Imaging at 1.25 and 2.20pm has been obtained of the field containing the galaxy (R.D1) found at redshift z = 5.34 by Dey, et al. (1998). This galaxy has been detected at 1.25pnl, while the lower redshift (,z = 4.02) galaxy also found in the same field by Dey, et al. was detected at both 1.2 and 2.2pn1. The colors of both of these galaxies are suggestive of significant reddening of a young stellar population. Combined with photometric observations of other high redshift systems, this shows that dust is an important component of young galaxies even at redshifts in excess of 5. The extinction corrected, monochromatic luminosity of R.D1 at 1500 ~ is 1-2 magnitudes greater than a typical star forming galaxy at z w3
International audienceUsing NOEMA and ALMA 3mm line scans, we measure spectroscopic redshifts of six...
We present new constraints on the evolution of the early-type galaxy color-magnitude relation (CMR) ...
We present optical and near-infrared photometry for a sample of 96 dusty, far-infraredluminous galax...
Imaging at 1.25 and 2.20 μm has been obtained of the field containing the galaxy (RD1) found at reds...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z ...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z ...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z=...
International audienceCandidates for the modest galaxies that formed most of the stars in the early ...
We use very deep near-infrared photometry of the Hubble Deep Field-South taken with ISAAC on th...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z=...
The acquisition of deep near-IR imaging with Wide Field Camera 3 on the Hubble Space Telescope has p...
Although dust emission at cosmological distances has only been detected a little more than a decade ...
First we present new infrared counts of field galaxies from more than 20 square arcminutes to a limi...
International audienceWe report Atacama Large Millimetre Array (ALMA) observations of four high-reds...
International audienceUsing NOEMA and ALMA 3mm line scans, we measure spectroscopic redshifts of six...
We present new constraints on the evolution of the early-type galaxy color-magnitude relation (CMR) ...
We present optical and near-infrared photometry for a sample of 96 dusty, far-infraredluminous galax...
Imaging at 1.25 and 2.20 μm has been obtained of the field containing the galaxy (RD1) found at reds...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z ...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z ...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z=...
International audienceCandidates for the modest galaxies that formed most of the stars in the early ...
We use very deep near-infrared photometry of the Hubble Deep Field-South taken with ISAAC on th...
Near-infrared imaging and spectroscopy have been obtained of the gravitationally lensed galaxy at z=...
The acquisition of deep near-IR imaging with Wide Field Camera 3 on the Hubble Space Telescope has p...
Although dust emission at cosmological distances has only been detected a little more than a decade ...
First we present new infrared counts of field galaxies from more than 20 square arcminutes to a limi...
International audienceWe report Atacama Large Millimetre Array (ALMA) observations of four high-reds...
International audienceUsing NOEMA and ALMA 3mm line scans, we measure spectroscopic redshifts of six...
We present new constraints on the evolution of the early-type galaxy color-magnitude relation (CMR) ...
We present optical and near-infrared photometry for a sample of 96 dusty, far-infraredluminous galax...