J/ApJ/703/2217Lensing measurement of SDSS galaxy clusters. I. (Sheldon+, 2009)

Cross-correlation weak lensing of SDSS galaxy clusters. I. Measurements. Sheldon E.S., Johnston D.E., Scranton R., Koester B.P., McKay T.A., Oyaizu H., Cunha C., Lima M., Lin H., Frieman J.A., Wechsler R.H., Annis J., Mandelbaum R., Bahcall N.A., Fukugita M. <Astrophys. J., 703, 2217-2231 (2009)> =2009ApJ...703.2217SADC_Keywords: Gravitational lensing ; Clusters, galaxyKeywords: dark matter - galaxies: clusters: general - gravitational lensing - large-scale structure of universeAbstract: This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in Sloan Digital Sky Survey. The photometrically selected cluster sample, known as MaxBCG, includes ∼130000 objects between redshift 0.1 and 0.3, ranging in size from small groups to massive clusters. We split the clusters into bins of richness and luminosity and stack the surface density contrast to produce mean radial profiles. The mean profiles are detected over a range of scales, from the inner halo (25kpc/h) well into the surrounding large-scale structure (30Mpc/h), with a significance of 15 to 20 in each bin. The signal over this large range of scales is best interpreted in terms of the cluster-mass cross-correlation function. We pay careful attention to sources of systematic error, correcting for them where possible. The resulting signals are calibrated to the ∼10% level, with the dominant remaining uncertainty being the redshift distribution of the background sources.Description: The clusters used in this study are drawn from a superset of the recently released MaxBCG catalog of Koester et al. (2007, Cat. J/ApJ/660/239, 2007ApJ...660..221K). The galaxies used for cluster selection and shear measurement were drawn from the SDSS. The area used for this study is somewhat smaller than the SDSS data release 4 (Adelman-McCarthy et al. 2006, Cat. II/267; superseded by Cat. II/294).File Summary:

FileName Lrecl Records Explanations

ReadMe 80 . This file table1.dat 348 588 The ΔΣ data for MaxBCG clusters

See also: II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) J/ApJ/703/2232 : Weak lensing of SDSS galaxy clusters. III. (Sheldon+, 2009) J/ApJ/690/670 : The Sloan lens ACS Survey. VIII. (Treu+, 2009) J/ApJ/660/239 : MaxBCG catalog of 13823 galaxy clusters from SDSS (Koester+, 2007) J/ApJ/668/643 : Multiply imaged gravitational lens systems (Limousin+, 2007) J/ApJ/641/169 : Spectroscopy in lens fields (Momcheva+, 2006)Byte-by-byte Description of file: table1.dat

Bytes Format Units Label Explanations

1 A1 --- Type [L/N] Bin type: Number, N, or Luminosity, L 3- 14 E12.6 --- Bin Mean number or luminosity in bin (1) 16- 27 E12.6 Mpc Rad Radius in units of Mpc/h 29- 41 E13.6 Msun/pc2 DelSig Lensing measurement ΔΣ (2) 43- 54 E12.6 Msun/pc2 e_DelSig The 1σ error in Delsig (2) 56- 68 E13.6 --- Corr0 C_{0}column value of correlation matrix 70- 82 E13.6 --- Corr1 C_{1}column value of correlation matrix 84- 96 E13.6 --- Corr2 C_{2}column value of correlation matrix 98-110 E13.6 --- Corr3 C_{3}column value of correlation matrix 112-124 E13.6 --- Corr4 C_{4}column value of correlation matrix 126-138 E13.6 --- Corr5 C_{5}column value of correlation matrix 140-152 E13.6 --- Corr6 C_{6}column value of correlation matrix 154-166 E13.6 --- Corr7 C_{7}column value of correlation matrix 168-180 E13.6 --- Corr8 C_{8}column value of correlation matrix 182-194 E13.6 --- Corr9 C_{9}column value of correlation matrix 196-208 E13.6 --- Corr10 C_{10}column value of correlation matrix 210-222 E13.6 --- Corr11 C_{11}column value of correlation matrix 224-236 E13.6 --- Corr12 C_{12}column value of correlation matrix 238-250 E13.6 --- Corr13 C_{13}column value of correlation matrix 252-264 E13.6 --- Corr14 C_{14}column value of correlation matrix 266-278 E13.6 --- Corr15 C_{15}column value of correlation matrix 280-292 E13.6 --- Corr16 C_{16}column value of correlation matrix 294-306 E13.6 --- Corr17 C_{17}column value of correlation matrix 308-320 E13.6 --- Corr18 C_{18}column value of correlation matrix 322-334 E13.6 --- Corr19 C_{19}column value of correlation matrix 336-348 E13.6 --- Corr20 C_{20}column value of correlation matrix

Note (1): The units are 10^{10}L☉/h^{2}for the Luminosity bins.Note (2): In units of h*M☉/pc^{2}.

History: From electronic version of the journalReferences: Johnston et al. Paper II. 2007arXiv0709.1159J Sheldon et al. Paper III. 2009ApJ...703.2232S Cat. J/ApJ/703/2232 Rozo et al. 2010ApJ...708..645R(End)Greg Schwarz [AAS], Emmanuelle Perret [CDS] 04-Nov-2011

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