From post

The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies

, , , , , , , , , , , , , , , и . (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed.

 

Другие публикации лиц с тем же именем

Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , и 3 other автор(ы). (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, , , и . (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.The number density and mass density of star-forming and quiescent galaxies at 0.4 &lt; z &lt; 2.2, , , , , , , , , и 2 other автор(ы). (2011)cite arxiv:1104.2595 Comment: Submitted to the Astrophysical Journal. The release of EAZY v2.0 will accompany the publication of the manuscript in the journal.The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies, , , , , , , , , и 6 other автор(ы). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , и 9 other автор(ы). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , и 20 other автор(ы). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , и 5 other автор(ы). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , и 7 other автор(ы). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.Halpha and 4000 Angstrom Break Measurements for ~3500 K-selected Galaxies at 0.5&lt;z&lt;2.0, , , , , и . (2011)cite arxiv:1103.0279 Comment: Submitted to ApJ, high-resolution version can be downloaded at https://www.cfa.harvard.edu/~mkriek/papers/.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , и . (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.