J/A+A/578/A79       Galaxy clusters in SDSS Stripe 82       (Durret+, 2015)

Galaxy clusters in the SDSS Stripe 82 based on galaxy photometric redshifts. Durret F., Adami C., Bertin E., Hao J., Marquez I., Martinet N., Maurogordato S., Sauvaget T., Scepi N., Takey A., Ulmer M.P. <Astron. Astrophys. 578, A79 (2015)> =2015A&A...578A..79D 2015A&A...578A..79D
ADC_Keywords: Clusters, galaxy ; Redshifts Keywords: surveys - galaxies: clusters: general - cosmology: large-scale structure of Universe Abstract: The discovery of new galaxy clusters is important for two reasons. First, clusters are interesting per se, since their detailed analysis allows us to understand how galaxies form and evolve in various environments and second, they play an important part in cosmology because their number as a function of redshift gives constraints on cosmological parameters. We have searched for galaxy clusters in the Stripe 82 region of the Sloan Digital Sky Survey, and analysed various properties of the cluster galaxies. Based on a recent photometric redshift (hereafter photo-z) galaxy catalogue, we built a cluster catalogue by applying the Adami & MAzure Cluster FInder (AMACFI). Extensive tests were made to fine-tune the AMACFI parameters and make the cluster detection as reliable as possible. The same method was applied to the Millennium simulation to estimate our detection efficiency and the approximate masses of the detected clusters. Considering all the cluster galaxies (i.e. within a 1Mpc radius of the cluster to which they belong and with a photo-z differing by less than ±0.05 from that of the cluster), we stacked clusters in various redshift bins to derive colour-magnitude diagrams and galaxy luminosity functions (GLFs). For each galaxy brighter than Mr←19.0, we computed the disk and spheroid components by applying SExtractor, and by stacking clusters we determined how the disk-to-spheroid flux ratio varies with cluster redshift and mass. Description: Table A1 (in the Appendix) is a catalogue of clusters of galaxies detected in the Stripe 82 region of the Sloan Digital Sky Survey, in order of increasing right ascension. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 37 3663 Catalogue of clusters of galaxies detected in the Stripe 82 region of SDSS -------------------------------------------------------------------------------- See also: J/MNRAS/413/3059 : 4098 galaxy clusters in SDSS Stripe 82 (Geach+, 2011) J/other/RAA/11.309 : Nearby early-type galaxies in Stripe 82 (Jiang+, 2011) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Seq [1/3663] Cluster number 6- 15 F10.6 deg RAdeg Right ascension (J2000.0) 18- 26 F9.6 deg DEdeg Declination (J2000.0) 28- 31 F4.2 --- z [0.15/0.7] Cluster photometric redshift 33 I1 --- Nsig [3/9] Cluster detection level (in σ's) 35- 37 I3 --- Ngal [11/102] Number of galaxies within a radius of 1Mpc of the cluster centre and with a photometric redshift differing by less than 0.04(1+z) from the cluster redshift -------------------------------------------------------------------------------- Acknowledgements: Florence Durret, durret(at)iap.fr
(End) Patricia Vannier [CDS] 23-Mar-2015
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