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Pascal A. Oesch

Identifiers

  • name variant Pascal A. Oesch 0.60 · backfill

Papers (37)

  1. One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN astro-ph.GA · 2026 · author #5
  2. Life After the Quasar: Overmassive Black Holes and Remnant Ionised Bubbles in and Around Two z~6.6 Galaxies astro-ph.GA · 2026 · author #2
  3. How I Wonder What You Are -- JWST's Little Red Dots do not TWINKLE astro-ph.GA · 2026 · author #18
  4. PANORAMIC: The Dawn of Massive Quiescent Galaxies I. Number Density and Cosmic Variance from 1000 arcmin$^2$ NIRCam Imaging astro-ph.GA · 2026 · author #6
  5. Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$ astro-ph.GA · 2026 · author #16
  6. Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot astro-ph.GA · 2026 · author #7
  7. A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy astro-ph.GA · 2025 · author #18
  8. A GLIMPSE into the very faint-end of the H$\beta$+[OIII]$\lambda\lambda$4960,5008 luminosity function at z=7-9 behind Abell S1063 astro-ph.GA · 2025 · author #12
  9. The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10 astro-ph.GA · 2025 · author #23
  10. Before its time: a remarkably evolved protocluster core at z=7.88 astro-ph.GA · 2025 · author #2
  11. The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions astro-ph.GA · 2025 · author #14
  12. Novel $z\sim~10$ auroral line measurements extend the gradual offset of the FMR deep into the first Gyr of cosmic time astro-ph.GA · 2025 · author #6
  13. The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths astro-ph.GA · 2024 · author #22
  14. Spatial distribution of stellar mass and star formation activity at 0.2<z<1.2 across and along the Main Sequence astro-ph.GA · 2018 · author #4
  15. RELICS: High-Resolution Constraints on the Inner Mass Distribution of the z=0.83 Merging Cluster RXJ0152.7-1357 from strong lensing astro-ph.CO · 2018 · author #28
  16. Dependence of galaxy clustering on UV-luminosity and stellar mass at $z \sim 4 - 7$ astro-ph.GA · 2018 · author #3
  17. "Big Three Dragons": a z = 7.15 Lyman BreakGalaxy Detected in [OIII] 88 $\mu$m, [CII] 158 $\mu$m, and Dust Continuum with ALMA astro-ph.GA · 2018 · author #15
  18. RELICS: A Strong Lens Model for SPT-CLJ0615-5746, a z=0.972 Cluster astro-ph.GA · 2018 · author #23
  19. A Low Lyman Continuum Escape Fraction of $<10\%$ for Extreme [OIII] Emitters in an Overdensity at z$\sim3.5$ astro-ph.GA · 2018 · author #3
  20. RELICS: Strong Lensing analysis of the galaxy clusters Abell S295, Abell 697, MACS J0025.4-1222, and MACS J0159.8-0849 astro-ph.CO · 2018 · author #29
  21. RELICS: Strong-lensing analysis of the massive clusters MACS J0308.9+2645 and PLCK G171.9-40.7 astro-ph.CO · 2018 · author #28
  22. Millimeter mapping at z~1: dust-obscured bulge building and disk growth astro-ph.GA · 2018 · author #10
  23. RELICS: Strong Lens Models for Five Galaxy Clusters From the Reionization Lensing Cluster Survey astro-ph.GA · 2017 · author #19
  24. Rotation in [CII]-emitting gas in two galaxies at a redshift of 6.8 astro-ph.GA · 2017 · author #4
  25. The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies astro-ph.GA · 2017 · author #2
  26. The Dust Attenuation of Star-forming Galaxies at $z\sim3$ and Beyond: New Insights from ALMA Observations astro-ph.GA · 2017 · author #2
  27. A massive, quiescent galaxy at redshift of z=3.717 astro-ph.GA · 2017 · author #6
  28. Dark-ages reionization and galaxy-formation simulation - VI. The origins and fate of the highest known redshift galaxy astro-ph.GA · 2016 · author #7
  29. 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 astro-ph.GA · 2015 · author #6
  30. Quantifying the UV continuum slopes of galaxies to z~10 using deep Hubble and Spitzer/IRAC observations astro-ph.GA · 2015 · author #3
  31. Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1 astro-ph.GA · 2015 · author #18
  32. Lyman-alpha Emission from a Luminous z=8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization astro-ph.GA · 2015 · author #8
  33. High-precision Photometric Redshifts from Spitzer/IRAC: Extreme [3.6]-[4.5] Colors Identify Galaxies in the Redshift Range z~6.6-6.9 astro-ph.GA · 2014 · author #4
  34. The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization astro-ph.CO · 2014 · author #6
  35. A Tentative Detection of an Emission Line at 1.6 {\mu}m for the z~12 Candidate UDFj-39546284 astro-ph.CO · 2013 · author #8
  36. The X-ray Star Formation Story as Told by Lyman Break Galaxies in the 4 Ms CDF-S astro-ph.CO · 2012 · author #6
  37. Confirmation of the compactness of a z=1.91 quiescent galaxy with Hubble Space Telescope's Wide Field Camera 3 astro-ph.CO · 2010 · author #8

Mentions

  • 1301.0317 #8 · backfill · confidence 0.70 Pascal A. Oesch
  • 2601.20929 #7 · arxiv_oai · confidence 0.70 Pascal A. Oesch
  • 1210.3357 #6 · backfill · confidence 0.70 Pascal A. Oesch
  • 2508.10099 #23 · arxiv_oai · confidence 0.70 Pascal A. Oesch
  • 2408.05273 #22 · arxiv_oai · confidence 0.70 Pascal A. Oesch
  • 1004.1411 #8 · backfill · confidence 0.70 Pascal A. Oesch

Frequent Coauthors