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J/MNRAS/458/582  Coma clusters and filaments galaxies FIR survey (Fuller+, 2016)

H-ATLAS: the far-infrared properties of galaxies in and around the Coma cluster. Fuller C., Davies J.I., Smith M.W.L., Valiante E., Eales S., Bourne N., Dunne L., Dye S., Furlanetto C., Ibar E., Ivison R., Maddox S., Sansom A., Michalowski M.J., Davis T. <Mon. Not. R. Astron. Soc., 458, 582-602 (2016)> =2016MNRAS.458..582F (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Photometry, infrared ; Photometry, millimetric/submm Keywords: galaxies: clusters: individual: Coma - galaxies: ISM - galaxies: photometry - infrared: galaxies Abstract: We describe a far-infrared survey of the Coma cluster and the galaxy filament it resides within. Our survey covers an area of ∼150 deg2 observed by Herschel H-ATLAS (Herschel Astrophysical Terahertz Large Area Survey) in five bands at 100, 160, 250, 350 and 500µm. The SDSS spectroscopic survey (mr≤17.8) is used to define an area (within the virial radius) and redshift selected (4268<v<9700km/s) sample of 744 Coma cluster galaxies - the Coma Cluster Catalogue. For comparison, we also define a sample of 951 galaxies in the connecting filament - the Coma Filament Catalogue. The optical positions and parameters are used to define appropriate apertures to measure each galaxy's far-infrared emission. We have detected 99 of 744 (13 per cent) and 422 of 951 (44 per cent) of the cluster and filament galaxies in the SPIRE 250um band. We consider the relative detection rates of galaxies of different morphological types finding that it is only the S0/Sa population that shows clear differences between the cluster and filament. We find no differences between the dust masses and temperatures of cluster and filament galaxies with the exception of early-type galaxy dust temperatures, which are significantly hotter in the cluster than in the filament (X-ray heating?). From a chemical evolution model, we find no evidence for different evolutionary processes (gas loss or infall) between galaxies in the cluster and filament. Description: We have undertaken a Herschel FIR survey of the Coma cluster and the galaxy filament it resides within. Our survey covers an area of ∼150 deg2 observed in five bands at 100, 160, 250, 350 and 500um. We have used the SDSS spectroscopic survey to define an area and redshift selected sample of 744 Coma cluster galaxies - the CCC. For comparison, we also define in a similar way a sample of 951 galaxies in the connecting filament - the CFC. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 74 774 Herschel far infrared measurements of Coma Cluster Catalogue galaxies tableb1.dat 74 951 Herschel far infrared measurements of Coma Filament Catalogue galaxies
See also: VII/42 : GMP catalogue: galaxies in the Coma cluster (Godwin+ 1983) J/ApJS/97/77 : Catalog of Coma Cluster Galaxies (Doi+ 1995) J/A+AS/122/409 : Photometric catalogue of Coma (Lobo+, 1997) J/A+A/384/383 : Halpha galaxies in A1367 and Coma (Iglesias-Paramo+, 2002) J/A+A/419/47 : XMM X-ray fluxes in Coma cluster (Finoguenov+, 2004) J/ApJS/169/225 : Photometry of galaxies in Coma cluster (Eisenhardt+, 2007) J/AJ/137/4436 : Coma cluster VLA survey (Miller+, 2009) J/ApJS/190/43 : Deep GALEX observations of the Coma cluster (Hammer+, 2010) J/A+A/553/A91 : Halpha3 survey of Virgo and Coma galaxies (Fossati+, 2013) J/MNRAS/445/2385 : HST/ACS Coma Cluster Survey. X. (den Brok+, 2014) J/A+A/576/A16 : Halpha3 V. Coma cluster (Gavazzi+, 2015) Byte-by-byte Description of file: tablea1.dat tableb1.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Object Object name (1) 8- 9 I2 h RAh Right ascension (J2000) 11- 12 I2 min RAm Right ascension (J2000) 14- 15 I2 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- 25 I2 arcsec DEs Declination (J2000) 26 A1 --- l_S500 3σ upper limit flag on S500 27- 29 I3 mJy S500 Herschel/SPIRE 500um flux density 31- 33 I3 mJy e_S500 ? 1σ rms uncertainty on S500 34 A1 --- l_S350 3σ upper limit flag on S350 35- 38 I4 mJy S350 Herschel/SPIRE 350um flux density 40- 42 I3 mJy e_S350 ? 1σ rms uncertainty on S350 43 A1 --- l_S250 3σ upper limit flag on S250 44- 47 I4 mJy S250 Herschel/SPIRE 250um flux density 49- 52 I4 mJy e_S250 ? 1σ rms uncertainty on S250 53 A1 --- l_S160 3σ upper limit flag on S160 54- 58 I5 mJy S160 Herschel/PACS 160um flux density 60- 63 I4 mJy e_S160 ? 1σ rms uncertainty on S160 64 A1 --- l_S100 3σ upper limit flag on S100 65- 69 I5 mJy S100 Herschel/PACS 100um flux density 71- 74 I4 mJy e_S100 ? 1σ rms uncertainty on S100
Note (1): Sources names CCCNNN for Coma Cluster Catalogue galaxies (table A1) and CFCNNN for Coma Filament Catalogue galaxies (table B1).
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 26-May-2017
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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