[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-history 1292] SN 1993J (Prabhu)




Date: Tue, 3 Aug 93 11:16:47 IST
From: iiap!tpp@iiap.ernet.in (Dr.T.P.Prabhu)
Subject: SN93J

  Dear Dr. Kato,
  
  I had mailed the following data on SN93J in BVRI(Cousins) bands some time
  back but it bounced. I am trying again. I would like to receive your
  updated photometry for beyond May 15. Since we are using uucp protocol
  by remote login from the nearest node, we can at present access files
  of size NOT MORE THAN 40kbytes at a time. May I request you to send the
  data in smaller files?
 
  Best regards,
  
  Tushar Prabhu
  tpp@iiap.ernet.in
  3  Aug  1993
-----------------------------------------------------------------------------  

  Supernova 1993J: CCD photometric results.
  
  Y. D. Mayya, T. P. Prabhu, Ram Sagar, A. Subramaniam, A. K. Pati,
  Indian Institute of Astrophysics, Bangalore 560034, India
  
  K. P. Singh, Tata Institute of Fundamental Research, Bombay 400005, India
  
  Gopal-Krishna, National Centre for Radio Astrophysics, Pune 411007, India
  
  Telescope : 2.3m reflector, Vainu Bappu Observatory, Kavalur, India
  Instrument: Prime Focus CCD camera with GEC 8603 chip 
  Method    : Differential photometry with star B as standard. Correction
              for colour coefficient in transformation equations is made.

       Date       V        B-V      V-R     V-I 
       1993
    APR 14.68   10.957    0.521    0.390 
    APR 15.67   10.898    0.497    0.397
    APR 16.68   10.865    0.530    0.425
    APR 17.65   10.869    0.630    0.406
    APR 18.62   10.847    0.576    0.396
    APR 19.62   10.885    0.675    0.426
    APR 21.61   10.976    0.780    0.473   0.520
    APR 22.59   11.049    0.876    0.475
    APR 24.60   11.267    0.935    0.557   0.637
    MAY 21.61   12.473    1.269    0.686
    MAY 23.64   12.538    1.392    0.707

    Star B      11.900    0.500    0.300    0.600  Comparison; assumed mag
              +/-0.018 +/-0.023 +/-0.008 +/-0.008  rms of correction
	      
    Star A      11.407    0.539    0.306    0.604  Check star; derived mag
              +/-0.016 +/-0.021 +/-0.022    0.010  rms of derived mag
	     


Return to Home Page

Return to the Powerful Daisaku Nogami

vsnet-adm@kusastro.kyoto-u.ac.jp

Powered by ooruri technology