activity
20002013
most citedMassive stars exploding in a He-rich circumstellar medium. I. Type Ibn (SN 2006jc-like) events

203 citations · 632 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2013

Observational study of the extremely slow nova V1280 Scorpii

H. Naito, S. Mizoguchi, A. Arai +10

We present multi-color light curves and optical spectra of V1280 Scorpii obtained from 2007 to 2012. It is shown that V1280 Sco is the extremely slow nova and the mass of white dwa…

astro-ph.HE2011★ 63 cited

Evidence for Type Ia Supernova Diversity from Ultraviolet Observations with the Hubble Space Telescope

Xiaofeng Wang, Lifan Wang, Alexei V. Filippenko +93

We present ultraviolet (UV) spectroscopy and photometry of four Type Ia supernovae (SNe 2004dt, 2004ef, 2005M, and 2005cf) obtained with the UV prism of the Advanced Camera for Sur…

astro-ph2008★ 203 cited

Massive stars exploding in a He-rich circumstellar medium. I. Type Ibn (SN 2006jc-like) events

A. Pastorello, S. Mattila, L. Zampieri +26

We present new spectroscopic and photometric data of the type Ibn supernovae 2006jc, 2000er and 2002ao. We discuss the general properties of this recently proposed supernova family…

astro-ph2003★ 113 cited

Variable Star Network: World Center for Transient Object Astronomy and Variable Stars

T. Kato, M. Uemura, R. Ishioka +4

Variable Star Network (VSNET, http://www.kusastro.kyoto-u.ac.jp/vsnet/) is a global professional-amateur network of researchers in variable stars and related objects, particularly…

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★ 31 cited

Superhumps in the Rarely Outbursting SU UMa-Type Dwarf Nova, HO Delphini

T. Kato, D. Nogami, M. Moilanen +1

We observed the 1994, 1996 and 2001 outbursts of HO Del. From the detection of secure superhumps, HO Del is confirmed to be an SU UMa-type dwarf nova with a superhump period of 0.0…