Mathematics – Logic
Scientific paper
Apr 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35099081a&link_type=abstract
VizieR On-line Data Catalog: J/A+A/509/A81. Originally published in: 2010A&A...509A..81A
Mathematics
Logic
Surveys, Clusters: Galaxy, Redshifts
Scientific paper
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.
(1 data file).
Adami Chris
Arnouts Stephane
Benoist Christophe
Blaizot Jérémy
Cappi Alberto
No associations
LandOfFree
Candidate clusters detected in six CFHTLS fields (Adami+, 2010) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Candidate clusters detected in six CFHTLS fields (Adami+, 2010), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Candidate clusters detected in six CFHTLS fields (Adami+, 2010) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1191552