The Astrophysical Journal (Jan 2024)

PROVABGS: The Probabilistic Stellar Mass Function of the BGS One-percent Survey

  • ChangHoon Hahn,
  • Jessica Nicole Aguilar,
  • Shadab Alam,
  • Steven Ahlen,
  • David Brooks,
  • Shaun Cole,
  • Axel de la Macorra,
  • Peter Doel,
  • Andreu A. Font-Ribera,
  • Jaime E. Forero-Romero,
  • Satya Gontcho A Gontcho,
  • Klaus Honscheid,
  • Song Huang,
  • Theodore Kisner,
  • Anthony Kremin,
  • Martin Landriau,
  • Marc Manera,
  • Aaron Meisner,
  • Ramon Miquel,
  • John Moustakas,
  • Jundan Nie,
  • Claire Poppett,
  • Graziano Rossi,
  • Amélie Saintonge,
  • Eusebio Sanchez,
  • Christoph Saulder,
  • Michael Schubnell,
  • Hee-Jong Seo,
  • Małgorzata Siudek,
  • Federico Speranza,
  • Gregory Tarlé,
  • Benjamin A. Weaver,
  • Risa H. Wechsler,
  • Sihan Yuan,
  • Zhimin Zhou,
  • Hu Zou

DOI
https://doi.org/10.3847/1538-4357/ad19c8
Journal volume & issue
Vol. 963, no. 1
p. 56

Abstract

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We present the probabilistic stellar mass function (pSMF) of galaxies in the DESI Bright Galaxy Survey (BGS), observed during the One-percent Survey. The One-percent Survey was one of DESI’s survey validation programs conducted from 2021 April to May, before the start of the main survey. It used the same target selection and similar observing strategy as the main survey and successfully observed the spectra and redshifts of 143,017 galaxies in the r 100 × more galaxies. Moreover, we present the statistical framework for subsequent population statistics measurements using BGS, which will characterize the global galaxy population and scaling relations at low redshifts with unprecedented precision.

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