J/A+A/552/A8  454 VCC galaxies revised coordinates  (di Serego Alighieri+, 2013)

The Herschel Virgo Cluster Survey. XIII. Dust in early-type galaxies. di Serego Alighieri S., Bianchi S., Pappalardo C., Zibetti S., Auld R., Baes M., Bendo G., Corbelli E., Davies J.I., Davis T., De Looze I., Fritz J., Gavazzi G., Giovanardi C., Grossi M., Hunt L.K., Magrini L., Pierini D., Xilouris E.M. <Astron. Astrophys., 552, A8 (2013)> =2013A&A...552A...8D 2013A&A...552A...8D
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs ; Positional data Keywords: galaxies: elliptical and lenticular, cD - galaxies: clusters: general - galaxies: ISM - dust, extinction Abstract: We study the dust content of a large optical input sample of 910 early-type galaxies (ETG) in the Virgo cluster, also extending to the dwarf ETG, and examine the results in relation to those on the other cold ISM components. We have searched for far-infrared emission in all galaxies in the input sample using the 250um image of the Herschel Virgo Cluster Survey (HeViCS). This image covers a large fraction of the cluster with an area of ∼55 square degrees. For the detected ETG we measured fluxes in five bands from 100 to 500um, and estimated the dust mass and temperature with modified black-body fits. Dust is detected above the completeness limit of 25.4mJy at 250um in 46 ETG, 43 of which are in the optically complete part of the input sample. In addition, dust is present at fainter levels in another six ETG. We detect dust in the four ETG with synchrotron emission, including M 87. Description: The sample of ETG to be searched for dust within HeViCS was selected at optical wavelengths using the GOLDMine compilation (Gavazzi et al. 2003A&A...400..451G 2003A&A...400..451G, http:goldmine.mib.infn.it), which is mostly based on the Virgo Cluster Catalogue (VCC, Binggeli et al. 1985, Cat. J/AJ/90/1681, 1993A&AS...98..275B 1993A&AS...98..275B), including all morphological types from -3 to 2 (i.e. galaxies earlier than S0a-S0/Sa) and excluding galaxies with radial velocity larger than 3000km/s, since these are background galaxies; we have retained galaxies without a measured radial velocity. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 42 454 Revised coordinates for VCC galaxies (accuracy=1.2arcsec) -------------------------------------------------------------------------------- See also: J/AJ/90/1681 : The Virgo Cluster Catalog (VCC) (Binggeli+, 1985) J/MNRAS/419/3505 : The HeViCS Bright Galaxy Sample (Davies+, 2012) J/MNRAS/428/1880 : FIR properties of VCC galaxies (Auld+, 2013) J/A+A/562/A106 : Planck submillimetre sources in Virgo Cluster (Baes+, 2014) J/A+A/573/A129 : HeViCS. SPIRE point-source catalogs (Pappalardo+, 2015) J/A+A/574/A126 : HeViCS. XVIII. Star-forming dwarf galaxies (Grossi+, 2015) http://goldmine.mib.infn.it : GOLDMINE Home Page Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- VCC VCC number 6- 7 I2 h RAh Right ascension (J2000) 9- 10 I2 min RAm Right ascension (J2000) 12- 16 F5.2 s RAs Right ascension (J2000) 17 A1 --- DE- Declination sign (J2000) 18- 19 I2 deg DEd Declination (J2000) 21- 22 I2 arcmin DEm Declination (J2000) 24- 27 F4.1 arcsec DEs [0/60] Declination (J2000) 30- 34 F5.1 arcsec Off [0.3/195] Offset from original position 36- 39 F4.1 mag Pmag Photographic total apparent blue magnitude 41- 42 I2 --- TT [-1/20] Morphological T-type -------------------------------------------------------------------------------- History: * 26-Aug-2013: From electronic version of the journal * 06-Nov-2013: Corrected positions (in declination) from author References: Davies et al., Paper I 2010A&A...518L..48D 2010A&A...518L..48D Cortese et al., Paper II 2010A&A...518L..49C 2010A&A...518L..49C Clemens et al., Paper III 2010A&A...518L..50C 2010A&A...518L..50C Smith et al., Paper IV 2010A&A...518L..51S 2010A&A...518L..51S Grossi et al., Paper V 2010A&A...518L..52G 2010A&A...518L..52G Baes et al., Paper VI 2010A&A...518L..53B 2010A&A...518L..53B de Looze et al., Paper VII 2010A&A...518L..54D 2010A&A...518L..54D Davies et al., Paper VIII 2012MNRAS.419.3505D 2012MNRAS.419.3505D, Cat. J/MNRAS/419/3505 Magrini et al., Paper IX 2011A&A...535A..13M 2011A&A...535A..13M Corbelli et al., Paper X 2012A&A...542A..32C 2012A&A...542A..32C Pappalardo et al., Paper XI 2012A&A...545A..75P 2012A&A...545A..75P Auld et al., Paper XII 2013MNRAS.428.1880A 2013MNRAS.428.1880A, Cat. J/MNRAS/428/1880 De Looze et al., Paper XIV 2013MNRAS.436.1057D 2013MNRAS.436.1057D Baes et al., Paper XV 2014A&A...562A.106B 2014A&A...562A.106B, J/A+A/562/A106 Davies et al. Paper XVI 2014MNRAS.438.1922D 2014MNRAS.438.1922D Pappalardo et al., Paper XVII 2015A&A...573A.129P 2015A&A...573A.129P, J/A+A/573/A129 Grossi et al. Paper XVIII 2015A&A...574A.126G 2015A&A...574A.126G, J/A+A/574/A126
(End) Patricia Vannier [CDS] 26-Aug-2013
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