Visual magnitude estimates by VSOLJ members
object YYYYMMDD(UT) mag code AURAB 20250217.489 73 Mhh.VSOLJ AURAB 20250226.439 73 Mhh.VSOLJ CETomicron 20250217.486 38 Mhh.VSOLJ CETomicron 20250226.436 36 Mhh.VSOLJ CMAHL 20250226.500 123 Mhh.VSOLJ CMAPU 20250226.502 <141 Mhh.VSOLJ GEMAW 20250226.524 <151 Mhh.VSOLJ GEMIR 20250226.522 <151 Mhh.VSOLJ GEMU 20250226.525 141 Mhh.VSOLJ GEMUV 20250226.522 <150 Mhh.VSOLJ HYAV748 20250226.531 120 Mhh.VSOLJ LEOR 20250217.487 60 Mhh.VSOLJ LEOR 20250226.438 62 Mhh.VSOLJ LEOX 20250226.527 <147 Mhh.VSOLJ MONHQ 20250226.519 131 Mhh.VSOLJ MONR 20250226.514 120 Mhh.VSOLJ MONU 20250217.487 57 Mhh.VSOLJ MONU 20250226.437 58 Mhh.VSOLJ MONV651 20250226.517 109 Mhh.VSOLJ ORICN 20250226.504 126 Mhh.VSOLJ ORICZ 20250226.509 135 Mhh.VSOLJ ORIV1159 20250226.503 139 Mhh.VSOLJ ORIV344 20250226.511 <148 Mhh.VSOLJ OT_J064833.4+065624 20250226.516 <148 Mhh.VSOLJ TAUSU 20250226.508 117 Mhh.VSOLJ TAUV1434 20250226.506 <146 Mhh.VSOLJ
Observer: Hiroyuki Maehara (Okayama, Japan) Instruments: 30cmL, 4.2cmB(10x)
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp