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T. Yamashita

4 papers hereh-index 4181 citations7 works total

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

author position
  • middle author3

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

fields
  • astro-ph1
  • astro-ph.CO1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • T. Yamashita — 48 papers, h 15
  • T. Yamashita — 41 papers, h 17
  • T. Yamashita — 38 papers, h 40
  • T. Yamashita — 36 papers, h 32
  • T. Yamashita — 9 papers, h 9
  • T. Yamashita — 5 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
20072010
collaborators

4 papers

astro-ph.CO2010

Infrared/optical - X-ray simultaneous observations of X-ray flares in GRB 071112C and GRB 080506

T. Uehara, M. Uemura, K. S. Kawabata +13

We investigate the origin of short X-ray flares which are occasionally observed in early stages of afterglows of gamma-ray bursts (GRBs). We observed two events, GRB 071112C and GR…

astro-ph.SR2009

Optical and Near-Infrared Photometric Observation during the Superoutburst of the WZ Sge-Type Dwarf Nova, V455 Andromedae

R. Matsui, M. Uemura, A. Arai +17

We report on optical and infrared photometric observations of a WZ Sge-type dwarf nova, V455 And during a superoutburst in 2007. These observations were performed with the KANATA (…

astro-ph.HE2009

Early phase observations of extremely luminous Type Ia Supernova 2009dc

M. Yamanaka, K. S. Kawabata, K. Kinugasa +31

We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is $Δm…

astro-ph2007

Discovery of a WZ Sge-Type Dwarf Nova, SDSS J102146.44+234926.3: Unprecedented Infrared Activity during a Rebrightening Phase

M. Uemura, A. Arai, T. Krajci +26

Several SU UMa-type dwarf novae, in particular, WZ Sge-type stars tend to exhibit rebrightenings after superoutbursts. The rebrightening phenomenon is problematic for the disk inst…

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