The Astrophysical Journal (Jan 2025)

The NGC 3109 Satellite System: The First Systematic Resolved Search for Dwarf Galaxies Around an SMC-mass Host

  • Amandine Doliva-Dolinsky,
  • Burçin Mutlu-Pakdil,
  • Denija Crnojević,
  • Dhayaa Anbajagane,
  • Jeffrey L. Carlin,
  • Jonah Medoff,
  • David J. Sand,
  • Erik Tollerud,
  • Sungsoon Lim,
  • Paul Bennet,
  • Alex Drlica-Wagner,
  • Catherine E. Fielder,
  • Jonathan R. Hargis,
  • Kai Herron,
  • Laura Congreve Hunter,
  • Michael G. Jones,
  • Ananthan Karunakaran,
  • Annika H. G. Peter,
  • Aaron J. Romanowsky,
  • Kristine Spekkens,
  • Jay Strader,
  • Beth Willman,
  • Julio A. Carballo-Bello,
  • William Cerny,
  • Astha Chaturvedi,
  • Nitya Kallivayalil,
  • Clara E. Martínez-Vázquez,
  • Gustavo E. Medina,
  • Noelia E. D. Noël,
  • Andrew B. Pace,
  • Alex H. Riley,
  • Joanna D. Sakowska,
  • Adam Smercina,
  • Kathy Vivas,
  • Monika Adamów,
  • Clecio R. Bom,
  • Yumi Choi,
  • Peter S. Ferguson,
  • Mahdieh Navabi,
  • Alfredo Zenteno,
  • (DELVE Collaboration)

DOI
https://doi.org/10.3847/1538-4357/ade9b8
Journal volume & issue
Vol. 989, no. 1
p. 21

Abstract

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We report the results of the deepest search to date for dwarf galaxies around NGC 3109, a barred spiral galaxy with a mass similar to that of the Small Magellanic Cloud (SMC), using a semiautomated search method. Using the Dark Energy Camera, we survey a region covering a projected distance of ∼70 kpc of NGC 3109 ( D = 1.3 Mpc, R _vir ∼ 90 kpc, M ∼ 10 ^8 M _* ) as part of the MADCASH and DELVE-DEEP programs. We introduce a newly developed semiresolved search method, used alongside a resolved search, to identify crowded dwarf galaxies around NGC 3109. Using both approaches, we successfully recover the known satellites Antlia and Antlia B. We identified a promising candidate, which was later confirmed to be a background dwarf through deep follow-up observations. Our detection limits are well defined, with the sample ∼80% complete down to M _V ∼ −8.0, and include detections of dwarf galaxies as faint as M _V ∼ −6.0. This is the first comprehensive study of a satellite system through resolved stars around an SMC mass host. Our results show that NGC 3109 has more bright ( M _V ∼ −9.0) satellites than the mean predictions from cold dark matter models, but well within the host-to-host scatter. A larger sample of LMC/SMC-mass hosts is needed to test whether or not the observations are consistent with current model expectations.

Keywords