J/MNRAS/413/3059    4098 galaxy clusters in SDSS Stripe 82   (Geach+, 2011)

4098 galaxy clusters to z∼0.6 in the Sloan Digital Sky Survey equatorial Stripe 82. Geach J.E., Murphy D.N.A., Bower R.G. <Mon. Not. R. Astron. Soc., 413, 3059-3067 (2011)> =2011MNRAS.413.3059G 2011MNRAS.413.3059G
ADC_Keywords: Clusters, galaxy ; Redshifts ; QSOs Keywords: catalogues - galaxies: clusters: general - large-scale structure of Universe Abstract: We present a catalogue of 4098 photometrically selected galaxy clusters with a median redshift =0.32 in the 270deg2 "Stripe 82" region of the Sloan Digital Sky Survey (SDSS), covering the celestial equator in the Southern Galactic Cap (-50°<RA<59°, |DE|≤1.25). Owing to the multi-epoch SDSS coverage of this region, the ugriz photometry is ∼2mag deeper than single scans within the main SDSS footprint. We exploit this to detect clusters of galaxies using an algorithm that searches for statistically significant overdensities of galaxies in a Voronoi tessellation of the projected sky. Description: We have chosen to distribute the full catalogue in Hierarchical Data Format (HDF, version 5). This format provides a natural way for us to release both the 'top level' cluster properties (coordinate, redshift, etc.) and a wide range of other information, including various richness classifications, and information for each of the constituent galaxies. However, for simple access, we also provide a "supplementary QSO sightline catalogue". File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file clusters.dat 186 4098 Stripe 82 cluster catalogue, top level qsos.dat 88 18295 Supplementary QSO sightline catalogue clusters.hdf5 512 529861 Full catalogue in Hierarchical Data Format (HDF, version 5) -------------------------------------------------------------------------------- Byte-by-byte Description of file: clusters.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Cluster Cluster sequential number 6- 23 E18.15 deg RAdeg Cluster right ascension (J2000) 25- 43 E19.15 deg DEdeg Declination (J2000) 45- 62 E18.15 deg RA1deg BCG right ascension (J2000) (1) 64- 82 E19.15 deg DE1deg BCG declination (J2000) (1) 84- 86 I3 --- Ngal Number of galaxies assigned to cluster 88-105 E18.15 --- z Cluster redshift 107-126 A20 --- n_z Code describing composite average of galaxy redshifts (unexplained) 128-145 E18.15 rad r80 Angular radius containing 80% of the members 147-164 E18.15 --- C Concentration index (C=r80/r20) 166 I1 --- R [1/4]?=- Richness class 168-186 E19.15 --- Agc ?=- Richness estimator (amplitude of the angular correlation function) -------------------------------------------------------------------------------- Note (1): BCG = Brightest Cluster Galaxy -------------------------------------------------------------------------------- Byte-by-byte Description of file: qsos.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- QSO QSO identification number 8- 17 F10.8 deg Sep Separation from cluster center, in degrees 19- 28 F10.8 Mpc R Separation from cluster center, in Mpc 30- 34 F5.3 --- zQSO QSO redshift 36- 43 F8.4 deg RAdeg QSO right ascension (J2000) 45- 52 F8.5 deg DEdeg QSO declination (J2000) 54- 57 F4.1 mag Vmag QSO V magnitude 59- 66 F8.6 --- zCl Cluster redshift 68- 79 F12.8 deg RAcdeg Cluster right ascension degrees (J2000) 81- 88 F8.5 deg DEcdeg Cluster declination (J2000) -------------------------------------------------------------------------------- History: Copied at http://www.physics.mcgill.ca/~jimgeach/stripe82
(End) Patricia Vannier [CDS] 15-Dec-2011
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