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4,599
The Properties of High Redshift Galaxies
, 2000
"... Abstract. In recent years, a variety of techniques at optical, near-infrared, sub-mm, and radio wavelengths have opened complementary windows on the high-redshift Universe. Here we review the current understanding of the general properties of the z�2 galaxies detected in the optical (Lyman-break gal ..."
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Abstract. In recent years, a variety of techniques at optical, near-infrared, sub-mm, and radio wavelengths have opened complementary windows on the high-redshift Universe. Here we review the current understanding of the general properties of the z�2 galaxies detected in the optical (Lyman
High redshift galaxy surveys
, 809
"... A brief overview on the current status of the census of the early universe population is given. Observational surveys of high redshift galaxies provide direct opportunities to witness the cosmic dawn and to have better understanding of how and when infant galaxies evolve into mature ones. It is a mu ..."
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A brief overview on the current status of the census of the early universe population is given. Observational surveys of high redshift galaxies provide direct opportunities to witness the cosmic dawn and to have better understanding of how and when infant galaxies evolve into mature ones. It is a
High-Redshift Galaxies: The HDF and More
, 1998
"... Abstract. We review our present knowledge of high-redshift galaxies, emphasizing particularly their physical properties and the ways in which they relate to present-day galaxies. We also present a catalogue of photometric redshifts of galaxies in the Hubble Deep Field and discuss the possibilities t ..."
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Abstract. We review our present knowledge of high-redshift galaxies, emphasizing particularly their physical properties and the ways in which they relate to present-day galaxies. We also present a catalogue of photometric redshifts of galaxies in the Hubble Deep Field and discuss the possibilities
Lyα emission in high-redshift galaxies ⋆
, 2007
"... received; accepted Context. A significant fraction of the high-redshift galaxies show strong Lyα emission lines. For redshifts z>5, most known galaxies belong to this class. However, so far not much is known about the physical structure and nature of these objects. Aims. Our aim is to analyse the ..."
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Cited by 2 (0 self)
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received; accepted Context. A significant fraction of the high-redshift galaxies show strong Lyα emission lines. For redshifts z>5, most known galaxies belong to this class. However, so far not much is known about the physical structure and nature of these objects. Aims. Our aim is to analyse
Stellar Masses of High–Redshift Galaxies
, 2002
"... Abstract. We present constraints on the stellar–mass distribution of distant galaxies. These stellar mass estimates derive from fitting population–synthesis models to the galaxies ’ observed multi-band spectrophotometry. We discuss the complex uncertainties (both statistical and systematic) that are ..."
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generally find a lack of high–redshift galaxies (z> 2) with masses comparable to those of present–day “L ∗ ” galaxies. At z < 1.8, galaxies with L ∗ –sized masses do emerge, but with a number–density below that at the present epoch. Thus, it seems massive, present–day galaxies were not fully
The nature of high redshift galaxies
- Astrophys. J. submitted
, 1998
"... With the dramatic recent advances in observational astronomy, more and more pieces of the puzzle of galaxy formation and evolution are becoming available. Some of the important puzzle pieces include the number densities, colours, sizes, ..."
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Cited by 4 (0 self)
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With the dramatic recent advances in observational astronomy, more and more pieces of the puzzle of galaxy formation and evolution are becoming available. Some of the important puzzle pieces include the number densities, colours, sizes,
Results 1 - 10
of
4,599
