ATLAS17jiv: discovery of a bright supernova candidate in NGC 7187
ATel #10633; K. W. Smith, S. J. Smartt (Queen's University Belfast), D. E. Wright (University of Minnesota), J. Tonry, L. Denneau, B. Stalder, A. Heinze, H. Weiland (IfA, University of Hawaii), A. Rest (STScI)
on 11 Aug 2017; 16:44 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Ken Smith (k.w.smith@qub.ac.uk)
Subjects: Optical, Supernovae
Referred to by ATel #: 10639
ATLAS is a twin 0.5m telescope system on Haleakala and Mauna Loa. Both
units are operational and are robotically surveying the sky. Two
filters are used, cyan and orange (denoted c and o, all mags in AB
system), more information on http://www.fallingstar.com. While
carrying out the primary mission for NEOs, we search for and publicly
report stationary transients (see Tonry et al. ATel #8680)
We report a new transient source, most likely a supernova in the
galaxy NGC 7187. We discovered ATLAS17jiv (AT2017gah)
on MJD 57975.49 == 2017-08-10.49 UTC at m_o = 15.69 +/- 0.03.
ATLAS17jiv is 43.56 arcseconds from the centre of NGC 7187 which is at z=0.008906 or d=33Mpc (from
NED). Implying an absolute magnitude of M = -16.98 (assuming m-M = 32.6
and (A_r+A_i)/2 = 0.068). A summary of the transient's properties are
summarised below. Follow up observations are encouraged.
Forced photometry yielded a first 3.1sigma detection of o=18.47 on 57970.408, indicating the object
is at least 5 days old.
Name | ATLAS Name | RA (J2000) | Dec (J2000) | Disc. MJD | Disc. Date | Disc Mag
AT2017gah | ATLAS17jiv | 22:02:42.43 | -32:47:33.4 | 57975.49 | 20170810.49 | 15.69 o
Obs. MJD mag err filter
57970.408 18.47 0.30 o
57970.415 18.32 0.24 o
57975.495 15.69 0.03 o
57975.503 15.71 0.03 o
57975.505 15.72 0.03 o
57975.511 15.74 0.04 o