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The Next Generation Virgo Cluster Survey (NGVS). I. Introduction to the Survey

  • Authors: Laura Ferrarese, Patrick Côté, Jean-Charles Cuillandre, S. D. J. Gwyn, Eric W. Peng, Lauren A. MacArthur, Pierre-Alain Duc, A. Boselli, Simona Mei, Thomas Erben, Alan W. McConnachie, Patrick R. Durrell, J. Christopher Mihos, Andrés Jordán, Ariane Lançon, Thomas H. Puzia, Eric Emsellem, Michael L. Balogh, John P. Blakeslee, Ludovic van Waerbeke, Raphaël Gavazzi, Bernd Vollmer, J. J. Kavelaars, David Woods, Nicholas M. Ball, S. Boissier, Stéphane Courteau, E. Ferriere, G. Gavazzi, Hendrik Hildebrandt, P. Hudelot, M. Huertas-Company, Chengze Liu, Dean McLaughlin, Y. Mellier, Martha Milkeraitis, David Schade, Chantal Balkowski, Frédéric Bournaud, R. G. Carlberg, S. C. Chapman, Henk Hoekstra, Chien Peng, Marcin Sawicki, Luc Simard, James E. Taylor, R. Brent Tully, Wim van Driel, Christine D. Wilson, Todd Burdullis, Billy Mahoney, and Nadine Manset

Ferrarese et al. 2012 The Astrophysical Journal Supplement Series 200 4.

  • Provider: AAS Journals

Caption: Figure 5.

Region surveyed by the NGVS overlaid on the Galactic extinction map from Schlegel et al. (1998). The gray scale corresponds to E( BV) values, as shown in the legend at the bottom. The area in red shows the footprint of the NGVS, which covers an area of 104 deg 2, as well as four "background" fields (4 deg 2 in total) that are located three virial radii (≈16.5 deg) from the cluster center. The crosses indicate the location of M87 and M49, which mark the centers of Virgo's two main substructures. Blue and magenta lines show grids in ecliptic and Galactic coordinates, respectively. The NGVS—the largest contiguous field mapped to this depth at optical wavelengths ( g = 25.9 mag, 10σ)—defines a low-extinction sight line at relatively high Galactic latitude ( lang b rang ~ 74°) and low ecliptic latitude ( langβ rang ~ 14°).

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