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Disambiguierung von "Whitaker, Katherine E."

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Ages of massive galaxies at $0.5 < z < 2.0$ from 3D-HST rest-frame optical spectroscopy

, , , , , , , , , , , , und . (2016)cite arxiv:1603.02689Comment: 13 pages, 15 figures, accepted for publication in ApJ.

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Richard Whitaker

Dagmar Whitaker

Katherine Hester

Katherine Mayes

Katherine Kämpchen

 

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Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , und 3 andere Autor(en). (2013)cite arxiv:1305.1943Comment: 6 pages, 4 figures, resubmitted to the Astrophysical Journal Letters after minor revisions.The Star-formation Mass Sequence out to z=2.5, , , und . (2012)cite arxiv:1205.0547Comment: Submitted to the Astrophysical Journal Letters, 6 pages, 5 figures. NMBS IR+UV SFRs are now available at http://www.astro.yale.edu/nmbs/Data_Products.html.Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7, , , , , , und . (2014)cite arxiv:1405.0490Comment: 14 pages, 8 figures. Re-submitted to ApJ.Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z=1.522, , , , , , und . (2019)cite arxiv:1902.09564Comment: 8 pages, 5 figures, resubmitted to ApJL following referee report.Ages of massive galaxies at $0.5 < z < 2.0$ from 3D-HST rest-frame optical spectroscopy, , , , , , , , , und 3 andere Autor(en). (2016)cite arxiv:1603.02689Comment: 13 pages, 15 figures, accepted for publication in ApJ.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , und 15 andere Autor(en). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.First spectroscopic observations of the galaxies that reionized the Universe, , , , , , , , , und 23 andere Autor(en). (2023)cite arxiv:2308.08540Comment: 29 pages, 7 figures, 2 tables.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , und 7 andere Autor(en). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , und . (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , und 10 andere Autor(en). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.