J/AZh/84/1110          Brightness of SN 2006X                   (Lipunov+, 2007)
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Optical observations of gamma-ray bursts, the discovery of supernovae 2005bv,
2005ee, 2006ak, search of transients at telescope-robot MASTER.
     Lipunov V.M., Kornilov V.G., Krylov A.V., Tyurina N.V., Belinski A.A.,
     Gorbovskoy E.S., Kuvshinov D.A., Gritsyk P.A., Antipov G.A., Borisov G.V.,
     Sankovich A.V., Vladimirov V.V., Vybornov V.I., Kuznetsov A.S.
    <Astron. Zh. 84, 1110 (2007)>
    =2007AZh....84.1110L
    =2007ARep...51.1004L
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ADC_Keywords: Gamma rays ; Supernovae

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.

Objects:
    ----------------------------------------------------------
       RA   (2000)   DE      Designation(s)
    ----------------------------------------------------------
    12 22 53.9   +15 48 32   SN 2006X = SN 2006X
    ----------------------------------------------------------

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table9.dat     20      120   Brightness of SN 2006X
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Table 5: Photometry of GRB 060926 obtained on the MASTER telescope
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 Beginning of Middle of   Exposure  Magnitude  Flux      Flux after
 exposure,s   exposure,s     s                           correction
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   76         91  1*30  17.3  0.3  (1.4+/-0.3)*10^-13^  (4.3+/-1.0)*10^-12^
  150        165  1*30  18.5  0.3  (4.6+/-1.1)*10^-14^  (1.4+/-0.4)*10^-12^
  165        343  5*30  19.3  0.3  (2.2+/-0.5)*10^-14^  (6.9+/-1.7)*10^-13^
  255        432  5*30  18.9  0.3  (3.2+/-0.8)*10^-14^  (9.9+/-2.4)*10^-13^
  343        519  5*30  18.5  0.3  (4.6+/-1.1)*10^-14^  (1.4+/-0.3)*10^-12^
  432        608  5*30  18.3  0.3  (5.8+/-1.3)*10^-14^  (1.7+/-0.4)*10^-12^
  519        707  5*30  18.4  0.3  (5.1+/-1.2)*10^-14^  (1.6+/-0.4)*10^-12^
  608        804  5*30  18.7  0.3  (3.9+/-0.9)*10^-14^  (1.2+/-0.3)*10^-12^
  707       1001  5*30  20.0  0.3  (1.2+/-0.3)*10^-14^  (3.6+/-0.9)*10^-13^
  804       1200  5*30  20.1  0.3  (1.1+/-0.3)*10^-14^  (3.3+/-0.8)*10^-13^
  901       1298  5*30 >20.1  0.3 <(1.1+/-0.3)*10^-14^ <(3.3+/-0.8)*10^-13^
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Byte-by-byte Description of file: table9.dat
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   Bytes Format Units   Label     Explanations
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   1- 12  F12.4 d       JD        [2453772/2453861] Julian date
  15- 20  F6.3  mag     Vmag      V magnitude
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(End)                                       Veta Avedisova (INASAN)  28-Nov-2009
