The Astrophysical Journal (Jan 2024)

The Ultraviolet Luminosity Function at 0.6 < z < 1 from UVCANDELS

  • Lei Sun,
  • Xin Wang,
  • Harry I. Teplitz,
  • Vihang Mehta,
  • Anahita Alavi,
  • Marc Rafelski,
  • Rogier A. Windhorst,
  • Claudia Scarlata,
  • Jonathan P. Gardner,
  • Brent M. Smith,
  • Ben Sunnquist,
  • Laura Prichard,
  • Yingjie Cheng,
  • Norman Grogin,
  • Nimish P. Hathi,
  • Matthew Hayes,
  • Anton M. Koekemoer,
  • Bahram Mobasher,
  • Kalina V. Nedkova,
  • Robert O’Connell,
  • Brant Robertson,
  • Sina Taamoli,
  • L. Y. Aaron Yung,
  • Gabriel Brammer,
  • James Colbert,
  • Christopher Conselice,
  • Eric Gawiser,
  • Yicheng Guo,
  • Rolf A. Jansen,
  • Zhiyuan Ji,
  • Ray A. Lucas,
  • Michael Rutkowski,
  • Brian Siana,
  • Eros Vanzella,
  • Teresa Ashcraft,
  • Micaela Bagley,
  • Ivano Baronchelli,
  • Guillermo Barro,
  • Alex Blanche,
  • Adam Broussard,
  • Timothy Carleton,
  • Nima Chartab,
  • Alex Codoreanu,
  • Seth Cohen,
  • Y. Sophia Dai,
  • Behnam Darvish,
  • Romeel Davé,
  • Laura DeGroot,
  • Duilia De Mello,
  • Mark Dickinson,
  • Najmeh Emami,
  • Henry Ferguson,
  • Leonardo Ferreira,
  • Keely Finkelstein,
  • Steven Finkelstein,
  • Timothy Gburek,
  • Mauro Giavalisco,
  • Andrea Grazian,
  • Caryl Gronwall,
  • Shoubaneh Hemmati,
  • Justin Howell,
  • Kartheik Iyer,
  • Sugata Kaviraj,
  • Peter Kurczynski,
  • Ilin Lazar,
  • John MacKenty,
  • Kameswara Bharadwaj Mantha,
  • Alec Martin,
  • Garreth Martin,
  • Tyler McCabe,
  • Charlotte Olsen,
  • Lillian Otteson,
  • Swara Ravindranath,
  • Caleb Redshaw,
  • Zahra Sattari,
  • Emmaris Soto,
  • Bonnabelle Zabelle,
  • the UVCANDELS team

DOI
https://doi.org/10.3847/1538-4357/ad5540
Journal volume & issue
Vol. 972, no. 1
p. 8

Abstract

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UVCANDELS is a Hubble Space Telescope Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields—GOODS-N, GOODS-S, EGS, and COSMOS—covering a total area of ∼426 arcmin ^2 . This is ∼2.7 times larger than the area covered by previous deep-field space UV data combined, reaching a depth of about 27 and 28 ABmag (5 σ in 0.”2 apertures) for F275W and F435W, respectively. Along with new photometric catalogs, we present an analysis of the rest-frame UV luminosity function (LF), relying on our UV-optimized aperture photometry method, yielding a factor of 1.5 increase over H-isophot aperture photometry in the signal-to-noise ratios of galaxies in our F275W imaging. Using well-tested photometric redshift measurements, we identify 5810 galaxies at redshifts 0.6 < z < 1, down to an absolute magnitude of M _UV = −14.2. In order to minimize the effect of uncertainties in estimating the completeness function, especially at the faint end, we restrict our analysis to sources above 30% completeness, which provides a final sample of 4726 galaxies at −21.5 < M _UV < −15.5. We performed a maximum likelihood estimate to derive the best-fit parameters of the UV LF. We report a best-fit faint-end slope of $\alpha =-{1.359}_{-0.041}^{+0.041}$ at z ∼ 0.8. Creating subsamples at z ∼ 0.7 and z ∼ 0.9, we observe a possible evolution of α with redshift. The unobscured UV luminosity density at M _UV < −10 is derived as ${\rho }_{{\rm{U}}{\rm{V}}}={1.339}_{-0.030}^{+0.027}\,(\times {10}^{26}\,{\rm{e}}{\rm{r}}{\rm{g}}\,{{\rm{s}}}^{-1}\,{{\rm{H}}{\rm{z}}}^{-1}\,{{\rm{M}}{\rm{p}}{\rm{c}}}^{-3})$ using our best-fit LF parameters. The new F275W and F435 photometric catalogs from UVCANDELS have been made publicly available on the Barbara A. Mikulski Archive for Space Telescopes.

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