The `Virgo Photometry Catalogue' (VPC) is the first independently calibrated general catalogue of galaxies to cover the Virgo cluster since the `Catalog of Galaxies and Clusters of Galaxies' of Zwicky et al. (1961,1963). It contains 1180 galaxies (including background objects) within a 23 square-degree region centred on the cluster's core. Photographic surface photometry is presented for 1067 galaxies in the U band, for 1020 galaxies in the B_J band and for 1020 galaxies in the R_C band. All total magnitudes and total colours are extrapolated according to a new system; denoted `t' to distinguish it from the `T' system already in use. This paper outlines: the scope of the VPC, the new extrapolation system, some recent findings based on the c...
We present a new catalog of galaxies in the wider region of the Virgo cluster, based on the Sloan Di...
The Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited survey of the Virgo Clu...
International audienceThe Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 d...
Surface photometry is one area of extragalactic studies in which information is urgently needed by o...
We use deep optical photometry from the Next Generation Virgo Cluster Survey (NGVS) to investigate t...
International audienceWe use deep optical photometry from the Next Generation Virgo Cluster Survey [...
International audienceWe use deep optical photometry from the Next Generation Virgo Cluster Survey [...
We use deep optical photometry from the Next Generation Virgo Cluster Survey (NGVS) to investigate t...
International audienceWe report on a large-scale study of the distribution of globular clusters (GCs...
The Virgo Cluster is the dominant mass concentration in the Local Supercluster and the largest colle...
This thesis describes the implementation and results of a prograunue of photometry of the relativel...
The Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 deg(2) MegaCam instrume...
International audienceThe Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited s...
The Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 deg 2 MegaCam instrumen...
We present a new catalog of galaxies in the wider region of the Virgo cluster, based on the Sloan Di...
The Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited survey of the Virgo Clu...
International audienceThe Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 d...
Surface photometry is one area of extragalactic studies in which information is urgently needed by o...
We use deep optical photometry from the Next Generation Virgo Cluster Survey (NGVS) to investigate t...
International audienceWe use deep optical photometry from the Next Generation Virgo Cluster Survey [...
International audienceWe use deep optical photometry from the Next Generation Virgo Cluster Survey [...
We use deep optical photometry from the Next Generation Virgo Cluster Survey (NGVS) to investigate t...
International audienceWe report on a large-scale study of the distribution of globular clusters (GCs...
The Virgo Cluster is the dominant mass concentration in the Local Supercluster and the largest colle...
This thesis describes the implementation and results of a prograunue of photometry of the relativel...
The Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 deg(2) MegaCam instrume...
International audienceThe Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited s...
The Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 deg 2 MegaCam instrumen...
We present a new catalog of galaxies in the wider region of the Virgo cluster, based on the Sloan Di...
The Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited survey of the Virgo Clu...
International audienceThe Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 d...