Add to ORKGnone1noNear-infrared surveys provide one of the best opportunities to investigate the cosmic evolution of galaxies and their mass assembly. We briefly review the main results obtained so far with the K20 and other recent near-IR surveys on the redshift distribution, the evolution of the luminosity function and luminosity density, the nature of old and dusty EROs, the evolution of the galaxy stellar mass function, the properties of the galaxies in the "redshift desert" and the nature of luminous starbursts at z~2.noneCimatti A.Cimatti A
We present new results on the cosmological evolution of the near-infrared (near-IR) galaxy luminosit...
The discovery of the Cosmic Infrared Background (CIB) in 1996, together with recent cosmological sur...
We explore effects of luminosity evolution in normal galaxies by means of a spectrophotometric model...
In the last decade, optical and near-infrared surveys played a crucial role to unveil and decipher t...
Infrared surveys provide essential insights on galaxy evolution. If near-IR studies suggest a mild e...
We present the galaxy rest-frame near-IR Luminosity Function (LF) and its cosmic evolution to $z\si...
Using Hubble Space Telescope and ground-based U through K- band photometry from the Great Observator...
Spectroscopic redshifts have been measured for nine K-band luminous galaxies at 1.7<z<2.3, selected ...
We present a redshift survey of 124 galaxies, from an imaging $K$-band survey complete to $K\simeq 1...
We discuss the constraints set on galaxy evolution by a variety of data from deep extragalactic surv...
AKARI's all-sky survey resolves the far-infrared emission in many thousands of nearby galaxies, prov...
Context. Studies of the generation and assembly of stellar populations in galaxies largely benefit f...
Over the last decade optical spectroscopic surveys have characterized the low redshift galaxy popula...
Thesis (Ph. D.)--University of Hawaii at Manoa, 1992.Includes bibliographical references.Microfiche....
Phenomenological models for evolution of dusty galaxies and E/S0 galaxies, respectively, are develop...
We present new results on the cosmological evolution of the near-infrared (near-IR) galaxy luminosit...
The discovery of the Cosmic Infrared Background (CIB) in 1996, together with recent cosmological sur...
We explore effects of luminosity evolution in normal galaxies by means of a spectrophotometric model...
In the last decade, optical and near-infrared surveys played a crucial role to unveil and decipher t...
Infrared surveys provide essential insights on galaxy evolution. If near-IR studies suggest a mild e...
We present the galaxy rest-frame near-IR Luminosity Function (LF) and its cosmic evolution to $z\si...
Using Hubble Space Telescope and ground-based U through K- band photometry from the Great Observator...
Spectroscopic redshifts have been measured for nine K-band luminous galaxies at 1.7<z<2.3, selected ...
We present a redshift survey of 124 galaxies, from an imaging $K$-band survey complete to $K\simeq 1...
We discuss the constraints set on galaxy evolution by a variety of data from deep extragalactic surv...
AKARI's all-sky survey resolves the far-infrared emission in many thousands of nearby galaxies, prov...
Context. Studies of the generation and assembly of stellar populations in galaxies largely benefit f...
Over the last decade optical spectroscopic surveys have characterized the low redshift galaxy popula...
Thesis (Ph. D.)--University of Hawaii at Manoa, 1992.Includes bibliographical references.Microfiche....
Phenomenological models for evolution of dusty galaxies and E/S0 galaxies, respectively, are develop...
We present new results on the cosmological evolution of the near-infrared (near-IR) galaxy luminosit...
The discovery of the Cosmic Infrared Background (CIB) in 1996, together with recent cosmological sur...
We explore effects of luminosity evolution in normal galaxies by means of a spectrophotometric model...