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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

Uwe Brammer

Joachim Brammer

 

Other publications of authors with the same name

Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim2$, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1912.01619Comment: 30 pages, 10 figures, accepted in ApJ.Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z=3.35: A Detailed Look at an Early Progenitor of Local Most Massive Ellipticals, , , , , , , , , and . (2014)cite arxiv:1406.0002Comment: 15 pages, 7 figures. Submitted to ApJ. Comments welcome.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.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.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.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.