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researcher

P. Gao

4 papers hereh-index 343.4k citations122 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph.SR1
same name
  • P. Gao — 4 papers, h 23
  • P. Gao — 2 papers, h 68
  • P. Gao — 2 papers, h 12
  • P. Gao — 1 paper, h 1
  • P. Gao — 1 paper, h 19
  • P. Gao — 1 paper, h 6

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20162019
most citedSulfur Hazes in Giant Exoplanet Atmospheres: Impacts on Reflected Light Spectra

72 citations · 84 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2019★ 12 cited

Retrieval of Chemical Abundances in Titan's Upper Atmosphere from Cassini UVIS Observations with Pointing Motion

Siteng Fan, Donald E. Shemansky, Cheng Li +3

Cassini/UVIS FUV observations of stellar occultations at Titan are well suited for probing its atmospheric composition and structure. However, due to instrument pointing motion, on…

astro-ph.EP2017★ 72 cited

Sulfur Hazes in Giant Exoplanet Atmospheres: Impacts on Reflected Light Spectra

Peter Gao, Mark S Marley, Kevin Zahnle +2

Recent work has shown that sulfur hazes may arise in the atmospheres of some giant exoplanets due to the photolysis of H2​S. We investigate the impact such a haze would have on…

astro-ph.EP2016

Hypotheses for near-surface exchange of methane on Mars

Renyu Hu, A. Anthony Bloom, Peter Gao +2

The Curiosity rover recently detected a background of 0.7 ppb and spikes of 7 ppb of methane on Mars. This in situ measurement reorients our understanding of the Martian environmen…

astro-ph.SR2016

Precise Near-Infrared Radial Velocities

Peter Plavchan, Peter Gao, Jonathan Gagne +31

We present the results of two 2.3 micron near-infrared radial velocity surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ~46,000)…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.