Results 41 to 50 of about 100,039 (213)
High redshift galaxy surveys [PDF]
SPIE Proceedings, 2008 Plenary talk given on 25 June at the SPIE 2008 symposium on "Astronomical Instrumentation" in Marseiile, 10 ...
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The Properties of High Redshift Galaxies [PDF]
, 2001 Summary of the Discussion Session on ``Evolution with Redshift'' at the Conference on The Evolution of Galaxies. I - Observational Clues, edited by J.M. Vilchez, G. Stasinska and E. Perez, Astrophysics and Space Science (Kluwer, The Netherlands). 10 Latex pages plus 2 encapsulated postscript figures.
Mauro Giavalisco, Daniela Calzetti
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The circumgalactic medium of high-redshift galaxies [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2014 Abstract We study the properties of the circumgalactic medium (CGM) of high-z galaxies in the metal enrichment simulations presented in Pallottini et al. At z = 4, we find that the simulated CGM gas density profiles are self-similar, once scaled with the virial radius of the parent dark matter halo.
PALLOTTINI, ANDREA +2 more
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In Pursuit of High Redshift Galaxies
, 2016 International ...
RAMPAZZO, ROBERTO +9 more
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The formation of high-redshift submillimetre galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 MNRAS Accepted; Revised version includes expanded discussion of simulated radio properties of ...
Narayanan, Desika +6 more
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The IRX–β relation of high-redshift galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT The relation between infrared excess (IRX) and UV spectral slope (βUV) is an empirical probe of dust properties of galaxies. The shape, scatter, and redshift evolution of this relation are not well understood, however, leading to uncertainties in estimating the dust content and star formation rates (SFRs) of galaxies at high ...
Philip F. Hopkins +8 more
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Globular clusters as the relics of regular star formation in ‘normal’ high-redshift galaxies [PDF]
, 2015 We present an end-to-end, two-phase model for the origin of globular clusters (GCs). In the model, populations of stellar clusters form in the high-pressure discs of high-redshift ($z>2$) galaxies (a rapid-disruption phase due to tidal perturbations from
J. Kruijssen
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Modelling galaxy clustering at high redshift [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 We discuss the theoretical interpretation of observational data concerning the clustering of galaxies at high redshifts. Building on the theoretical machinery developed by Matarrese et al. (1997), we make detailed quantitative predictions of galaxy clustering statistics for a variety of cosmological models, taking into account differences in spatial ...
MOSCARDINI, LAURO +3 more
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The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation [PDF]
, 2015 The observed high covering fractions of neutral hydrogen (HIHI) with column densities above ∼1017 cm−2 around Lyman-Break Galaxies (LBGs) and bright quasars at redshifts z ∼ 2–3 has been identified as a challenge for simulations of galaxy formation.
A. Rahmati +6 more
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Galaxies at High Redshift and Reionization
, 2007 ASP Conference Series, Vol. 395 (50 years of NRAO, eds A. Bridle, J. Condon & G. Hunt)
Richard G. McMahon +9 more
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