ATLAS19ggw (AT2019dhc): discovery of a candidate SN in UGC 08752 (93 Mpc)
ATel #12650; K. W. Smith, O. McBrien, S. J. Smartt, A. McCormack (Queen's University Belfast), L. Denneau, H. Flewelling, A. Heinze, J. Tonry, H. Weiland (IfA, University of Hawaii), B. Stalder (LSST) A. Rest (STScI), P. Clark, M. Fulton, D. O'Neill, D. R. Young (Queen's University Belfast), D. E. Wright (University of Minnesota)
on 11 Apr 2019; 14:50 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 #: 12653
ATLAS is a twin 0.5m telescope system on Haleakala and Mauna Loa which is robotically surveying the sky above declination -40 with a cadence of 2 days (Tonry et al. 2018, PASP, 13, 064505). Two filters are used, cyan and orange (denoted c and o; all mags quoted are in the AB system). While carrying out the primary mission for Near Earth Objects, we search for and publicly report stationary transients to the IAU Transient Name Server. More information is on http://www.fallingstar.com. We are submitting Astronomer's Telegrams for transients that are either within 100 Mpc, or have some other interesting feature to bring to the community's attention, such as bright nuclear transients, slowly rising or rapidly fading objects.
We report a new transient source, most likely a supernova in the galaxy UGC 08752. We discovered ATLAS19ggw (AT2019dhc) on MJD 58581.47 == 2019-04-08.47, at m_o = 19.02 +/- 0.18. There was no detection by ATLAS on MJD 58579.52 == 2019-04-06.52. ATLAS19ggw is offset by 2.90 arcsec south, 1.98 arcsec east from UGC 08752, which is at z = 0.021 or d = 92.5 Mpc (from NED), implying an absolute magnitude of M = -15.83 (assuming m-M = 34.83 and A_r = 0.026 and A_i = 0.019). A summary of the transient's properties is shown below. Followup observations are encouraged.
Name | ATLAS Name | RA (J2000) | Dec (J2000) | Disc. MJD | Disc Mag | Offset from host
AT2019dhc | ATLAS19ggw | 13:50:33.01 | +35:07:50.6 | 58581.47 | 19.02 o | 3.51 arcsec
This work has made use of data from the Asteroid Terrestrial-impact Last Alert System (ATLAS) project. ATLAS is primarily funded to search for near earth asteroids through NASA grants NN12AR55G, 80NSSC18K0284, and 80NSSC18K1575; byproducts of the NEO search include images and catalogs from the survey area. The ATLAS science products have been made possible through the contributions of the University of Hawaii Institute for Astronomy, the Queen's University Belfast, and the Space Telescope Science Institute.
