Bridging Star-forming Galaxy and AGN Ultraviolet Luminosity Functions at z =4 with the SHELA Wide-field Survey

Matthew L. Stevans, Steven L. Finkelstein, Isak Wold, Lalitwadee Kawinwanichakij, Casey Papovich, Sydney Sherman, Robin Ciardullo, Jonathan Florez, Caryl Gronwall, Shardha Jogee, Rachel Somerville, L. Y.Aaron Yung

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Abstract

We present a joint analysis of the rest-frame ultraviolet (UV) luminosity functions of continuum-selected star-forming galaxies and galaxies dominated by active galactic nuclei (AGNs) at z ∼4. These 3740 z ∼4 galaxies are selected from broadband imaging in nine photometric bands over 18 deg2 in the Spitzer/HETDEX Exploratory Large Area Survey field. The large area and moderate depth of our survey provide a unique view of the intersection between the bright end of the galaxy UV luminosity function (M AB < -22) and the faint end of the AGN UV luminosity function. We do not separate AGN-dominated galaxies from star-formation-dominated galaxies, but rather fit both luminosity functions simultaneously. These functions are best fit with a double power law for both the galaxy and AGN components, where the galaxy bright-end slope has a power-law index of -3.80 ±0.10 and the corresponding AGN faint-end slope is . We cannot rule out a Schechter-like exponential decline for the galaxy UV luminosity function, and in this scenario the AGN luminosity function has a steeper faint-end slope of . Comparison of our galaxy luminosity function results with a representative cosmological model of galaxy formation suggests that the molecular gas depletion time must be shorter, implying that star formation is more efficient in bright galaxies at z =4 than at the present day. If the galaxy luminosity function does indeed have a power-law shape at the bright end, the implied ionizing emissivity from AGNs is not inconsistent with previous observations. However, if the underlying galaxy distribution is Schechter, it implies a significantly higher ionizing emissivity from AGNs at this epoch.

Original languageEnglish (US)
Article number63
JournalAstrophysical Journal
Volume863
Issue number1
DOIs
StatePublished - Aug 10 2018

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • galaxies: active
  • galaxies: evolution
  • galaxies: high-redshift
  • galaxies: luminosity function mass function
  • galaxies: statistics
  • quasars: general

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    Stevans, M. L., Finkelstein, S. L., Wold, I., Kawinwanichakij, L., Papovich, C., Sherman, S., Ciardullo, R., Florez, J., Gronwall, C., Jogee, S., Somerville, R., & Yung, L. Y. A. (2018). Bridging Star-forming Galaxy and AGN Ultraviolet Luminosity Functions at z =4 with the SHELA Wide-field Survey. Astrophysical Journal, 863(1), [63]. https://doi.org/10.3847/1538-4357/aacbd7