Independent Discovery of a Probable Nova in M31
ATel #16758; K. Hornoch (Astronomical Institute, Ondrejov, Czech Republic), M. Zejda (DTPA, Masaryk University, Brno, Czech Republic), H. Kucakova and M. Wolf (Charles University, Prague, Czech Republic), A. W. Shafter (SDSU)
on 7 Aug 2024; 20:09 UT
Distributed as an Instant Email Notice Novae
Credential Certification: Allen W. Shafter (ashafter@sdsu.edu)
Subjects: Optical, Nova, Transient
Referred to by ATel #: 16770
We report the independent discovery of a probable rising nova found during our survey of the central region of M31. The object was discovered on a co-added 1620-s Sloan g CMOS frame taken on 2024 Aug. 7.054 UT with the 0.8-m telescope at Zdanice. The object is visible also on a co-added 1620-s Sloan r and Sloan i CMOS frames taken with the same instrumentation on Aug. 7.056 and 7.057 UT, respectively, and also on three prediscovery co-added R-band CCD frames taken on Aug. 6.924, 6.936, and 6.946 UT with the 0.65-m telescope at Ondrejov. The object was subsequently found barely visible also on a prediscovery CCD frames taken on Aug. 5.891 and 5.896 UT with the 0.65-m telescope
at Ondrejov.
The object was independently discovered on Aug. 7.142 UT by J. Zhao and designated
as PNV J00424486+4115420 = AT 2024rnm.
The object was designated by us as M31N 2024-08b and is located at R.A. = 0h42m44s.87, Decl. = +41o15'41".7 (equinox 2000.0), which is 6.2" east and 26.8" south of the center of M31 (see link to discovery image below).
The following magnitudes were obtained using the 0.65-m telescope at Ondrejov (D65) and the 0.8-m telescope at Zdanice (D80):
Date [UT] | Mag | Err | Filter | Telescope
2024-08-01.062 | >19.7 | | Sloan g | D80
2024-08-03.845 | >19.4 | | R | D65
2024-08-05.891 | 19.0 | 0.4 | R | D65
2024-08-05.896 | 19.2 | 0.4 | R | D65
2024-08-06.924 | 18.4 | 0.3 | R | D65
2024-08-06.936 | 18.2 | 0.25 | R | D65
2024-08-06.946 | 18.3 | 0.25 | R | D65
2024-08-07.054 | 18.43 | 0.10 | Sloan g | D80
2024-08-07.056 | 18.6 | 0.15 | Sloan r | D80
2024-08-07.057 | 18.4 | 0.2 | Sloan i | D80
As with all extragalactic novae, follow-up spectroscopic and photometric observations to confirm the nova's nature and determine its spectroscopic class and rate of decline (speed class) are encouraged.
Discovery image