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Michael A. Pahre
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, Mail Stop 20, Cambridge, MA 02138
Office: (617) 495-7073; FAX 495-7073
mpahre@cfa.harvard.edu cfa-www.harvard.edu/~mpahre/

Education

1992-1998
Ph. D. in Astronomy, California Institute of Technology

1985-1989
A. B. Cum Laude, Harvard University, concentration: physics and astronomy

Employment Experience

2001-      
Astronomer, Harvard-Smithsonian Center for Astrophysics.
1998-2001
Hubble Postdoctoral Fellow and Associate of the Harvard College Observatory, Harvard-Smithsonian Center for Astrophysics, Faculty Sponsor: J. P. Huchra.
1992-1998
Research Assistant, Department of Astronomy, California Institute of Technology. Supervisors: S. G. Djorgovski, S. E. Persson, J. R. Mould.
1993-1995
Teaching Assistant, Department of Astronomy, California Institute of Technology.

1992
Teaching Fellow, Department of Astronomy, Harvard University.

1991-1992
Astronomer, Harvard-Smithsonian Center for Astrophysics, Submillimeter Array Group. Supervisor: P. T. P. Ho.
1989-1991
Secondary School Physics Teacher, U. S. Peace Corps Volunteer, Nkroful, Ghana.

1987-1988
Research Assistant, Harvard-Smithsonian Center for Astrophysics, Speckle Imaging Group. Supervisors: C. Papaliolios and P. Nisenson.

Fellowships and Awards

Robert J. Trumpler Award,
2001, Astronomical Society of the Pacific
Hubble Fellowship,
1998-2001
Kingsley Graduate Fellowship,
1994-1995
Jesse L. Greenstein Graduate Fellowship,
1993-1994

Professional Organizations

American Astronomical Society
(1992-  )

Research Interests

Elliptical Galaxies:
Scaling relations, evolution, stellar populations.
Stellar Populations:
Surface brightness fluctuations (near-infrared and optical), color gradients, Local Group.
Faint Field Galaxy Population:
Galaxy counts, redshift surveys, galaxy evolution.
High-Redshift Universe:
Protogalaxies, QSO luminosity function.
Clusters of Galaxies:
Multicolor detection techniques, Butcher-Oemler effect.
Instrumentation:
Infrared imaging detectors, wide-field multi-object spectroscopy.

Professional Activities

SIRTF:
IRAC Instrument GTO Science Team Panels on ``Galaxies'' and ``The Early Universe'' (1998-  )

Review Panels:
HST (Cycle 8), NASA (ROSS-99), Chandra (Cycle 2)

CfA:
co-organizer of Optical/IR Division lunch talk series (1998-  )

Referee:
numerous times for ApJ and MNRAS

Citations:
papers have been cited more than 500 times in the scientific literature since 1994.

Outreach:
work has been cited in popular articles in Science and Science News

Student:
Harvard undergraduate Nicholas Siegler:

Grants (Past, Current, and Pending)

HST
Archival Research, Cycle 6, The Evolution of Elliptical Galaxies in Clusters, Co-I (for institutional reasons), 8/1996-7/1997, $47,771

HST
Hubble Post-doctoral Fellowship, A Multi-color Search for Distant Clusters of Galaxies, 2/1998-1/2001, $190,694

HST
Archival Research, Cycle 9, Color Gradients in Elliptical Galaxies at $z = 0.5$: An Indicator of Galaxy Formation Processes, 4/2000-3/2001, $37,690

HST
Archival Research, Cycle 9, Co-I for The Fundamental Plane of Cluster Ellipticals at $z=0.18$: Establishing the Local Baseline, 4/2000-3/2001, $7,608 (SAO portion of total $45,234)

SAO
Research Equipment Proposal, Moderate Dispersion Grating for the Hectospec, FY2001, $75,000

NASA
Long-Term Space Astrophysics, The Evolution of ``Normal'' Galaxies and the Star Formation Rate Measured at Infrared Wavelengths, 5/2001-4/2006, $732,607 (pending)

References

Presentations of Work

Talks
 
Poster Papers
(lead author only)

About this document ...

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The translation was initiated by Michael Andrew Pahre on 2008-01-24


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Michael Andrew Pahre 2008-01-24