Brightness of SN 2006X Virtual Observatory Resource

Authors
  1. Lipunov V.M.
  2. Kornilov V.G.
  3. Krylov A.V.
  4. Tyurina N.V.
  5. Belinski A.A.,Gorbovskoy E.S.
  6. Kuvshinov D.A.
  7. Gritsyk P.A.
  8. Antipov G.A.
  9. Borisov G.V.,Sankovich A.V.
  10. Vladimirov V.V.
  11. Vybornov V.I.
  12. Kuznetsov A.S.
  13. Published by
    CDS
Abstract

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 (F_E_~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.

Keywords
  1. gamma-ray-astronomy
  2. supernovae
Bibliographic source Bibcode
2007AZh....84.1110L
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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/84/1110
IVOA Identifier IVOID
ivo://CDS.VizieR/J/AZh/84/1110

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History

2010-02-01T03:28:32Z
Resource record created
2010-02-01T03:28:32Z
Created
2017-07-05T06:59:09Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr