J/MNRAS/419/3505 The HeViCS Bright Galaxy Sample (Davies+, 2012)
The Herschel Virgo Cluster Survey. VIII. The Bright Galaxy Sample.
Davies J.I., Bianchi S., Cortese L., Auld R., Baes M., Bendo G.J.,
Boselli A., Ciesla L., Clemens M., Corbelli E., De Looze I.,
di Serego Alighieri S., Fritz J., Gavazzi G., Pappalardo C., Grossi M.,
Hunt L.K., Madden S., Magrini L., Pohlen M., Smith M.W.L., Verstappen J.,
Vlahakis C.
<Mon. Not. R. Astron. Soc., 419, 3505-3520 (2012)>
=2012MNRAS.419.3505D 2012MNRAS.419.3505D
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs ; Photometry, infrared
Keywords: galaxies: clusters: individual: Virgo - galaxies: general -
galaxies: ISM
Abstract:
We describe the Herschel Virgo Cluster Survey and the first data that
cover the complete survey area (four 4x4deg2 regions). We use these
data to measure and compare the global far-infrared properties of 78
optically bright galaxies that are selected at 500um and detected in
all five far-infrared bands. We show that our measurements and
calibration are broadly consistent with previous data obtained by the
IRAS, ISO, Spitzer and Planck. We use SPIRE and PACS photometry data
to produce 100-, 160-, 250-, 350- and 500-um cluster luminosity
distributions.
Description:
We have obtained ∼64deg2 of data over four fields covering a large
part of the Virgo Cluster using the SPIRE/PACS parallel scan-map mode.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 73 78 The Herschel Virgo Cluster Survey Bright Galaxy
Sample: observations and far-IR flux densities
table4.dat 74 78 The Herschel Virgo Cluster Survey Bright Galaxy
Sample: intrinsic properties
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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/552/A8 : 454 VCC galaxies revised coordinates (di Serego Alighieri+ 2013)
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: table1.dat
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Bytes Format Units Label Explanations
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1- 8 A8 --- Name Galaxy name
10- 11 I2 h RAh Right ascension (J2000) (1)
13- 14 I2 min RAm Right ascension (J2000) (1)
16- 19 F4.1 s RAs Right ascension (J2000) (1)
21 A1 --- DE- Declination sign (J2000) (1)
22- 23 I2 deg DEd Declination (J2000) (1)
25- 26 I2 arcmin DEm Declination (J2000) (1)
28- 31 F4.1 arcsec DEs Declination (J2000) (1)
33- 36 I4 km/s HV Heliocentric velocity (2)
38- 41 F4.1 Mpc Dist Distance (2)
43- 46 F4.2 Jy F500 Herschel/SPIRE far-infrared flux at 500um
48- 52 F5.2 Jy F350 Herschel/SPIRE far-infrared flux at 350um
54- 58 F5.2 Jy F250 Herschel/SPIRE far-infrared flux at 250um
60- 65 F6.2 Jy F160 Herschel/PACS far-infrared flux at 160um
67- 72 F6.2 Jy F100 Herschel/PACS far-infrared flux at 100um
73 A1 --- n_Name [*] Note on NGC 4567 and 4568 (3)
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Note (1): The coordinates are obtained from centroiding the 500um data.
Note (2): From GOLDMINE database, http://goldmine.mib.infn.it/
Note (3): NGC 4567 and 4568 are very close together and so it is difficult to
separate the measurements of one from the other.
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Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
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1- 8 A8 --- Name Galaxy name
10- 15 F6.2 mag BMAG Absolute B magnitude
17- 21 F5.2 [Msun] logM* Stellar mass (1)
23- 26 F4.2 [Msun] logMHI ?=- HI mass (3)
28- 31 F4.2 [Msun] logMd ?=- Dust mass (2)
33- 36 F4.2 [Msun] e_logMd ?=- rms uncertainty on logMd
38- 41 F4.1 K Td ?=- Dust temperature (2)
43- 45 F3.1 K e_Td ?=- rms uncertainty on Td
47- 51 F5.2 [Lsun] logL* Stellar luminosity (0.4-2.5um)
53- 57 F5.2 [Lsun] logLFIR Far-infrared luminosity (100-500um)
59- 62 F4.2 --- ?=- Mean optical depth τ
64- 68 F5.1 --- M*/MHI ?=- Stellar-to-atomic gas mass ratio (3)
70- 74 F5.1 --- MHI/Md ?=- Atomic gas-to-dust mass ratio (3)
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Note (1): The B-, V- and H-band magnitudes, used to calculate stellar mass,
are taken from the GOLDMINE data base.
Note (2): The mean fractional dust mass and temperature errors are approximately
19 and 6 per cent, respectively.
Two galaxies have no dust mass and temperatures listed because their SEDs are
not well fitted by a thermal spectrum. Stellar luminosities were calculated
using SDSS and 2MASS data. Far-infrared luminosities were calculated using
the data from this paper.
Note (3): Seven galaxies have no detected atomic hydrogen.
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History:
From electronic version of the journal
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
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, J/MNRAS/428/1880
di Serego Alighieri et al., Paper XIII 2013A&A...552A...8D 2013A&A...552A...8D, J/A+A/552/A8
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