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researcher

S. Mathur

4 papers here

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

author position
  • middle author3
  • last author1

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

fields
  • astro-ph.SR2
  • astro-ph.EP1
  • astro-ph.IM1
ORCID 0000-0002-0129-0316
same name
  • S. Mathur — 199 papers, h 47
  • S. Mathur — 162 papers, h 64
  • S. Mathur — 134 papers, h 56
  • S. Mathur — 57 papers, h 25
  • S. Mathur — 30 papers, h 18
  • S. Mathur — 20 papers, h 12

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
20092024
most citedAsteroseismology of the solar analogs 16 Cyg A & B from Kepler observations

199 citations · 337 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.EP2020★ 51 cited

TOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star

Brett C. Addison, Duncan J. Wright, Belinda A. Nicholson +91

We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS…

astro-ph.SR2012★ 199 cited

Asteroseismology of the solar analogs 16 Cyg A & B from Kepler observations

T. S. Metcalfe, W. J. Chaplin, T. Appourchaux +34

The evolved solar-type stars 16 Cyg A & B have long been studied as solar analogs, yielding a glimpse into the future of our own Sun. The orbital period of the binary system is too…

astro-ph.SR2009★ 74 cited

The CoRoT target HD175726: an active star with weak solar-like oscillations

B. Mosser, E. Michel, T. Appourchaux +17

Context. The CoRoT short runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report observations of the star HD1757…

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