ATLAS discoveries of optical transients
ATel #9651; J. Tonry, L. Denneau, B. Stalder, A. Heinze, A. Sherstyuk (IfA, University of Hawaii), A. Rest (STScI), K. W. Smith, S. J. Smartt (Queen's University Belfast)
on 19 Oct 2016; 13:00 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Ken Smith (k.w.smith@qub.ac.uk)
Subjects: Optical, Supernovae, Transient
We report the following transients found by the ATLAS survey (see Tonry et al. ATel #8680). ATLAS is a twin 0.5m telescope system on Haleakala and Mauna Loa. The first unit is operational on Haleakala is robotically surveying the sky. Two filters are used, cyan and orange (denoted c and o, all mags in AB system), more information is on http://www.fallingstar.com. All transients have been registered with the IAU.
Host galaxy identifications and redshifts are from NED or the Pan-STARRS1 3Pi image stack, and absolute magnitude calculations include an estimate of Milky Way foreground extinction at the filter wavelength.
Name | ATLAS Name | RA (J2000) | Dec (J2000) | Disc. MJD | Disc. Date | Disc Mag | z | Notes
AT2016hff | ATLAS16dkq | 19:25:51.18 | -31:21:16.5 | 57667.26 | 20161006.26 | 17.38 c | | 1.
AT2016hfh | ATLAS16dlb | 19:21:21.14 | +47:14:27.2 | 57668.27 | 20161007.27 | 18.07 c | | 2.
AT2016hfc | ATLAS16dkf | 00:20:11.44 | +47:28:56.4 | 57668.39 | 20161007.39 | 18.33 c | | 3.
AT2016gzs | ATLAS16dic | 07:52:43.19 | +58:41:38.0 | 57668.58 | 20161007.58 | 17.39 c | | 4.
AT2016hgd | ATLAS16dmf | 09:59:07.46 | +50:59:05.6 | 57674.63 | 20161013.63 | 17.74 o | 0.025544 | 5.
AT2016hfe | ATLAS16dkv | 20:06:45.56 | -31:00:44.2 | 57675.24 | 20161014.24 | 17.44 o | 0.039661 | 6.
AT2016hgb | ATLAS16dlz | 00:43:36.60 | +41:56:32.1 | 57677.52 | 20161016.52 | 17.67 o | | 7.
1. No obvious host.
2. NED reports that the likely host (2.22 arcsec away) is 2MASX J19212135+4714264
3. NED reports that the likely host (16.2 arcsec away) is 2MASX J00201167+4728401
4. NED reports that the likely host (4.02 arcsec away) is 2MASX J07524342+5841346
5. NED reports that the likely host (18.66 arcsec away) is UGC 05356, with spectroscopic z=0.025544, hence mu=35.20, A_o=0.032, M_o=-17.49
6. NED reports that the likely host (7.55 arcsec away) is ESO 461- G 040, with spectroscopic z=0.039661, hence mu=36.09, A_o=0.326, M_o=-18.98
7. This object is a probable M31 nova.