[vsnet-alert 14922] Re: Possible bright CV in Peg? - PNV J23272715+0855391
Denis Denisenko
d.v.denisenko at gmail.com
Fri Sep 14 07:24:15 JST 2012
MASTER-Tunka automatic photometry of PNV J23272715+0855391 = SDSS
J232727.14+085538.7 (unfiltered with USNO-B1.0 R2 zeropoint):
20120913.659 13.11C MASTER-Tunka
20120913.662 13.14C MASTER-Tunka
20120913.665 13.07C MASTER-Tunka
20120913.668 13.04C MASTER-Tunka
20120913.671 13.08C MASTER-Tunka
20120913.674 13.10C MASTER-Tunka
MASTER is known for systematically providing "brighter" magnitudes
compared to other observers by as much as 0.5m, so this does not
necessarily mean the brightening of the object since the discovery by
K. Itagaki.
Denis Denisenko
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