Paper
24 February 2003 The Galaxy Evolution Explorer
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
Author Affiliations +
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.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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, and Jennifer Zsoldas "The Galaxy Evolution Explorer", Proc. SPIE 4854, Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation, (24 February 2003); https://doi.org/10.1117/12.460034
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KEYWORDS
Sensors

Galactic astronomy

Space operations

Ultraviolet radiation

Imaging spectroscopy

Space telescopes

Telescopes

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