THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY
By L. Ferrarese, P. Côté, J. Cuillandre, S. Gwyn, E. Peng, L. MacArthur, Pierre-Alain Duc, A. Boselli, S. Mei, T. Erben and 42 more. 2012
313 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/138b62d1d902173cab080a09eb1cfc22ecea810d
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- The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function (2012, methodology): “A much improved coverage of these parameters will soon be provided by the Next Generation Virgo Cluster Survey (Ferrarese et al. 2012) as shown in Ferrarese (2012).”
- CATALOG OF ULTRA-DIFFUSE GALAXIES IN THE COMA CLUSTERS FROM SUBARU IMAGING DATA (2016, background): “Recently, Mihos et al. (2015) found quite low SB (μ0 > 27 Vmag arcsec −2) galaxies in the Virgo cluster, and Boselli et al. (2016) noted that UDGs are easily detected in the Virgo cluster by the NGVS survey (Ferrarese et al. 2012).”
- GALAXIES AT THE EXTREMES: ULTRA-DIFFUSE GALAXIES IN THE VIRGO CLUSTER (2015, methodology): “Subsequent inspection of the deep NGVS imaging (Ferrarese et al. 2012) confirms all objects, providing deep u∗giz data9 with sub-arcsecond seeing.”
- CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products (2012, methodology): “…to re-analyse the CFHT Red Sequence Cluster Survey (RCS2, see for example van Uitert et al. 2011), and analyse the CFHT i′band imaging survey of the SDSS Stripe 82 region, the Next Generation Virgo Survey (NGVS, Ferrarese et al. 2012), and the Kilo Degree Survey (KiDS) on the VLT Survey Telescope.”
- APPROXIMATELY A THOUSAND ULTRA-DIFFUSE GALAXIES IN THE COMA CLUSTER (2015, background): “…Koganei, Tokyo, 184-8584 Japan 4 SOKENDAI (The Graduate University for Advanced Studies), Mitaka, Tokyo, 181-8588, Japan and low SBs, in clusters (e.g., Binggeli & Cameron 1991; Bothun et al. 1991; Ulmer et al. 1996, 2011; Adami et al. 2006b, 2009; Lieder et al. 2012; Ferrarese et al. 2012).”
- Simulating galaxy formation with the IllustrisTNG model (2017, background): “E-mail: pillepich@mpia-hd.mpg.de † Alfred P. Sloan Fellow neous environments – in isolation, or as members of rich groups and clusters (e.g. Ferrarese et al. 2012).”
- Globular clusters as the relics of regular star formation in ‘normal’ high-redshift galaxies (2015, methodology): “The Next Generation VirgoCluster Survey (Ferrarese et al. 2012) as well as the lensing results from Hudson, Harris & Harris(2014) now cover a large sample of galaxies all the way out to their virial radii, implying a slight increase of the dark matter mass per unit GC mass relative toSpitler &…”
- The ATLAS3D project - XXIX. The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images (2014, methodology): “• The LSB–optimized NGVS at the CFHT (Ferrarese et al. 2012) reaches 29 mag arcsec−2 in the g–band, a value checked comparing the surface brightness profile of the galaxy M49 with previously determined ones in the literature.”
- The ATLAS3D project XV: benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, fundamental plane and mass plane (2012, background): “The only real solution to the problem is to obtain deeper photometry so that Re values converge and become essentially independent of the adopted profiles (Kormendy et al. 2009; Ferrarese et al. 2012).”
- Illuminating Low Surface Brightness Galaxies with the Hyper Suprime-Cam Survey (2017, background): “Ferrarese et al. 2012; Duc et al. 2015; Fliri & Trujillo 2016; Trujillo & Fliri 2016).”