The Astrophysical Journal (Jan 2024)

A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55

  • M. McNanna,
  • K. Bechtol,
  • S. Mau,
  • E. O. Nadler,
  • J. Medoff,
  • A. Drlica-Wagner,
  • W. Cerny,
  • D. Crnojević,
  • B. Mutlu-Pakdıl,
  • A. K. Vivas,
  • A. B. Pace,
  • J. L. Carlin,
  • M. L. M. Collins,
  • P. S. Ferguson,
  • D. Martínez-Delgado,
  • C. E. Martínez-Vázquez,
  • N. E. D. Noel,
  • A. H. Riley,
  • D. J. Sand,
  • A. Smercina,
  • E. Tollerud,
  • R. H. Wechsler,
  • T. M. C. Abbott,
  • M. Aguena,
  • O. Alves,
  • D. Bacon,
  • C. R. Bom,
  • D. Brooks,
  • D. L. Burke,
  • J. A. Carballo-Bello,
  • A. Carnero Rosell,
  • J. Carretero,
  • L. N. da Costa,
  • T. M. Davis,
  • J. De Vicente,
  • H. T. Diehl,
  • P. Doel,
  • I. Ferrero,
  • J. Frieman,
  • G. Giannini,
  • D. Gruen,
  • G. Gutierrez,
  • R. A. Gruendl,
  • S. R. Hinton,
  • D. L. Hollowood,
  • K. Honscheid,
  • D. J. James,
  • K. Kuehn,
  • J. L. Marshall,
  • J. Mena-Fernández,
  • R. Miquel,
  • M. E. S. Pereira,
  • A. Pieres,
  • A. A. Plazas Malagón,
  • J. D. Sakowska,
  • E. Sanchez,
  • D. Sanchez Cid,
  • B. Santiago,
  • I. Sevilla-Noarbe,
  • M. Smith,
  • G. S. Stringfellow,
  • E. Suchyta,
  • M. E. C. Swanson,
  • G. Tarle,
  • N. Weaverdyck,
  • P. Wiseman,
  • DES & DELVE Collaboration

DOI
https://doi.org/10.3847/1538-4357/ad07d0
Journal volume & issue
Vol. 961, no. 1
p. 126

Abstract

Read online

We report results from a systematic wide-area search for faint dwarf galaxies at heliocentric distances from 0.3 to 2 Mpc using the full 6 yr of data from the Dark Energy Survey (DES). Unlike previous searches over the DES data, this search specifically targeted a field population of faint galaxies located beyond the Milky Way virial radius. We derive our detection efficiency for faint, resolved dwarf galaxies in the Local Volume with a set of synthetic galaxies and expect our search to be complete to M _V ∼ (−7, −10) mag for galaxies at D = (0.3, 2.0) Mpc. We find no new field dwarfs in the DES footprint, but we report the discovery of one high-significance candidate dwarf galaxy at a distance of ${2.2}_{-0.12}^{+0.05}\,\mathrm{Mpc}$ , a potential satellite of the Local Volume galaxy NGC 55, separated by 47′ (physical separation as small as 30 kpc). We estimate this dwarf galaxy to have an absolute V -band magnitude of $-{8.0}_{-0.3}^{+0.5}\,\mathrm{mag}$ and an azimuthally averaged physical half-light radius of ${2.2}_{-0.4}^{+0.5}\,\mathrm{kpc}$ , making this one of the lowest surface brightness galaxies ever found with $\mu =32.3\,\mathrm{mag}\,{\mathrm{arcsec}}^{-2}$ . This is the largest, most diffuse galaxy known at this luminosity, suggesting possible tidal interactions with its host.

Keywords