Add to ORKGTo circumvent the spatial effects of resolution on galaxy classification, the images of 233 objects of known redshift in the Hubble Deep Field (HDF) and its flanking fields that have redshifts in the range 0.20 0.5 are seen to be more chaotic than those of their nearer counterparts. Furthermore, the spiral structure in distant early-type spirals appears to be less well developed than it is in nearby early galaxies
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
The morphological properties of high-redshift galaxies are investigated using a sample of 507 object...
We report 328 redshifts, b_J magnitudes and b_J--r_F colors of galaxies measured in a redshift surve...
To circumvent the spatial effects of resolution on galaxy classification, the images of 233 objects ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS an...
We have carried out a study of the luminosity function (LF) of galaxies in the region of the Hubble ...
A redshift survey has been carried out in the region of the Hubble Deep Field North using the Low Re...
Detection and photometry of sources in the U_n, G, ℛ, and K_s bands in a 9 × 9 arcmin^2 region of th...
A spectroscopic survey of over 400 field galaxies has been completed in three fields for which we ha...
A clustering analysis is performed on two samples of ~600 faint galaxies each, in two widely separat...
This paper presents the results of a photometric redshift study of galaxies in the Hubble Deep Field...
I am currently analyzing the emission line spectra of the 600 galaxies from the sample of Cohen et a...
Photometric redshifts have been determined for the galaxies in the Hubble Deep Field. The resulting ...
International audienceWe tested the performance of photometric redshifts for galaxies in the Hubble ...
We combine the photometric redshift data of Fernandez-Soto et al. (1997) with the morphological data...
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
The morphological properties of high-redshift galaxies are investigated using a sample of 507 object...
We report 328 redshifts, b_J magnitudes and b_J--r_F colors of galaxies measured in a redshift surve...
To circumvent the spatial effects of resolution on galaxy classification, the images of 233 objects ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS an...
We have carried out a study of the luminosity function (LF) of galaxies in the region of the Hubble ...
A redshift survey has been carried out in the region of the Hubble Deep Field North using the Low Re...
Detection and photometry of sources in the U_n, G, ℛ, and K_s bands in a 9 × 9 arcmin^2 region of th...
A spectroscopic survey of over 400 field galaxies has been completed in three fields for which we ha...
A clustering analysis is performed on two samples of ~600 faint galaxies each, in two widely separat...
This paper presents the results of a photometric redshift study of galaxies in the Hubble Deep Field...
I am currently analyzing the emission line spectra of the 600 galaxies from the sample of Cohen et a...
Photometric redshifts have been determined for the galaxies in the Hubble Deep Field. The resulting ...
International audienceWe tested the performance of photometric redshifts for galaxies in the Hubble ...
We combine the photometric redshift data of Fernandez-Soto et al. (1997) with the morphological data...
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
The morphological properties of high-redshift galaxies are investigated using a sample of 507 object...
We report 328 redshifts, b_J magnitudes and b_J--r_F colors of galaxies measured in a redshift surve...