We measure redshifts for 67 galaxies in the field of six cluster candidates from the ESO Imaging Survey (EIS). The cluster candidates are selected in the EIS patches C and D among those with estimated mean redshifts 0.5 95% confidence level). Two of these systems have mean redshift in agreement with the redshift estimate given by the matched filter algorithm (\u394z = \ub1 0.1). The other two systems have significantly lower redshifts. We discuss the implications of our results in the context of our ongoing research projects aimed at defining high-redshift optically-selected cluster samples. Based on observations collected at the European Southern Observatory (La Silla, Chile), Proposal ID: 62.O-060
Galaxy clusters can be used as a sensitive probe for cosmology. A large cluster catalog that extends...
International audienceWe present spectroscopic observations of galaxies in 4 clusters at z = 0.7-0.8...
Astronomy and Astrophysics, 435, pp. 781-798, http://dx.doi.org./10.1051/0004-6361:20041850Internati...
Using EFOSC2 at the 3.6m ESO telescope, we obtained redshifts for 68 galaxies in the field of six cl...
We measure redshifts for 67 galaxies in the field of six cluster candidates from the ESO Imaging Sur...
International audienceContext: This paper reports the results obtained on the photometric redshifts ...
We have carried out an investigation of the properties of low redshift EIS clusters using both spec...
We use publicly available V-band imaging data from the wide-angle surveys conducted by the ESO Imagi...
6 pagesThis paper presents preliminary results of a spectroscopic survey being conducted at the VLT ...
The ESO Distant Cluster Survey (EDisCS) is a photometric and spectroscopic study of the galaxy clust...
International audienceWe present the ESO Distant Cluster Survey (EDisCS), a survey of distant galaxy...
31 pages, 23 figures, accepted for publication in A&AInternational audienceAims. We present spectros...
Astronomy and Astrophysics, 490, pp. 945-963, http://dx.doi.org./10.1051/0004-6361:20066830Internati...
© ESO 2015. Context. The discovery of new galaxy clusters is important for two reasons. First, clust...
Galaxy clusters can be used as a sensitive probe for cosmology. A large cluster catalog that extends...
International audienceWe present spectroscopic observations of galaxies in 4 clusters at z = 0.7-0.8...
Astronomy and Astrophysics, 435, pp. 781-798, http://dx.doi.org./10.1051/0004-6361:20041850Internati...
Using EFOSC2 at the 3.6m ESO telescope, we obtained redshifts for 68 galaxies in the field of six cl...
We measure redshifts for 67 galaxies in the field of six cluster candidates from the ESO Imaging Sur...
International audienceContext: This paper reports the results obtained on the photometric redshifts ...
We have carried out an investigation of the properties of low redshift EIS clusters using both spec...
We use publicly available V-band imaging data from the wide-angle surveys conducted by the ESO Imagi...
6 pagesThis paper presents preliminary results of a spectroscopic survey being conducted at the VLT ...
The ESO Distant Cluster Survey (EDisCS) is a photometric and spectroscopic study of the galaxy clust...
International audienceWe present the ESO Distant Cluster Survey (EDisCS), a survey of distant galaxy...
31 pages, 23 figures, accepted for publication in A&AInternational audienceAims. We present spectros...
Astronomy and Astrophysics, 490, pp. 945-963, http://dx.doi.org./10.1051/0004-6361:20066830Internati...
© ESO 2015. Context. The discovery of new galaxy clusters is important for two reasons. First, clust...
Galaxy clusters can be used as a sensitive probe for cosmology. A large cluster catalog that extends...
International audienceWe present spectroscopic observations of galaxies in 4 clusters at z = 0.7-0.8...
Astronomy and Astrophysics, 435, pp. 781-798, http://dx.doi.org./10.1051/0004-6361:20041850Internati...