Add to ORKGWe present a new automated cluster search algorithm, stressing its advantages relatively to others available in the literature. Applying it to the photometric data of the ESO Imaging Survey (EIS, Renzini & da Costa 1997) allowed us to produce, with a high degree of confidence, a new catalogue of cluster candidates up to z approximately equal to 1.1
International audienceWe present the ESO Distant Cluster Survey (EDisCS), a survey of distant galaxy...
We present spectroscopic confirmation of a z = 0.99 galaxy cluster discovered using data from the Wi...
Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test...
We present a new algorithm to search for distant clusters of galaxies on catalogues deriving from im...
High redshift galaxy clusters have traditionally been a fruitful place to study galaxy evolution. I ...
We measure redshifts for 67 galaxies in the field of six cluster candidates from the ESO Imaging Sur...
The evolution of galaxy clusters and their members above z >= 1 is largely unclear at present due to...
© ESO 2015. Context. The discovery of new galaxy clusters is important for two reasons. First, clust...
We describe a new method (Poisson probability method, PPM) to search for high-redshift galaxy cluste...
Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test...
Astronomy and Astrophysics, 435, pp. 781-798, http://dx.doi.org./10.1051/0004-6361:20041850Internati...
We present a new cluster-finding algorithm based on a combination of the Voronoi Tessellation and Fr...
Galaxy clusters can be used as a sensitive probe for cosmology. A large cluster catalog that extends...
We present and analyze the optical and X-ray catalogs of moderate-redshift cluster candidates from t...
Context. Cosmological parameters can be constrained by counting clusters of galaxies as a function o...
International audienceWe present the ESO Distant Cluster Survey (EDisCS), a survey of distant galaxy...
We present spectroscopic confirmation of a z = 0.99 galaxy cluster discovered using data from the Wi...
Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test...
We present a new algorithm to search for distant clusters of galaxies on catalogues deriving from im...
High redshift galaxy clusters have traditionally been a fruitful place to study galaxy evolution. I ...
We measure redshifts for 67 galaxies in the field of six cluster candidates from the ESO Imaging Sur...
The evolution of galaxy clusters and their members above z >= 1 is largely unclear at present due to...
© ESO 2015. Context. The discovery of new galaxy clusters is important for two reasons. First, clust...
We describe a new method (Poisson probability method, PPM) to search for high-redshift galaxy cluste...
Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test...
Astronomy and Astrophysics, 435, pp. 781-798, http://dx.doi.org./10.1051/0004-6361:20041850Internati...
We present a new cluster-finding algorithm based on a combination of the Voronoi Tessellation and Fr...
Galaxy clusters can be used as a sensitive probe for cosmology. A large cluster catalog that extends...
We present and analyze the optical and X-ray catalogs of moderate-redshift cluster candidates from t...
Context. Cosmological parameters can be constrained by counting clusters of galaxies as a function o...
International audienceWe present the ESO Distant Cluster Survey (EDisCS), a survey of distant galaxy...
We present spectroscopic confirmation of a z = 0.99 galaxy cluster discovered using data from the Wi...
Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test...