The Galaxy Evolution Explorer:: A space ultraviolet survey mission

被引:1935
作者
Martin, DC
Fanson, J
Schiminovich, D
Morrissey, P
Friedman, PG
Barlow, TA
Conrow, T
Grange, R
Jelinsky, PN
Milliard, B
Siegmund, OHW
Bianchi, L
Byun, YI
Donas, J
Forster, K
Heckman, TM
Lee, YW
Madore, BF
Malina, RF
Neff, SG
Rich, RM
Small, T
Surber, F
Szalay, AS
Welsh, B
Wyder, TK
机构
[1] CALTECH, Pasadena, CA 91125 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Lab Astrophys Marseille, F-13376 Marseille, France
[4] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[5] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[6] Yonsei Univ, Ctr Space Astrophya, Seoul 120749, South Korea
[7] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA
[8] CALTECH, NASA IPAC Extragalact Database, Pasadena, CA 91125 USA
[9] NASA, Goddard Space Flight Ctr, Astron & Solar Phys Lab, Greenbelt, MD 20771 USA
[10] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
关键词
galaxies : evolution; galaxies : general; space vehicles : instruments; surveys; ultraviolet : galaxies; ultraviolet : general;
D O I
10.1086/426387
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 Angstrom). The surveys include an all-sky imaging survey (m(AB) similar or equal to 20.5), a medium imaging survey of 1000 deg(2) (m(AB) similar or equal to 23), a deep imaging survey of 100 deg(2) (m(AB) similar or equal to 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.
引用
收藏
页码:L1 / L6
页数:6
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