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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 2.

NGVS survey area, shown in heavy red, compared to the regions covered by a number of multi-wavelength surveys of the Virgo cluster (primarily at non-optical wavelengths). The different surveys are indicated in the legend at the top of the figure (the light gray area shows the region covered by UKIDSS/LAS; see the text for complete details). Complete coverage over the entire NGVS survey area is also available in the IR, optical, 21 cm H i line, and X-rays from 2MASS, SDSS, ALFALFA, and ROSAT, respectively.

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