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Proceedings Paper

The Galaxy Evolution Explorer
Author(s): Christopher Martin; Thomas Barlow; William Barnhart; Luciana Bianchi; Brian K. Blakkolb; Dominique Bruno; Joseph Bushman; Yong-Ik Byun; Michael Chiville; Timothy Conrow; Brian Cooke; Jose Donas; James L. Fanson; Karl Forster; Peter G. Friedman; Robert Grange; David Griffiths; Timothy Heckman; James Lee; Patrick N. Jelinsky; Sug-Whan Kim; Siu-Chun Lee; Young-Wook Lee; Dankai Liu; Barry F. Madore; Roger Malina; Alan Mazer; Ryan McLean; Bruno Milliard; William Mitchell; Marco Morais; Patrick F. Morrissey; Susan G. Neff; Frederic Raison; David Randall; Michael Rich; David Schiminovich; Wes Schmitigal; Amit Sen; Oswald H. W. Siegmund; Todd Small; Joseph M. Stock; Frank Surber; Alexander Szalay; Arthur H. Vaughan; Timothy Weigand; Barry Y. Welsh; Patrick Wu; Ted Wyder; C. Kevin Xu; Jennifer Zsoldas
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Paper Abstract

The Galaxy Evolution Explorer (GALEX), a NASA Small Explorer Mission planned for launch in Fall 2002, will perform the first Space Ultraviolet sky survey. Five imaging surveys in each of two bands (1350-1750Å and 1750-2800Å) will range from an all-sky survey (limit mAB~20-21) to an ultra-deep survey of 4 square degrees (limit mAB~26). Three spectroscopic grism surveys (R=100-300) will be performed with various depths (mAB~20-25) and sky coverage (100 to 2 square degrees) over the 1350-2800Å band. The instrument includes a 50 cm modified Ritchey-Chrétien telescope, a dichroic beam splitter and astigmatism corrector, two large sealed tube microchannel plate detectors to simultaneously cover the two bands and the 1.2 degree field of view. A rotating wheel provides either imaging or grism spectroscopy with transmitting optics. We will use the measured UV properties of local galaxies, along with corollary observations, to calibrate the UV-global star formation rate relationship in galaxies. We will apply this calibration to distant galaxies discovered in the deep imaging and spectroscopic surveys to map the history of star formation in the universe over the red shift range zero to two. The GALEX mission will include an Associate Investigator program for additional observations and supporting data analysis. This will support a wide variety of investigations made possible by the first UV sky survey.

Paper Details

Date Published: 24 February 2003
PDF: 15 pages
Proc. SPIE 4854, Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation, (24 February 2003); doi: 10.1117/12.460034
Show Author Affiliations
Christopher Martin, California Institute of Technology (United States)
Thomas Barlow, California Institute of Technology (United States)
William Barnhart, Orbital Sciences Corp. (United States)
Luciana Bianchi, Johns Hopkins Univ. (United States)
Brian K. Blakkolb, Jet Propulsion Lab. (United States)
Dominique Bruno, Orbital Sciences Corp. (United States)
Joseph Bushman, Orbital Sciences Corp. (United States)
Yong-Ik Byun, Yonsei Univ. (South Korea)
Michael Chiville, Orbital Sciences Corp. (United States)
Timothy Conrow, California Institute of Technology (United States)
Brian Cooke, Jet Propulsion Lab. (United States)
Jose Donas, Lab. d'Astrophysique de Marseille (France)
James L. Fanson, Jet Propulsion Lab. (United States)
Karl Forster, California Institute of Technology (United States)
Peter G. Friedman, California Institute of Technology (United States)
Robert Grange, Lab. d' Astrophysique de Marseille (France)
David Griffiths, Orbital Sciences Corp. (United States)
Timothy Heckman, Johns Hopkins Univ. (United States)
James Lee, Yonsei Univ. (South Korea)
Patrick N. Jelinsky, Univ. of California/Berkeley (United States)
Sug-Whan Kim, Yonsei Univ. (S. Korea)
Siu-Chun Lee, Applied Sciences Lab., Inc. (United States)
Young-Wook Lee, Yonsei Univ. (South Korea)
Dankai Liu, Jet Propulsion Lab. (United States)
Barry F. Madore, Carnegie Institute of Washington (United States)
Roger Malina, Lab. d'Astrophysique de Marseille (France)
Univ. of California/Berkeley (United States)
Alan Mazer, Jet Propulsion Lab. (United States)
Ryan McLean, California Institute of Technology (United States)
Bruno Milliard, Lab. d'Astrophysique de Marseille (France)
William Mitchell, Orbital Sciences Corp. (United States)
Marco Morais, California Institute of Technology (United States)
Patrick F. Morrissey, California Institute of Technology (United States)
Susan G. Neff, NASA Goddard Space Flight Ctr. (United States)
Frederic Raison, California Institute of Technology (United States)
David Randall, Jet Propulsion Lab. (United States)
Michael Rich, Univ. of California/Los Angeles (United States)
David Schiminovich, California Institute of Technology (United States)
Wes Schmitigal, Jet Propulsion Lab. (United States)
Amit Sen, Jet Propulsion Lab. (United States)
Oswald H. W. Siegmund, Univ. of California/Berkeley (United States)
Todd Small, California Institute of Technology (United States)
Joseph M. Stock, Univ. of California/Berkeley (United States)
Frank Surber, Jet Propulsion Lab. (United States)
Alexander Szalay, Johns Hopkins Univ. (United States)
Arthur H. Vaughan, Jet Propulsion Lab. (United States)
Timothy Weigand, Orbital Sciences Corp. (United States)
Barry Y. Welsh, Univ. of California/Berkeley (United States)
Patrick Wu, Jet Propulsion Lab. (United States)
Ted Wyder, California Institute of Technology (United States)
C. Kevin Xu, California Institute of Technology (United States)
Jennifer Zsoldas, Orbital Sciences Corp. (United States)

Published in SPIE Proceedings Vol. 4854:
Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation
J. Chris Blades; Oswald H. W. Siegmund, Editor(s)

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