J/MNRAS/418/1409    Compact groups of galaxies in SDSS DR7       (Mendel+, 2011)

Compact groups in theory and practice. IV. The connection to large-scale structure. Mendel J.T., Ellison S.L., Simard L., Patton D.R., McConnachie A.W. <Mon. Not. R. Astron. Soc., 418, 1409-1422 (2011)> =2011MNRAS.418.1409M 2011MNRAS.418.1409M
ADC_Keywords: Surveys ; Clusters, galaxy ; Morphology ; Redshifts Keywords: galaxies: evolution - galaxies: groups: general - galaxies: interactions - galaxies: photometry - galaxies: structure Abstract: We investigate the properties of photometrically selected compact groups (CGs) in the Sloan Digital Sky Survey. In this paper, the fourth in a series, we focus on understanding the characteristics of our observed CG sample with particular attention paid to quantifying and removing contamination from projected foreground or background galaxies. Based on a simple comparison of pairwise redshift likelihoods, we find that approximately half of CGs in the parent sample contain one or more projected (interloping) members; our final clean sample contains 4566 galaxies in 1086 CGs. Description: In Paper III (Cat. J/MNRAS/395/255) we describe the photometric selection of CGs from the SDSS Data Release 6 (Adelman-McCarthy et al., 2008, Cat. II/282/), which included imaging of the entire SDSS-II Legacy Survey area. Since that paper, SDSS Data Release 7 (DR7; Abazajian et al., 2009ApJS..182..543A 2009ApJS..182..543A) has provided an additional ∼1200deg2 of spectroscopic data, completing spectroscopic observations of the SDSS-II Legacy Survey footprint. In what follows we use galaxy catalogues drawn from SDSS DR7 and, where available, supplement the CG samples in Paper III with updated spectroscopic information. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 60 1086 Properties of CGs initially presented in Paper III tablea2.dat 85 4566 Individual member galaxies of the groups in tablea1 -------------------------------------------------------------------------------- See also: J/MNRAS/395/255 : Compact groups of galaxies in SDSS DR6 (McConnachie+, 2009) J/A+A/514/A102 : SDSS DR7 groups of galaxies (Tago+, 2010) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- --- [SDSSCGA] 8- 12 I05 --- GrID [3/2296] Group ID in catalog "A" (G1) 14- 15 I2 h RAh Right ascension (J2000) of geometric group centre 17- 18 I2 min RAm Right ascension (J2000) of geometric group centre 20- 24 F5.2 s RAs Right ascension (J2000) of geometric group centre 26 A1 --- DE- Declination sign (J2000) of geometric group centre 27- 28 I2 deg DEd Declination (J2000) of geometric group centre 30- 31 I2 arcmin DEm Declination (J2000) of geometric group centre 33- 37 F5.2 arcsec DEs Declination (J2000) of geometric group centre 39- 43 F5.3 --- zest Estimated redshift of the group, determined from the joint probability of group member redshifts 45- 50 F6.4 --- e_zest rms uncertainty on zest, determined from the 1σ width of the joint redshift probability 51- 52 I2 --- NM09 Number of group members in the original Paper III photometric group catalogue (i.e. prior to cleaning) 54 I1 --- Nclean Number of remaining group members after application of the cleaning algorithm described in Section 2.2.1. 56- 60 F5.2 Mpc RT10 ? Distance to the nearest rich group in the Tago et al. (2010, Cat. J/A+A/514/A102) catalogue, estimated following the description in Section 3.1 (in h70-1Mpc) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- --- [SDSSCGA] 8- 12 I05 --- GrID [3/2296] Group ID (G1) 13 A1 --- --- [.] 14 I1 --- Gal Galaxy ID in group (G1) 16- 33 A18 --- objID Galaxy object ID within the SDSS 35- 36 I2 h RAh Right ascension (J2000) of the galaxy 38- 39 I2 min RAm Right ascension (J2000) of the galaxy 41- 45 F5.2 s RAs Right ascension (J2000 of the galaxy 47 A1 --- DE- Declination sign (J2000) of the galaxy 48- 49 I2 deg DEd Declination (J2000) of the galaxy 51- 52 I2 arcmin DEm Declination (J2000) of the galaxy 54- 58 F5.2 arcsec DEs Declination (J2000) of the galaxy 60- 65 F6.3 --- zsp ? Spectroscopic redshift 67- 72 F6.4 --- e_zsp ? rms uncertainty on zsp 74- 78 F5.3 --- zph Photometric redshift 80- 85 F6.4 --- e_zph rms uncertainty on zph -------------------------------------------------------------------------------- Global Notes: Note (G1): designation in PaperIII (McConnachie et al. 2009, J/MNRAS/395/255). Catalogue "A" is defined as the flux-limited sample with extinction- corrected r-band Petrosian magnitudes in the range 14.5-18.0mag. Groups are assigned integer numbers, and galaxies in the group are assigned a decimal number which integer part represents the group ID. History: From electronic version of the journal References: McConnachie et al., Paper I 2008MNRAS.387.1281M 2008MNRAS.387.1281M Brasseur et al., Paper II 2009MNRAS.392.1141B 2009MNRAS.392.1141B McConnachie et al., Paper III 2009MNRAS.395..255M 2009MNRAS.395..255M, Cat. J/MNRAS/395/255
(End) Patricia Vannier [CDS] 23-Jul-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