Discovery of the heavily obscured supernova 2002cv

被引:23
作者
Di Paola, A
Larionov, V
Arkharov, A
Bernardi, F
Garatti, ACO
Dolci, M
Di Carlo, E
Valentini, G
机构
[1] Osserv Astron Roma, INAF, I-00136 Rome, Italy
[2] St Petersburg State Univ, Astron Inst, St Petersburg 198504, Russia
[3] Isaac Newton Inst Chile, St Petersburg Branch, St Petersburg, Russia
[4] Cent Astron Observ, St Petersburg, Russia
[5] Osservatorio Astron Teramo, OACT, INAF, Teramo, Italy
[6] Univ Roma Tor Vergata, Rome, Italy
关键词
supernovae : general; supernovae : individual : SN2002cv; infrared : galaxies;
D O I
10.1051/0004-6361:20021168
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
On the 13th of May 2002, supernova 2002cv was discovered using a near-infrared camera working at the AZT-24 1.1 m telescope at Campo Imperatore (AQ-Italy). After the infrared detection a simultaneous photometric follow-up was started at optical wavelengths. The preliminary results confirm a heavily obscured object with a V-K color not lower than 6 mag, making SN 2002cv the most reddened supernova ever observed. This finding, along with the recent discovery of another obscured supernova, suggests a critical revision of the rates known to date. The estimate of the visual extinction and the light curves are provided here. These latter indicate that our SN 2002cv observations are the earliest available for a type-Ia supernova at IR wavelengths.
引用
收藏
页码:L21 / L24
页数:4
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