SN 2018ivc

Follow up observations of SN 2018ivc in M77 on 2018-11-29.399

Magnitude C = 14.73 +/- 0.03

Observer: M. Kendurkar, GSNST, Canada

AT 2018jeo

We observed AT 2018jeo on 2018-11-29.248

Observed magnitude C = 16.81 +/- 0.08
Observer: M. Kendurkar, GSNST , Canada

Observation: 2017eaw

2017eaw, Type IIP in NGC 6946
Discovered 2017-05-14.238 by Patrick Wiggins, mag 12.8 at discovery
R.A. = 20h34m44s.238, Decl. = +60°11'36".00

TCP J00420310+4102331

TCP J00420310+4102331 in M31 on 2018-10-17.876

CV = 16.84 +/- 0.05

Observer: M. Kendurkar, GSNST, Canada

SN 2018hfn (GSNST 2018-ah)

M. Kendurkar reported a discovery of a new transient and now it's classified as Supernova SN 2018hfn. ( https://wis-tns.weizmann.ac.il/object/2018hfn )
Follow up observations of SN 2018hfn on 2018-10-13.116
V = 14.80 +/- 0.01
Observer: M. Kendurkar, GSNST

AT 2018grm = (GSNST 2018-ae)

Follow up observations of our discovery AT 2018grm = (GSNST 2018-ae) on 2018-09-22.040

CV = 20.55 +/- 0.75

Observer: Malhar R. Kendurkar, GSNST Team

SN 2018fub

Supernova SN 2018fub in 2MASX J00403068-5041153.
Date of Observations: 2018-09-07.237
CV Magnitude: +17.71 +/- 0.06
Observer: Malhar R. Kendurkar, GSNST Team

Followup: AT2018fhy

After further investigation, AT2018fhy is probably 2MASS J00431056+4116574, a possible globular cluster in M31. The fact that it's made up of many stars, some of variable type RR Lyrae, explains the variations in magnitude we observed. Thanks to Emmanuel Conseil for the information.