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Star Forming Rates Between Z=0.25 And Z=1.2 From The Cadis Emission Line Survey
ASTRONOMY & ASTROPHYSICS, no. 1 (2003): 65-78
摘要
The emission line survey within the Calar Alto Deep Imaging Survey (CADIS) detects emission line galaxies by a scan with an imaging Fabry-Perot interferometer. It covers 5 fields of >100 square' each in three wavelengths windows centered on lambdasimilar or equal to700, 820, and 920 nm, and reaches to a typical limiting line flux of 3x10(...更多
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