Re: [vsnet-chat 2074] BV sequence for V1333 Aql > The GCVS4.1 claims a peak magnitude of 14.8, so perhaps it is readily > accessible only to those with large telescopes (or smaller ones + CCD). The quoted GCVS maximum seems to be a rather exceptional value. Recent reports (cf. IAUCs) indicate usual optical maxima are around mag 16. At the time of charting, it did look readily accessible, since several 14.5-15.0 mag dwarf novae were already on the program (as are reported in VSNET now). Aside from usual outbursts, there was a report (in ApJ letter, last year?) of recurrent short optical flashes. I wonder whether this phenomenon has been confirmed, and whether is accesible to eyes. Regards, Taichi Kato