Results 41 to 50 of about 147,516 (226)
KILOPARSEC-SCALE DUST DISKS IN HIGH-REDSHIFT LUMINOUS SUBMILLIMETER GALAXIES [PDF]
Astrophysical Journal, 2016 We present high-resolution (0.″16) 870 μm Atacama Large Millimeter/submillimeter Array (ALMA) imaging of 16 luminous ( ) submillimeter galaxies (SMGs) from the ALESS survey of the Extended Chandra Deep Field South.
J. Hodge +23 more
semanticscholar +1 more source
On the Number of Galaxies at High Redshift [PDF]
Galaxies, 2015 The number of galaxies at a given flux as a function of the redshift, z, is derived when the z-distance relation is non-standard. In order to compare different models, the same formalism is also applied to the standard cosmology. The observed luminosity function for galaxies of the zCOSMOS catalog at different redshifts is modeled by a new luminosity ...
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THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: MOLECULAR GAS RESERVOIRS IN HIGH-REDSHIFT GALAXIES [PDF]
, 2016 We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (ASPECS) that targets an ∼1 arcmin2 region in the Hubble Ultra Deep Field (UDF), a blind survey of CO emission (tracing molecular gas) in the 3 and 1 mm ...
R. Decarli +31 more
semanticscholar +1 more source
The fate of high-redshift massive compact galaxies [PDF]
, 2016 Massive high-redshift quiescent compact galaxies (nicknamed red nuggets) have been traditionally connected to present-day elliptical galaxies, often overlooking the relationships that they may have with other galaxy types.
I. G. D. L. Rosa +6 more
semanticscholar +1 more source
High-redshift galaxy populations and their descendants [PDF]
Monthly Notices of the Royal Astronomical Society, 2009 16 pages, 17 figures, submitted to ...
Guo, Q., White, S.
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Why do high-redshift galaxies show diverse gas-phase metallicity gradients? [PDF]
, 2016 Recent spatially resolved observations of galaxies at z ∼ 0.6–3 reveal that high-redshift galaxies show complex kinematics and a broad distribution of gas-phase metallicity gradients.
Xiangcheng Ma +10 more
semanticscholar +1 more source
Morphological Classification of High Redshift Galaxies [PDF]
Astrophysics and Space Science, 2001 4 pages, 3 encapsulated figures. Proceedings of the Euroconference "The Evolution of Galaxies.I- Observational clues." held in Granada (Spain), 23-27 May, 2000.
Pignatelli, E., Fasano, G.
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RECONCILING THE STELLAR AND NEBULAR SPECTRA OF HIGH-REDSHIFT GALAXIES [PDF]
, 2016 We present a combined analysis of rest-frame far-UV (FUV; 1000–2000 Å) and rest-frame optical (3600–7000 Å) composite spectra formed from very deep Keck/LRIS and Keck/MOSFIRE observations of a sample of 30 star-forming galaxies with , selected to be ...
C. Steidel +5 more
semanticscholar +1 more source
Galaxy halo occupation at high redshift [PDF]
Monthly Notices of the Royal Astronomical Society, 2002 13 pages, 5 figures, Submitted to MNRAS, minor ...
Bullock, James S. +2 more
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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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