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researcher

P. Rekhi

4 papers here

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

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • P. Rekhi — 1 paper

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
20242026
most citedBa Enrichment in Gaia MS+WD Binaries: Tracing s-Process Element Production

8 citations · 8 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2026

Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context

Imri A. Dickstein, Maayane T. Soumagnac, Eran O. Ofek +4

We report the discovery of 11 X-ray flares from 7 M dwarfs previously unknown to exhibit flaring activity, by cross-matching eROSITA observations of bright, nearby M dwarfs with th…

astro-ph.SR2026

IK Pegasi and the Double-merger Path to Type Ia Supernovae

Na'ama Hallakoun, Sahar Shahaf, Sagi Ben-Ami +3

Recent Gaia astrometry has revealed thousands of main-sequence + white-dwarf binaries (MS+WD) at separations of ~0.1-10 au, including a subset hosting unusually massive (>~0.8 Msun…

astro-ph.SR2025

Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts

Param Rekhi, Sahar Shahaf, Sagi Ben-Ami +4

The recently identified Gaia population of main-sequence--white dwarf (MS+WD) binaries at separations of ∼1 AU, often with moderate eccentricities, is not readily re…

astro-ph.SR2024★ 8 cited

Ba Enrichment in Gaia MS+WD Binaries: Tracing s-Process Element Production

Param Rekhi, Sagi Ben-Ami, Na'ama Hallakoun +3

A large population of intermediate-separation binaries, consisting of a main-sequence (MS) star and a white dwarf (WD), has recently emerged from Gaia's third data release (DR3), p…

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