(1993 May 8)
subject: VS observations SN1993J etc.
Visual magnitude estimates by VSOLJ members
object YYMMDD(UT) mag code
R Boo 930507.593 123 Ths
Z Cam 930507.498 117 Yad
YZ Cnc 930507.508 116 Yad
R CrB 930505.598 60 Yad
930506.506 60 Yad
930507.460 66 Ths
930507.506 60 Yad
T CrB 930507.588 99 Ths
R Crv 930507.578 73 Ths
chi Cyg 930505.599 54 Yad
930506.657 54 Yad
P Cyg 930506.658 49 Yad
g Her 930506.507 52 Yad
930507.510 53 Yad
FI Hya 930507.500 89 Yad
930507.581 90 Ths
R Leo 930507.507 89 Yad
T Leo 930507.563 <131 Ths
R Sct 930506.658 58 Yad
S UMa 930507.503 87 Yad
930507.505 87 Yad
Z UMa 930506.506 73 Yad
930507.509 74 Yad
SW UMa 930507.552 <132 Ths
BC UMa 930507.559 <133 Ths
BZ UMa 930507.469 <126 Ths
CH UMa 930507.457 <140 Ths
CY UMa 930507.555 <132 Ths
R Vir 930507.502 97 Yad
SS Vir 930507.569 88 Ths
HV Vir 930507.574 <133 Ths
3C273 930507.571 125 Ths
SN1993J 930507.455 122 Ths seq: TB inst:60L
930507.495 124 Yad seq: TB inst:16L
Observer's code:
Ths: S.Takahashi(Shiga, Japan) instruments: 60L, 20R, 12B
Yad: M.Yamada(Ishikawa,Japan) instruments:16L,5.6B
* Takahashi comments that R CrB is fainter than usual.
* Takahashi comments that 3C273 is brighter than usual, which is consistent
with the radio activity reported in recent IAUC.
vsnet-adm@kusastro.kyoto-u.ac.jp