0000000000765130

AUTHOR

Gabriel B. Brammer

showing 3 related works from this author

The GLASS-JWST Early Release Science Program. III. Strong lensing model of Abell 2744 and its infalling regions

2023

We present a new high-precision, JWST-based, strong lensing model for the galaxy cluster Abell 2744 at $z=0.3072$. By combining the deep, high-resolution JWST imaging from the GLASS-JWST and UNCOVER programs and a Director's Discretionary Time program, with newly obtained VLT/MUSE data, we identify 32 multiple images from 11 background sources lensed by two external sub-clusters at distances of ~160" from the main cluster. The new MUSE observations enable the first spectroscopic confirmation of a multiple image system in the external clumps. Moreover, the re-analysis of the spectro-photometric archival and JWST data yields 27 additional multiple images in the main cluster. The new lens mode…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics of Galaxies (astro-ph.GA)FOS: Physical sciencesAstrophysics - Astrophysics of GalaxiesAstrophysics - Cosmology and Nongalactic Astrophysics
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The Evolution of the Rest-frame V-band Luminosity Function from z=4: A Constant Faint-end Slope over the Last 12 Gyr of Cosmic History

2012

We present the rest-frame V-band luminosity function (LF) of galaxies at 0.4<z<4.0, measured from a near-infrared selected sample constructed from the NMBS, the FIRES, the FIREWORKS, and the ultra-deep NICMOS and WFC3 observations in the HDFN, HUDF, and GOODS-CDFS, all having high-quality optical to mid-infrared data. This unique sample combines data from surveys with a large range of depths and areas in a self-consistent way, allowing us to (1) minimize the uncertainties due to cosmic variance; and (2) simultaneously constrain the bright and faint ends with unprecedented accuracy over the targeted redshift range, probing the LF down to 0.1 L* at z~3.9. We find that (1) the faint end is fai…

PhysicsCOSMIC cancer databaseCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCosmic varianceAstrophysics::Cosmology and Extragalactic AstrophysicsRedshiftGalaxyLuminositySpace and Planetary ScienceMagnitude (astronomy)HaloAstrophysics::Galaxy AstrophysicsLuminosity function (astronomy)Astrophysics - Cosmology and Nongalactic Astrophysics
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Spectroscopic Confirmation of an Ultramassive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals

2014

et al.

PhysicsActive galactic nucleusStellar massStar formationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of GalaxiesRedshiftGalaxyStarsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Elliptical galaxySpectral energy distributionAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysics
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