John 3:
5. Jesus answered, "I tell you the truth, no one can enter the kingdom of God unless he is born of water and the Spirit.
6. Flesh gives birth to flesh, but the Spirit gives birth to spirit.
7. You should not be surprised at my saying, 'You must be born again.'
17. For God did not send his Son into the world to condemn the world, but to save the world through him.
18. Whoever believes in him is not condemned, but whoever does not believe stands condemned already because he has not believed in the name of God's one and only Son.
John 4:
24. God is spirit, and his worshipers must worship in spirit and in truth."
John 8:
16. But if I do judge, my decisions are right, because I am not alone. I stand with the Father, who sent me.
Peter I:
3:18 For Christ died for sins once for all, the righteous for the unrighteous, to bring you to God. He was put to death in the body but made alive by the Spirit,
3:19 through whom also he went and preached to the spirits in prison
3:20 who disobeyed long ago when God waited patiently in the days of Noah while the ark was being built. In it only a few people, eight in all, were saved through water,
4:6 For this is the reason the gospel was preached even to those who are now dead, so that they might be judged according to men in regard to the body, but live according to God in regard to the spirit.
4:11 If anyone serves, he should do it with the strength God provides, so that in all things God may be praised through Jesus Christ.
Peter II:
3: 7 By the same word the present heavens and earth are reserved for fire, being kept for the day of judgment and destruction of ungodly men.
Ishiah 45:18
For this is what the LORD says-- he who created the heavens, he is God; he who fashioned and made the earth, he founded it; he did not create it to be empty, but formed it to be inhabited-- he says: "I am the LORD, and there is no other.
By myself I have sworn, my mouth has uttered in all integrity a word that will not be revoked:
Before me every knee will bow; by me every tongue will swear. (Isaiah 45:23)
+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
+ Dongchan Kim +
+ Department of Astronomy +
+ University of Virginia +
+ Charlottesville, VA 22904 +
+ Tel: (434) 924-7494, Fax: (434) 924-3104 +
+ +
+ "For God so loved the world that he gave his one and only Son, +
+ that whoever believes in him shall not perish but have eternal life (John 3:16)." +
+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
John 14:10
The Spirit himself testifies with our spirit that we are God's children. - Romans 8:16.
For this is what the Lord says- he who created the heavens, he is God; he who fashioned and made the earth, he founded it;
he did not create it to be empty, but formed it to be inhabited- he says:
"I am the Lord , and there is no other. (Isaiah 45:18)
Church help line: required amount, received amount from church, donated amount from people have to match.
Otherwise, delete the list.
Davin's SSN: 217-73-7364
Suvin's TIN: 975-73-9410
Forwarding addresses are:
USA: DongChan Kim
4565 N. Figueroa St.
Los Angeles, CA 90065
U.S.A
Korea: Postal Code: 626-810
DongChan Kim
BumEh-Ri 684-9
MulGum-Up, YangSan-City, KyoungSangNam-Do
S. Korea
0523-385-0495
626-810
palomar observatory job
university of arizona job
steward observatory job
keck observatory job
mauna kea observatory job
DongChan Kim
KangNam-Gu, ApGuJung-Dong
HanYang Apt. #9-109
Seoul 135-794, Korea
0551-267-1611
Zip code: 135-230
DongChan Kim
KangNamGu, IlWonDong 615-1,
GaePo HanShin Apt. 104 Dong 405 Ho,
Seoul, KOREA
TIAA/CREF, contact number -> C5547819, U5547817, 3456137, uid=dongkim2, p=honolulu100, shin,Tel 1 800 842-2252
106069 (7280)
YangSan City MulGumUp BumEhRi 684-9
MapoGu DoWhaDong 22, ChangGang BLD 1222Ho, 82-2-719-0400
IBAMA: Brazil Environment Beurou
Tonex: 02) 3444-0741, jungijipjingi, talchifilter
575-672706
208-528-2090
JeongPanggiup: 02) 275-9116, hudaeyoung ganyisechuckgi.
Book: Ilsayusa.
Magnetic shields.
Electrosensor.
Sendai city recycling center.
cosmos tongsang, noodle machine
ln -s /img1/archives /img1/wwwned/httpd_demo/archives
dry batteries: Foster McLean (Bulding 261).
:g/+[1234567890]d/s/+/+0/g
:g/-[1234567890]d/s/-/-0/g
:g/ [1234567890]h/s/ /+/g
:g/ [1234567890]h/s/ /-/g
:g/ [1234567890]\./s/ / 0/g
:g/ -[1234567890]\./s/-/ -/g
:g/+[1234567890]d/s/+/+0/g
:g/-[1234567890]d/s/-/-0/g
%s/HI ,-,/ - , - ,HI , - ,/g %s/2cm ,-,/2.00E-02, - ,2cm , - ,/g
%s/6cm,-,/6.00E-02, - ,6cm, - ,/g
%s/6cm ,-,/6.00E-02, - ,6cm , - ,/g
%s/6cm ,-,/6.00E-02, - ,6cm , - ,/g
%s/11cm,-,/1.10E-01, - ,11cm, - ,/g
%s/18cm,-,/1.80E-01, - ,18cm, - ,/g
%s/21cm,-,/2.10E-01, - ,21cm, - ,/g
%s/20cm,-,/2.00E-01, - ,20cm, - ,/g
%s/20cm ,-,/2.00E-01, - ,20cm, - ,/g
/crystal/gump/g /conv -sexhrs /g / equ B1950 equ B1950/g
/sexhrs/decdeg/g ra.in > cra1950 ra.in > cra2000 ra.in > ra2000 /0 equ B1950/0 equ J2000/g
Inflation with relativistic velocity = time expansion? How to accelerate infinite mass into relativistic velocity?
AUTHOR Nayler, G. H. F.
TITLE Dictionary of mechanical engineering / G.H.F. Nayler.
EDITION 4th ed.
IMPRINT Warrendale, Pa. : Society of Automotive Engineers ; Oxford,
[England] ; Boston : Butterworth-Heinemann, c1996.
COLLATION vii, 454 p. : ill. ; 24 cm.
SUBJECT Mechanical engineering -- Dictionaries.
TITLE Illustrated dictionary of mechanical engineering : English,
German, French, Dutch, Russian / [V.V. Schwartz ... et al.]
IMPRINT The Hague ; Boston : M. Nijhoff Publishers ; Hingham, MA :
Distributors for the U.S. and Canada, Kluwer Boston, 1984.
COLLATION 416 p. : ill. ; 25 cm.
NOTE Includes indexes.
Dictionaries, Polyglot.
ALT AUTHOR Shvarts, V. V. (Vladimir Vladislavovich)
LOCATION CALL NO. STATUS
Aero TJ9 .I37 1984 LIB USE ONLY
TITLE McGraw-Hill dictionary of mechanical and design engineering /
Sybil P. Parker, editor in chief.
IMPRINT New York : McGraw-Hill Book Co., c1984.
COLLATION 387 p. ; 22 cm.
SUBJECT Mechanical engineering -- Dictionaries.
Engineering design -- Dictionaries.
ALT AUTHOR Parker, Sybil P.
McGraw-Hill Book Company.
ALT TITLE Dictionary of mechanical and design engineering.
LOCATION CALL NO. STATUS
EERL Ref TJ9 .M395 1984 LIB USE ONLY
AUTHOR Newmark, Maxim.
TITLE Illustrated technical dictionary, containing standard technical
definitions of current terms in the applied sciences, graphic
and industrial arts, and mechanical trades; including air
navigation, meteorology, shipbuilding, synthetics and plastics;
with illustrations, technical data, and interconversion tables.
Edited by Maxim Newmark.
IMPRINT New York, The Philosophical library [1944]
COLLATION 3 p. l., vi, 352 p. illus., diagrs. 24 cm.
NOTE RETRO 3.
SUBJECT Technology -- Dictionaries.
LOCATION CALL NO. STATUS
Mil-8 Ref T9 .N4 LIB USE ONLY
Tape copy:
dd if=/dev/nrst1 of=dev/nrst0 bs=20b
How to calculate "BS"?
Do "tcopy /dev/nrst1" and do ^c(capital) see size.
"bs=size/512"
특허
http://www.kipo.go.kr
enscript -G -fCourier10 -pjj j
qpr -Pqms2 -d jj
Andrew Baek: 310-422-9955, 714-738-8747
MyoungJun Lee: 714-521-0905
Jonathan Kang: 310-282-2322
Institute for Educational Leadership: Harold Hokins
10122
jetprint -Plaser146 -oduplex print_file_name
YongK Kim: 364-8230
promiser's group?
Study how Twian become #1 laptop manufacturer?
if cdrom drive on piaf doesn't working
do swap -s.
Call PTO 703-308-1202 if not received.
4328795 : Smokeless tobacco pipe
Water+carbon filter, DaeYoung Gumsok, 02-645-6227
ACCO USA, Inc.
770 South ACCO Plaza
Wheeling, IL 60090-6070
800-222-6462
847) 405-9000
Fax 800-247-1317
Fax 847-405-9020
Fax 847-541-5750 > old one
Global motors
Ring Binders:
double lock: 5354142
ring design: 4552478
Stockwell Office Product
P.O. Box ?5144
Westborough, MA 01581
823-1 Yeoksam-dong, Kangnam-ku
Seoul, Korea 135-784
Tel. 82-2-568-6077
Fax 82-2-567-9383
1.CD-ROM 검색 및 분석
(PATROM)
(CAPS)
(JPP)
(EP-A)
2.Web Site
PATROM
MicroPatent
USPTO
JPO
Derwent
IBM
3. On-line
DIALOG
PATOLIS
DaeWoo Motors Company
ADDRESS:
T.404-030, 199 Chungchun-dong, Pupyong-gu, Inchon, Korea
Tel: (032) 520-2114 Fax: (032) 524-4362
Kim TaeGou
http://www.trade.co.kr=com.trade
Kokuyo
Kokuyo Co., Ltd.
Public Relations Department
1-1 Oimazato Minami 6-chome Higashinariku, Osaka-shi 537 Japan
Arthur B. Moore
Chief Patent Counsel
Avery Dennison
Corporate Center
P.O. Box 7090
Pasadena, CA 91109-7090
ph: 818-304-2231
sunglasses: 5,382,986;5,114,218;
KyoBo MunGo: 교보문고
Emie's Food, Wholesome and hutty Food: Veggie burger
Economist : kimsu@www.joongang.co.kr
YoungJieuJip:BuGok-Dong, EuWang-City, KyoungGiDo.
Kokuyo Co., Ltd.
Public Relations Department
1-1 Oimazato Minami 6-chome Higashinariku, Osaka-shi 537 Japan
Havard Bussiness School Video
Gas Lighter
Green Earth Office Supply
There are four requirements for patentability: statutory class, useful, novel, and unobvious.
Submit tips for saving natural resources to the major newspaper :
ex. how to save wood consumption, ..
New business ans new product (dosol,8000)
Hanguk's marketing (20,000)
sinsangpoom gabalei 7 gaji sunggongbiguel (18,000).
China Risk(6,800)
Green.net: Patent search engine (http:www.gnk.co.kr), 90,000 won.
Monami:8p3*9L, second:5?>F?,GJ
Environmentally friendly product. rules for evaluating it and suggest it to Govenment.
Paper punch: 5503052, 5490440, 5429445, 5386638, 5247863, 5239904, 5150998, 4727610 (7/160, 227/156), 4724734 (83/549, 83/571), 4656907, 3906633, 3592092, D350564, D295192, D251600, D250,270, D250,269, 4240572 (ref)
Water spray: 5501400, 5464129, 5323968
EuroMax Icepan.
Think various ways of recycling: ex) bring old gift basket, you will be given phone card.
Vinegar drink
Give Him a Life: Hyun, HeaRan (Irvine), 714-509-4724
Binder:바인 다
Patent giseul JoungBo center:특허기술정보센터
Korea Inventor's club한국발명진흥회
World Wide Stationery Manufacturing Co. Ltd., Hong Kong
Binder Works, Inc.
591-T S. Walnut St.
La Habra, CA 90631-6035 USA
562-691-1941 FAX: 562-691-0791 Custom Ring
Bindertek
Sausalito, CA 94965 USA 415-332-8688 FAX: 415-332-2641 Binders, Filing Systems.
Beaverite Products, Inc., Information Packaging Products Div.
Beaver Falls, NY 13305 USA
800-424-6337 FAX: 315-346-1575
Mfrs. Of Binders For Industry, School. Specialists In All Types O f Binders
Charles Leonard: 310-715-7465
We hereby guarantee that we will treat your invention confidential and
will never start to produce, develope
or market your invention before coming to an agreement in writing, and
that all information received from you will
be confined to the staff in our company or to the persons directly
responsible for the development and manufacture
Make purse-like reusable carrier and give a $0.5 back to the people who bring it to the store.
WincomSoft, TongHap Graphic SW.
Ask to establish research institute within Southern Baptist Church
to do reforming laws and constitutions (prevent before not after). Solve root problem.
American Public Transit Association
1201 New York Avenue N.W., Washington, DC 20005
Tel: (202) 898-4000; Fax: (202) 898-4070; E-mail: info@apta.com
http://www.apta.com/
I would recommend you go to your local library and search the reference
section for the 1996 MANA book. This is the official guide for the
Marketing Association of North America. Each group of marketing companies
are listed by category of what they specialize in, and their locality,
phone, and fax is included.
Fred Ferino
miggs@asan.com: guiding catcher
JaeSoo Yoo: Korea Venture business information center chairman (02-557-2141)
JoengHyo An: KoKo Silver:631-6394
www.travelweb.com
Health pipe: DaeYoung Metal
Korea Invention JinHeung Association Patent to Bussiness connecting center 02-557-1077
www.cotis.net: import/export informaion net
Environment management complex rend support devision(02-519-0211-3.
Korea natural resources recycle coaperation industry support dev. 2)37739782~9
Korea industrial design promotion, Dadam Design.
Nedit
Hyundai Motor Company
140-2, Kye-dong, Chongro-ku
Seoul, 110-793, Korea
vice.president@whitehouse.gov
Science Experiment:www.jasontech.com
Telemarketing: TongPanLife, Nissen
Recycling theme park (recycle center, exchange center, food mart, ..)
Inventors' web site: http://www.nrc.ca/corpserv/nrc.html
World Fra: 2-517-8227, mini-vaccumm.
Search Japaneses web site with Korean: www.idetect.com
3-dimmensional cad assitent center: 0345-496-1052.
TV problems in Korea: Jin SeungHo Reporter, Choson IlBo
Static elliminator: SeoJin Tech, 6500won, 032-872-6142
10 best CEOs: Samsung Economic research center
ID : qqq13879
password : qqq13879
DongChan Kim
Group Practice: GOOD SAMARITAN MEDICAL PRACTICE ASSOCIATION
PCP Specialty: 3637262 - PEDIATRICS
Non-PCP Specialty: PEDIATRICS
3323 W Olympic Blvd Ste 210
Los Angeles, CA 90019
(213) 733-0127
Cho, Won Joon, MD
Group Practice: HPG-HUNTINGTON MEM HOSP
PCP Specialty: 396648419 - PEDIATRICS
Non-PCP Specialty: No Specialties
65 N Madison Ave Ste 310
Pasadena, CA 91101
(626) 796-5384
MRA Korea Branch: SeokKyu Kang, President of HoSeo University.
CIGNA Member service - 1-800-344-0557
North Korea: Hepa-B solution
Try looking at a program called Vdraft
They have a web site at http://www.vdraft.com
MS-Zone (static elliminator)
Kiki-rang, Toro-rang, 080-728-7288, traffic educational cd-rom
EMF detector: TRIFIELD METER(Cat. # A150) $139.00,
Trifield Extended Range Meter (Cat. # A155) $189.95
Magmetic Field detector: ElectroSensor (Cat. #A144) $24.95
SAFE RANGE EMF METER (Cat. # A140) $29.95
ORDER BY PHONE: 1 - 8 8 8 - L E S S - E M F, Practical Product
book: Why Didn't I think of That
Patrom: ID: qqq17448, qqq17448, DongChan
1/20won: cholesterol suppression, JBB-1, SungMin Byun: Life Science Institute.
dangryo:IlYang Pahmarcy
(1101) 800-426-528-1407-000-5557-131-501
800-426-528-1421-766-1219-993-888
nursing pad: 572376,
linux Customer Account number is 0021257 and passwd is DongChan
linux: passwd dckim, 12345
http://terraserver.microsoft.com/
rmt/1l
rmt/0m
creation musium, show them details of the creation process.
Show real experiment and let them feel.
https://nbs-web02.jpl.nasa.gov/
makuhariMese: 043-296-0001 (convention center), 043-296-9999 (event hall).
Big site (03-5530-1100)
flounder: special protain
Yi: 577-6091, 395-2518
KOTRA
Avery Dennison Korea, Ltd.
5Fl.,Cheongku Bldg., 517-5, Shinsa-Dong, Kangnam-Ku, Seoul, Korea 135-120
Consumer Information Phone: (82)-2-545-4939 Fax: (82)-2-546-1829
Technical Support Phone: (82)-2-545-4939 Fax: (82)-2-546-1829
Sup Hur, 82-2-264-5890
Avery China: 86-21-6482-1208, Fax: 86-21-6482-1210
Semire: 2-593-0021, fax:2-592-4275
AVERY K & M 3528 Boulevard Torrance, CA 90503 Tel:310 543 1553
National Transportation Safety Board
490 L'Enfant Plaza East, S.W.
Washington, D.C. 20594
Attn: Office of Safety Recommendations
http://www.wal-mart.com/win/how.html
yi@shemesh.gsfc.nasa.gov
yi@lodur-gw.srl.caltech.edu
UNFPA(UN F Population A)
JingYoung Yi, 2-844-7564
floppy: volcheck
KyoungBoo: TongDaeMoonGu YoungDoo (1290380), KB Bld.
927-5826/7, 928-5115, fax:928-5115, YoungKwan Kim
Island mission: SangSu Kim, 011-733-8555, 032-564-8501/2 (JinSan Ko)
104794-0030587 (HyunJu Han), KEB: 114-18-19598 (Kim)
Flex-o-lite signal night flasher, 3500378, 4237405
tiff?
Young-Soo KIM
23 Sherrick Green Road
Dollis Hill
London, NW10 1LB
UK Patent application number: 9822718.4
Woody Haralson: QVC
Third street elementary school
SERRA LASER CENTER
1740 N. Orangethorpe Park
Anaheim, California 92801-1138
http://www.serralaser.com
Tel: (714) 680-6211 Fax: (714) 680-6213
dckim, astro1, thomasregister
2631-2736
IP: 140.109.177.59
DNS: 140.109.177.3
140.109.1.10
gateway: 140.109.177.1
netmask: 255.255.255.0
You will need to decide what you are compiling into the kernel, and what as modules, but should take the above points into consideration. The actual
choices are made during the compilation, by the second of the following sequence of instructions:
cd /usr/src/linux
make menuconfig
make dep clean modules modules_install zImage
Read Mail
Subject: CREDIT CARD 05/19/1999
DEAR DONG CHAN KIM,THANK YOU FOR
YOUR MESSAGE.FIRST YOU NEED TO SET
UP THE CREDIT CARD AS A PAYEE.FILL
OUT THE FORM THERE ON ADD PAYEE.
WAIT FOR IT TO BE SETUP (5 BUSINESS
DAYS).TO YOUR SYSTEM.THAN CLICK ON
BILL PAYMENTS .THEN MAKE PAYMENTS.
THAT'S IT.AND FOR ANY OTHER COMPANYS
YOU WANT TO SETUP.
REGARDS, CARROLL
Having done that, the module dependencies need to be mapped out. This is done with the following command:
UKIRT/99B/10
AA user name: ygm534ty
passwd:acy502sr
amazon dckim.uva honolulu!
masan-ch.ed.kyongnam.kr
sun cream: italia cancer institute
ibm: dckim, inventor
Otugi Ballpen
EndSection
sndconfig
DMA=01, irq=10, es1878pnp
melalueca: eunju1, 20664753
www.catalog-news.com
Edit /etc/sysconfig/harddisks and uncomment the line with USE_DMA=1.
This re-enables DMA which speed up my buffered disk reads by a factor of 5 (from 4 MB/sec to 20 MB/sec).
Use the "hdparm -T -t /dev/hda" command to check the performance if you are interested.
-------------------
Check out Trib-Gel - its a Cold Welding Agent -and will readily join metal
parts as one part is forced or inserted into another - it is an alternative
to adhesives in many applications and it is much stronger. It gives instant
strength -it has no cure or cooling time -because it makes a genuine cold
pressure welds. You can read the story at www.tribtech.com. There are many
innovative assembly solutions illustrated in the application notes. This is
a new idea that innovators and inventors should be aware of.
-------------------
uni graphics solution
freezed tofu
Asia File
Plot 16, Kaw. Perindustrian
Bayan Lepas, Fasa IV, Mukim 12,
Bayan Lepas,
11900 Penang, Malaysia
Tel: 04-6426601, Fax:04-642-6602
LimSoonHee
kangsoochoi
forJesus
Nature: dckim, dongchan
mug that removes garlic
psnup -2 -w21.6cm -h28.0cm psfile.ps | lpr
psnup -w21.5cm -h26.5cm -2 test.ps > test1.ps
KangYong Lee: ChangWon City SangNamTong 45-1, SeungWon Apt. 312Dong 1085Ho (0551-266-8284)(T641-010)
Leadingedge: Mega SangSa, Game_BonBu (dancing machine)
seoul@kipa.org
www.bizkr.com:internet trade support software, Laicos too check it out
(http://etlars.etri.re. kr: provides prospective bussiness items in 21st century
anon-ftp.ipac.caltech.edu
DongChan;searchjob
dongckim;dongchan;jobbank
ttp://www.microsoft.com/msdownload/iebuild/ime5_win32/en/ime5_win32.htm
tp://www.unionway.com/ts/index.html
SamilGongup: doorlock that unlocks with pull, push, or turn (2-335-1197)
WonBang Electronics: EM warnning alarm (02-2214-4757)
www.sba.gov
process brown rice to more palatable
Make Payment
Your payment has been scheduled with transaction number 365001.
If you're using money management or spreadsheet software, don't forget to download your payments before you sign off.
UNFPA: UN population ..
JongTae: 551-261-8070
Park Fax: 551-294-0065
Park Tel: 551-297-4025
Choi JunDoSaNim: 8665-6634 (CP: 0930-159-643)
Anti-hack software
http://www.silkroad21.com
PHP web-db programming guide(JJH).
WangKun? (2841-3963, ext14, Ms Seo).
Simbad: t778extr, passwd: e7x7t8
nature:dckim, dongchan
mysql: rlogin iaa1 and cd /usr/local/mysql/bin and type mysql -h iaa1
HanGul97: 79734541-00000208
suction cup
hansoft:dongckim, 435718
checkgalpi-pen
regedit,edit-find,productkey input, next number is the product number
www.daewootrade.com
http://www.william-a-kolb.com/billko/poohstainste.html: pooh ring watch $24.95
http://www.imageexchange.com/featured/mocala/4627.shtml: $30.0
http://store.yahoo.com/freethought/sailmoonrinw1.htm: 6.95
Wang Chien Shien, 2841-3963, fax: 2841-3964, www.cswang.org
Garlic ordor: Pacelery will remove it completely
napster, Gnutella, freenet
Tanita breath alert: bad breath buster
Bushnel: $400.0 telescope
www.kojima.net: spelling checker, Y5800
www.powertank.com
v-commerce: online shop supplier
hohyunkim
http://mybible.pe.kr/page1.html
www.kitf.co.kr: small company program
netian: dongckim, 12345
Dukpyo: 02-517-3931~2, 핸드폰) 011-351-6171
For the first two images, I have removed cosmic rays from near the object, but not the entire image. There should be few if any cosmic rays in the third image.
Most data parameters of interest should be in the header. The gain in each image has been converted to 1. from an original 1.74. Readnoise is 10e.
The data is photometric with a photometric solution of:
m=-2.5*log(cnts/et)+(25.47+-0.01)-(0.07+-0.01)*(am-1.0)
Given name: DongChan
Family name: Kim
Nickname: dckim
Your MediaRing ID: 6188555
Your MediaRing account e-mail: kim@asiaa.sinica.edu.tw
Your Password: 12345
etoys: dongchan, Your Confirmation Number is: Your Order Confirmation Number is: 000825192930
consummer can check credit of the company
Caltech: We are committed to making a good faith effort in achieving the goals of
this program. As a major part of our strategy, Tina Lowenthal of the
Purchasing Services Department leads our small and disadvantaged business
outreach activities.
Bongchul: 2632-5112, hp 011-9975-5112
www.tradecard.com)는 뉴욕에 본사를, 홍콩에 사무소를 두고있다.
./S98sshd
browser invention
41622
www.bigtrust.com
computer+ion-generator
http://www.venturezip.com;dongchankim, dongchan
hyejinchung@hotmail.com
bestbuyer.dreamwiz.com/maindream/index.php3
www.willsearch.co.kr:internet TV
K4HVD-Q9TJ9-6CRX9-C9G68-RQ2D3
global communications technology
ccie, ccna
world ongly P.O. Box 63, Taichung, Taiwan, R.O.C. Address : No.258, Yungming St, Dali City.Taichung, Taiwan Telephone : 886-4-4076771 Fax : 886-4-4076757, 4076758
www.cherrycorp.com: keyboard
www.belkin.com: mouse
keyboard: http://www.genovation.com/computer/custom.html#pictures
sma: sma_web, smasma@$10
patent display: 02-557-1077(ext.교환 501~7).
SNU: sinkisul changup network
hchen@net.com
portable water quality analyzer: Techno
Storex: 2195 Place Thimlns, St. Laurent, QC
H4R 1K8, Canada
Media matrix: market research organization
honeycom: ordor elliminator(8000won, 02-555-4464)
www.cryptotelecom.com: cryptocam
S7S global net (snsgp.com)
jobsqure: dongchankim, dongchan
H1: kim@asiaa.sinica.edu.tw
dongchan
mechanical watch with feeling
02-837-1808: ear vacuum
Electopia: vacuum mop; 031-872-5033
Carson Electric: car refrigirator: 0346-557-0120
Hot touch: Academitech: 02-992-5431
Dust mask: Korea 3M
Winners: safty plug, STM, 02-477-7242
tofu maker: ionmag, 28,5000, 02-859-8682
caption camera: gyelim21.com
www.doctortex.com: anti-EMR apron
Can cap: ideabank114@orgio.net
finger DDR: myhome.hananet.net/~sam6417
sendmemail.com-ask customer to request what ad. he want to receive?
passwd:chb212123
church revolution consulting
www.kotis.net www.eckorea.com www.ec21.com www.digitalkorea.com www.eto.com altavista
freshness sensor for fish check all biosensors in industry
bestbuyer.co.kr, clickprice.co.kr halfclub.com
factory direct market hosting
한글
findall: dongkim2, 1234
저장성 이우
patent:dongchankim, 123456, posting number: 15880
nong: 1528
okBible: dongkim, abc123
psnup -2 -w8in -h11in
Corinthians I 1:18
Corinthians I 2:10 (but God has revealed it to us by his Spirit. The Spirit searches all things, even the deep things of God.)
Corinthians II 2:5 - 1. Now it is God who has made us for this very purpose and has given us the Spirit as a deposit, guaranteeing what is to come.
hancomm:dongkim2,1234
Mail Payments to: AT&T Universal Card
P.O. Box 8029
South Hackensack, NJ 07606
Spy war between the USA and Japan (roket)
Holy Spirit: 2 Cor. 3-5 (search Holy Spirit).
353-04-486820
EunJu: 670914-2637726
hst: dongkim, 7inagn2g, or dckim, 2wv1lnc (one el)
KAL: dongkim2, 12345
Kim, JiHee: 018-310-5684, 365joyful@hanmail.net
NorthWest: Dr Dongchan Kim, 496191452, 1234
S Kim: 310-288-0227
Empas or http://www.usenetsolution.com, Bada Mailer, Bada mail collector
Mathew, 11:12-14(John=Elijah)
전자거래분쟁조정위원회
sunlee@lvcm.com
Auto_repair_shop service price list
How to lose a guy in 10 days
What, then, was the purpose of the law?
It was added because of transgressions until the Seed to whom the promise referred had come.
The law was put into effect through angels by a mediator. (Gal 3:19)
UAL: 00617136295
Yamato: 0505-693-1131
------------------------
NVIDIA_GLX-1.0-1541.i386.rpm
NVIDIA_kernel-1.0-1541.src.rpm
or maybe
RedHat 7.1, one CPU, uniprocessor kernel
NVIDIA_GLX-1.0-1541.i386.rpm
NVIDIA_kernel-1.0-1541.rh71up.i386.rpm
.........................
Install the RPMs. The commands needed are:
rpm --rebuild NVIDIA_kernel-1.0-1512.src.rpm
rpm -ivh /usr/src/redhat/RPMS/i386/NVIDIA_kernel-1.0.1512.i386.rpm
rpm -ivh NVIDIA_GLX-1.0-1512.i386.rpm
Edit your /etc/X11/XF86Config-4 file: Change the line containing Driver "vga
(or Driver "vesa") to read Driver "nvidia". Also, make sure that within the
Section "module" part of the file, you have a line that says Load "glx", and
that you comment out (put a # character at the start of the line) the lines
reading Load "GLcore" and Load "dri".
Becuase I'm not completely sure about the refresh rates I'm using, I've
added the line Option "UseEdidFreqs" "on" into the Section "Driver" part of
the XF86Config-4 file. Note that this only works with the nVidia drivers,
and not with the vesa drivers described above.
-------------------
9. I then moved to the directory where I copied those two files. (most likely /home/whatevername if you followed my way). Then, I issued the following commands:
rpm --rebuild NVIDIA_kernel-1.0-1541.src.rpm
rpm -Uvh /usr/src/redhat/RPMS/i386/NVIDIA_kernel-1.0-1541.i386.rpm
rpm --rebuild NVIDIA_GLX-1.0-1541.src.rpm
rpm -Uvh /usr/src/redhat/RPMS/i386/NVIDIA_GLX-1.0-1541.i386.rpm
-------------------
mkdir /mnt/windows
mount -t vfat /dev/hda1 /mnt/windows
--------------------
JaeIl Bank: 328-20-059821
School of Earth and Environmental Sciences
College of Natural Sciences
Seoul National University, NS89
San 56-1, Shinrim-9 dong, Kwanak-ku
Seoul, 151-747, Korea
텍스쿨: 양천구 신정4동 985-3, 502호, 536-7992, 2698-1072
gmc: astro!
radiokorea: dongkim2, 12345
MODERN COSMOLOGY AND THE CHRISTIAN IDEA OF GOD
ochid: dongkim2
Young earth creationist
iris_data, fissurvey, irlab106
% xgterm
xgterm: error while loading shared libraries: libncurses.so.4: cannot open
shared object file: No such file or directory
This is a known problem with how the binary was built and RH7/8 systems.
The simplest solution is to just create a symlink to satisfy the
dependency, i.e. as 'root' do
# cd /usr/lib
# ln -s libncurses.so.5 libncurses.so.4
Alternatively you could recompile the system from the sources and you should
then be able to run xgterm normally.
Additionally, you may encounter another problem starting xgterm under RH8
caused by the xgterm trying to write a /var/run/utmp entry without the
proper permissions, this causes the window to appear briefly and then shut
down. The workaround is to either start it as "xgterm -ut" to disable
this utmp entry, or else change the permissions on the binary as root using
# chown root:root xgterm
# chmod g+s xgterm
미국영화 협의회 (MPAA)
mount /dev/sda /mnt/disk - usb hdd
no page number: \pagestyle{empty}
add line in /etc/fstab to use hdb1
astrof: ATI radion ve, via tech, vt8233ac97
하나님을 믿으면 인생의 항로가 자동조정이다
누가복음 15장, 불신자에게 무엇이 중요한지 알려라!
Extinction in Different Bandpasses
----------------------------------
Assuming an R_V=3.1 extinction curve, the dust maps should be multiplied
by the value in the final column to determine the extinction in a given
passband. The standard optical-IR bandpasses are represented by the CTIO
and UKIRT transmission curves. For further details, see Appendix B of the text.
Filter name LamEff A/A(V) A/E(B-V)
---------------- ------ ------- --------
Landolt U 3372 1.664 5.434
Landolt B 4404 1.321 4.315
Landolt V 5428 1.015 3.315
Landolt R 6509 0.819 2.673
Landolt I 8090 0.594 1.940
CTIO U 3683 1.521 4.968
CTIO B 4393 1.324 4.325
CTIO V 5519 0.992 3.240
CTIO R 6602 0.807 2.634
CTIO I 8046 0.601 1.962
UKIRT J 12660 0.276 0.902
UKIRT H 16732 0.176 0.576
UKIRT K 22152 0.112 0.367
UKIRT L' 38079 0.047 0.153
Gunn g 5244 1.065 3.476
Gunn r 6707 0.793 2.590
Gunn i 7985 0.610 1.991
Gunn z 9055 0.472 1.540
Spinrad R 6993 0.755 2.467
APM b_J 4690 1.236 4.035
Stromgren u 3502 1.602 5.231
Stromgren b 4676 1.240 4.049
Stromgren v 4127 1.394 4.552
Stromgren beta 4861 1.182 3.858
Stromgren y 5479 1.004 3.277
Sloan u' 3546 1.579 5.155
Sloan g' 4925 1.161 3.793
Sloan r' 6335 0.843 2.751
Sloan i' 7799 0.639 2.086
Sloan z' 9294 0.453 1.479
WFPC2 F300W 3047 1.791 5.849
WFPC2 F450W 4711 1.229 4.015
WFPC2 F555W 5498 0.996 3.252
WFPC2 F606W 6042 0.885 2.889
WFPC2 F702W 7068 0.746 2.435
WFPC2 F814W 8066 0.597 1.948
DSS-II g 4814 1.197 3.907
DSS-II r 6571 0.811 2.649
DSS-II i 8183 0.580 1.893
You may receive in time of need, guidance in life's problems, a knowledge of Jesus Christ, hope for the future, peace of mind, and an assurance of eternal life.
CFHT: dongckim, 12345
tdump test3.tab columns=@col.list pwidth=256
tdump k00091m0738.tab columns=@col.list pwidth=256 cdfile="" pfile="" > k00091m0738.txt
col.list
----------
SMA
INTENS
INT_ERR
ELLIP
ELLIP_ERR
PA
PA_ERR
X0
Y0
MAG
MAG_LERR
MAG_UERR
B4
B4_ERR
STOP
Joshep, Daniel, Jehoshua - triumph after hardship
日本國 兵庫縣 寶塚市 泉が丘 12-22
Day-age theory: Gerald Schroeder, Russell Humphreys
raw data directory
/net/subway1/user1/jjsohn/POP/CFH12K/Data/Zsource
reduced data
/net/subway1/user1/jjsohn/POP/CFH12K/Data/Flipsdata/Acomb
JAXA: iris_data, fissurvey
visa: 4642, 11/28, -70
핵산: 30억쌍, 500페이지 200만권부량, 1000m^3 (10x10x10)
iloveschool: tongchankim 12345
미우라 아야코, 엔도 슈사코 (신성일 목사님으로 부터)
동물창조의 순서를 책으로. 창세기 포함.
The Selfish Gene by Richard Dawkins
<과학과 기독교: 충돌 또는 결합(Science and Christianity: Conflict or Coherence)>
Size of the human - if wind blows, too small or large size will have big problems - Size of the Earth matters
캄브리아기 (5억 4천만년전 - 4억 9천만년전) 중 5억 3천만년전 과 5억2천만년전 사이에 거의 대부분의 동물들이
나타났음 (창세기 1장 20절의 수상식물과 공중의 새의 창조와 관련있음). 50종류의 문, 현재 약 37문의 동물들이 있음.
이를 캄브리아 폭발이라고 부르며 다윈의 진화나무를 꺼꾸로 세워놓은것 같이 보임.
영국 이매뉴엘 칼리지: 창조론 교육
공현표, 한원영 (항공우주공학), 김덕호 (응용화학), 변준석 (법학과), 임동균 (사범대)
L_FIR
1.915e53*1.26e-14(2.58*f3+f4)*C*zq^2 - C=1.4-1.8
or
8.00e26*FIR*zq^2 (FIR=1.26e-14(2.58*f3+f4)) = 10.08e12*(2.58*f3+f4)*zq^2
data all.amh read {z 2 f3 29 f4 30 s 38} set z=(z*(1+0.5*z))**2. set l=1.008e13*(2.58*f3+f4)*z set l=lg(l) print {l}
ebonart@hanmir.com
1. catalog sale
2. do-it yourself merchandise
3. read trend - nike vs. rebok
4. flexible work hour (gem stone selling)
5. hagen-daz - best quality
6. upside down udon house
7. calendar starts with November
8. hotdog+sandwich+french-fry, different looking style
9. nature company
10. tooth-paste for business women (ebis set - toothpaste+brush)
11. cafe-de-avang (ganda-eki), toriba: standing coffee shop (aoto coffee machine, sell sandwich, best quality cups, spoons, etc... check interior)
주소서비스회사(directory service company), 신용조사회사 (credit service company)
www.eylangs.com: cosmetic
광두: 017-588-8548
종태: 011-586-5735
병규: 011-564-4512
덕표: 011-351-6171
추제: 011-865-4703
봉철: 011-9975-5112
기철: 018-305-7902
상현: 016-312-8292
농협: 07002843452
강용: 011-846-8288, 상남동 45-1 성원 아파트, 312-1805
유만: 019-417-0902
병천: 019-351-4535
재만: 011-9817-5193
누나: 011-9311-5718
형건: 016-598-5718
현희: 016-780-0145
원종: 011-898-7983
군석: 011-864-9290
동만: 011-9926-0184
용익: 019-295-3621
MyoungSuk: 011-579-5606
JangWan: 582-9798 (H), 585-2255 (W), 011-9534-9798, 55-636-2855 (Hacheung)
DongSu: 055-541-0161
yongTek: 017-844-2798
SangHo: 273-3787, Dawon 81
sangun: 055-277-1432
김인환 목사님: 011-336-0827
동수: 011-558-1343, 경남진해시 석동 139-1
석봉토스트, 연봉 1억신화
Church of New Nations (CNN)
9532 Oakhurst Drive, Columbia, MD 21046. (301) 362-1536 / www.i-CNN.org
hanmail: dongkim12345, 641217 -2829817
AA: 7R869K6
pgplot: /root/pgplot/makemake /root/pgplot linux g77_gcc
in root directory gunzip pgplot5.2.tar.gz
738 tar xvf pgplot5.2.tar
744 mkdir /usr/local/pgplot
745 cd /usr/local/src
746 cp ~/pgplot5.2.tar .
747 gunzip -c pgplot5.2.tar.gz | tar xvof -
748 gzip pgplot5.2.tar
749 gunzip -c pgplot5.2.tar.gz | tar xvof -
751 cd /usr/local/pgplot
752 cp /root/pgplot/drivers.list .
753 vi drivers.list
755 /root/pgplot/makemake /root/pgplot linux g77_gcc
765 cd /usr/local/pgplot
767 make
768 make clean
769 vi ~/.bashrc
770 source ~/.bashrc
772 ./pgdemo1
wip: change f2c to g2c in makewip and
do ./makewip -pgplot /root/pgplot -xlib "/usr/X11R6/lib"
A matter of day, The Science of God
www.linuxcompatible.org/thread27947-1.html
ellipse i12540p5708a.fits x0=303.67 y0=327.53 ell=0.0 sma0=15
http://www.koreandc.com/restaurant/list.cfm
ear wax remover (one side wet, other side dry)
http://www.kstudent.com
옜� 옜�(Moral Majority), 옜� 옜옜 옜 옜옜 옜� 옜� 옜옜� 옜�(Christian Coalition)� 옜 옜� 옜옜 옜� 옜 옜옜.
My HMO insurance number is 141289171 and address is
"P.O. Box 6233, Rochville, MD 20845" and phone number is 301-255-4000.
quixtar: 3506053, dph199111
geico: 4021075793, FED-4GJDEI-6BEC2J, u:dongkim12345, p:123456
nicmos archive ftp: veilleux62957, ftp://archive.stsci.edu/
---------------------------------------------
componentN Npar
value1 lowerlimit upperlimit stepsize tolerance fix(-1)/free(0)
stepsize should be fixed if linked (F1/F2(0.333), W1/W3(6548/6583), width=1
---------------------------------------------
# Sun 22:41:04 06-Jun-93
begin test_i1 #file name of initial
task specfit
components 4
linear
gaussian
gaussian
gaussian
linear1 2
2.693334E-16 1.000000E-18 9.000000E-13 1.000000E-17 1.000000E-5 0
0. -5.000000E-15 5.000000E-15 1.000000E-20 1.000000E-5 -1
gaussian2 4
7.357765E-15 1.000000E-18 1.000000E-11 0.333 1.000000E-5 4
7391.481 6550. 8500. 0.99463 1.000000E-5 4
520.6982 10. 3000. 1. 1.000000E-4 4
1. 0. 1. 0.01 1.000000E-5 -1
gaussian3 4
3.102005E-14 5.000000E-18 5.000000E-11 1.000000E-16 1.000000E-5 0
7409.43 6570. 8500. 0.5 1.000000E-4 0
569.231 10. 3000. 5. 1.000000E-4 0
1. 0. 1. 0.1 1.000000E-5 -1
gaussian4 4
2.209539E-14 1.000000E-18 3.000000E-11 1.000000E-16 1.000000E-5 0
7431.388 6580. 8500. 0.5 1.000000E-4 0
520.6982 10. 3000. 10. 1.000000E-4 0
1. 0. 1. 0.1 1.000000E-5 -1
specfit spec=test.imh init=test_i1 final=test_f1 Sample=7300-7500 plotdata=yes plot_file=test_d1
specfit spec=f27.fits init=f27.2a final=f27.2b Sample=7200-7500 plotdata=yes plot_file=test_d1
need sffx.d
-------------------------
begin fx.d
task specfit
intervals 0
---------------------------------------------
1-800-FOR-MERCEDES
1-800-367-6372EDES
I have a 95 C280 and recently replaced my temp bulb in my cluster. It was fairly easy, and I did not pull off my steering wheel or have any specailty tools. I pulled the tweeter cover to the left of the console and then pulled the tweeter off to the side. Next, pulled off the heater duct cover(under the tweeter)-it comes out with two screws then by depressing two small clips in the bottom of the heater duct cover. I then had enough room to fit my hand behind the cluster and carefully push it out. I did however, cut a small bit of coat hanger, fashioned a small loop on one end(to fit over my thumb) and the other end I bent over in a small catch, to aid me. Once I got it pulled loose, unclipped the two connections on the back, I was able to(at the correct angle) pull the cluster free.
hope that helps,
-M
Mercedes-Benz C180, C200, C220, C230 & C250 (Haynes)
WDBHA24G7XA788989
Tee imprint, astronomy, physics, any high-tech or pure science department
ex) ngc123 observed on Oct.23, 2003
ByungChun 016-560-4674
Yoshiro Kajii, hesede@mwd.biglobe.ne.jp, kyascho@hotmail.com
UMID: SSN, PIN: 641217, Directory ID: dkim21, U ID:641217
the insurers offer first-time accident forgiveness.
Mother: 06-27
United: dongkim, dongkim2,00326843130 - old
saralee789@hotmail.com
astrof, dckim, dckim123
Jeong Kim, Landover, Maryland, Lucent Technologies president of its Carrier Networks business unit within Lucent's Data Networking Systems (DNS) group
President of Lucent Optical Networking Group
Institute For Systems Research &
Electrical and Computer Engineering DepartmentA.V. Williams Bldg (bldg # 115) room #2405, University of Maryland
College Park, MD 20742-3285
Dept. of Electrical and Computer Engineering University of Maryland College Park, MD 20742
enscript j.cl --margins=30:0:0:0 -oj30
psnup -2 j30 > j30a
libra:C옜
juno: dongkim.2, 12345
cox.com
Genius research
reflection tape for highway patrom cars
orchid.ess.sunysb.edu: dbs 7399
xhost problem: use ssh -X instead of ssh.
Steve Kim: 461 N Faring Road, L.A. CA 90077 (310-288-0227)
FCC: Kevin Martin
mizutani osamu, Kids, your are not wrong!
mr vegetable market
cellphone: cash, door key,
Thimoty 6:17
PID: 3187
Title: The Evolution of Activity in Massive Gas-Rich Mergers
% U$eRnAm3: MERGER_EVOLUTION
% p4$sw0Rd: paxvobiscum
IRS data: username: veilleux@astro.umd.edu and then: r$ChM3rG, PID: 3187
try username: veilleux@astro.umd.edu
and then: r$ChM3rG
Spitzer Observations of a Complete Sample of Luminous Infrared Galaxies in the Local Universe
PID: 3672
Jeff Lee: Lee and associates) - send mail
Davin: 710414975
Suvin: JR1683600
masterrhee@aol.com, Lee JunGu, 4068 Rosamora Court, Mclean, VA 22101
greenhouse effect, if blocks sunlight, photosysthesis rate changes that effect animal life
1 Peter 4:6, explanation
2 Peter 1:17
Write letter to the riches!
i-CNN, GMC, KCM, KBS, UMKC, Samil, Kosta, IKEA, Hanarum, Lotte, KoreanKorner, restraunt, UMKGSA, cooking, library open hours, parking rate,
Eggcups: /usr/sbin/prelink /usr/lib/libdbus*so*
Sell top 20 best selling items
wpines.com: sticker
VGX:vgx pharmasutical
MAC: 00:0F:1F:23:91:D9
sinho.jung@duke.edu
EIf Atochem korea
produce talk database
Bae TaeHo, sinjeung 옜� (121-140) 옜 옜� 옜�325 옜옜옜옜� 1108-1202
bb= llx lly urx ury
-----------
I simply issued the command:
modprobe -r ehci-hcd
and the drive was immediately detected, mounted, and available for use.
Every time I boot I must re-issue this command for it to work again.
Not sure why removing the "ehci-hcd " does this...but it works.
2.) su
3.) enter root password
4.) mkdir /mnt/external
5.) mount /dev/sda1 /mnt/external -t ntfs
6.) cd /mnt/external
7.) ls
This will mount your hard disk to the folder /mnt/external.
NOTE: The "/dev/sda1" bit varries according to your USB port. It could be "/dev/sda2" or "/dev/sdb1" etc... To find out what it is try the program "usbview". I think knoppix has usbview.
YoenSuk Kim, 808-384-0949-cell?, 808-599-4705-home
---------
user: slirgs
pwd: #StarBursts!
ml-1740-1
BOX puts axes around the plot region, labelling the lower and left
according to the values set by LIMITS and TICKSIZE. If the arguments
are included (default 1 2 0 0) they are used as ILABEL arguments for
the bottom, left, top and right hand axes respectively, where 0 means
no labels, 1 and 2 specify the direction of ticks (see AXIS), 3
means omit both tickmarks and labels, and 4 means omit the axis entirely.
1 2 0 0; b l t r; 0=no label, 1,2=dir, 3=omit tick and label
옜 옜� 옜 옜� 602 옜 옜옜옜� 9�
redhat: dongkim2, 12345
Rev. Jae Young Heo: 2735 Piedmont Ave. #3, Montrose, CA 91020
818-249-5037 (H), paulheo@yahoo.com
rpmbuild -rebuild filename.src.rpm
happo:dongkim1,12345
yahoo: dongckim2, 123456 - old?
yahoo: dongkim12345, 123456 - new
Hyunjum: 640807
Mihyang: 630221
boundingbox: llx, lly, urx, ury
14402 Pebble Hill Ln,
North Potomac, MD 20878
aas ID: 10336, passwd: dongch - working, oasis u:dk3wc, 63301
sturm@mpe.mpg.de, b@E5q!y, id=3237
if we don't have enough thickness of air, meteors will hit incessently without being burnt by entering thich air.
realtime cityscape
---------
yoojung food and good fellowship afterwards :) [ 2005/11/22 ] D
옜 I agree...it's the people that the non-believers will notice first, so when christians show genuine love and care, it draws people in. Food makes the fellowship a lot more natural :) [ 2005/11/22 ] D
tim praying for them [ 2005/11/23 ] D
David i actually think that through friends you can get those non-believers... just asking them to come will suffice =P [ 2005/11/25 ] D
----------
198365703 옜� 옜� 옜 busan U hakbun
kcmission@hotmail.com - 123456
JungRang-Ku, SangBong2Dong 130-28 Na, HyunHee, Zip 131-222
start_gui
color printer:
login to ursa, print to 'lpr -P tek850' for paper, or 'lpr -P tek850t' for transparency.
/n/ftp/pub/
------------
ref:
Title:
The QSO -- Ultraluminous Infrared Galaxies Connection
Authors:
Veilleux, S.; Kim, D.-C.; Sanders, D. B.
Journal:
QSO hosts and their environments, Proceedings of an international workshop, held January 10-12, 2001, in Granada, Spain Edited by Isabel M�rquez, Josefa Masegosa, Ascencion Del Olmo, Lucas Lara, Emilio Garc�a, and Josefina Molina. Dordrecht: Kluwer Academic / Plenum Publishers, 2001 xvii, 376 p. ISBN 0306466627, p.165
Publication Date:
00/2001
Origin:
AUTHOR
Bibliographic Code:
2001qhte.conf..165V
Scientific A: 750657389, 123456, 20742, number
Here are some links to various on-line teaching resources: Ned Wright's Cosmology Tutorial | Pasachoff On-Line, featuring Astronomy, From the Earth to the Universe | Nick Strobel's Introductory Astronomy Notes | The IDEA Program: Initiative to Develop Education through Astronomy | AAS Education Initiative | The Jason Project | Astro Camp | The American Physical Society's Forum on Education | The HTML Astronomy Classroom Project (HACP)
---------
dopcor - dopler correction
Jessica Kim
16400 S. Westland Dr.
Gaithersburg, MD 20877
sumspec - Try changing the declaration of rcomp in Xcsao/xcplot.x from extern to int
gilbut: dongkim2, a12345
img plot wip directory - faith:/mnt/removable/img/uigs/plot/fits
--------
Average Ultraviolet Quasar Spectra in the Context of Eigenvector
Spectra were normalized by their own continuum flux in the wavelength range 1430�1470, where no strong lines are observed/expected.
Composite spectra were generated by median-combining the averaged spectra of individual AGNs.
This procedure ensures that only the most typical features will be revealed and that some unusual features, such as narrow absorption (often lost in the noise), unusually strong (narrow) lines, and noise spikes, will be omitted in the composites.
A median also works better than an average when the individual spectra do not cover the same spectral region (see � 4 for details regarding line profiles of the composites).
The composites have been binned to 0.5 per resolution element and have a typical S/N � 50 (see Table 1).
Evolution of ULIGs:
(1) merger - giant shocks - super-starbursts + galactic winds - elliptical
galaxies (Joseph, 1999)
(2) merger - H2inflow (starbursts) - cold ULIRGs - warm ULIRGs+QSOs optical QSOs (Sanders, 1999)
(3) merger/s - extreme starburst + galactic wind (inflow + outflow) -
FeII/BAL composite IR-QSOs - standard QSOs and ellipticals (L퓈ari et al., 2003)
Galactic extinction correction
deredshift
normalized
median-combined
binned to 0.1A
--------
[m] Install Macromedia Flash Player 7 into Mozilla user
directory: /home/dckim/.mozilla
[o] Install Macromedia Flash Player 7 into Opera user
directory: /home/dckim/.opera
[a] All
Please choose a directory: a
WARNING: An older version of the Macromedia Flash Player has been detected in
/home/dckim/.mozilla/plugins.
The installer will overwrite this existing binary.
WARNING: An older version of the Macromedia Flash Player has been detected in
/home/dckim/.opera/plugins.
The installer will overwrite this existing binary.
-----------
Local ERO, normal, and blue quasars in SDSS DR3 catalog.
blank lines can be removed from a file with any of the following:
:v/./d, or :%!cat -s
If you want to get rid of duplicate blank lines, but leave the first blank line intact, try:
:%!sed /./,/^$/!d
Be aware that you may need to get rid of trailing whitespace first. This can be accomplished with
:%s/[ ^I]*$/
-fTimes-Roman7
Catherine.Ishida@SubaruTelescope.org
xlsfonts | more, helvetica times utopia lucida luxi baekmuk fixed nimbus
10x20 7x13bold
12x24 7x14
5x8 8x13
6x10 8x13bold
6x12 8x16
6x13 9x15
6x13bold 9x15bold
6x9 fixed
7x13
www.3min.co.kr - comdream
www.wizisland.co.kr
Paul Stauffer, 6 Treworthy Rd, Gaithersburg, MD 20878
Chan Yang Park
859 N. Mountain Ave. #18B
UPLAND, CA 91786
1-909 -932-0066
1-909-767-9916
Key: B77471
Being Smart About Gifted Children: A Guidebook For Parents And Educators (Paperback)
* Helping Gifted Children Soar: A Practical Guide for Parents and Teachers by Carol Ann Strip
* Guiding the Gifted Child: A Practical Source for Parents and Teachers by James T. Webb
* The Social and Emotional Development of Gifted Children: What Do We Know? by Maureen Neihart
* Losing Our Minds: Gifted Children Left Behind by Deborah L., Ph.d. Ruf
* The Survival Guide for Parents of Gifted Kids: How to Understand, Live With, and Stick Up for Your Gifted Child by Sally Yahnke, Ph.D. Walker
Education of the Gifted and Talented, Fifth Edition
Education of the Gifted and Talented, Fifth Edition by Gary A. Davis and
fdisk and do mkfs -t ext3 /dev/sda1
You need to set UID and GID to the values used on faith.
grep dckim /etc/passwd
dckim:x:5721:567:Dong Chan Kim:/home/dckim:/bin/tcsh
Then while the disk is plugged into the laptop where you are root chown 5721:567 /dckim
D.C.: 158km^2 = 12.6x12.6
Oahu: 1600km^2 = 40x40
Hawaii: 10500km^2 = 100x100
Cheju: 1825km^2 =42x42
University of Maryland
Department of Astronomy
Computer & Space Sciences Building, Rm. 1253
301-405-3057 (Office)
301-314-9067 (Fax)
read habitable planet paper and do again
globat: dongkim, iraf123 (seopyong)
globat cancellation number: 0NKQD4YX
delta: 2576715243, pin: 1234
onesuite.com: calling card
http://was-1.umd.edu/phrearningstatement/earningstatement?printindind=N&saveprintearind=Save+Change&action=saveprintearind&action=saveprintearind&uid=108186347&usminstcd=01&ssn=575439918&fromapp=null
Leschkircherstr.17B, 81829 Munich, Germany, tel: 0049-89-4202-4266
MRA, Gate's foundation, media monitor this week's, international branch, PD addressfor all nations, send letter to inform they have responsibility for culture.
Mario.Schweitzer@mpe.mpg.de, Astro!
Myungkook James Jee
Yokohama_student
read Joe's paper
to do sql search: http://cas.sdss.org/dr5/en/tools/search/sql.asp
to retrieve sdss image: http://das.sdss.org/DR5-cgi-bin/DAS
Daum, yokohama university
optical depth on earth http://spiff.rit.edu/classes/phys440/lectures/optd/optd.html
http://72.14.209.104/search?q=cache:xPz_0h2-DNoJ:spiff.rit.edu/classes/phys440/lectures/optd/optd.html+optical+depth&hl=en&gl=us&ct=clnk&cd=6
check email on June 22, 2006
check aligned 3 components in ULIRGs
Galactic extinction correction - use dust.pro to get embv value coordinates are Galactic not equitorial, output value is E(B-V).
For following objects, the naming convention 'SDSShhmm+ddmm' was used, with the hhmm giving the ra in hours and minutes, and the +ddmm or -ddmm giving the declination in degrees and minutes. Column 2: RA. The object's right ascension, in decimal degrees. Column 3: DEC. The object's declination in decimal degrees.
L function: MNRAS 360, 839
set z=0.1*1 set dl1=z*(1+0.5*z) set dl2=(1-1/sqrt(1+z)) set dl2=dl2*2*(1+z) print {z dl1 dl2}
0409257 - ero qso powered by bb about 0.03 to 0.1 eddington limit, estimated column density from xmm data - apply.
enhanced K wrt R is due to extinction in optical and agn emission (point-like) in nir.
nir emission could also be from host galaxy (ref: mainieri et al 2002, mignoli et al 2004).
check formation of spheroids (Menci+ 2004).
fig4 = k vs f(2-10kev) plot, log(x/o)
fig5 = r-k vs x/o, mention ero fraction in sdss qso.
ref this paper for x-ray properties of the ero
0301019 - bal troughs are caused are by outflow of qso not galaxies in los.
bal ~ broad UV absorption qso, 12% of all qso (weymann+ 1991), mostly in rqq.
A_l = E(l-V) + R_v x E(B-V), E(l-V) = A_l - A_V (extinction law).
fraction of outflow
0304564 - bal velocity ~ 10,000 to 30,000km/s.
0305541 - photosperic radius and outflow speed prop to M'^2 and M'^-1. L_edd/c = momentum. bh outflow formulae
0308345 - radio galaxy is proto-quasar, reddened qso 3.1 to A_v to 7.3, once outflow blow out cocoon, it becomes qso
0309524 - outflow formulae for qso
check if we have narrow-line qso in our sample.
0311561 - bal, caii 3934, 3969, sample spectra for bal, bal condition for caii, most of the red spectra shows caii whereas blue shows [NeIII]3969 emission
blueshifted caII - general properties of bal
aa, 443, 903, 2005 - bal = 20% of qso pop, from jhk' color, you can estimate sf episode, see fig5.
BAls are redder - menou+2001,
Galactic extinction correction
deredshift
normalized
median-combined
binned to 0.1A
tprint X0170101tot1alif4ttagfcal.fits, col=풵AVE FLUX ERROR� > flx.asc
l60.f
character*28 a
do 100 i=1,118
open (unit=1, status='old', file='j.d')
read(1,10)a,z,f60
10 format(a28,f5.0,a95,f6.2,a13)
rl60=2.5E13*f60*(z*(1.+0.5*z))**2.
rl60=log10(rl60)
write(7,20)a,z,f60,rl60
20 format(a28,f6.4,f8.5,f8.2)
100 continue
120 close (unit=1)
stop
end
1sigma = 68.26%, 2sigma=95.46%, 3sigma=99.73%
mark ra dec el white major minor pa
mark 111.5 40.5 el white 10 10 60
mark 2h46m45s 61d47m57s el white 10 10 60
mark 23h55m01.91s -0d06m41.7s el green 10 10 50
mark 23h55m01.91s -0d06m41.7s el green 1 1 50
http://cas.sdss.org/dr4/en/tools/crossid/upload.asp
SELECT
p.objID, p.ra, p.dec, p.run, p.rerun, p.camCol, p.field, p.obj,
dbo.fPhotoTypeN(p.type) as type,
p.modelMag_u, p.modelMag_g, p.modelMag_r, p.modelMag_i, p.modelMag_z
FROM #x x, #upload u, PhotoTag p
WHERE u.up_id = x.up_id and x.objID=p.objID
ORDER BY x.up_id
get E(B-V), use /mnt/removable/IDLCode/get_dust
velocity_dispersion of SDSS:
The instrumental dispersion of the SDSS spectrograph is 69 km s-1 per pixel, and the resolution is ~ 90 km s-1.
rv.fxcor: velocity dispersion
http://spectro.princeton.edu/
lambda=10**(coeff0+coeff1*i)
splot spSpec-MJD-plate-fiber.fit[0][*,X], X=1,2,3,4
!./lineprotect.pl protect.dat 0.027863;more linep1
$pwz3 = $plz / 600.; # redshifted region width, in um for SH, and LH
$pwz5 = $plz / 600.*8.; # redshifted region width, in um for SL
push @out, sprintf("%10.5f%10.5f%10.5f%10.5f\n",$plz,$pwz,$pwz3,$pwz5);
line width=l/600
first: angular resolution=5.4", 20cm, nvss: resolution=45"
FIRST and NVSS both observed the sky at 20cm (1.4 GHz), but with very different spatial resolution.
FIRST has a 5.4" beam with astrometrical errors of 0.5-1", while NVSS has a 45" beam with 1-7" astrometric accuracy.
FIRST therefore distinguishes small-scale structures with accurate positions, but underestimates flux for extended sources.
NVSS has less accurate positional measurements and cannot distinguish small-scale structures,
but measures more accurate fluxes for extended sources and can find low-surface brightness objects missed by FIRST.
exptime=53.9sec
aa = zeropoint, kk = extinction coefficient, airmass
f/f0 = counts/exptime * 10**(0.4*(aa + kk * airmass))
mag = -2.5 * log10(f/f0), f/f0 = counts/(10**8 * flux20)
-----
I have had some problems like this, too. One possibility could be a bad
dmask file, a problem I have had a couple of times. I would check the
relevant bmask files and look for a jailbar pattern at the 8-count
level. I've fixed my code again to better avoid these exposures.
If that's not it, it could be a problem with counting the frames; I've
had a few of those, too. I could take a look at it if you want.
--------------
Filters/Images/Compose
Layer/colors/level
narrow-line seyfert 1 galaxy (Osterbrock & Pogge 1985):
H_beta < 2000 km/s, [OIII]5007 / Hb < 3.0
idl help:
IDL>?for
IDL> X = [ 1.8, -2.7, 0.7, -0.5, -1.3, -0.9, 0.6, -1.5, 2.5, 3.0]
IDL> Y = [-4.7, 9.8, -3.7, 2.8, 5.1, 3.9, -3.6, 5.8, -7.3, -7.4]
IDL> PRINT, CORRELATE(X, Y)
% Compiled module: CORRELATE.
-0.979907
IDL> print, linfit(x,y)
% Compiled module: LINFIT.
0.615019 -3.20599
IDL> text=rd_tfile(filename)
IDL> data=rd_tfile(filename)
or
OPENR, lun, 'test.dat', /GET_LUN
;header = STRARR(3)
;READF, lun, header
rows = 19
data = FLTARR(2, rows)
READF, lun, data
x = [ 0, 1, 2, 3, 4, 5]
y = [ 1, 1.5, 2, 2.5, 3, 3.5]
x = data(0,*)
y = data(1,*)
;z = data(2,*)
x = REFORM(x)
y = REFORM(y)
;z = REFORM(z)
print, correlate(x,y)
print, linfit(x,y)
x = [ 1, 2, 3, 4, 5]
y = [ 1.5, -10, -25, 3, 10.8]
x = data(0,*)
y = data(1,*)
x = REFORM(x)
y = REFORM(y)
print, correlate(x,y)
print, linfit(x,y)
If I didn't know how many rows were in the data file in the example above, I might have used the EOF command to read the data until I got to the end of the file.
pressure = FLTARR(10000)
temperature = FLTARR(10000)
humidity = FLTARR(10000)
p = 0.0
t = 0.0
h = 0.0
count = 0
WHILE (NOT EOF(lun)) DO BEGIN
READF, lun, p, t, h
pressure(count) = p
temperature(count) = t
humidity(count) = h
count = count + 1
ENDWHILE
pressure = pressure(0:count-1)
temperature = temperature(0:count-1)
humidity = humidity(0:count-1)
PRINT, CORRELATE(X, Y)
print, linfit(x,y)
OPENR, lun, 'lrna.d', /GET_LUN
rows = 15
data = FLTARR(2, rows)
READF, lun, data
x = data(0,*)
y = data(1,*)
x = REFORM(x)
y = REFORM(y)
print, correlate(x,y)
print, linfit(x,y)
print, x, y
close, lun
arr1=sin((findgen(100)/35.)^2.5)
arr1=arr1+2
arr2=2+sin((findgen(100)/35.)^2.0)
plot, arr1, arr2
plot, arr1<2>(-1.5), arr2
openw, 1, 'arr.dat'
for i=0,99 do printf, 1, i, arr1[i], arr2[i]
close, 1
readcol,'arr.dat',i,arr1,arr2
Galactic extinction correction - use dust.pro to get embv value coordinates are Galactic not equitorial, output value is E(B-V).
Carefirst/BC/BS/Bule Choice - ID=XIC903184165, G#=7J63, dongkim2, 123456
continuum input.fits output.fits high=3 low=3 or=100 ty=dif
25825
impact factor:
1997-2005
ApJ, ApJS, (2.948, 1.946), (1.953, 2.075), (2.543, 3.749), (2.822, 3.475), (5.921, 5.214), (6.187, 4.749), (6.604, 6.247), (6.237, 15.231), (6.308,14.428)
AJ, 2003-5.647
PASP, 1998, 0.955
Astron Nachr, 2005, 0.871
continuum subtraction: continuum s094215.12+090015.8aez.fits output.fits high=3 low=3 or=50 ty=dif
iso orientation: http://www.intprog.umd.edu/sparkplug/common/images/ies/InternOrientationVolunteer.pdf
Huwongum옜� 옜옜 848601-04-043129 (옜�:옜옜 옜옜옜�)
homeless - good spoon
american value agenda 10 republican party
japaneses properties in korea
chb: 58504181345
bangsong weonehae pyoungga sim-i-gug choi jeoung kyu bujang
optical specgtra 3c273: K. L. Thompson, ApJ, 395, 403-417, 1992.
M(BH)= S. Paltani (LAM, Marseille), M. Turler (ISDC, Geneva), 6.59 10^9with a 1 sigma confidence interval 5.69-8.27 10^9 Mohis estimate is more than one order of magnitude larger than that obtained in aprevious study using Balmer lines.
2005A&A...435..811P PALTANI, S.; TU... THE MASS OF THE BLACK HOLE IN 3C 273.
logM_BH=8.92, ApJ 637, pp669, 2006,
Liu, Yi; Jiang, Dong Rong; Gu, Min Feng
nref: works in csh @faith - setenv nref /n/faith1/dckim/nicmos/nicmos1/
also works in bash with export nref=/home/dckim/iraf/nic/
atmospheric absorption line: A-band (7600-7630), B-band (6860-6890)
Jamison property, David lee
American Southern Baptist Church Korean Assembly
Rev. SungBin Park, Memphis Korean Baptist Church
sdss extinction: g=0.73*u, r=0.53*u, i=0.40*u, z=0.29*u
sandiego onnuri church, chansu cho
1 parsec: 3.08568025 � 10^18 cm
1 solar luminosity: 3.827 � 10^33ergs/s.
wip, device/vcps
$as2 = 20./$dl[$i]/1000.*206265.; #20kpc in as scale
#$as = $as2/$pix/2.; 10kpc/2 in pixel unit
$as = $as2/2.; #10kpc/2 in arcsec unit
MBC complaint zero, Sep. 28, 7:20PM
OIII_1666 1666 1665.85
AlIII_1857 1857 1857.40
CIII_1909 1909 1908.73
CII_2326 2326 2326.00
NeIV_2439 2439 2439.50
MgII_2799 2799 2799.12
NeV_3347 3347 3346.79
NeV_3427 3427 3426.85
OII_3727 3727 3727.09
OII_3730 3730 3729.88
Hh_3799 3799 3798.98
Oy_3836 3836 3836.47
HeI_3889 3889 3889.00
K_3935 3935 3934.78
H_3970 3970 3969.59
He_3971 3971 3971.19
SII_4072 4072 4072.30
Hd_4103 4103 4102.89
G_4306 4306 4305.61
Hg_4342 4342 4341.68
OIII_4364 4364 4364.44
Hb_4863 4863 4862.68
OIII_4933 4933 4932.60
OIII_4960 4960 4960.30
OIII_5008 5008 5008.24
Mg_5177 5177 5176.70
Na_5896 5896 5895.60
OI_6302 6302 6302.05
OI_6366 6366 6365.54
NI_6529 6529 6529.03
NII_6550 6550 6549.86
Ha_6565 6565 6564.61
NII_6585 6585 6585.27
Li_6708 6708 6707.89
SII_6718 6718 6718.29
SII_6733 6733 6732.67
CaII_8500 8500 8500.36
CaII_8544 8544 8544.44
CaII_8665 8665 8664.52
ebay: dongkim2, 641217, (& pal gm, honolulu100!)
-------------------------------------------------------------------------
NICMOS data reduction
1. do Mr. StayPuft correction (idl code)
setenv nref 'path'
to run undopuft, mv all n6* files to some other directory.
(or remove all *fits files other than images?)
.r undopuft.pro
.r runpuft
2. calnica
a. mv raw, cal, ima, files to ori
mv *raw.fits ori
mv *cal.fits ori
mv *ima.fits ori
b. mv *.raw1 to *.raw to run calnica
see cal.cl calnica n9og01woq_raw.fits n9og01woq.fits
export nref="/home/dckim/iraf/nic/"
need *pht.fits and *mask/flt/tdd.fits files
3. pedsky
choose best one from cal, psk, psu
4. SAA correction
setenv nref '/mnt/removable/dckim/nicmos/nic/'
need lib directory
cd /faith1/dckim/nicmos/nicmos2, or cp lib directory to . and start idl
idl> !path = 'lib:'+!path
idl> saa_clean,'n9og08edq_psk.fits','n9og08edq_saa.fits',/tv,/fit
5. drizzle
cp chmask.fits to current directory
to run drizzle, epar driz_cr to change 'background' to 'backest1'.
-------------------------------------------------------------------------
IRS extraction:
SL - automatic column, no sky subtraction
SH, LH - full aperture extraction
to get upper limits:
1. fit continuum (1/2 order) and get RMS
2. set height=3xRMS, set width=lambda/600 for SH/LH, =lambda/200 for SL
3. flux result is 3 sigma upper limit
Spitzer Space Telescope - Guaranteed Time Observer Proposal #30334
IRS Spectroscopy of Starburst-Dominated ULIRGs at 2 < z < 3
Principal Investigator: James R. Houck
Institution: Cornell University
Co-Investigators:
Vandana Desai, Caltech
Science Category: high-z galaxies (z>0.5)
Observing Modes: IrsMap
Hours Approved: 34.9
Abstract:
We request 34.9 hours of Spitzer time to obtain mid-infrared IRS LL1
spectra of 16 extreme (f(24)/f(R) > 1000) infrared sources selected
from the NOAO Deep Wide-Field Survey Bootes field. Each target
displays a 1.6 micron rest-frame stellar bump indicating that 1) it
has a redshift in the range 2 < z < 3; and 2) its infrared luminosity
is primarily generated by reprocessed starlight, rather than
AGN-heated dust. These spectra will allow us to study the
mid-infrared properties of the most luminous starburst-dominated
galaxies to z=3. We will also confirm the stellar bump as an
indicator of starburst domination and calibrate the bump photometric
redshifts for extreme, high redshift sources.
Spitzer Space Telescope - Guaranteed Time Observer Proposal #105
Spectroscopic Study of Distant ULIRGs II
Principal Investigator: James R. Houck
Institution: Cornell University
Science Category: ULIRGS/LIRGS/HLIRGS
Observing Modes: IracMap IrsStare
Hours Approved: 85.3
Abstract:
Ultraluminous Infrared Galaxies (ULIRGs) have bolometric luminosities
of quasars but they outnumber the QSOs with same optical luminosities.
Even though several of the nearby ULIRGs have been studied extensively
many questions regarding their dust content and energetics remain, and
little is known about the more distant ones. We propose to extend our
knowledge of these objects and explore the potential evolution in
their properties with redshift by obtaining full low-res spectra of a
sample of ULIRGs with redshifts up to 0.5.
Molecular Hydrogen content in nearby galaxies: Houck, James R.
Spitzer Space Telescope - Guaranteed Time Observer Proposal #97
Molecular hydrogen content in nearby spirals
Principal Investigator: James R. Houck
Institution: Cornell University
Science Category: nearby galaxies (z<0.05, v_sys<15,000 km/s)
Observing Modes: IrsStare
Hours Approved: 2.0
Abstract:
It is believed that the ratio of molecular to atomic hydrogen remains
constant as a function of radius in late type spirals. The reason why
the former is not detected is that current methods of estimating the
molecular gas mass are based on indirect CO measurements which are
metallicity depended. If the H2 to HI ratio is constant then
molecular gas could potentially constitute a considerable fraction of
the dark matter of a galaxy. We wish to examine this hypothesis by
directly mapping the molecular hydrogen profile, using the mid-IR H2
lines, in one edge-on and one face-on spiral galaxy.
/n/ultra1/drupke/spitzer/smart/smart
PRINCIPLES OF DEVELOPMENT
hongbw@gmail.com
By faith we understand that the universe was formed at God's command, so that what is seen was not made out of what was visible.
Hebrews 11:3
Exotic Earths: Forming Habitable Worlds with Giant Planet Migration Hot Earths?
The first and foremost of these is, of course, scientific merit.
Because the committee is rather small and must cover a wide range of astrophysical expertise,
it is essential that proposals make very clear just what scientific questions will be addressed by the proposed observations.
The committee often wishes to see these goals placed in a larger context;
i.e., how these questions relate to major unresolved astrophysical questions.
kpno07a, dckim07a, 12345
kpno07b, dckim07b, 12345
umd: dkim21, Dongkim1!
VideoJug.com, eHow.com, ViewDo.com, WikiHow.com
Leavy & Frank: zakimdon8, !choisun, 14kimeun2, !potomac, kimsuvnr7r, !
651-41 Yeoksam-Dong, Kangnam-Gu, Seoul, KOREA
Fat person: bacteroidetes -small, firmicutes -large, nature 12/21/2006, Jeffery Gorden
ys94@georgetown.edu
Schneider (2006) - number of Jupiter-like planet
Sangkyun Park: 14903 Alpine Meadow Lane, Silver Spring, MD 20906
solid angle=surface area / r^2 steradian
imcopy s003657.17m100810.6.fits[*,1] s003657.17m100810.6a.fits
deredden s003657.17m100810.6a.fits s003657.17m100810.6ae.fits 0.0346660
dopcor s003657.17m100810.6ae.fits s003657.17m100810.6aez.fits 0.1877 flux+
diffraction spike
to get dss images in batch mode
dss2 red -i ./dss.in
sv background memory dump mode:
/home/dckim/package/Skyview_3.5/bin/skyview -n < do.sv
The fact that the asteroid belt has such a well-defined, high concentration of asteroids suggests two things. One, that they are fragments of a planet that broke-up long ago, or two, that they are rocks that never managed to accumulate into a genuine planet.
Currently, scientists tend to favor the latter explanation.
According to Eric Chaisson and Steve McMillan, the authors of the text book "Astronomy Today", 1993 edition,
"There is far too little mass in the belt to constitute a planet, and the marked chemical differences between individual asteroids strongly suggest that the asteroids could not all have originated in a single planet.
Instead, astronomers believe that the strong gravitational field of Jupiter continuously disturbs the motions of these chunks of primitive matter, nudging and pulling at them, thereby prohibiting them from aggregating into a planet.
The existence and composition of the asteroid belt joins the general properties of the planets and their moons on our list of features that any theory of solar system formation must explain."
Here is a good web page about the asteroids: http://www.seds.org/nineplanets/nineplanets/asteroids.html
Earth - James F. Luhr
ApJ 556, p727, gamma-ray burst properties
compusa: comp12345-old, iraf123,
erebates.compusa.com: dckim,umd,iraf123,dongkim2, 123456
Yoon, YoungSoo, 3235 Computer & Space Science, Building #224
velocity of light in dark matter, vacuum, material, ether...
Your e-mail has been forwarded by Veberly. Would you like to share your suggestions regarding EE meterials? Thank you.
My cellular phone is 240-731-1004 and
2mass - six times longer (6x) than the 7.8s exposure time used for each sky location in the survey.
soribada, dongkim12345, 12345
cell phone: 240-505-6292
umd facility: Work Control Center Office of Facilities Administration Facilities Management 301-405-3202 http://www.facilities.umd.edu/ios
sunkyung, manna, princeton
Orbital forcing of the martian polar layered deposits, Nature 419, 375-377 (26 September 2002) , Jacques Laskar1, Benjamin Levrard1 and John F. Mustard2
white granite walled house. Bible verse (Acts 16:31) appears on the wall depending on certain direction. Could use some lighting bulb to illuminate letters and use special form of letter shapes.
Farm Bureau
navy: %HoNolulu10!
to plot xdr file:
IDL> restore,"IRAS11119_3257_all.xdr"
IDL> restore,"pgaveragenonfirsed.xdr"
IDL> restore,"UGC5101_total.xdr"
IDL> object=memstor.aar
IDL> w1=object.data.wave
IDL> f1=object.data.flux
IDL> plot,w1,f1
You can load tbl files by clicking 'browse' tab in smart and
after that if you click 'view' tab, it will open 'idea' window.
It preserve all information just as xdr file does.
39 years old, 100, young rich's real estate investment secret
;change ;local=reform(fframe(108:116,75:110)) to local=reform(fframe(104:116,75:110)) in lhdeglitchb.pro
pyramid: Kate Spence - Nature, Vol. 408 p.320, 16th November 2000, BC 2467? - BC2485-BC2475 ( http://216.239.51.104/search?q=cache:UmGQTIqhhd8J:www.americanscientist.org/template/AssetDetail/assetid/35115%3F%26print%3Dyes+pyramid+build+date+precession&hl=en&ct=clnk&cd=1&gl=us)
dell: umd, dongkim2, inspiron 8600 service code: bfttk51 -old?
dell: gmail, hon1 - home/home office
wiki: dongkim, 12345
1. DongChan Kim's parents:
Father's name: DukSang Kim
Date and place of birth: 09/18/1917, Masan, Korea
Mother's name: JongRyun Shin
Date and place of birth: 06/23/1927, Masan, Korea
Address they lived before passed away: 2-11 Odong-dong, Masan, Korea
2. EunJu Kim (DongChan Kim's wife)'s parents:
Father: DaeWon Yoo
Date and place of birth: 02/28/1942, GoHeung, Korea
Mother: YoungGil Chang
Date and place of birth: 12/10/1943, SoonChun, Korea
Current address: 15 tong 7 ban, 334-11 Chunho-dong, Kangdong-gu, Seoul, Korea
.com nuLnu2Fnu.pro
read_sed.xdr.pro:nuLnu2Fnu,source='IRAS00091-0738_sed.xdr',output='IRAS00091-0738_sed.asc',dl=100.0
dump -o -f /media/usbdisk/dckim/j (=to) /dev/hda3 (=from)
costco-dongkim2
ChangRae Lee - Native speaker, novelist
MinJin Lee - Free Food For Millionaires, novelist
Robert Lee Illustration and Design
IDL batch job: @file_name
fedora upgrade error:
cd /usr/share/gdm/themes
ln -s Bluecurve Default
cd Bluecurve
ln -s Bluecurve.xml Default.xml
gravity - why weak? smeared out to 11-dim and we see left-over. If dark matters are
around us, what happens to the law of gravity?
"Neptune's south pole is currently tilted toward the Sun, just as the Earth's south pole is tilted toward sun during summer in the southern hemisphere," explains Orton. "But on Neptune the Antarctic summer lasts 40 years instead of a few months, and a lot of solar energy input during that time can make big temperature differences between the regions in continual sunlight and those with day-night variations. This is a likely factor in Neptune having the strongest winds of any planet in the solar system; sometimes, the wind blows there at more than 2,000 kilometers per hour," said Orton.
3 Ways to make protype:
1. fabathome.org
2. engadget.com
3. emachineshop.com
Install Apache:
adobe & shareware korea: potomac, 12345
Many Worlds in One: The Search for Other Universes
The Cosmic Landscape: String Theory and the Illusion of Intelligent Design
Christian astronomer - ask to give lecture of creation science to their church.
Ask Ashley to correct grammer.
compile c++ code: g++
class=variable, object=specific variable, method=function
class can contain variable and function, but struct can contain variable only
csc: dckim@astro.umd.edu, 123456
case number: 0607-0000375414
i140, dongchankim, Poto1234, LIN0706153811, niw: LIN0709953123
if you get error on LL reduction, change flat path
hancoke@yahoo.com, Park, YoungSoo, cell ph 213)819-1333, work)213-748-5678
490, apgujungdong, hanyang apt 9-109ho
yoeksam 695-41 (25/5), dot.com villa 301ho.
gsfc: dckim, 12345
box: b l t r, 0-no label, 1&2 - direction of ticks, 3 - omit ticks and labels, 4-omit all
log-log plot (axis.sm): take log on x, y, limits log limits, box 4 4 4 4
idl tip:
x1=findgen(10)
y1=findgen(10)
for i=0, 9 do print,x1(i),y1(i)
pyraf error :
ImportError: libf2c.so: cannot open shared object file: No such file or directory
solved after I have placed libf2c.so to /usr/lib
EE revision???, when and how?
(1) NTFS (for Windows partition)
(2) EXT3 (for Linux partition)
(3) FAT32 (for the External HD, which I use in both Windows and Linux partitions)
fc6 installation:
windows (ntfs) first and fc6 (ext3, LVM, default setup)
IRAF v.2.14 installation under fc6:
1. login as a root
adduser iraf; passwd iraf iraf123
mkdir /iraf; mkdir /iraf/iraf; mkdir /iraf/iraf/local
mkdir /iraf/imdir???
vi /etc/passwd and make change as in the following example (csh, not bash)
iraf:x:312:12:IRAF system login:/iraf/iraf/local:/bin/csh.
chown iraf /iraf; chown iraf /iraf/iraf; chown iraf /iraf/iraf/local
chgrp iraf /iraf; chgrp iraf /iraf/iraf; chgrp iraf /iraf/iraf/local
2. login as iraf
mkdir /iraf/irafbin; mkdir /iraf/irafbin/bin.redhat; mkdir /iraf/irafbin/noao.bin.redhat
mkdir /iraf/x11iraf; mkdir /iraf/extern; mkdir /iraf/extern/stsdas; mkdir /iraf/extern/tables
mkdir /iraf/extern/stsdas/bin.redhat; mkdir /iraf/extern/tables/bin.redhat
cp as.pcix.gen.gz /iraf/iraf
cp ib.rhux.x86.gz /iraf/irafbin/bin.redhat
cp nb.rhux.x86.gz /iraf/irafbin/noao.bin.redhat
cp stsdas37.tar.gz /iraf/extern/stsdas
cp stsdas37.bin.redhat.tar.gz /iraf/extern/stsdas/bin.redhat
cp tables37.tar.gz /iraf/extern/tables
cp tables37.bin.redhat.tar.gz /iraf/extern/tables/bin.redhat
cd /iraf/iraf; tar -xvzf as.pcix.gen.gz
cd /iraf/irafbin/bin.redhat; tar -xvzf ib.rhux.x86.gz
cd /iraf/irafbin/noao.bin.redhat; tar -xvzf nb.rhux.x86.gz
cd /iraf/extern/stsdas; tar -xvzf stsdas37.tar.gz
cd /iraf/extern/stsdas/bin.redhat; tar -xvzf stsdas37.bin.redhat.tar.gz
cd /iraf/extern/stsdas; python python/compileall.py ./python; python python/compileall.py ./python/*
cd /iraf/extern/tables; tar -xvzf tables37.tar.gz
cd /iraf/extern/tables/bin.redhat; tar -xvzf tables37.bin.redhat.tar.gz
setenv iraf /iraf/iraf/
cd $iraf/unix/hlib; cp extern.pkg.NOAO extern.pkg (or edit original extern.pkg to include external packages you want to include)
source irafuser.csh; ./install -n
if everything works ok,
login as a root (su and enter rootpasswd);
./install; exit from root; cd to iraf home; source .login; rehash (to update excutables);
note on FC6: cl (login.cl was already generated).
if you have error message of "os_mach; undefined variable", add "set os_mach = linux" under the "setenv mach redhat" in /iraf/iraf/unix/hlib/cl.csh
X11-IRAF installation:
1. download pre-compiled binary from "http://iraf.net/downloads/".
1. tar -xvzf x11iraf-v1.5DEV-bin.redhat.tar.gz;
2. login as root;
2. mv bin.redhat/* /usr/local/bin; mv lib.redhat/* /usr/local/lib; mv include/* /usr/local/include ; mv app-defaults /usr/lib/X11/app-defaults; mkdir /usr/man; mkdir /usr/man/man1; mv man/* /usr/man/man1
STScI Python v2.5 installation (login as root (bash))
1. install Tcl/Tk
unpack tcl and tk; tar xzvf tcl8.3.5-src.tar.gz; tar xzvf tk8.3.5-src.tar.gz
cd tcl8.3.5/unix; ./configure --enable-shared; make; make install
cd tk8.3.5/unix; ./configure --enable-shared; make; make install
if get error (bash3.1 or larger on FC6, CentOS 5),
delete "'" character in two lines in tcl8.3.5/unix/configure and one line in tk8.3.5/unix/configure
(i.e., change /etc/.relid' to /etc/.relid).
2. install latest version of Python
a. do the following changes (uncomment and set proper path, see below) in Python-2.5.1/Modules/Setup.dist in order to make "Tkinter" working
# *** Always uncomment this (leave the leading underscore in!):
_tkinter _tkinter.c tkappinit.c -DWITH_APPINIT \
# *** Uncomment and edit to reflect where your Tcl/Tk libraries are:
-L/usr/local/lib \
# *** Uncomment and edit to reflect where your Tcl/Tk headers are:
-I/usr/local/include \
# *** Uncomment and edit to reflect your Tcl/Tk versions:
-ltk8.3 -ltcl8.3 \
# *** Always uncomment this; X11 libraries to link with:
-lX11
note: works without setting proper paths for "X11 header and X11 lib files"
b. cd Python-2.5.1; ./configure; make; make install
if "make" gives error messages (can't find libtcl8.3.so/tk8.3.so),
cp /usr/local/lib/tk8.3.so and /usr/local/lib/tcl8.3.so to /usr/lib (and /usr/local/lib/tcl8.3 and /usr/local/lib/tk8.3 not required in CentOS5?).
3. install libf2c
a. tar -xvzf libf2c.tar.gz; cd libf2c_stsci; make -f makefile.linux
b. mkdir /usr/local/libf2c;
cp libf2c.a /usr/local/libf2c; cp libf2c.a /usr/local/lib; cp libf2c.a /usr/lib;
cp f2c.h /usr/local/libf2c; cp f2c.h /usr/local/lib; cp f2c.h /usr/lib; or
cp -r libf2c_stsci /usr/local/libf2c (preferred).
4. install Pmw
tar -xvzf Pmw.1.2.tar.gz; cp -r Pmw /usr/local/lib/python2.5/site-packages
5. install stsci python 2.5;
a. tar xzvf stsci_python-2.5.tar.gz
unset F77; unset F2C (bash), unsetenv F77; unsetenv F2C (csh/tcsh)
b. cd stsci_python-2.5/numpy-1.0.3
python setup.py install
c. cd stsci_python-2.5/convolve
python setup.py install
d. cd stsci_python-2.5/image
python setup.py install
f. cd stsci_python-2.5/ndimage
python setup.py install
g. cd stsci_python-2.5/
python setup.py install --with-f2c=/usr/local/libf2c #(path_to_f2c)
Now, reboot system and build iraf (mkiraf).
to start pyraf, type pyraf
if you get error '/iraf/irafunix/hlib/mach.h', login as iraf; cp -r /iraf/iraf/unix /iraf/irafunix.
MAC tiger installation to pc:
1. Download VMWare files for patched Mac OS X Tiger Intel from your favorite torrent site. (Hint: Use the search function).
2. Copy tiger-x86-flat.img from the archive to an external USB drive (its 6gb)
3. Download Ubuntu Live CD (link) be sure you get the Live CD!!
4. Burn the ubuntu iso, stick it in your pc, and boot it! (make sure you have your bios set to boot to CD)
5. Once ubuntu boots and the gui finally comes up, hook up the USB drive you copied the 6gb image to. A window should pop up showing the contents of the drive. Take note of where its mounted. It should be /Devices/Yourdrivesvolumename
6. Open a terminal window and cd to that directory (/Devices/Yourdrivesvolumename). Do an ls to make sure you are in the right place (you should see the 6gb img file.
7. In the terminal window type:
sudo dd bs=1048576 if=./tiger-x86-flat.img of=/dev/hda
Replace hda with the correct drive! If you only have one drive, its probably hda. Thats what mine was. You are about to erase this entire drive so make sure youve got it right and make sure you want to do this! Hit enter. It takes a while took my vaio about 9 minutes.
8. When its done, remove the ubuntu disc and shut down the pc. Disconnect your usb drive. Thats it! When you power it back on, OS X should boot!
For whatever reason, mine hangs when its loading. If this happens to you, boot with the -x option (hit a button at the darwin screen when you boot your pc. enter -x and hit enter). Should work without any problems, and I dont see any restrictions being in safe mode.
Youll notice there is a login screen, and you dont know the password! This image was created by deadmoo and we can easily change his password. Reboot the machine again. Again, hit a button at the darwin screen. This time type -v and hit enter. At the command prompt screen type:
sh /bin/sh
passwd curtis
(change the password to what you like)
ubuntu: sudo ...
daum: dongkim12345, honolulu
Install x11 to mac (http://macsingularity.org/x11/):
X11 is installed by default in Leopard (Mac OSX10.5).
It is in Tiger "Optional Installs.mpkg" on Tiger DVD and in "Packages" folder on Panther CD #3.
caution: Don't put X11.app in the dock (http://forums.macosxhints.com/showthread.php?t=80171)
edit .xinitrc to change "windows manager".
Installing IRAF on Mac (http://macsingularity.org/iraf-on-macos-x/):
Introduction
You really need 3 things to run IRAF:
* Apple's X11 (see the X11 tab at the top)
* IRAF (from the download page)
* X11IRAF (mainly xgterm)
You will run X11, run xgterm within x11, and run IRAF from the xgterm.
Getting IRAF up and running
The easiest way to install IRAF is to use the Mac OS X installers I have created.
You can find them both for Intel or for PPC from the download page
(http://macsingularity.org/downloads/).
Making the iraf user account
Step 1. Do not launch the package file just yet, you must first make the IRAF user.
IRAF requires the creation of a user on the machine named "iraf" who owns all the iraf files.
Creating the User is easy though.
Open up System Preferences and click on the Accounts Click on the + button... and set it up so.
The login picture doesn't matter of course.
Make the IRAF User an Admin by checking the box.
Click save, and you're done creating the IRAF user.
Step 2. Double-clicking the downloaded file should launch Apple’s built in decompression helper program.
You’ll be greeted by a folder containing a .pkg installer, the Installing PC IRAF users guide in PDF format, and a README file.
If you have already downloaded the .pkg installer from contrib as your normal login, you should probably go ahead and move it to Shared folder that’s in /Users, or if that doesn’t work try copying it to the Drop Box in the Iraf User’s Public folder.
Step 3, Installation. Now you can log out of Mac OS X via the Apple menu and then log back in as the Iraf User,
or if you’re running Panther or later use fast user switching to switch to the IRAF User.
As you log into MacOS X for the first time "as the Iraf User" things will look odd on your OS X desktop.
The dock will seem big, the background will probably be diffrent.
Find the IRAF .pkg installer, or go "download it" and double-click the .pkg file inside the folder
after you’ve decompressed and expanded the archive.
You should be familiar with the MacOS X installer. Simply follow the on-screen instructions.
In MacOS 10.1 and again 10.3, when the installer is done, it will likely seem to work and then at the end say "Errors occured when installing the software, try again".
Ignore that. It should work just fine, you can check in the Finder or Terminal to see that all the files are there in /iraf.
For some reason this does not happen in Jaguar.
Now it’s time to use the Terminal. You can stay logged in as ‘iraf’ for this. Launch "Terminal.app" from /Applications/Utilities, change directories to /iraf/iraf/unix/hlib/ and run the IRAF install script.
Note: The first time you run a command with sudo it’ll give you a lecture on using it.
Each time you run a command with sudo it will ask for your password (not the root password.)
Only administrators can run sudo. This is why it’s helpful that you make the iraf user an admin. Just to simplify this process.
% cd /iraf/iraf/unix/hlib
% sudo ./install
Follow the install scripts onscreen instructions. The script should run without any errors.
You can choose either /usr/bin or /usr/local/bin as the iraf local comands directory,
I believe /usr/bin/ is the default… this has the advantage of being in your PATH by default.
You’re done! IRAF is installed. Now back to your normal login account.
You can log out of OS X as IRAF and go back to your normal account.
First Time Setup
So, this part should be familiar to you.
It’s probably best to make an iraf directory in your home directory, so startig in your home directory:
% mkdir iraf
% cd iraf
% mkiraf
This makes you an iraf directory that will store your iraf parameter files and other things.
The login.cl file generated will determine your terminal type, so it will ask you to choose.
If you’re going to install X11IRAF, then xgterm is probably a good choice.
If you’re going to use X-Windows but not xgterm then go with xterm.
Otherwise, if you plan on just using the OS X terminal, pick vt100.
If the mkiraf step doesn’t work, and you get a command not found problem,
then you need to add /usr/local/bin to your path.
Alternatively, you can pick /usr/bin when you run the iraf install script at the beginning.
For information on changing your path check out the unix page or also here (PATH=/usr/local/bin:~/bin:$PATH) on changing the path in the bash shell.
The bash shell is the shell by default for new users, so you may very well be using bash.
Now type in your iraf directory
% cl
and all should be working. IRAF is running on your Mac.
However, most users will want X11 to get the full benefits of IRAF.
Scisoft 2007.11.1 Released
updated Python to version 2.5.1.
correct some minor issue with the bash version of the irafuser.bash script when running unde OSX 10.5 Leopard. Missing GCC runtime fortran libraries are also now included.
Once the Setup.bash script has been sources (see the Installing instruction), you should add the following line to your .bash_profile:
export DISPLAY=127.0.0.1:0.0
This will enable all Scisoft X11 applications to start from Terminal.app
If get error saying can't install it on "/", do the following from terminal:
"sudo installer -pkg path/Scisoft_OSX_macintel_2007.11.1.pkg -target /".
http://blogplus.net/GoE.aspx?idx=2462094&path=http://blog.joins.com/dh1218/8882109 - > you are here
multiboot: http://ubuntuforums.org/archive/index.php/t-376677.html
shell tutorial: http://www.cyberciti.biz/nixcraft/linux/docs/uniqlinuxfeatures/lsst/
iraf install script:http://mjhutchinson.com/journal/2006/11/05/install_iraf_on_ubuntu_edgy_amd64
doiraf
-------------------------
#!/bin/bash
PID=`pidof ds9`
if [ ! $PID ]; then
ds9 &
fi
cd ~/iraf
xgterm -sbr -fn 9x15 -sl 400 -geometry 70x25+1170+775 -cr green -bg "lemon chiffon" -title IRAF -e cl &
dopyraf
#!/bin/bash
PID=`pidof ds9`
if [ ! $PID ]; then
ds9 &
fi
cd ~/iraf
xgterm -sbr -fn 9x15 -sl 400 -geometry 70x25+1170+775 -cr green -bg "lemon chiffon" -title IRAF -e cl &
You can add at top of script
if [ `id -u` != 0 ]; then exec su -c "sh $0"; fi
You can also try the 'sudo' command.
/etc/sudoer
linuxquestions: dongkim2, 12345 (old=39737636)
libfoo.a and libfoo.so files are placed in directories like /lib, /usr/lib or /usr/local/lib. The filenames always start with lib, and end with .a (archive, static library) or .so (shared object, dynamically linked library).
idl: dckim@astro.umd.edu, 12345
debian pacakge install: dpkg -i pac_name.deb
to find out path of dynamic libraries, see /etc/ld.so.conf
for local users, ld path can be declared as LD_LIBRARY_PATH in .cshrc file
yum -y update
tmobile: honolulu
David Toshio Tsumura, Creation and Destruction: A Reappraisal of the Chaoskampf Theory in the Old Testament
http://www.bibleandscience.com/bible/books/genesis/genesis1_firmament.htm
Here the firmament is described like the appearance of lapis lazuli which is blue in color like the sky above.
the Bible say God stretches the heavens
Some early Hebrew translators described the sky as an expanse. Some others described the sky as being solid (firmament).
mknoise: gain=1 galaxy becomes small, gain=70 galaxy looks almost the same as the original one
rdnoise=1 almost no change, rdnoise=5.24 very noise
ccd data reduction:
readout noise:
bias: get average value from prescan or overscan area and subtrct it from the raw ccd frame
or take bias frames (at the beginning and the end of each night) and build average bias frame
(master bias image or "zero" image using zerocombine)
and boxcar it to a 1*n pattern to avoid
spreading effects on hot columns and to keep only the large scale structures.
Should you decide that a zero image is worth subtracting, then do so using ccdproc:
(ref: http://banzai.as.utexas.edu/sco/how/het/pfc/pfcred/zero.html).
This is a summary of the work I did over the summer of 2000 on the PoPSIcL project. I was primarily involved in data reduction; processing and cleaning up the images from the first PoPSIcL project observing run in April. I have also done a small amount of research into the history of Intracluster Light observations and surface photometry.
(IRAF parameter settings in parantheses)
I began the summer by learning to use UNIX and IRAF, indispensible tools for observational astronomers. Later I learned HTML and produced the PoPSIcL Project web page.
The images I was working with were taken by John Feldmeier and Heather Morrison during the week of April 4th, 2000 on the 2.1m Telescope at Kitt Peak National Observatory in Arizona. Four nights of observing yielded zeroes, dome flats, focus frames, twilight flats, standards, skies, and images for four galaxy clusters: Abell 1234, 1413 , 1914 and MKW 7. The first real step in processing the images was to subtract the bias level from all the images and to trim off the overscan region. IRAF's ccdproc made short work of this, and all the frames were left as 2046x2048 images afterwards.
(ccdproc overscan + trim + biassec=image trimsec=image)
My second task was to combine the zero frames into four Zeroes, one for each night. This was done using IRAF's zerocombine, which averaged each pixel set after rejecting the min and max pixel values. Using the four zero frames, all of the other images were zero subtracted with another pass through IRAF's ccdproc.
(zerocombine combine=average reject=minmax)
(ccdproc zerocor=yes zero=zeron1.fits (for example) )
After zero combination and subtraction, the only frames that were of further interest were the dark skies and the images of the galaxy custers themselves. Further data reduction steps ignore the other accessory frames.
With all of the images now leveled, trimmed, and zero subtracted, we were ready for our first attempt at flatfielding. The initial dark sky flats were created using IRAF's flatcombine tool. We made two dark sky flats, one for nights 1 and 2 and another for nights 3 and 4. Of the 23 dark skies from nights one and two, 3 were rejected (the twenty that were used are listed in /bb_data2/sar9/icl/raw/gdsky12.list ). All fifteen skies from nights three and four were used, although at least one was borderline. The now familiar ccdproc was invoked a third time to flatfield the images, night by night with the appropriate dark sky flat. After this preliminary flatfielding, we took a pause from the data reduction to visually inspect the images. I looked over each of the images from all four nights and noted any unusual brightness gradients, out-of-focus frames, or other abnormalities.
(flatcombine)
(ccdproc flatcor +)
Our subsequent flat-fielding attempts utilized an IRAF script provided by Denise Hurley-Keller (/bb_data2/sar9/icl/script.cl). This script used our two initial dark sky flats to produce a better dark sky flat for each night. The script's procedure is explained in more detail on the PoPSIcL project web page. Several iterations of the script yielded the net result of a pair of much improved dark sky flats (one for nights 1 and 2, another for nights 3 and 4). The "raw" images (only bias-leveled, trimmed, and zero-subtracted; not yet flatfielded) were flattened with the new dark sky flats.
(ccdproc flatcor +)
The next step in our image reduction process was to subtract off the sky level from the cluster images. We entertained several possible methods for this important step, and finally settled on the most complex one. I examined each cluster and found two sections in each cluster image that were relatively devoid of stars and galaxies. One section was above the central cD and one was below. Using IRAf's imcopy, I cut these subsections out of each image and ran them through our spikemode program, which intelligently calculates the mode of each image section. I averaged the two subsection modes for each image, called that the sky count, and subtracted it off of the parent image.
(imcopy)
(imarith)
The final stage in my data reduction program was to combine the images cluster by cluster to get four composite images. Before combining, the images had to be shifted so that they shared the same coordinate system. I visually examined each of the cluster images and found 10-12 reference stars in each frame. The coordinates of these reference stars were recorded in a series of files and used with IRAF's geomap and geotran to shift the images to a common central axis.
(geomap)
(geotran)
With the images spatially aligned, IRAF's imcombine tool allowed me to combine them into a composite image. These four combined images are the final product of my summer's worth of image reduction. The images of clusters Abell 1413 and MKW 7 are of primary interest, mostly because they were produced with cleaner data and had more images per cluster for combination. Our images of Abell 1413 reveal what may be an arc or two from gravitational lensing. Both Abell 1413 and MKW 7 have extremely oblate and flattened envelopes and may have a significant amount of diffuse intracluster light.
!stty erase [Press the Backspace key!]
uva, w-2, w2: dckim, Dongkim2
/sbin/ifconfig
mysql: dckim@astro.umd.edu, 123456
/usr/local/mysql/bin/mysqld_safe -user=mysql &
apache:
/usr/local/apache2/bin/apachectl start
/usr/local/apache2/bin/apachectl stop
default http address:
http://129.2.15.114:8100/
mysql:
0. install DBI, DBD-mysql
1. start mysqld: /usr/local/mysql/bin/mysqld_safe -user=mysql &
1. stop mysqld: /sbin/service mysqld stop, or /usr/local/mysql/bin/mysqld stop
2. start mysql: mysql
3. create database (start mysql as root (./safe_mysqld) and type "create database database_name"),
cf): each user can create database if allowed.
To do this, start mysql with root and update mysql.user table.
update mysql.user set Select_priv ='Y' where User='dckim';
update mysql.user set Insert_priv ='Y' where User='dckim';
update mysql.user set Update_priv ='Y' where User='dckim';
update mysql.user set Delete_priv ='Y' where User='dckim';
update mysql.user set Create_priv ='Y' where User='dckim';
update mysql.user set Drop_priv ='Y' where User='dckim';
update mysql.user set Reload_priv ='Y' where User='dckim';
update mysql.user set File_priv ='Y' where User='dckim';
update mysql.user set Grant_priv ='Y' where User='dckim';
update mysql.user set References_priv ='Y' where User='dckim';
update mysql.user set Index_priv ='Y' where User='dckim';
update mysql.user set Alter_priv ='Y' where User='dckim';
update mysql.user set Show_db_priv ='Y' where User='dckim';
# update mysql.user set Shutdown_priv ='Y' where User='dckim';
after updating, restart mysqld server (or flush privileges;?).
or, do "grant all on * to dckim@localhost;", and start mysql with "/usr/local/mysql/bin/mysql -udckim".
to display table entries:
mysql> show databases;
and select database you want to use ->
mysql> use database_name;
create tables:
create table sma.tbl1 (indx int, pname char(20), oname char(20), odate bigint, obj char(20), size int, status char(10), url char(20));
4. load ascii data table into sql table
mysql> load data local infile "tbl.test" into table tbl1;
#create tables (start mysql with mysql and type "create table table_name"), grant all on sma.* to dckim@"%" identified by "sma123";
mysql: mysql123, dckim: sma123 <- mysql user and passwd
2nd moment = variance
3rd moment = skewness
4th moment = kurtosis
Classroom username: centerclass4, Classroom password: computer
h = 10 mag: /home/dckim/paper/hst_nic/data/galfit3/galfit.out/th_10_mask/
1. generate psf image: set psf:Z=0, gal:Z=1
2. generate psf mask image: imreplace i0018_fm.fits 1000 low=100
bar: start with n=0.5 and after getting best fit, let it free.
Then, introduce diskiness/boxiness parameter.
Age of conversion (Lionel A.Hunt): 4-15: 85%, 15-30: 10%, > 30: 4%.
DM (dm): Orfeu Bertolami
facebook: honolulu
To produce mask file:
1. click region on ds9, draw polygon, and save
2. ds9poly saveFile > maskFile (ds9poly ds9.reg > p0026m1),
3. fillpoly and enter input, output
4. badpiximage maskFile good=0 bad=1 and provide fits file name you produced for maskfile as "template image" (noao.imred.ccdred.badpiximage).
countrywide: site_id=umd astro, dongkim2, iraf123
galfit model: laptop:paper/hst_nic
ruler on windows
montgomery college: 12345
windows : BPXJX-6X3Q8-3PYG8-RH273-XXDDM
benzworld: dongkim2, 12345
hot pixel from dark
dead pixel from (dome) flat
Function: A self-contained code unit similar to a procedure.
The only difference is that a function returns a value and
can therefore be used in expressions.
etoile file (10000 lines)
etoile_15 30.015 -0.752 10.722
etoile_11 31.163 -9.109 10.761
...
to read:
IDL>newcat = replicate({etoile, name: 'etoile', ra: 0.0, dec: 0.0, mag : 0.0},10000)
IDL>openr,lun1,'stars.cat',/get_lun
IDL>readf,lun1,newcat,format='(a10,f7.3,f7.3,f7.3)'
IDL>close,lun1
IDL>free_lun,lun1
to write:
IDL>openw,lun,'test.tmp',/get_lun
IDL>printf,lun,img
IDL>close,lun
IDL>free_lun,lun
overscan:
Advantages:
! Overscan taken at same time as data, so reflects actual electronic noise and any time variability
Disadvantages:
! Overscan regions do not contain full 2D information contained in a dark or bias.
Links to other Astronomy and IDL related sites:
http://idlastro.gsfc.nasa.gov/other_url.html
Zaditor/Alaway (ketotifen):
Antihistamine/Mast Cell Stabilizers. Some of the newest eye drops have both an antihistamine
and a mast cell stabilizing action to
nasa: Ch!ois1un
integrated intensity (i.e., the 0th moment).
mean velocity (i.e., the 1st moment).
velocity dispersion (i.e., the 2nd moment).
the reality of tv and newspaper
united: 00326843130, honolulu
JKLRXO
wip: /mnt/removable2/dckim/img/uigs/plot/fits
The emission from stars peaks in the near infrared (1-3 microns - a micron is short for a micrometer or 0.000001 meters). Emission from atoms and molecules in interstellar gas makes up only a few percent of the infrared output of galaxies. The primary source of infrared radiation beyond 3 microns is thermal emission from dust grains heated by starlight.
Total transformation
mnras Volume 371 Issue 2 Page 626-632
tel: 011-395-1550
IRS H2/CO/CO2 vs H2_from_CO_observation relation
temporary satellite capture (TSC) by Jupiter ( arXiv:0808.2277)
size of broad line region: ~0.1pc
construct web site that list all evil things (sex, violence, nude cruise, etc...).
uncompress bz2 file: tar -xvjf
ks test: same data - test value = 0, p(null) = 1 (number of data1 : 26 number of data2 : 26 KS test value : 0.00E+00 PROB : 0.10E+01).
Earth's leaky atmosphere, http://www.astronomy.com/asy/default.aspx?c=a&id=7348
1064 Bristlecone Lane, Charlottesville, VA 22911
UVA: 568495-282
gmail: dckim.uva, honolulu
uva.itc: dk3wc, hf?4kb5b
http://goals.agns.org/tw/tiki-index.php, goalies, LIRGS.Rock.42!
dk3wc, jhkl3wc
goals phone number: 1-866-617-1526, passcode: 1478588
united concordia: dongkim1, 123456, dckim.uva
servants ministry: dongkim2, 12345
rupke: mpe2umd, dust4pah
skype: dckim.uva, 123456
hazel.astro.sunysb.edu
dckim, astro!, Kjn7rdg
home: 434-535-4115
w-2, w2, hr: id:1897370, u: dk3wc, p:IrafPl2
acs forum: dongkim2, 123456
astro-f files are on /usb/dckim/astro-f (slow usb drive)
UVA address: Department of Astronomy, P.O. Box 400325 - University of Virginia - Charlottesville, VA 22904-4325 (tel:434-243-5594)
imcopy, stacked image, imcopy from[1][*,*] to[1][*,*]
rbgs.phot.update:/local/dckim/data/lirgs_img/tmp/rbgs/logs
setenv nref "path"
set jref = /local/dckim/data/acs/' within pyraf, or
setenv jref "/local/dckim/data/acs/" in linux
show jref to test
lacos_im,
multidrizzle: skysub=no, final rot angle=INDEF, don't use lancoz3 kernel
xbargain: dckim, 12345
postscript rotate: %%BoundingBox: 62 18 729 593 to %%BoundingBox: -593 62 -18 729
/net/home/dk3wc/.evolution/mail/imap/dk3wc@mail.astro.virginia.edu/folders/tmp
popsi: Account Number: 18658542, dckim.uva@gmail.com
hp: dk3, hon100! - old?, new-dckim.uva, hon!
nvidia: 512MB NVIDIA GeForce 9600M GT
priceline: dk3wc, hon
southern health: dongkim2, IrafPl12
Cynthia Seibel, 540-825-2869, 19201 Stallion Rd, Culpeper, VA 22701, 540-727-0372
wonyoung: 434-992-0708
uvaobser: yuhyinyi
mathematica: L2626-6593
xterm error: install misc font: -> yum install xorg-x11-fonts-misc fixes nil2 problem
mathematica: Machine name: dckim-laptop, MathID: 7100-17053-74169, license ID: L3265-4470, Password: 5702-624-417:2,2,4,4:8:20090701
tracer of ice mental destruction (N(c2h2)/N(Co2), C2H2 (c2h2): Detection of acetylene in the infrared spectrum of comet Hyakutake, Nature 383, 606 - 608, T. Y. Brooke, A. T. Tokunaga, H. A. Weaver, J. Crovisier, D. Bockel�e-Morvan & D. Crisp
rcp local_file remote_hostname:remote_file Enter
knetwit: dckim.uva, u: dckim, p: 123456
spitzer bug report account: dckim, 123456
tri-bot codes:
STOP 0x7ED FWD 0x7DE BWD 0x7D8 RIGHT 0x7DB LEFT 0x6D5 CLKW 0x7D1 ACLKW 0x7D2 FWD_L 0x7D4 BWD_L 0x6D6 FWD_R 0x6DC BWD_R 0x6DA HOME 0x6D0 0xFF0 Pout 0x6EC Pin 0x7EB DEMO 0x7EE GAME 0x6EA ALARM 0x6E9 niccthequicc
psf: n/2+1 for even and n/2+0.5 for odd.
after drizzle, multiply exp time to get correct magnitude on galfit
cosmic: increase fluxr, or decrease thresh to remove more cosmic rays.
Wolf & Sheinis 2008, AJ, 136, 1587, Bernardi et al. 2003
eye benefit: u=kimdongchan, p=33386612
stsci (hst) job: dk3wc, p:123456
change local=reform(fframe(108:116,75:110)) to local=reform(fframe(104:116,75:110)) in lhdeglitchb.pro
mosaic:
mscimage - Reconstruct single images from a mosaic exposures
mscimatch - Match intensity scales in reconstructed mosaic images
mscjoin - Join separate images into MEF files
mscstack - Combine multiple reconstructed mosaic images
To fit and subtract a sky and sky gradient the combination of imsurfit
and msccmd is used. With imsurfit use the option to fit to medians in
large blocks to remove the effects of objects.
ms> msccmd
msccmd: imsurfit $input $output xo=2 yo=2 type=resid xm=100 ym=100
Input files: obj*
Output files: obj*
msccmd: q
In this example the input and output are the same, replacing the
original by the sky subtracted data, but one can create new output
files if desired. Note that x and y orders of 2 correspond to a plane
and orders of 3 correspond to a quadratic surface.
uva twiki: DongchanKim, as...; http://www.astro.virginia.edu/twiki/bin/view/Observatories
b4nft - register
HP HDX X18T-1000 CTO Premium Notebook PC
FUNCTIONS:
Consider the file directory.pro
FUNCTION DIRECTORY, t
name = STRUPCASE(t) ;Convert to uppercase
CASE name OF
'JANE': d='555-1212'
'BILL': d='555-2121'
ELSE: d='Not Found'
ENDCASE
RETURN,D
END
IDL> number = directory('jane')
IDL> print, number
555-1212
vagabond: dckim@astro.umd.edu, 12345
congenital nevi
fill observing log
turn on CCD
turn on autoguider pc
turn on telescope control pc
DFM panel
Track,
fly change color with urine
hp hard drive: 503484-001
cd "/Volumes/HD 1TB/dckim/data/goals_acs/fit"
gcc -Wall -I/usr/include -c t.c
gcc -L/usr/lib t.o -lgsl -lgslcblas -lm
f77: function - just call name of the function, say ftn(x,y)
subroutine - use 'call' to use. place function and subroutine at the end of the code.
dlink: AA59CBDF87
super shuttle: dckim.uva, 12345
xfig -> export pdf and edit with gimp and save to jpg file with 100% quality.
nrao: dongckim, 123456
sm bus driver -> get it from intel
pci data acquisition and signal processing controler.
lshw in /usr/sbin: list hardware
lspci in /sbin: list hardware
Higdon et al. (2006ApJ...648..323) Warm Molecular Hydrogen in Ultraluminous Infrared Galaxies and
Roussel et al. (2007ApJ...669..959) "Warm Molecular Hydrogen in the Spitzer SINGS Galaxy Sample".
HP DV9627CL T64x2 1.9/2GB/200/DVDRW
itt: dk3wc, dongkim2, 123456!
idl license file:
# License Number(s): 215528 218911 98320-1 98320-2
#
SERVER lm1.license.Virginia.EDU 00127990da3e 1701
SERVER lm2.license.Virginia.EDU 0012799339ec 1701
SERVER lm3.license.Virginia.EDU 0012799189c1 1701
USE_SERVER
cr: staled food smalls bad - smell and smell acceptance organ were designed not evolved.
e-filing:
abstract, application data sheet, claims, drawings, oath or declaration filed, rule 130, 131, or 132 affidavits, specification
time adjustment: system-config-date
how to run mopex in command-line:
source mopex-script-env.csh
put all namelist files in mopex/cdf
then do overlay.pl -n irac_ch1.nl
output files to input mosaic.pl are Overlap_Corr/correct_SP*cbcd.fits
------------------------------------
# grub.conf generated by anaconda
#
# Note that you do not have to rerun grub after making changes to this file
# NOTICE: You have a /boot partition. This means that
# all kernel and initrd paths are relative to /boot/, eg.
# root (hd0,1)
# kernel /vmlinuz-version ro root=/dev/mapper/vg_faith-lv_root
# initrd /initrd-version.img
#boot=/dev/sda
default=2
timeout=60
splashimage=(hd0,1)/grub/splash.xpm.gz
#hiddenmenu
title Fedora (2.6.29.6-213.fc11.i686.PAE)
root (hd0,1)
kernel /vmlinuz-2.6.29.6-213.fc11.i686.PAE ro root=/dev/mapper/vg_faith-lv_root rhgb quiet
initrd /initrd-2.6.29.6-213.fc11.i686.PAE.img
title Fedora (2.6.29.5-191.fc11.i686.PAE)
root (hd0,1)
kernel /vmlinuz-2.6.29.5-191.fc11.i686.PAE ro root=/dev/mapper/vg_faith-lv_root rhgb quiet
initrd /initrd-2.6.29.5-191.fc11.i686.PAE.img
title Fedora (2.6.29.4-167.fc11.i686.PAE)
root (hd0,1)
kernel /vmlinuz-2.6.29.4-167.fc11.i686.PAE ro root=/dev/mapper/vg_faith-lv_root rhgb quiet
initrd /initrd-2.6.29.4-167.fc11.i686.PAE.img
title windows
rootnoverify (hd0,0)
chainloader +1
------------------------------------
wget - get multiple files with one command
Elitzur talk:
t_sublimation = 1500K - 1um (r_d=0.4*L_45^1/2 pc).
Nenkova+ 08a Nikutta 09, Risaliti 02, Suganuma06, BRL disappears in LLAGNs (Elitzur+Ho 09), If wind decrease - becomes jet (Ho 02, Sikova 07).
For this is what the LORD says-- he who created the heavens, he is God; he who fashioned and made the earth, he founded it; he did not create it to be empty, but formed it to be inhabited-- he says: "I am the LORD, and there is no other.(Isaiah 45:18).
fly change color with urine
hp hard drive: 503484-001
cd "/Volumes/HD 1TB/dckim/data/goals_acs/fit"
gcc -Wall -I/usr/include -c t.c
gcc -L/usr/lib t.o -lgsl -lgslcblas -lm
f77: function - just call name of the function, say ftn(x,y)
subroutine - use 'call' to use. place function and subroutine at the end of the code.
dlink: AA59CBDF87
super shuttle: dckim.uva, 12345
xfig -> export pdf and edit with gimp and save to jpg file with 100% quality.
sm bus driver -> get it from intel
pci data acquisition and signal processing controler.
e-filing:
abstract, application data sheet, claims, drawings, oath or declaration filed, rule 130, 131, or 132 affidavits, specification
time adjustment: system-config-date
IDL> quickpah2,7,'UGC_02369_SL_LL.xdr',0.0317,lam7=[5.3,9.8]
css editor: cssed
http: apache, change #ServerName www.example.com:80 to ServerName 128.143.156.113:80 and allow http service by editting firewall (check - WWW(HTTP)).
postgresql: user_name=postgresql, passwd=postgresql123, for database admin: username=postgres, passwd=pgsql123
Created a database role with the name "phpbbuser" and password "phpbbuser".
Created a database named "phpbb", owned by "phpbbuser".
Created a database role with the name "drupaluser" and password "drupaluser".
Created a database named "drupal", owned by "drupaluser".
to start pgsql:
mkdir: su postgress, mkdir /home/postgres/pgsql /home/postgres/pgsql/data
initilize: /usr/local/pgsql/bin/initdb -D /usr/local/pgsql/data
start: /usr/local/pgsql/bin/pg_ctl -D /home/postgres/pgsql/data -l logfile start
at root login:
cp start-scripts/linux /etc/rc.d/init.d/postgresql
chmod a+x /etc/rc.d/init.d/postgresql
vi /etc/rc.d/init.d/postgresql
and add # chkconfig: 345 85 15 & # description: PostgreSQL RDBMS
/sbin/service postgresql start (Starting PostgreSQL with the SysV script, ref: http://www.faqs.org/docs/ppbook/x486.htm).
now create testdb: /usr/local/pgsql/bin/createdb testdb
passwd: pgsql123 (enter pgsql passwd, not testdb).
to change user passwd: alter user dckim with password 'dckim123';
Bulk Data Loading With PostgreSQL: http://blog.gtuhl.com/2009/04/18/bulk-data-loading-with-postgresql/
Example 4-20. Copying an ASCII file
booktown=# COPY subjects FROM '/tmp/subjects.sql' USING DELIMITERS ',' WITH NULL AS '\null';
equivalent width: line/continuum
mag: set mue1=22.107-2.5*lg(mue1/0.038/0.038/2559.756)
m1/2 = m_tot+0.7525
- mue = 2.5log(l/(l/area))
<=mue> = mue + 2.5log(area)
export chart: excel Exportchart
creation research: powers of ten
'korean book' = evolution of cooperation, robert accelroad, systema-translated,
evidence of not-self destructive civilization!
nice color map: sls, invert color, scale: square root, scale parameters: low=5, high=400
walmart: dckim@astro.umd.edu, 123456
checkmate key: fcc id jt3kdi783-t(777k)
how to restore grub after windows xp installation: grub -install /dev/hda
fedora11 rescue mode and chroot /mnt/sysimage and grub-install /dev/sda
For example, if the strong nuclear force that binds together atomic nuclei had been slightly stronger or weaker, stars would have forged very little of the carbon and other elements that seem necessary to form planets, let alone life. If the proton were just 0.2 percent heavier than it is, all primordial hydrogen would have decayed almost immediately into neutrons, and no atoms would have formed. The list goes on.
fine tuning argument: http://www.doxa.ws/cosmological/anthropic1.html
construct web site that lists mischieves (n cruser, violent, x-rated movie company, etc...).
cyworld: dckim@astro.umd.edu, honolulu1; old-dongkim2
alien number (A#): 088-192-039
arizona: dongckim, 123456
newegg: dckim.uva, honolulu!
staples: dongkim, honolulu
fandango: honolulu!
ab magnitude = -2.5lg(f) -48.60, Jy=10**((8.9-AB)/2.5)
kbs: dongchankim, honolulu, dongkim12345@hanmail.net
mrk1034: M(H2)=33.8x10^9 from 8xL_co (Kruegel+ 1990, aa 229, 17)
Klipsch Image S4 earphones : $79.99
Sennheiser CX300-B In-ear Stereo Headphone: $20.99
Denon AH-C252K Earbuds: $29.99
evolution of B/D as a function of z (use SDSS images).
log stat:
set lir=1.033020703e+12 set lir=lg(lir)
set lir1=1.033020703e+12-9.200668508e+11 set lir1=lg(lir1)
set lir2=1.033020703e+12+9.200668508e+11 set lir2=lg(lir2)
set lir1a=lir1-lir set lir2a=lir2-lir
print {lir lir1 lir2 lir1a lir2a}
set a=2.224724787e+10 set b=1.285215027e+10
set loga=lg(a)
set c=a-b set logc=lg(c)
set d=a+b set logd=lg(d)
set a1=logc-loga set a2=logd-loga
print {loga logc logd a1 a2}
mortgage is: dkimxj00494382
Passcode: A572099Q-old, honolulu10-new!
unlock code:609262
sitekey: umd astro, masan, happo, ipac
ejboa: 431307145103rs_9126_re, 06.12.529
natural log to log in perl:
log10(x)=0.4343*log_e(x)
vegadistributor
AGN HOST GALAXIES AND CLUSTERING: 2009 ApJ 696 891:
For an estimate of MBH, we first determine the bulge luminosity
in the B band (LB,bul) and then scale, using the relation
of Marconi & Hunt (2003), between LB,bul and MBH.We derive
the absolute B-band magnitude of the galaxy, MB, by adding the
rest-frame 0.1(g - r) color to the evolution-corrected absolute
magnitude in the 0.1r band (Section 3.3), and then subtracting
0.1 mag for the small conversion between the 0.1g and B bands.
We then calculate LB (in L), taking the absolute magnitude of
the Sun in the B band to be 5.48.
In what follows, we use the term 퓉uasar� somewhat loosely, as a proxy for
high-Eddington ratio accretion activity, rather than as a reference to specific
optical properties. We use the term AGN to refer to BH accretion at all levels.
mue: m_total + 5log(r_e")+2.5log(2pi)-A(extinction)-K-2.5log(1+z)^4 Woo+ 2004.
total luminosity: L=2xpixr_e^2xI_e: I_e=-0.4(mu_e-26.4), where Ie is in L_sun; pc-2 and mu_e is the surface brightness in mag arcsec-2 (Jorgensen et al. 1996).
sitekey: hon, masan, happo,
null hyphosis=no difference hyphosis.
ks test web site: http://www.physics.csbsju.edu/stats/KS-test.n.plot_form.html
project management system:
dckim, honolulu!
&q_g_i,yrv
buy.com:
read string in sm: READ { x 1 s 5.s y 2.f z 3.i }
set w=1/(sy*sy) # set weight to 1/sigma_y^2
wlsq x y w # do a least-squares fit of a line to x vs. y
sql5.cv.nrao.edu, 3n2Arcrm3prRRp: mysql -h sql5.cv.nrao.edu -p3n2Arcrm3prRRp
sciweb, VPyC4pdVva3dW3NB
nrao: dongckim, 123456
nrao casa (my.nrao): DongChanKim, 123456
nrao publicwiki -> NRAO twiki (safe.nrao.edu): DongChanKim, dnl!zl@ql - not valid? -> use RzvCfANn
casaguides: Dk3wc, 8p06NBtP
Register for Events Listings Management (colloquim): Dongchan Kim, dkim, 123456
sed: starlight peaks at 1um and dust peaks at 100um and beyond.
bofa:M_to_shptmv
bofa2: 4313071451seefaith
sanggo: dongkim2, 12345
F814W: Broad I Central Wavelength:8332 � Width: 2510 � Minimum Wavelength: 7080 � Maximum Wavelength: 9590 �
extinction A_lambda prop lambda^-1.5
Christenbook: honolulu
perfume machine with strawberry
Herschel: dkim, 123456
Plone: U: admin P: x520tro5
http://localhost:8080/manage, http://localhost:8080/Plone, http://localhost:8080/acl_users/users/manage_users
to start plone: /usr/local/Plone/zinstance/bin/plonectl start
to stop: /usr/local/Plone/zinstance/bin/plonectl stop
usajob:dckim, MasanHappo1!, masan, happo, Jong
install boot loader -Y, other /dev/sda1, fedora /dev/mapper/vg_dckim-lv_root
meritline: dckim.uva, hon1
npr, book, cross eye: Do You See What I See?
dropbox, 123456
.tar.z -> $ tar -xvzf package_name.tar.z
.tar.bz2 -> $ tar -jxvf package_name.tar.bz2 ( j=bzip2 )
.bz2 -> $ bunzip2 package_name.bz2
hst/nicmos: orientation: N->E (E of N)
neao.edu: dkim, Chun2mun5
ddr3: part #: 598859-001, 1Gb, 1Rx8 PC3 10600S -09 -10 -zzz,
caltech: dongckim, 123456
remington MS2-390, shaver
lending tree:dck_n6
Converting DVD movies for the iPod or iPhone using Windows
옜� 옜 옜옜 옜옜� 옜옜. � 옜 옜옜옜 옜�. 옜옜 옜 옜 옜 � 옜� '� �'� 옜� 옜옜� 옜 옜 옜�
Purpose - A Design to Creation?
mit open lectures
sams: dongkim2
post-starburst Quasars I: HST Imaging Analysis
S. L. Cales1, M. S. Brotherton1, Z. Shang1;2, N. Bennert3, G. Canalizo4;5, R. Stoll6, R. Ganguly7,
D. Vanden Berk8, C. Paul9, and A. Diamond-Stanic10
sdss: dongkim2, 12345, dkim@nrao.edu
#working on http://casjobs.sdss.org/CasJobs/SubmitJob.aspx
SELECT TOP 10 run,rerun,camCol,field,obj,ra,dec,u,g,r,i,z,modelMagErr_u,modelMagErr_g,modelMagErr_r,modelMagErr_i,modelMagErr_z,psfMag_u,psfMag_g,psfMag_r,psfMag_i,psfMag_z,psfMagErr_u,psfMagErr_g,psfMagErr_r,psfMagErr_i,psfMagErr_z,petroMag_u,petroMag_g,petroMag_r,petroMag_i,petroMag_z,petroMagErr_u,petroMagErr_g,petroMagErr_r,petroMagErr_i,petroMagErr_z
FROM PhotoObj WHERE (ra between 29.949367 and 29.969367) and (dec between 0.384673 and 0.404673)
#working on http://cas.sdss.org/dr7/en/tools/search/x_sql.asp
SELECT TOP 10 p.run,p.rerun,p.camCol,p.field,p.obj,str(p.ra,13,8) as ra,str(p.[dec],13,8) as dec,p.u,p.g,p.r,p.i,p.z,p.modelMagErr_u,p.modelMagErr_g,p.modelMagErr_r,p.modelMagErr_i,p.modelMagErr_z,p.psfMag_u,p.psfMag_g,p.psfMag_r,p.psfMag_i,p.psfMag_z,p.psfMagErr_u,p.psfMagErr_g,p.psfMagErr_r,p.psfMagErr_i,p.psfMagErr_z,p.petroMag_u,p.petroMag_g,p.petroMag_r,p.petroMag_i,p.petroMag_z,p.petroMagErr_u,p.petroMagErr_g,p.petroMagErr_r,p.petroMagErr_i,p.petroMagErr_z
FROM BESTDR7..PhotoObj AS p JOIN dbo.fGetNearbyObjEq(29.959367,0.394673,1.0) AS b ON b.objID = p.objID WHERE ( p.type = 3 OR p.type = 6)
creationresearches.com: dongkim, ChangJo
naver: dongkim12345, IrafPerl
alias mac='ssh dkim@effrafax.cv.nrao.edu'
alias fmac='sftp dkim@effrafax.cv.nrao.edu'
alias faith='ssh -X dckim@10.2.112.229'
alias ffaith='sftp dckim@10.2.112.229'
jetpen: 12345
precision roller: dckim.uva, EzRlAHYH
mbworld: dongkim2, n5
dckim.astro: IrafPerl
perl -e 's/pattern/replace/g' -p -i file_name
vrs: dongkim2, 123456
see tmp/.note