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UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxies

R. Bouwens, G. Illingworth, P. Oesch, M. Franx, I. Labbe, M. Trenti, P. van Dokkum, C. Carollo, V. Gonzalez, and D. Magee. (2011)cite arxiv:1109.0994 Comment: 33 pages, 24 figures, 7 tables, submitted to ApJ.

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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 UncertaintiesR. Bouwens, P. Oesch, G. Illingworth, R. Ellis, and M. Stefanon. (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 complexesR. Bouwens, P. van Dokkum, G. Illingworth, P. Oesch, M. Maseda, B. Ribeiro, and D. Lam. (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 TimeR. Smit, R. Bouwens, M. Franx, G. Illingworth, I. Labbé, P. Oesch, and P. van Dokkum. (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 FieldsR. Bouwens, P. Oesch, I. Labbe, G. Illingworth, G. Fazio, D. Coe, B. Holwerda, R. Smit, M. Stefanon, P. van Dokkum and 7 other author(s). (2015)cite arxiv:1506.01035Comment: 22 pages, 14 figures, 6 tables, submitted to the Astrophysical Journal.Normal, Dust-Obscured Galaxies in the Epoch of ReionizationY. Fudamoto, P. Oesch, S. Schouws, M. Stefanon, R. Smit, R. Bouwens, R. Bowler, R. Endsley, V. Gonzalez, H. Inami and 19 other author(s). (2021)cite arxiv:2109.10378Comment: 16 pages, 7 figures, 4 tables, published in Nature.A dusty compact object bridging galaxies and quasars at cosmic dawnS. Fujimoto, G. Brammer, D. Watson, G. Magdis, V. Kokorev, T. Greve, S. Toft, F. Walter, R. Valiante, M. Ginolfi 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.Expanded Search for z~10 Galaxies from HUDF09, ERS, and CANDELS Data: Evidence for Accelerated Evolution at z>8?P. Oesch, R. Bouwens, G. Illingworth, I. Labbe, M. Trenti, V. Gonzalez, C. Carollo, M. Franx, P. van Dokkum, and D. Magee. (2011)cite arxiv:1105.2297 Comment: 13 pages, 12 figures, submitted to ApJ.Cosmic Reionization after Planck: The Derived Growth of the Ionizing Background now matches the Growth of the Galaxy UV Luminosity DensityR. Bouwens, G. Illingworth, P. Oesch, J. Caruana, B. Holwerda, R. Smit, and S. Wilkins. (2015)cite arxiv:1503.08228Comment: 16 pages, 10 figures, 3 tables, submitted to the Astrophysical Journal, Figure 6 shows the main result of the paper, Table 1 includes a compilation of the many key constraints on the ionisation state of the universe at z>6.Gas Fraction and Depletion Time of Massive Star Forming Galaxies at z~3.2: No Change in Global Star Formation Process out to z>3E. Schinnerer, B. Groves, M. Sargent, A. Karim, P. Oesch, B. Magnelli, O. LeFevre, L. Tasca, F. Civano, P. Cassata and 1 other author(s). (2016)cite arxiv:1610.03656Comment: 24 pages plus 16 pages references and 5 figures, ApJ, accepted.Newly Discovered Bright z~9-10 Galaxies and Improved Constraints on Their Prevalence Using the Full CANDELS AreaR. Bouwens, M. Stefanon, P. Oesch, G. Illingworth, T. Nanayakkara, G. Roberts-Borsani, I. Labbe', and R. Smit. (2019)cite arxiv:1905.05202Comment: 21 pages, 12 figures, 6 tables, to be resubmitted to the Astrophysical Journal after helpful referee report.

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Disambiguation of "Oesch, P. A."