26 citations · 26 across the 1 of their papers we have counts for
6 papers
Molecular gas in CLASH brightest cluster galaxies at
G. Castignani, M. Pandey-Pommier, S. L. Hamer +4
Brightest cluster galaxies (BCGs) are excellent laboratories to study galaxy evolution in dense Mpc-scale environments. We have observed in CO(1-0), CO(2-1), CO(3-2), or CO(4-3), w…
Molecular gas and star formation activity in LIRGs in clusters at intermediate redshifts
G. Castignani, P. Jablonka, F. Combes +10
We investigate the role of dense Mpc-scale environments in processing molecular gas of cluster galaxies as they fall into the cluster cores. We consider luminous infrared…
Environmental processing in cluster core galaxies at z=1.7
G. Castignani, F. Combes, P. Salomé
Today, the brightest cluster galaxies (BCGs) are passive and very massive galaxies at the center of their clusters, and they still accrete mass through swallowing companions and ga…
Molecular gas in distant brightest cluster galaxies
G. Castignani, F. Combes, P. Salomé +1
The stellar mass assembly of brightest cluster galaxies (BCGs) is still debated. We have observed in CO with the IRAM-30m two star forming BCGs belonging to SpARCS clusters, 3C 244…
Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection
Euclid Collaboration, R. Adam, M. Vannier +56
Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clust…
Molecular gas in radio galaxies in dense Mpc-scale environments at
G. Castignani, F. Combes, P. Salomé +4
We investigate the role of dense Mpc-scale environment in processing molecular gas in distant Low luminosity radio galaxies (LLRGs) in galaxy (proto-)clusters. We have selected wit…