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Disambiguation of "Oesch, Pascal A."

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Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST

, , , , , , , , , , , , , , , , , , , , , , , and . (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.

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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.Rapid Reionization by the Oligarchs: The Case for Massive, UV-Bright, Star-Forming Galaxies with High Escape Fractions, , , , , and . (2019)cite arxiv:1907.13130Comment: Submitted to ApJ. Figure 5 features a compilation of LyC leakers and (hopefully) motivates an $f_esc$-$\Sigma_SFR$ connection. Figures 8, 9, and Table 1 profile the öligarchs". Figure 10 compares with "democratic" reionization. Comments very welcome!.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.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.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.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , and 14 other author(s). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization, , , , , , , , , and 24 other author(s). (2022)cite arxiv:2212.04026Comment: 17 pages, 8 figures, 4 tables, submitted to ApJ, comments welcome.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.