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researcher

R. Kotak

185 papers hereh-index 6318.4k citations334 works total

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

author position
  • first author8
  • middle author128
  • last author4

Across the 140 of 185 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR59
  • astro-ph.HE52
  • astro-ph34
  • astro-ph.CO16
  • astro-ph.IM16
  • astro-ph.GA6
same name
  • R. Kotak — 9 papers, h 2
  • R. Kotak — 2 papers, h 3
  • R. Kotak — 1 paper
  • R. Kotak — 1 paper, h 0

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
19972026
most citedThe Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

2.7k citations · 17.7k across the 182 of their papers we have counts for

collaborators
Showing 2002Show all

3 papers · 1 filter

astro-ph2002★ 17 cited

A new look at the pulsating DB white dwarf GD 358:Line-of-sight velocity measurements and constraints on model atmospheres

Rubina Kotak, Marten H. van Kerkwijk, J. C. Clemens +1

We report on our findings of the bright, pulsating, helium atmosphere white dwarf GD 358, based on time-resolved optical spectrophotometry. We identify 5 real pulsation modes and a…

astro-ph2002★ 8 cited

Pulsating or not? A search for hidden pulsations below the red edge of the ZZ instability strip

Rubina Kotak, Marten H. van Kerkwijk, J. Christopher Clemens +1

The location of the red edge of the ZZ Ceti instability strip is defined observationally as being the lowest temperature for which a white dwarf with a H-rich atmosphere (DA) is kn…

astro-ph2002★ 24 cited

Time-resolved optical spectroscopy of the pulsating DA white dwarf HS 0507+0434B: New constraints on mode identification and pulsation properties

Rubina Kotak, Marten H. van Kerkwijk, J. Christopher Clemens

We present a detailed analysis of time-resolved optical spectra of the ZZ Ceti white dwarf, HS 0507+0434B. Using the wavelength dependence of observed mode amplitudes, we deduce th…

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