Electronic Telegram No. 2417
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
CBAT Director:  Daniel W. E. Green; Room 209; Dept. of Earth and Planetary
 Sciences; Harvard University; 20 Oxford St.; Cambridge, MA  02138; U.S.A.
e-mail:  cbat@iau.org; cbatiau@eps.harvard.edu
URL http://www.cfa.harvard.edu/iau/cbat.html


SUPERNOVA 2010gv
     Further to CBETs 2404 and 2408, D. Balam and E. Chisholm, National
Research Council of Canada, obtained CCD images of 2010gv on Aug. 13.33 UT
using the 1.82-m Plaskett telescope, showing the new object at R.A. =
17h58m22s.57, Decl. = +50d47'34".3 (equinox 2000.0), which is 2".3 east and
1".2 N north the core of the faint galaxy SDSS J175822.33+504733.1, noting
that there is no source visible at this position on the Sloan Digital Sky
Survey DR7 images (to limiting R magnitude about 22) or on the Palomar Sky
Survey.  Using the SDSS catalogue star SDSS J175818.72+504702.2 as a
secondary standard and converting the SDSS magnitudes to the Kron_Cousins
system, they derive a differential magnitude of R = 15.85.


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2010 CBAT
2010 August 17                   (CBET 2417)              Daniel W. E. Green