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researcher

S. Yurchenko

21 papers hereh-index 191.7k citations58 works total

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

author position
  • middle author14
  • last author6

Across the 20 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP14
  • astro-ph.SR2
  • astro-ph.IM1
  • cs.CV1
  • physics.atm-clus1
  • physics.chem-ph1
same name
  • S. Yurchenko — 156 papers, h 59
  • S. Yurchenko — 10 papers, h 30
  • S. Yurchenko — 8 papers, h 4
  • S. Yurchenko — 7 papers, h 11
  • S. Yurchenko — 1 paper, h 1

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
20102024
most citedTau-REx I: A next generation retrieval code for exoplanetary atmospheres

285 citations · 1.7k across the 21 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.EP2020★ 169 cited

Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) IV. A spectral inventory of atoms and molecules in the high-resolution transmission spectrum of WASP-121 b

H. J. Hoeijmakers, J. V. Seidel, L. Pino +22

Aims: We survey the transmission spectrum of WASP-121 b for line-absorption by metals and molecules at high spectral resolution, and elaborate on existing interpretations of the op…

astro-ph.EP2020★ 22 cited

Ions in the Thermosphere of Exoplanets: Observable Constraints Revealed by Innovative Laboratory Experiments

Jérémy Bourgalais, Nathalie Carrasco, Quentin Changeat +7

With the upcoming launch of space telescopes dedicated to the study of exoplanets, the \textit{Atmospheric Remote-Sensing Infrared Exoplanet Large-survey} (ARIEL) and the \textit{J…

astro-ph.EP2020★ 27 cited

A weak spectral signature of water vapour in the atmosphere of HD 179949 b at high spectral resolution in the L-band

Rebecca K. Webb, Matteo Brogi, Siddharth Gandhi +5

High resolution spectroscopy (R > 20,000) is currently the only known method to constrain the orbital solution and atmospheric properties of non-transiting hot Jupiters. It does so…

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