Figure 7 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 7.

UV-to-Hα ratio plotted as a function of age since the onset of star formation for a range of SFHs (single stellar population, single bursts, rising, and constant star formation) computed using the Bruzual & Charlot (2003) models. The shaded band shows the expected ﹩{\mathrm{log}}_{10}[\nu {L}_{\nu }(1500)/{L}_{{\rm{H}}\alpha }]﹩ value for constant star formation, after accounting for a range of metallicities as well as different IMFs. See text for a description of the models.

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