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- W1542895667 abstract "In this thesis, metal poor galaxies at 0.4 4.7 have been searched for and investigated in a sample of 600 faint emission line galaxies from four fields of the Calar Alto Deep Imaging Survey (CADIS). Employing an imaging Fabry-Perot interferometer, CADIS detects emission lines in three waveband windows, free of night-sky emission lines, at 700 nm, 820 nm, and 920 nm. Metal poor galaxies at 0.4 3 , and with model predictions, indicates that bright Ly-alpha galaxies are so rare beyond z=5 that a non-evolving population can be excluded.%%%%In dieser Arbeit werden metallarme Galaxien bei 0.4 4.7 anhand eines Samples von 600 schwachen Emissionsliniengalaxien von dem Calar Alto Deep Imaging Survey (CADIS) gesucht und untersucht. CADIS weist Emissionsliniengalaxien mit Hilfe eines Fabry-Perot-Interferometers in drei Wellenlaengenintervallen nach, die in Fenster minimaler Nachthimmelsemission bei 700 nm, 820 nm, und 920 nm platziert sind. Metallarme Galaxien bei 0.4 3 sowie mit Modellvorhersagen deutet an, dass helle Lyman-alpha Galaxien so selten bei z>5 sind, dass eine sich nicht entwickelnde Population ausgeschlossen werden kann." @default.
- W1542895667 created "2016-06-24" @default.
- W1542895667 creator A5048044337 @default.
- W1542895667 date "2002-12-01" @default.
- W1542895667 modified "2023-10-06" @default.
- W1542895667 title "Emission Line Galaxies from CADIS : High Redshift Lyman-Alpha Galaxies and Metal Poor Galaxies at Medium Redshift" @default.
- W1542895667 doi "https://doi.org/10.11588/heidok.00003067" @default.
- W1542895667 hasPublicationYear "2002" @default.
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