Figure 3 from UVUDF: UV Luminosity Functions at the Cosmic High Noon

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UVUDF: UV Luminosity Functions at the Cosmic High Noon

Authors: Vihang Mehta, Claudia Scarlata, Marc Rafelski, Timothy Gburek, Harry I. Teplitz, Anahita Alavi, Michael Boylan-Kolchin, Steven Finkelstein, Jonathan P. Gardner, Norman Grogin, Anton Koekemoer, Peter Kurczynski, Brian Siana, Alex Codoreanu, Duilia F. de Mello, Kyoung-Soo Lee, and Emmaris Soto

2017 The Astrophysical Journal 838 29.

Provider: AAS Journals

Caption: Figure 3.

Redshift distribution of the selected-dropout samples. The gray, blue, and red histograms show the distribution of the photometric, grism, and spectroscopic redshifts for the dropout samples, respectively. The curves show the completeness associated with the corresponding dropout criteria for a range of observed UV magnitudes, as computed from our completeness simulations (Section 3). The right-hand axis gives the scale for the completeness values.

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