0000000000878455

AUTHOR

Katherine E. Whitaker

showing 2 related works from this author

Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST

2022

The first few 100 Myr at z > 10 mark the last major uncharted epoch in the history of the universe, where only a single galaxy (GN-z11 at z ≈ 11) is currently spectroscopically confirmed. Here we present a search for luminous z > 10 galaxies with JWST/NIRCam photometry spanning ≈1–5 μm and covering 49 arcmin2 from the public JWST Early Release Science programs (CEERS and GLASS). Our most secure candidates are two MUV ≈ −21 systems: GLASS-z12 and GLASS-z10. These galaxies display abrupt ≳1.8 mag breaks in their spectral energy distributions (SEDs), consistent with complete absorption of flux bluewards of Lyα that is redshifted to =+z12.40.3 0.1and=+z10.40.5 0.4. Lower redshift interlopers su…

DECOMPOSITIONII.594Early universeFOS: Physical sciences2291435PROPAGATION734595310Galaxies and CosmologyUNCERTAINTIESGalaxy evolutionGalaxy formationTO 8REIONIZATIONMASSIVE GALAXIESAstronomy and AstrophysicsBRIGHT ENDAstrophysics - Astrophysics of GalaxiesEVOLUTIONSTELLARSpace and Planetary Science5101 Astronomical SciencesAstrophysics of Galaxies (astro-ph.GA)High-redshift galaxiesJames Webb Space Telescope51 Physical Sciences
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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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