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S. Kiyota

63 papers hereh-index 221.9k citations294 works total

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

author position
  • middle author40
  • last author4

Across the 44 of 63 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR38
  • astro-ph14
  • astro-ph.HE10
  • astro-ph.CO1
same name
  • S. Kiyota — 8 papers, h 5
  • S. Kiyota — 2 papers
  • S. Kiyota — 1 paper, h 1
  • S. Kiyota — 1 paper, h 5

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
20012023
most citedASASSN-15lh: A Highly Super-Luminous Supernova

203 citations · 2.2k across the 63 of their papers we have counts for

collaborators
Showing 2003Show all

4 papers · 1 filter

astro-ph2003★ 12 cited

A New SU UMa-Type Dwarf Nova, QW Serpentis (= TmzV46)

D. Nogami, M. Uemura, R. Ishioka +11

We report on the results of the QW Ser campaign which has been continued from 2000 to 2003 by the VSNET collaboration team. Four long outbursts and many short ones were caught duri…

astro-ph2003★ 6 cited

On the Possibility of V4444 Sgr as a Recurrent Nova

T. Kato, H. Yamaoka, S. Kiyota

V4444 Sgr (Nova Sgr 1999) has been recently suggested to be a possible recurrent nova based on the detection of the preexisting dust, which may have been formed in a previous outbu…

astro-ph2003★ 21 cited

Period change of Superhumps in the WZ Sge-Type Dwarf Nova, HV Virginis

R. Ishioka, T. Kato, M. Uemura +12

After 10 years of quiescence, HV Vir underwent a superoutburst in January 2002. We report time-series observations clearly revealing the period change of ordinary superhumps during…

astro-ph2003★ 7 cited

Grazing Eclipsing Dwarf Nova CW Monocerotis: Dwarf Nova-Type Outburst in a Possible Intermediate Polar?

T. Kato, M. Uemura, S. Kiyota +10

We observed the 2002 October-November outburst of the dwarf nova CW Mon. The outburst showed a clear signature of a premaximum halt, and a more rapid decline after reaching the out…

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