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researcher

P. Royer

13 papers hereh-index 7142 citations10 works total

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

author position
  • middle author12
  • last author1

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR8
  • astro-ph.EP3
  • astro-ph.GA2
same name
  • P. Royer — 28 papers, h 24
  • P. Royer — 23 papers, h 20
  • P. Royer — 11 papers
  • P. Royer — 8 papers, h 6
  • P. Royer — 6 papers, h 5
  • P. Royer — 4 papers, h 38

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
20122025
most citedCombined analysis of the 12.8 and 15 μm JWST/MIRI eclipse observations of TRAPPIST-1 b

53 citations · 295 across the 13 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.SR2014★ 30 cited

The wind of W Hya as seen by Herschel. II. The molecular envelope of W Hya

T. Khouri, A. de Koter, L. Decin +18

The evolution of low- and intermediate-mass stars on the asymptotic giant branch (AGB) is mainly controlled by the rate at which these stars lose mass in a stellar wind. Understand…

astro-ph.SR2014★ 51 cited

Detailed modelling of the circumstellar molecular line emission of the S-type AGB star W Aquilae

T. Danilovich, P. Bergman, K. Justtanont +5

S-type AGB stars have a C/O ratio which suggests that they are transition objects between oxygen-rich M-type stars and carbon-rich C-type stars. As such, their circumstellar compos…

astro-ph.SR2014★ 30 cited

Herschel/PACS observations of the 69 μm band of crystalline olivine around evolved stars

J. A. D. L. Blommaert, B. L. de Vries, L. B. F. M. Waters +15

We present 48 Herschel/PACS spectra of evolved stars in the wavelength range of 67-72 μm. This wavelength range covers the 69 μm band of crystalline olivine ($\text{Mg}_{2-2x}\…

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