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首页> 外文期刊>The Astrophysical journal >THE GALAXY EVOLUTION EXPLORER; A SPACE ULTRAVIOLET SURVEY MISSION
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THE GALAXY EVOLUTION EXPLORER; A SPACE ULTRAVIOLET SURVEY MISSION

机译:星系演化浏览器;太空紫外线调查任务

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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 A). The surveys include an all-sky imaging survey (m_(AB) approx= 20.5), a medium imaging survey of 1000 deg~2 (m_(AB) approx= 23), a deep imaging survey of 100 deg2~ (m_(AB) approx= 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.
机译:我们概述了银河演化探测器(GALEX),这是美国宇航局于2003年4月28日发射的任务。GALEX正在执行首次太空UV天空勘测,包括在两个波段(1350-1750和1750-2750 A )。这些调查包括全天候成像调查(m_(AB)大约= 20.5),1000 deg〜2的中等成像调查(m_(AB)大约= 23),100 deg2〜(m_(AB )= 25),以及附近的星系测量。正在进行光谱(无缝隙)磨光测量(R = 100-200),具有各种深度和天空覆盖范围。许多目标与其他波段的现有或计划中的调查重叠。我们将使用测得的局部星系的紫外线特性,以及推论性观测值,来校准局部星系中紫外线与全球恒星形成率之间的关系。我们将将此校准应用于在深层成像和光谱调查中发现的遥远星系,以绘制红移范围0

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