|
Steve Majewski (Principal Investigator), University of Virginia
Website, Email
|
John Bahcall (1934-2005), Institute for Advanced Study
Website
Bahcall led the Oort limit project analysis. He
worked on developing a program to simulate the SIM PlanetQuest
observations of disk stars, and worked with Majewski's
group on developing and characterizing the proposed Oort
limit target samples.
|
|
Doug Geisler, Universidad de Concepción
Website, Email
Geisler is part of the program of identifying halo K giants
using photometry. He is a co-I in the Grid Giant Star
Survey (GGSS), and the PI of a SIM PlanetQuest
preparatory grant to do follow-up photometry and
spectroscopy of Grid stars. |
Wolfgang Gieren, Universidad de Concepción
Website, Email
Gieren is establishing and
characterizing the Cepheid target list, assisting with
spectroscopy of bulge stars, and the creation of the GGSS
and halo K giant samples.
|
|
Eva Grebel, Astronomisches Institut, Basel
Website, Email
Grebel is playing an active role in the search for tidal
tails around dwarf satellites and globular clusters. She
has been leading the search of the open cluster
literature to identify brightest member stars.
|
Carl Grillmair, Caltech/Spitzer Science Center
Website, Email |
|
Kathryn Johnston, Columbia University
Website, Email |
Ricky Patterson, University of Virginia
Website, Email
Patterson plays a key role in organizing the day-to-day
operations of many observational programs. He is
involved in the K giant samples for the halo and Oort
surveys, the project to determine proper motion of
globular clusters and dwarf galaxies, and the search for
tidal tails. |
|
I. Neill Reid, Space Telescope Science Institute
Website, Email
Reid leads the observational program to identify
Cepheid and Mira variables suitable for probing the
potential of the Galactic disk. He is also
collaborating in the Oort limit determination.
|
Takahiro Sumi, Princeton University
Website,alternate website, Email
|
|
David Spergel, Princeton University
Website, Email
Spergel is leading the analysis of
R0 and the study of
the bulge kinematics. He will construct a model for the
Galactic bar and explore implications for the formation of
the bar. He is also part of the disk and
tidal tail analysis efforts.
|
Scott Tremaine, Institute for Advanced Study
Website, Email Tremaine is leading the analysis of the hot halo
tracers. He is investigating phase-mixing in galaxies
formed by mergers to determine the influence of incomplete
mixing on halo tracers, and is continuing work on simulations of
SIM PlanetQuest observations of disk parameters and on the Oort
limit analysis. |
Back to Taking Measure of the Milky Way KP Home