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researcher

K. Shin

85 papers hereh-index 293.4k citations95 works total

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

author position
  • first author4
  • middle author60
  • last author3

Across the 67 of 85 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE69
  • astro-ph.IM6
  • astro-ph.CO4
  • astro-ph.GA3
  • astro-ph.SR3
same name
  • K. Shin — 38 papers, h 16
  • K. Shin — 27 papers, h 102
  • K. Shin — 12 papers, h 8
  • K. Shin — 7 papers, h 8
  • K. Shin — 7 papers, h 6
  • K. Shin — 6 papers, h 22

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
20192026
most citedA bright millisecond-duration radio burst from a Galactic magnetar

745 citations · 3.7k across the 76 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

The long period radio transient ASKAP J1448-68 is a cataclysmic variable

Geoffrey Mo, Akash Anumarlapudi, Iris de Ruiter +8

Wide-field time-domain radio surveys have recently unveiled a new class of Galactic radio emitter: long period radio transients (LPTs). Despite the rapid pace of discovery, their o…

astro-ph.SR2026

Discovery of over a thousand variable stars in Terzan 5 and Liller 1 with JWST

Kevin B. Burdge, Ilaria Caiazzo, Malina M. Desai +18

The Bulge Fossil Fragments Terzan 5 and Liller 1 host some of the densest stellar environments in the Galaxy, yet their variable star populations have remained largely unexplored d…

astro-ph.SR2026

Stars stably accreting from substellar objects

Aaron Householder, Kaitlyn Shin, Kevin B. Burdge +11

Substellar objects such as brown dwarfs and planets are generally expected to remain detached from their main-sequence host stars unless orbital decay or stellar expansion brings t…

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