VizieR Online Data Catalog: Massive quiescent ETG in clusters (Delaye+ 2014)

L. Delaye; M. Huertas-Company; S. Mei; C. Lidman; R. Licitra; A. Newman; A. Raichoor; F. Shankar; F. Barrientos; M. Bernardi; P. Cerulo; W. Couch; R. Demarco; R. Munoz; R. Sanchez-Janssen; M. Tanaka

VizieR Online Data Catalog: Massive quiescent ETG in clusters (Delaye+ 2014)

L. Delaye, M. Huertas-Company, S. Mei, C. Lidman, R. Licitra, A. Newman, A. Raichoor, F. Shankar, F. Barrientos, M. Bernardi, P. Cerulo, W. Couch, R. Demarco, R. Munoz, R. Sanchez-Janssen, M. Tanaka

Research School of Astronomy & Astrophysics

Research output: Other contribution

Abstract

Our targets have been selected according to the following criteria: (1) they cover a broad redshift range 0.84All clusters have HST/ACS WFC (Wide Field Camera) images in at least two bandpasses. The ACS WFC resolution is 0.05-arcsec/pix, and its field of view is 210-arcsecx204-arcsec. The ACS/WFC PSF width is around 0.11arcsec. Our ACS/WFC images were mostly obtained in a programme designed to find Type Ia supernovae in distant galaxy clusters (Dawson et al., 2009AJ....138.1271D). See Meyers et al. (2012ApJ...750....1M) for a description of how these data were processed. Three clusters (see below): RDCS J1252-2927, XMMU J2235.3-2557 and RX J0152-1357 had been previously targeted with the ACS camera on HST in the context of the ACS Intermediate Redshift Cluster Survey (Ford 2004, HST Proposal ID 10327, ACS Imaging of a High-Redshift Cluster of Galaxies; Postman et al. 2005ApJ...623..721P; Mei et al. 2009ApJ...690...42M) and these data have been included.

(1 data file).

Original language	English
Publication status	Published - 1 Jan 2015

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@misc{16835b3bf0004f00a938679ba69f40cc,

title = "VizieR Online Data Catalog: Massive quiescent ETG in clusters (Delaye+ 2014)",

abstract = "Our targets have been selected according to the following criteria: (1) they cover a broad redshift range 0.84All clusters have HST/ACS WFC (Wide Field Camera) images in at least two bandpasses. The ACS WFC resolution is 0.05-arcsec/pix, and its field of view is 210-arcsecx204-arcsec. The ACS/WFC PSF width is around 0.11arcsec. Our ACS/WFC images were mostly obtained in a programme designed to find Type Ia supernovae in distant galaxy clusters (Dawson et al., 2009AJ....138.1271D). See Meyers et al. (2012ApJ...750....1M) for a description of how these data were processed. Three clusters (see below): RDCS J1252-2927, XMMU J2235.3-2557 and RX J0152-1357 had been previously targeted with the ACS camera on HST in the context of the ACS Intermediate Redshift Cluster Survey (Ford 2004, HST Proposal ID 10327, ACS Imaging of a High-Redshift Cluster of Galaxies; Postman et al. 2005ApJ...623..721P; Mei et al. 2009ApJ...690...42M) and these data have been included. (1 data file).",

keywords = "Clusters: galaxy, Galaxies: optical, Morphology",

author = "L. Delaye and M. Huertas-Company and S. Mei and C. Lidman and R. Licitra and A. Newman and A. Raichoor and F. Shankar and F. Barrientos and M. Bernardi and P. Cerulo and W. Couch and R. Demarco and R. Munoz and R. Sanchez-Janssen and M. Tanaka",

year = "2015",

month = jan,

day = "1",

language = "English",

type = "Other",

}

TY - GEN

T1 - VizieR Online Data Catalog: Massive quiescent ETG in clusters (Delaye+ 2014)

AU - Delaye, L.

AU - Huertas-Company, M.

AU - Mei, S.

AU - Lidman, C.

AU - Licitra, R.

AU - Newman, A.

AU - Raichoor, A.

AU - Shankar, F.

AU - Barrientos, F.

AU - Bernardi, M.

AU - Cerulo, P.

AU - Couch, W.

AU - Demarco, R.

AU - Munoz, R.

AU - Sanchez-Janssen, R.

AU - Tanaka, M.

PY - 2015/1/1

Y1 - 2015/1/1

N2 - Our targets have been selected according to the following criteria: (1) they cover a broad redshift range 0.84All clusters have HST/ACS WFC (Wide Field Camera) images in at least two bandpasses. The ACS WFC resolution is 0.05-arcsec/pix, and its field of view is 210-arcsecx204-arcsec. The ACS/WFC PSF width is around 0.11arcsec. Our ACS/WFC images were mostly obtained in a programme designed to find Type Ia supernovae in distant galaxy clusters (Dawson et al., 2009AJ....138.1271D). See Meyers et al. (2012ApJ...750....1M) for a description of how these data were processed. Three clusters (see below): RDCS J1252-2927, XMMU J2235.3-2557 and RX J0152-1357 had been previously targeted with the ACS camera on HST in the context of the ACS Intermediate Redshift Cluster Survey (Ford 2004, HST Proposal ID 10327, ACS Imaging of a High-Redshift Cluster of Galaxies; Postman et al. 2005ApJ...623..721P; Mei et al. 2009ApJ...690...42M) and these data have been included. (1 data file).

AB - Our targets have been selected according to the following criteria: (1) they cover a broad redshift range 0.84All clusters have HST/ACS WFC (Wide Field Camera) images in at least two bandpasses. The ACS WFC resolution is 0.05-arcsec/pix, and its field of view is 210-arcsecx204-arcsec. The ACS/WFC PSF width is around 0.11arcsec. Our ACS/WFC images were mostly obtained in a programme designed to find Type Ia supernovae in distant galaxy clusters (Dawson et al., 2009AJ....138.1271D). See Meyers et al. (2012ApJ...750....1M) for a description of how these data were processed. Three clusters (see below): RDCS J1252-2927, XMMU J2235.3-2557 and RX J0152-1357 had been previously targeted with the ACS camera on HST in the context of the ACS Intermediate Redshift Cluster Survey (Ford 2004, HST Proposal ID 10327, ACS Imaging of a High-Redshift Cluster of Galaxies; Postman et al. 2005ApJ...623..721P; Mei et al. 2009ApJ...690...42M) and these data have been included. (1 data file).

KW - Clusters: galaxy

KW - Galaxies: optical

KW - Morphology

M3 - Other contribution

ER -

VizieR Online Data Catalog: Massive quiescent ETG in clusters (Delaye+ 2014)

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