KAIT Discovery and Robotic Follow-up of a young SN Ia in NGC5669
ATel #4823; W. Zheng, P. Blanchard, S. B. Cenko, A. V. Filippenko (UC Berkeley) and A. Cucchiara (UCO/Lick Observatory)
on 18 Feb 2013; 23:47 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Weikang Zheng (zwk@umich.edu)
Subjects: Optical, Supernovae, Transient
We report the discovery, with the 0.76-m Katzman Automatic Imaging Telescope
(KAIT) at Lick Observatory, of a possible new supernova in the nearby
galaxy NGC 5669. The new object, dubbed PSN J14324449+0953123 (by the
IAU), is located at (J2000.0) coordinates RA = 14:32:44.49, Dec =
+09:53:12.3. Following discovery in an unfiltered image obtained at
12:59 UT on 2013 Feb. 17, KAIT autonomously began a sequence of triggered
follow-up observations in the U, B, V, and clear (roughly R) filters
beginning only 4 minutes later. Using stars from the USNO-B1 catalog for
reference, we measure R = 17.6 mag at this time. Previous KAIT imaging on
2013 Feb. 15 revealed no emission at this location to a limit of R > 18.5 mag.
A CCD spectrum (range 340-800 nm) of the object was obtained on Feb. 18 UT
with the Kast double spectrograph on the Shane 3-m telescope at Lick Observatory.
It is dominated by a largely featureless blue continuum, with superimposed
narrow emission lines from the underlying host galaxy, consistent with
the reported redshift of 0.0046. These properties are suggestive of a
very young Type II supernova, and further observations are encouraged.