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researcher

S. Majewski

24 papers hereh-index 91.8k citations31 works total

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

author position
  • first author1
  • middle author16
  • last author1

Across the 18 of 24 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA12
  • astro-ph4
  • astro-ph.IM4
  • astro-ph.SR3
  • astro-ph.EP1
same name
  • S. Majewski — 660 papers
  • S. Majewski — 343 papers, h 90
  • S. Majewski — 42 papers, h 35
  • S. Majewski — 20 papers, h 42
  • S. Majewski — 9 papers, h 9
  • S. Majewski — 6 papers

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
19942026
most citedThe Apache Point Observatory Galactic Evolution Experiment (APOGEE)

1.8k citations · 2.8k across the 22 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2025

Characterizing TESS-Identified Quadruple and Higher Order Eclipsing Binaries: I. Speckle Imaging with DSSI and HRCam

Steven R. Majewski, James W. Davidson, Robert F. Wilson +9

NASA's TESS mission has unveiled a plethora of eclipsing binaries (EBs), among them hundreds of triples and higher order, hierarchical systems. These complex targets require follow…

astro-ph.SR2025

The TESS Ten Thousand Catalog: 10,001 uniformly-vetted and -validated Eclipsing Binary Stars detected in Full-Frame Image data by machine learning and analyzed by citizen scientists

Veselin B. Kostov, Brian P. Powell, Aline U. Fornear +36

The Transiting Exoplanet Survey Satellite (TESS) has surveyed nearly the entire sky in Full-Frame Image mode with a time resolution of 200 seconds to 30 minutes and a temporal base…

astro-ph.SR2015★ 14 cited

Characterizing the Rigidly Rotating Magnetosphere Stars HD 345439 and HD 23478

J. P. Wisniewski, S. D. Chojnowski, J. R. A. Davenport +8

The SDSS III APOGEE survey recently identified two new σ Ori E type candidates, HD 345439 and HD 23478, which are a rare subset of rapidly rotating massive stars whose large (kGa…

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