( en | de | ru )

 

Disambiguation

From post

копироватьудалитьдобавить публикацию в буфер
Measurement of rotation in two galaxies in the Epoch of Reionization from ALMA-detected CII emission

, , , , , , , , , , , и . (2017)cite arxiv:1706.04614Comment: 13 pages, 5 figues, 1 table, submitted.

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.

Pascal A Iten

Matthias Oesch

Claudia Oesch

Ottmar Oeschey

Daniel Oesch

 

Другие публикации лиц с тем же именем

Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , и 15 other автор(ы). (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.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, , , , , и . (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, , , , , , , , и . (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, , , , , , , , , и 2 other автор(ы). (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, , , , , , , , , и 6 other автор(ы). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.Rapid Reionization by the Oligarchs: The Case for Massive, UV-Bright, Star-Forming Galaxies with High Escape Fractions, , , , , и . (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!.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , и 14 other автор(ы). (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, , , , , , , , , и 24 other автор(ы). (2022)cite arxiv:2212.04026Comment: 17 pages, 8 figures, 4 tables, submitted to ApJ, comments welcome.The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization, , , , , , , , и . (2014)cite arxiv:1402.4129Comment: Re-submitted to ApJ after first positive referee report, 22 pages, 15 figures.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , и 10 other автор(ы). (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.