The galaxy evolution explorer: A space ultraviolet survey mission

D. Christopher Martin, James Fanson, David Schiminovich, Patrick Morrissey, Peter G. Friedman, Tom A. Barlow, Tim Conrow, Robert Grange, Patrick N. Jelinsky, Bruno Milliard, Oswald H.W. Siegmund, Luciana Bianchi, Yong Ik Byun, Jose Donas, Karl Forster, Timothy M. Heckman, Young Wook Lee, Barry F. Madore, Roger F. Malina, Susan G. NeffR. Michael Rich, Todd Small, Frank Surber, Alex S. Szalay, Barry Welsh, Ted K. Wyder

Research output: Contribution to journalReview articlepeer-review

1770 Citations (Scopus)


We give an overview of the Galaxy Evolution Explorer (GALEX), a NASA Explorer Mission launched on 2003 April 28. GALEX is performing the first space UV sky survey, including imaging and grism surveys in two bands (1350-1750 and 1750-2750 A). The surveys include an all-sky imaging survey (mAB ≃ 20.5), a medium imaging survey of 1000 deg2 (mAB ≃ 23), a deep imaging survey of 100 deg2 (mAB ≃ 25), and a nearby galaxy survey. Spectroscopic (slitless) grism surveys (R = 100-200) are underway with various depths and sky coverage. Many targets overlap existing or planned surveys in other bands. We will use the measured UV properties of local galaxies, along with corollary observations, to calibrate the relationship of the UV and global star formation rate in local 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 redshift range 0 < z < 2 and probe the physical drivers of star formation in galaxies. The GALEX mission includes a guest investigator program, supporting the wide variety of programs made possible by the first UV sky survey.

Original languageEnglish
Pages (from-to)L1-L6
JournalAstrophysical Journal
Issue number1 II
Publication statusPublished - 2005 Jan 20

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


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