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THE SWIFT GRB HOST GALAXY LEGACY SURVEY. II. REST-FRAME NEAR-IR LUMINOSITY DISTRIBUTION AND EVIDENCE FOR A NEAR-SOLAR METALLICITY THRESHOLD
(IOP PUBLISHING LTD, 2016)
We present rest-frame near-IR (NIR) luminosities and stellar masses for a large and uniformly selected population of gamma-ray burst (GRB) host galaxies using deep Spitzer Space Telescope imaging of 119 targets from the ...
From Peculiar Morphologies to Hubble–type Spirals: The relation between galaxy dynamics and morphology in star–forming galaxies at z ∼ 1.5
(Royal Astronomical Society, 2020)
We present an analysis of the gas dynamics of star-forming galaxies at z ∼ 1.5 using data from the KMOS Galaxy Evolution Survey. We quantify the morphology of the galaxies using HSTCANDELS imaging parametrically and ...
ALMA Observations Show Major Mergers among the Host Galaxies of Fast-growing, High-redshift, Supermassive Black Holes
(IOP Publishing, 2017)
We present new ALMA band-7 data for a sample of six luminous quasars at z similar or equal to 4.8, powered by fast-growing supermassive black holes (SMBHs) with rather uniform properties: the typical accretion rates and ...
The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
(Oxford University Press, 2015-07-03)
The evolution of the metal content of galaxies and its relations to other global properties [such as total stellar mass (M*), circular velocity, star formation rate (SFR), halo mass, etc.] provides important constraints ...
Study of intrinsic properties of HII galaxies at high redshift
(Instituto Nacional de Astrofísica, Óptica y Electrónica, 2015)
Study of intrinsic properties of HII galaxies at high redshift
(Instituto Nacional de Astrofísica, Óptica y Electrónica, 2015)
Correlations between mass, stellar kinematics, and gas metallicity in eagle galaxies
(Oxford University Press, 2020-05)
The metallicity of star-forming gas in galaxies from the eagle (Evolution and Assembly of GaLaxies and their Environments) simulations increases with stellar mass. Here, we investigate whether the scatter around this ...