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Disambiguation of "Oesch, P. A."

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UV Luminosity Functions at redshifts z~4 to z~10: 11000 Galaxies from HST Legacy Fields

, , , , , , , , , , , , , and . (2014)cite arxiv:1403.4295Comment: 47 pages, 29 figures, 8 tables, submitted to the Astrophysical Journal.

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Max P Oesch

Matthias Oesch

Claudia Oesch

Ottmar Oeschey

Iain P A Stitt

 

Other publications of authors with the same name

The z~6 Luminosity Function Fainter than -15 mag from the Hubble Frontier Fields: New Insights into the Impact of Magnification Uncertainties, , , , and . (2016)cite arxiv:1610.00283Comment: 27 pages, 16 figures, 5 tables, submitted to the Astrophysical Journal.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 HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1611.07038Comment: 11 pages, 6 figures, submitted to ApJ.A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z=7.730 using Keck/MOSFIRE, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1502.05399Comment: 6 pages, 4 figures, submitted to ApJL.Expanded Search for z~10 Galaxies from HUDF09, ERS, and CANDELS Data: Evidence for Accelerated Evolution at z>8?, , , , , , , , , and . (2011)cite arxiv:1105.2297 Comment: 13 pages, 12 figures, submitted to ApJ.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.A dusty compact object bridging galaxies and quasars at cosmic dawn, , , , , , , , , and 11 other author(s). (2022)cite arxiv:2204.06393Comment: 49 pages, 15 figures, 2 tables. Authors' version. Published in the 14 April issue of Nature.Normal, Dust-Obscured Galaxies in the Epoch of Reionization, , , , , , , , , and 19 other author(s). (2021)cite arxiv:2109.10378Comment: 16 pages, 7 figures, 4 tables, published in Nature.Gas Fraction and Depletion Time of Massive Star Forming Galaxies at z~3.2: No Change in Global Star Formation Process out to z>3, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1610.03656Comment: 24 pages plus 16 pages references and 5 figures, ApJ, accepted.