J/ApJS/199/22 UV to far-IR photometry of galaxies (Hernandez-Fernandez+, 2012)
UV to Far-IR catalog of a galaxy sample in nearby clusters: spectral energy distributions and environmental trends. Hernandez-Fernandez J.D., Iglesias-Paramo J., Vilchez J.M. <Astrophys. J. Suppl. Ser., 199, 22 (2012)> =2012ApJS..199...22H
ADC_Keywords: Clusters, galaxy ; Photometry, ultraviolet ; Photometry, SDSS ; Photometry, infrared ; Galaxies, photometry ; Surveys Keywords: catalogs - galaxies: clusters: general - galaxies: dwarf - galaxies: evolution - galaxies: interactions - ultraviolet: galaxies Abstract: In this paper, we present a sample of cluster galaxies devoted to study the environmental influence on the star formation activity. This sample of galaxies inhabits in clusters showing a rich variety in their characteristics and have been observed by the SDSS-DR6 down to MB~-18, and by the Galaxy Evolution Explorer AIS throughout sky regions corresponding to several megaparsecs. We assign the broadband and emission-line fluxes from ultraviolet to far-infrared to each galaxy performing an accurate spectral energy distribution for spectral fitting analysis. The clusters follow the general X-ray luminosity versus velocity dispersion trend of LX∝σ4.4c. Description: The cluster sample is observed in a sky area which is delimited by the intersection of observed sky areas of SDSS (DR6, Adelman-McCarthy et al. 2008, Cat. II/282) and Galaxy Evolution Explorer (GALEX; Martin et al. 2005ApJ...619L...1M) surveys. Both surveys are incomplete (at the moment of sample definition, 2008 March) and have smaller observed sky areas than the other ended surveys, Two Micron All Sky Survey (2MASS, Cat. II/246) and Infrared Astronomical Satellite (IRAS; Neugebauer et al. 1984ApJ...278L...1N; Cat. II/125 and II/156). In order to sample a broad range of environments, we select galaxy clusters observed by these surveys up to regions several virial radius beyond the virial region. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 86 16 Main properties of the cluster sample table3.dat 409 7822 Spectrophotometric catalog of cluster galaxies
See also: II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) VII/177 : Redshifts and Velocity Dispersions for Abell Clusters (Struble+ 1991) II/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989) II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) J/ApJ/694/992 : SED of cluster radio galaxies (Lin+, 2009) J/A+A/402/37 : UV to radio SED of galaxies in Virgo cluster (Boselli+, 2003) J/ApJ/554/L129 : X-ray luminosity-velocity dispersion relation (Mahdavi+, 2001) J/ApJ/534/114 : RASSCALS: X-ray and optical study (Mahdavi+, 2000) J/ApJ/496/39 : Properties of poor groups of galaxies. I. (Zabludoff+ 1998) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 20 A20 --- Cluster NED identification 21 A1 --- f_Cluster [*] Note on WBL 514 (1) 23- 29 F7.3 deg RAdeg NED right ascension in decimal degrees (J2000) 31- 38 F8.5 deg DEdeg NED declination in decimal degrees (J2000) 40- 45 F6.4 --- z Cluster average redshift 47- 51 F5.1 km/s Sig Cluster velocity dispersion 53- 56 F4.2 Mpc r200 radius 200 58- 60 I3 --- n200 no. of galaxies inside virial region with SDSS redshift 62- 65 I4 --- ntot no. of galaxies associated with each cluster selected by criteria exposed in Section 3.1 67- 71 F5.3 deg theta half-size of sky square region (θ_tot_) (2) 73- 74 A2 --- l_logLX [≤ ] Limit flag on logLX 75- 79 F5.2 Lsun logLX ? Bolometric X-ray luminosity (3) 81- 86 A6 --- Cl Cluster abbreviation as in table3 (added by CDS)
Note (1): * = The historical criterion is not applied. In the case of WBL 514, we have selected WBL 514 instead of MKW07 because this object is split into two clusters by a late reference (Struble & Rood 1991, Cat. VII/177). Note (2): Half-size of sky square region retrieved for each cluster, computed as suming the Local Universe approximation cz=HD, the small-angle approximation DP=Dxθ[rad], and a projected radius RP=7.1Mpc Note (3): Bolometric X-ray luminosity from Mahdavi & Geller (2001, Cat. J/ApJ/554/L129) except for WBL 213 (Mahdavi et al. 2000, Cat. J/ApJ/534/114).
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 4 I4 --- ID [0/7821] Identification number (1) 6- 23 A18 --- ObjID SDSS-DR6 Imaging Catalog identifier (2) 25- 42 A18 --- sObjID SDSS-DR6 Main Galaxy Sample identifier (SpecObjID) 44- 53 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 55- 63 F9.6 deg DEdeg Declination in decimal degrees (J2000) 65- 71 F7.5 --- z SDSS-DR6 spectroscopic redshift 73- 79 F7.5 --- e_z Uncertainty in z 81- 89 F9.6 mag FUVmag ?=-1 GALEX/FUV band AB magnitude 91- 98 F8.6 mag e_FUVmag ?=1 Uncertainty in FUVmag 100-101 I2 --- l_FUVmag [-1/1] Detection identifier for FUVmag (3) 103-111 F9.6 mag NUVmag ?=-1 GALEX/NUV band AB magnitude 113-120 F8.6 mag e_NUVmag ?=1 Uncertainty in NUVmag 122-123 I2 --- l_NUVmag [-1/1] Detection identifier for NUVmag (3) 125-133 F9.6 mag u'mag SDSS u' band AB magnitude (DR6) 135-142 F8.6 mag e_u'mag Uncertainty in umag 144 I1 --- l_u'mag  Detection identifier for umag (3) 146-154 F9.6 mag g'mag SDSS g' band AB magnitude (DR6) 156-163 F8.6 mag e_g'mag Uncertainty in gmag 165 I1 --- l_g'mag  Detection identifier for gmag (3) 167-175 F9.6 mag r'mag SDSS r' band AB magnitude (DR6) 177-186 F10.6 mag e_r'mag Uncertainty in rmag 188 I1 --- l_r'mag  Detection identifier for rmag (3) 190-198 F9.6 mag i'mag SDSS i' band AB magnitude (DR6) 200-209 F10.6 mag e_i'mag Uncertainty in imag 211 I1 --- l_i'mag  Detection identifier for imag (3) 213-221 F9.6 mag z'mag SDSS z' band AB magnitude (DR6) 223-230 F8.6 mag e_z'mag Uncertainty in zmag 232 I1 --- l_z'mag  Detection identifier for zmag (3) 234-242 F9.6 mag Jmag 2MASS J band AB magnitude 244-251 F8.6 mag e_Jmag Uncertainty in Jmag 253 I1 --- l_Jmag [0/1] Detection identifier for Jmag (3) 255-263 F9.6 mag Hmag 2MASS H band AB magnitude 265-272 F8.6 mag e_Hmag Uncertainty in Hmag 274 I1 --- l_Hmag [0/1] Detection identifier for Hmag (3) 276-284 F9.6 mag Ksmag 2MASS Ks band AB magnitude 286-293 F8.6 mag e_Ksmag Uncertainty in Ksmag 295 I1 --- l_Ksmag [0/1] Detection identifier for Ksmag (3) 297-305 F9.6 mag  IRAS 12 micron band AB magnitude 307-314 F8.6 mag e_ Uncertainty in  316 I1 --- l_ [0/1] Detection identifier for  (3) 318-326 F9.6 mag  IRAS 25 micron band AB magnitude 328-335 F8.6 mag e_ Uncertainty in  337 I1 --- l_ [0/1] Detection identifier for  (3) 339-347 F9.6 mag  IRAS 60 micron band AB magnitude 349-356 F8.6 mag e_ Uncertainty in  358 I1 --- l_ [0/1] Detection identifier for  (3) 360-367 F8.6 mag  IRAS 100 micron band AB magnitude 369-376 F8.6 mag e_ Uncertainty in  378 I1 --- l_ [0/1] Detection identifier for  (3) 380-389 F10.6 Msun/yr SFR Hα derived star formation rate 391-399 F9.6 Msun/yr e_SFR Uncertainty in SFR 401-402 I2 --- l_SFR [-2/1] Detection identifier for SFR (3) 404-409 A6 --- Cl Parent cluster identifier (4)
Note (1): Associated with the position of the galaxy inside the cluster galaxy sample. Note (2): Last digit numbers in these objID are erroneous. This column is ignored in VizieR database. Note (3): Flag as follows: 1 = Source detected on this band; 0 = Source undetected on this band (upper limit in flux); -1 = Source not observed on this band (flux is blank) -2 = Lower limit in flux. Note (4): Abbreviations: A = ABELL; B2 = B2 1621+38:[MLO2002] CLUSTER; N = NED; U = UGCl; W = WBL.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 23-Mar-2012
|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|