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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 4.

Histograms showing the g-band magnitude distributions of all NGVS galaxies. The blue and orange histograms show, respectively, bona fide members and galaxies found, after the fact, to have velocities that place them beyond the v = 3500 km s−1 boundary adopted for Virgo. The green histogram shows the one galaxy, EVCC1010, identified as a Virgo member in the EVCC, but not originally included in the NGVS catalog. The red and violet histograms show NGVS galaxies identified in the VCC and in the EVCC, respectively. Finally, the brown histogram show NGVS galaxies with a measured recessional velocity. The panel to the right is plotted on a logarithmic y-axis to better highlight small samples.

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