Date: Wed, 7 Apr 93 18:01:36 JST
From: tkato@kusastro.kyoto-u.ac.jp (Taichi Kato)
Subject: SN1993J, photometry at Ouda, Apr.6
CCD observations on Apr. 6 at Ouda Station, Kyoto University (Nara, Japan)
(60-cm reflector, fl=4.8m)
SN-starA starB-StarA
band* mid UT dmag N mid UT dmag N
---- ----------------------------------------------
V 930406.485 0.391 12 930406.486 0.452 13
B 930406.538 0.226 6 930406.538 0.397 6
Ic 930406.511 0.452 12 930406.511 0.456 14
---- ----------------------------------------------
V 930406.685 0.377 18 930406.694 0.490 15
B 930406.720 0.218 5 930406.720 0.428 5
Ic 930406.739 0.413 9 930406.739 0.481 9
band: uncorrected Ouda system
Using standard values of starB (V=11.90, B=12.40, Ic=11.30), we obtain
(first half)
SN: V=11.84, B=12.23, Ic=11.29
starA: V=11.45, B=12.00, Ic=10.84
(last half)
SN: V=11.79, B=12.19, Ic=11.23
starA: V=11.41, B=11.97, Ic=10.82
Condition was rather non-photometric, but the data suggest that supernova
is definitely on the rise.
Regards,
Taichi Kato (Kyoto University)

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