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T. Kato

7 papers hereh-index 14862 citations56 works total

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

author position
  • sole author1
  • first author4
  • middle author1

Across the 6 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph7
same name
  • T. Kato — 5 papers, h 26
  • T. Kato — 4 papers, h 21
  • T. Kato — 1 paper, h 12
  • T. Kato — 1 paper, h 1
  • T. Kato — 1 paper, h 19
  • T. Kato — 1 paper, h 18

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
20002003
collaborators
Showing 2002Show all

5 papers · 1 filter

astro-ph2002

Astrometric authentication of RX J2309.8+2135 as a nearby dwarf nova candidate

T. Kato, H. Yamaoka

RX J2309.8+2135 = 1RXS J230949.6+213523 is an X-ray source discovered through the ROSAT all-sky survey. The object was later identified with a star showing a spectrum resembling a…

astro-ph2002

NSV 10934: an Unusual ROSAT-Selected Dwarf Nova: An Analogous Object to HT Cam?

T. Kato, R. Stubbings, H. Yamaok +4

NSV 10934 was discovered as a large-amplitude suspected variable star of unknown classification. We noticed that the object is identified with a bright ROSAT X-ray source (1RXS J18…

astro-ph2002

Unusually Increased Activity of GZ Cnc

T. Kato, P. A. Dubovsky, R. Stubbings +1

GZ Cnc was discovered as a variable star by Takamizawa (Tmz V34), which turned out to a cataclysmic variable (CV). Past studies have shown that this object is a good candidate for…

astro-ph2002

Unusual Outbursting State of a Z Cam-Type Star HL CMa

T. Kato

HL CMa is a Z Cam-type dwarf nova which was discovered as an Einstein X-ray source. In addition to normal outbursts and standstills, we noticed the presence of "the third" outburst…

astro-ph2002

V893 Sco Is Not an ER UMa-Type Star

T. Kato, K. Matsumoto, M. Uemura

V893 Sco is a recently rediscovered bright eclipsing dwarf nova below the period gap. Most recently, Mason et al. (2001) proposed an idea that V893 Sco is an ER UMa-type dwarf nova…

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