THE EVOLUTION OF THE FAINT END OF THE UV LUMINOSITY FUNCTION DURING THE PEAK EPOCH OF STAR FORMATION

We present a robust measurement of the rest-frame UV luminosity function (LF) and its evolution during the peak epoch of cosmic star formation at . We use our deep near-ultraviolet imaging from WFC3/UVIS on the Hubble Space Telescope and existing Advanced Camera for Surveys (ACS)/WFC and WFC3/IR ima...

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Veröffentlicht in:	The Astrophysical journal 2016-11, Vol.832 (1), p.56
Hauptverfasser:	Alavi, Anahita, Siana, Brian, Richard, Johan, Rafelski, Marc, Jauzac, Mathilde, Limousin, Marceau, Freeman, William R., Scarlata, Claudia, Robertson, Brant, Stark, Daniel P., Teplitz, Harry I., Desai, Vandana
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CAMERAS Completeness Computer simulation COMPUTERIZED SIMULATION DENSITY DISTRIBUTION Evolution Galactic clusters GALACTIC EVOLUTION GALAXIES GALAXY CLUSTERS Galaxy distribution GRAVITATIONAL LENSES Hubble Space Telescope Infrared imaging LUMINOSITY MASS MONTE CARLO METHOD Monte Carlo simulation Polls & surveys RED SHIFT Sciences of the Universe Size distribution Slopes SPACE Space telescopes Star & galaxy formation Star formation STARS Stars & galaxies Statistical methods Stellar evolution Systematics TELESCOPES ULTRAVIOLET RADIATION Uncertainty
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