Author of the publication

Rest-Frame Optical Emission Lines in z~3.5 Lyman Break selected Galaxies: The Ubiquity of Unusually High OIII/Hbeta Ratios at 2 Gyr

, , , , , , , , and . (2014)cite arxiv:1401.5490Comment: 13 pages, 8 figures, 5 color, submitted to ApJ.

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. You can also use the button next to the name to display some publications already assigned to the person.

 

Other publications of authors with the same name

Lower-Luminosity Galaxies could reionize the Universe: Very Steep Faint-End Slopes to the UV Luminosity Functions at z&gt;=5-8 from the HUDF09 WFC3/IR Observations, , , , , , , , , and . (2011)cite arxiv:1105.2038 Comment: 6 pages, 4 figures, 1 table, submitted to Astrophysical Journal Letters.Discovery of Lyman Break Galaxies at z~7 from the ZFOURGE Survey, , , , , , , , , and 15 other author(s). (2013)cite arxiv:1304.4227Comment: Accepted in ApJ.Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies, , , , , , , , , and 28 other author(s). (2014)cite arxiv:1406.0183Comment: Submitted to Astrophysical Journal.Rest-Frame Optical Emission Lines in z~3.5 Lyman Break selected Galaxies: The Ubiquity of Unusually High OIII/Hbeta Ratios at 2 Gyr, , , , , , , , and . (2014)cite arxiv:1401.5490Comment: 13 pages, 8 figures, 5 color, submitted to ApJ.UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z&gt;=4 star-forming galaxies, , , , , , , , , and . (2011)cite arxiv:1109.0994 Comment: 33 pages, 24 figures, 7 tables, submitted to ApJ.The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7, , , , , , , , , and 17 other author(s). (2014)cite arxiv:1409.6791Comment: 20 pages, 11 figures, submitted to ApJ.The VLT LEGA-C Spectroscopic Survey: The Physics of Galaxies at a Lookback Time of 7 Gyr, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1603.05479Comment: Accepted for publication in ApJS - LEGA-C website: http://www.mpia.de/home/legac/index.html.Very low-luminosity galaxies in the early universe have observed sizes similar to single star cluster complexes, , , , , , and . (2017)cite arxiv:1711.02090Comment: 23 pages, 14 figures, 4 tables, submitted to the Astrophysical Journal, Figures 9 and 10 show comparisons with the sizes and luminosities of local star cluster complexes and evolved objects, respectively, Figure 11 presents our constraints on the z~6 proto-globular cluster LF.The Star Formation Rate Function for Redshift z~4-7 Galaxies: Evidence for a Uniform Build-Up of Star-Forming Galaxies During the First 3 Gyr of Cosmic Time, , , , , , and . (2012)cite arxiv:1204.3626Comment: 6 pages, 4 figures, 1 table, resubmitted to ApJ letters after responding to referee report.Most Luminous z=9-10 Galaxies: A First Determination of the Bright End of the z~9 and z~10 UV Luminosity Functions using all five CANDELS Fields, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1506.01035Comment: 22 pages, 14 figures, 6 tables, submitted to the Astrophysical Journal.