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The Next Generation Virgo Cluster Survey (NGVS). II. A Catalog of Galaxies in the Virgo Cluster

  • Authors: Laura Ferrarese, Patrick Côté, Lauren A. MacArthur, Joel C. Roediger, John P. Blakeslee, Michele Cantiello, Jean-Charles Cuillandre, Puragra Guhathakurta, Stephen Gwyn, Max M. Kurzner, Eric W. Peng, Matthew Santos, Eleanore B. Todd, Elisa Toloba, Pierre-Alain Duc, Patrick R. Durrell, Nicholas Fantin, Yuting Feng, Ariane Lançon, Sungsoon Lim, Chengze Liu, Deborah Lokhorst, Alessia Longobardi, Simona Mei, J. Christopher Mihos, Sanjaya Paudel, Thomas H. Puzia, Anand Raichoor, Rubén Sánchez-Janssen, Kaixiang Wang, Hongxin Zhang, Alessandro Boselli, Michael L. Balogh, Samuel Boissier, Eric Emsellem, J. J. Kavelaars, Alan W. McConnachie, Cameron R. Morgan, Chelsea Spengler, James E. Taylor, Matthew A. Taylor, Toby Brown, Sébastien Fabbro, Raphael Gavazzi, Hendrik Hildebrandt, Rashi Jain, Andrés Jordán, Rory Smith, Solveig Thompson, Haruka Yoshino, Wim van Driel, Ludovic van Waerbeke, Tyrone E. Woods, Jade Yeung

Laura Ferrarese et al 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 10.

Histogram showing the g-band magnitude distribution of NGVS galaxies classified as certain (Membership Class 0), likely (Membership Class 1), and possible (Membership Class 2) members, as well as galaxies found, after the fact, to have velocities that place them beyond the v = 3500 km s−1 boundary adopted for Virgo. Note that the latter histogram has been multiplied by a factor of 10 to make it easier to see it.

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