Brightness of SN 2006X (Lipunov+, 2007)

Details Brightness of SN 2006X (Lipunov+, 2007) Brightness of SN 2006X (Lipunov+, 2007)

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..80841110l&link_type=abstract

VizieR On-line Data Catalog: J/AZh/84/1110. Originally published in: 2007AZh....84.1110L; 2007ARep...51.1004L

Physics

Gamma Rays, Supernovae

Scientific paper

The results of observations over 2005-2006 years at the robotic telescope MASTER are presented. There are the first in the world observation of optical emission of GRB 050824 and GRB 060926 gamma-ray bursts. Our data combined with more later one gives the low of brightness drop t-0.55+/-0.05 for GRB 050824. We discovered optical flare for GRB 060926 around 500-700s. The power low spectral index (FE~E-beta) is equal beta=1.0+/-0.2. In the course of sky survey we have images of more than 90% possible sky. The virtual data-base and pipe-line was made. The limit to the orphan optical bursts rate is presented. We discovered 3 supernovae stars, they are the following: SN 2005bv (Ia-type) is the first one, opened from Russian territory, SN 2005ee is one of the most powerful among II-type supernovae, SN 2006ak (Ia-type). New method of the OT search after IPN-triangulation gamma-observation is proposed and tested.
(1 data file).

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