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Prediscovery Detection and Photometry of AT 2024zaq, a Probable Nova in M31

ATel #16878; K. Hornoch (Astronomical Institute, Ondrejov, Czech Republic), A. W. Shafter (SDSU)
on 25 Oct 2024; 17:27 UT
Distributed as an Instant Email Notice Novae
Credential Certification: Allen W. Shafter (ashafter@sdsu.edu)

Subjects: Optical, Nova, Transient

Referred to by ATel #: 16883, 16884

We report the prediscovery detection of a probable M31 nova AT 2024zaq discovered by R. Fidrich on 2024 Oct. 24.337 UT. During our survey of the central region of M31 we detected the probable nova first on a co-added 900-s R-band CCD frame taken on Oct. 24.151 UT with the 40-in reflector at SDSU's Mount Laguna Observatory and also on additional images taken with the same instrument as well as with the 0.65-m telescope at Ondrejov.

The following R-band magnitudes were obtained using the 40-in reflector at SDSU's Mount Laguna Observatory (MLO) and the 0.65-m telescope at Ondrejov (D65):

 
  Date [UT]    |  Mag   | Err  | Filter  | Telescope 
 
2024-10-23.146 | >19.7  |      | R       | MLO 
2024-10-24.151 |  16.56 | 0.03 | R       | MLO 
2024-10-24.738 |  16.09 | 0.08 | R       | D65 
2024-10-24.752 |  15.94 | 0.09 | R       | D65 
2024-10-25.173 |  16.24 | 0.03 | R       | MLO 
 
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.