2010A&A...509A..81A


Query : 2010A&A...509A..81A

2010A&A...509A..81A - Astronomy and Astrophysics, volume 509, A81-81 (2010/1-1)

Galaxy structure searches by photometric redshifts in the CFHTLS.

ADAMI C., DURRET F., BENOIST C., COUPON J., MAZURE A., MENEUX B., ILBERT O., BLAIZOT J., ARNOUTS S., CAPPI A., GARILLI B., GUENNOU L., LEBRUN V., LEFEVRE O., MAUROGORDATO S., McCRACKEN H.J., MELLIER Y., SLEZAK E., TRESSE L. and ULMER M.P.

Abstract (from CDS):

Counting clusters is one of the methods to constrain cosmological parameters, but has been limited up to now both by the redshift range and by the relatively small sizes of the homogeneously surveyed areas. In order to enlarge publicly available optical cluster catalogs, in particular at high redshift, we have performed a systematic search for clusters of galaxies in the Canada France Hawaii Telescope Legacy Survey (CFHTLS). We considered the deep 2, 3 and 4 CFHTLS Deep fields (each 1x1deg2), as well as the wide 1, 3 and 4 CFHTLS Wide fields. We used the Le Phare photometric redshifts for the galaxies detected in these fields with magnitude limits of i'=25 and 23 for the Deep and Wide fields respectively. We then constructed galaxy density maps in photometric redshift bins of 0.1 based on an adaptive kernel technique and detected structures with SExtractor at various detection levels. In order to assess the validity of our cluster detection rates, we applied a similar procedure to galaxies in Millennium simulations. We measured the correlation function of our cluster candidates. We analyzed large scale properties and substructures, including filaments, by applying a minimal spanning tree algorithm both to our data and to the Millennium simulations. We detected 1200 candidate clusters with various masses (minimal masses between 1.0x1013 and 5.5x1013 and mean masses between 1.3x1014 and 12.6x1014M) in the CFHTLS Deep and Wide fields, thus notably increasing the number of known high redshift cluster candidates. We found a correlation function for these objects comparable to that obtained for high redshift cluster surveys. We also show that the CFHTLS deep survey is able to trace the large scale structure of the universe up to z≥1. Our detections are fully consistent with those made in various CFHTLS analyses with other methods. We now need accurate mass determinations of these structures to constrain cosmological parameters. We have shown that a search for galaxy clusters based on density maps built from galaxy catalogs in photometric redshift bins is successful and gives results comparable to or better than those obtained with other methods. By applying this technique to the CFHTLS survey we have increased the number of known optical high redshift cluster candidates by a large factor, an important step towards using cluster counts to measure cosmological parameters.

Abstract Copyright:

Journal keyword(s): surveys - galaxies: clusters: general - large-scale structure of Universe

VizieR on-line data: <Available at CDS (J/A+A/509/A81): tablea.dat>

Nomenclature: Tables A.1-A.3: [ADB2010] DN-NN N=60+64+47. Tables A.4-A.6: [ADB2010] WN-NNN N=755+175+99.

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 ACO 85 ClG 00 41 37.8 -09 20 33           ~ 844 0
2 [LCG2009] SL2S Group J02140-0532 GrG 02 14 08.0316 -05 35 32.621           ~ 7 0
3 3XMM J222144.0-005306 GrG 22 21 43.74240 -00 53 02.5549           ~ 6 0

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2022.08.18-03:33:41

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