SN1994I new photometry

  Forwarded message:

>From visitor1@kibi.oao.nao.ac.jp Wed Apr 20 23:27:03 1994
To: tkato@kusastro.kyoto-u.ac.jp
Subject: SN1994I obserevational result

Hello Kato-sama,
   
  Because Dr. Hitoshi Yamaoka told me that the SN brightness should be 
reported to you, I am sending here a short report of preliminary 
result of 1994I brightness measured at the Okayama Astrophysical 
Observatory with RCA CCD during our observing run. 

   We used star 135(D) near the nucleus of M51, R-magnitude is 
   13.12. The thin cloud was there during our imaging, the 
   R-magnitude we obtained should have large uncertainty as noted.

1994 April 17.48 UT    13.24 +- 0.2 
1994 April 19.59 UT    13.28 +- 0.1 

   These value were measured from CCD images taken by 188cm telescope 
   at the Okayama Astrophysical Observatory. 
   The observers are J. Watanabe, National Astronomical Observatory
of Japan, A. Nakamura, H. Araki, Institute of Space and
Astronautical Science, H. Hasegawa, Astec Inc., and Y. Hirota,
Tokyo Gakugei University.

  Best regards,

-Junichi Watanabe
National Astronomical Observatory of Japan.