activity
20022004
most citedVery high column density and small reddening towards GRB 020124 at z = 3.20

112 citations · 188 across the 5 of their papers we have counts for

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astro-ph2004

The 2003 Superoutburst of an SU UMa-type Dwarf Nova, GO Comae Berenices

Akira Imada, Taichi Kato, Makoto Uemura +19

We photometrically observed the 2003 June superoutburst of GO Gom. The mean superhump period was 0.063059(13) d. The resultant data revealed that (1) the obtained light curve conta…

astro-ph2003★ 17 cited

Outburst and Post-Outburst Active Phase of the Black Hole X-ray Binary V4641 Sgr in 2002

M. Uemura, T. Kato, R. Ishioka +19

The black hole X-ray binary V4641 Sgr experienced an outburst in 2002 May which was detected at X-ray, optical, and radio wavelengths. The outburst lasted for only 6 days, but the…

astro-ph2003★ 112 cited

Very high column density and small reddening towards GRB 020124 at z = 3.20

J. Hjorth, P. Møller, J. Gorosabel +27

We present optical and near-infrared observations of the dim afterglow of GRB 020124, obtained between 2 and 68 hours after the gamma-ray burst. The burst occurred in a very faint…

astro-ph2003★ 23 cited

In-the-Gap SU UMa-Type Dwarf Nova, Var73 Dra with a Supercycle of about 60 Days

D. Nogami, M. Uemura, R. Ishioka +13

An intensive photometric-observation campaign of the recently discovered SU UMa-type dwarf nova, Var73 Dra was conducted from 2002 August to 2003 February. We caught three superout…

astro-ph2002★ 36 cited

Discovery of a Dwarf Nova Breaking the Standard Sequence of Compact Binary Evolution

M. Uemura, T. Kato, R. Ishioka +1

We revealed that the dwarf nova 1RXS J232953.9+062814 is an SU UMa-type system with a superhump period of 66.774+/-0.010 min. The short period strongly indicates that the orbital p…