Searching for filaments and large-scale structure around DAFT/FADA clusters

Bibcode
2016A&A...588A..69D
DOI
10.1051/0004-6361/201527655
Durret, F.; Márquez, I.; Acebrón, A.; Adami, C.; Cabrera-Lavers, A.; Capelato, H.; Martinet, N.; Sarron, F.; Ulmer, M. P.
Bibliographical reference

Astronomy and Astrophysics, Volume 588, id.A69, 19 pp.

Advertised on:
4
2016
Journal
Astronomy and Astrophysics
Number of authors
9
IAC number of authors
1
Citations
17
Refereed citations
16
Description
Context. Clusters of galaxies are located at the intersection of cosmic filaments and are still accreting galaxies and groups along these preferential directions. However, because of their relatively low contrast on the sky, filaments are difficult to detect (unless a large amount of spectroscopic data are available), and unambiguous detections have been limited until now to relatively low redshifts (z< ~ 0.3). Aims: This project is aimed at searching for extensions and filaments around clusters, traced by galaxies selected to be at the cluster redshift based on the red sequence. In the 0.4
Type
Refereed
Galaxies

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