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Disambiguation of "Brammer, Gabriel B."

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Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1

, , , , , , , , , , , , , , , , , , , and . (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.

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Friedrich Brammer

Friederike Brammer

Gregor Brammer

Joachim Brammer

Carl Brammer

 

Other publications of authors with the same name

The Grism Lens-Amplified Survey from Space (GLASS). V. Extent and spatial distribution of star formation in z~0.5 cluster galaxies, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1511.00686Comment: 18 pages, 15 figures, accepted for publication in ApJ.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2, , , , , , , , , and 14 other author(s). (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , and 5 other author(s). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , and 10 other author(s). (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.A substantial population of massive quiescent galaxies at z~4 from ZFOURGE, , , , , , , , , and 14 other author(s). (2013)cite arxiv:1312.4952Comment: 8 pages, 4 figures, 1 table, re-submitted to ApjL after second referee report.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , and . (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.Halpha and 4000 Angstrom Break Measurements for ~3500 K-selected Galaxies at 0.5&lt;z&lt;2.0, , , , , and . (2011)cite arxiv:1103.0279 Comment: Submitted to ApJ, high-resolution version can be downloaded at https://www.cfa.harvard.edu/~mkriek/papers/.Overturning the Case for Gravitational Powering in the Prototypical Cooling Lyman-alpha Nebula, , , , and . (2015)cite arxiv:1501.05312Comment: Accepted to ApJ; 21 pages in emulateapj format; 12 figures, 1 table.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.