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Baryonic Masses and Properties of Gaseous Satellite Galaxies

  • Authors: Jingyao Zhu, Yasmeen Asali, Mary E. Putman, Tobias Westmeier, W. J. G. de Blok, Barbara Catinella, Nathan Deg, Bi-Qing For, Dane Kleiner, Karen Lee-Waddell, Filippo M. Maccagni, D. J. Pisano, Austin X. Shen, Kristine Spekkens, Lister Staveley-Smith

Jingyao Zhu et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure B1.

Key ingredients of our injection method for assessing the H I sensitivity. Panel (1): dwarf H I column density profiles as a function of radius. The model dwarfs (Equation (B1)) are shown in solid lines, while the observed low-mass dwarfs from the literature (MH I < 107 M, from which the model parameters are derived) are shown in dashed lines (E. A. K. Adams & T. A. Oosterloo 2018; D. A. Hunter et al. 2021). Panels (2a) and (2b): the recovery rate as a function of injected dwarf mass. The WALLABY and MHONGOOSE example hosts shown here are at the median distance among each survey (Table 1). The red circles mark the MH I detectability thresholds at 25%, 50%, and 90% recovery rates.

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