We present a spectroscopic and photometric analysis for eight field galaxies in the direction of the galaxy cluster LCDCS-S001. The spectra were obtained with the GMOS instrument at the Gemini South Observatory. The objects were selected in an i' -band image and the multiobject spectroscopic observations were centred at 7500 Å. For the galaxies ID 440 and ID 461, we have determined redshifts of z = 0.7464 and 0.7465, respectively. For the other six galaxies we have confirmed the previous measurements of redshift. The redshifts of the field galaxies are in the range of 0.2201 < z < 0.7784.We determined the blue and visual luminosities and they are brighter than MB =−18.64. The galaxies ID 180, ID 266 and ID 461 follow the Faber–Jackson relat...
Context.This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequ...
We exploit the gravitational potential of massive cluster lenses to probe the emission-line properti...
Context. The discovery of new galaxy clusters is important for two reasons. First, clusters are inte...
We present a spectroscopic and photometric analysis for eight field galaxies in the direction of the...
We present kinematic parameters and stellar population properties of selected galaxies in the high-r...
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
We present the results of SPT-GMOS, a spectroscopic survey with the Gemini Multi-Object Spectrograph...
Context: .This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Se...
We present results from a spectroscopic study of ~4000 galaxies in a 6.2 square degree field in the ...
Accepted by Astronomy & Astrophysics. 24 pages, 10 figures, 10 tables (figures 3, 4, 5 and tables 1,...
We have performed a deep (35.5-h exposure) spectroscopic survey of extremely red (I -K > 4) galaxies...
We present the spectrophotometric properties of a sample of 141 emission-line galaxies at redshifts ...
We exploit the gravitational potential of massive cluster lenses to probe the emission-line properti...
. Although starburst galaxies have relatively flat spectral energy distributions, their strong optic...
We present the results of SPT-GMOS, a spectroscopic survey with the Gemini Multi-Object Spectrograph...
Context.This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequ...
We exploit the gravitational potential of massive cluster lenses to probe the emission-line properti...
Context. The discovery of new galaxy clusters is important for two reasons. First, clusters are inte...
We present a spectroscopic and photometric analysis for eight field galaxies in the direction of the...
We present kinematic parameters and stellar population properties of selected galaxies in the high-r...
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
We present the results of SPT-GMOS, a spectroscopic survey with the Gemini Multi-Object Spectrograph...
Context: .This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Se...
We present results from a spectroscopic study of ~4000 galaxies in a 6.2 square degree field in the ...
Accepted by Astronomy & Astrophysics. 24 pages, 10 figures, 10 tables (figures 3, 4, 5 and tables 1,...
We have performed a deep (35.5-h exposure) spectroscopic survey of extremely red (I -K > 4) galaxies...
We present the spectrophotometric properties of a sample of 141 emission-line galaxies at redshifts ...
We exploit the gravitational potential of massive cluster lenses to probe the emission-line properti...
. Although starburst galaxies have relatively flat spectral energy distributions, their strong optic...
We present the results of SPT-GMOS, a spectroscopic survey with the Gemini Multi-Object Spectrograph...
Context.This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequ...
We exploit the gravitational potential of massive cluster lenses to probe the emission-line properti...
Context. The discovery of new galaxy clusters is important for two reasons. First, clusters are inte...