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Disambiguation of "Oesch, Pascal A."

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The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization

, , , , , , , , and . (2014)cite arxiv:1402.4129Comment: Re-submitted to ApJ after first positive referee report, 22 pages, 15 figures.

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Pascal A Iten

Matthias Oesch

Claudia Oesch

Ottmar Oeschey

Daniel Oesch

 

Other publications of authors with the same name

Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.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 10 other author(s). (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.The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization, , , , , , , , and . (2014)cite arxiv:1402.4129Comment: Re-submitted to ApJ after first positive referee report, 22 pages, 15 figures.Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at $z$$\sim$$7$$-$$8$, , , , , , , , , and 6 other author(s). (2021)cite arxiv:2105.12133Comment: 21 pages, 12 figures, 2 tables. Submitted to ApJ.The Synchrony of Production & Escape: Half the Bright Ly$\alpha$ Emitters at $z\approx2$ have Lyman Continuum Escape Fractions $\approx50\%$, , , , , , , , , and 7 other author(s). (2021)cite arxiv:2110.11961Comment: Submitted to MNRAS. Figure 4 and Table 2 show key results from the stacks. Figure 8 presents a unifying scheme for the LyC duty cycle. Our companion paper (Matthee & Naidu et al. 2021) works out implications of these results for the cosmic UV background at $z\approx2-8$. Comments warmly welcomed and greatly appreciated!.(Re)Solving Reionization with Ly\alpha: How Bright Ly\alpha Emitters account for the $z\approx2-8$ Cosmic Ionizing Background, , , , , , , , , and 5 other author(s). (2021)cite arxiv:2110.11967Comment: Submitted to MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2021. Comments welcome.Lyman-alpha Emission from a Luminous z=8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization, , , , , , , , and . (2015)cite arxiv:1507.02679Comment: ApJL Submitted; 6 pages, 4 figures, 1 table.Inferred H\alpha Flux as a Star-Formation Rate Indicator at z ~ 4-5: Implications for Dust Properties, Burstiness, and the z = 4-8 Star-Formation-Rate Functions, , , , , and . (2015)cite arxiv:1511.08808Comment: 19 pages, 11 figures, 9 tables, submitted to ApJ.The Dust Attenuation of Star-forming Galaxies at $z\sim3$ and Beyond: New Insights from ALMA Observations, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1705.01559Comment: 8 pages, 4 figures, submitted to MNRAS.The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies, , , , , , , , , and 6 other author(s). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.