Correction: Photometric mass estimation and the stellar mass–halo mass relation for low mass galaxies (Monthly Notices of the Royal Astronomical Society (2023) 519:1 (871–883) DOI: 10.1093/mnras/stac3610)

Research output: Contribution to journalComment/debatepeer-review

Abstract

This is a correction to: Dennis Zaritsky and Peter Behroozi, Photometric mass estimation and the stellar mass–halo mass relation for low mass galaxies, Monthly Notices of the Royal Astronomical Society, Volume 519, Issue 1, May 2023, Pages 871–883, https://doi.org/10.1093/mnras/stac3610. Due to a mathematical error in our implementation, we presented an incorrect functional form for the best-fitting stellar mass–halo mass (SMHM) relation in the low mass regime. The corrected expression is Mh = 1010.02±0.02(M/108 M)0.77±0.02. This adjustment has no qualitative effect on the discussion or conclusions. This paper has been typeset from a TEX/LATEX file prepared by the author.

Original languageEnglish (US)
Pages (from-to)2696
Number of pages1
JournalMonthly Notices of the Royal Astronomical Society
Volume522
Issue number2
DOIs
StatePublished - Jun 1 2023

Keywords

  • dark matter
  • errata, addenda
  • galaxies: dwarf
  • galaxies: formation
  • galaxies: kinematics and dynamics
  • galaxies: nuclei
  • galaxies: structure

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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