Image Details

Choose export citation format:

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 9.

The number of H I–bearing satellite candidates within projected R200 versus the host halo mass. Points show individual hosts, colored by their H I sensitivity limits. Hosts with partial halo coverage (Table 1) are marked by upward arrows (four with Rcover/R200 = 70%–90% in full-size arrows, three with 90%−100% in half-size arrows). Error bars show binned means and 1σ scatter for two groups of our sample separated by median sensitivity: the deeper half with ﹩\mathrm{log}{M}_{{\rm{H}}\,{\rm\small{I}},{\rm{lim}}}\lt 6.7﹩ (in blue) and the rest with ﹩\mathrm{log}{M}_{{\rm{H}}\,{\rm\small{I}},{\rm{lim}}}\,\geqslant \,6.7﹩ (in yellow).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse