RA/DEC (2000)
00:42:47.190 +41:16:19.60
10.696625 +41.272111
Type
Nova
Redshift
Reporting Group
XOSS
Discovering Data Source
XOSS
Discovery Date
2022-11-12 12:37:11.712
TNS AT
Y
Public
Y
Host Name
M31
Discovery Mag
16.8
Filter
Clear-
Reporter/s
Mi Zhang, Qingchen Wang, Linbo Zhu , Yuqing Ren, Chunpeng Bi, Lanhe Ding, Leiming Tang, Jianlin Xu, Wenjie Zhou, Jingyuan Zhao, Jiangao Ruan, Guoyou Sun, Xing Gao and the PSP team

Spectra

 AT_2022zyr - 2022-11-12 15:19:26 Other / Other (None)z=
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   Binning factor: (rounded to nearest integer >1)
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Light curves

 ATLAS-MLO_ATLAS-01_orange
 ATLAS-HKO_ATLAS-02_orange
 Other_Other_Clear
   
Pointer position (MJD, Mag, Abs.Mag): (0.00, 0.00, 0.00)
Spectra
ID Obs-date (UT) Tel / Inst Exp-Time Observer/s Reducer/s Group Spectrum ascii file Spectrum fits file Spec. Type Assoc. Groups End prop. period Remarks
13862 2022-11-12 15:19:26 Other / Other 750 Kenta Taguchi, Masaaki Otsuka Kenta Taguchi None tns_2022zyr_2022-11-12_15-19-26_Other_Other.dat tns_2022zyr_2022-11-12_15-19-26_Other_Other.fits Object We performed the follow-up spectroscopic observation using the KOOLS-IFU attached to the 3.8-m Seimei telescope at Okayama Observatory. The spectral resolution is ~ 500 and the wavelength coverage is 4100-8900 A. The weather was partially cloudy.
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
orange-ATLAS ATLAS-MLO_ATLAS-01 2022-11-12 08:16:49 - 2022-11-12 08:16:49 2459895.8450116 - 2459895.8450116 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
316660 2022-11-12 08:16:49 2459895.8450116 16.574 0.136 ABMag orange-ATLAS ATLAS-MLO_ATLAS-01 30 Robot
orange-ATLAS ATLAS-HKO_ATLAS-02 2022-11-10 12:02:46 - 2022-11-10 12:02:46 2459894.0019213 - 2459894.0019213 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
316659 2022-11-10 12:02:46 2459894.0019213 18.33 ABMag orange-ATLAS ATLAS-HKO_ATLAS-02 30 Robot [Last non detection]
Clear- Other_Other 2022-10-31 17:15:48 - 2022-11-12 12:37:12 2459884.2193056 - 2459896.02583 4
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
316130 2022-11-12 12:37:12 2459896.02583 16.8 20.5 VegaMag Clear- Other_Other 300 Xing Gao
316381 2022-11-12 06:39:00 2459895.7770833 16.07 0.05 20.9 ABMag Clear- Other_Other Data taken with the 0.6/0.9m Schmidt telescope at Piszkesteto Station of Konkoly Observatory
316129 2022-11-11 12:21:19 2459895.0148 20.5 VegaMag Clear- Other_Other 300 Xing Gao [Last non detection]
316380 2022-10-31 17:15:48 2459884.2193056 20.9 ABMag Clear- Other_Other K. Sarneczky [Last non detection] Data taken with the 0.6/0.9m Schmidt telescope at Piszkesteto Station of Konkoly Observatory
AT Reports
ID Time received (UT) Sender Reporter/s Reporting group Disc. Data Source RA DEC Discovery date (UT) Discovery Mag. Filter Related files AT Type Host name Internal name Assoc. Groups End prop. period Remarks ADS Bibcode Unreal Auto classification
164356 2022-11-14 13:11:40 Ismael Perez-Fournon D. Galán,G. Aznar Menargues,Y. Calatayud-Borrás et al. ULL-ASTRO-MASTER ATLAS 00:42:47.190 +41:16:19.60 2022-11-12 08:16:49.000 16.574 orange-ATLAS PSN M31 ULL-ASTRO-MASTER ATLAS forced photometry. N
164198 2022-11-13 14:38:14 Jozsef Vinko A. Horti-David,K. Sarneczky,J. Vinko (Konkoly Observatory) et al. 00:42:47.100 +41:16:19.60 2022-11-12 06:39:00.000 16.07 Clear- PNV M31 Possible nova observed with the 0.6/0.9m Schmidt telescope at Piszkesteto Station of Konkoly Observatory N
164059 2022-11-12 13:16:00 Mi Zhang Mi Zhang,Qingchen Wang,Linbo Zhu et al. XOSS XOSS 00:42:47.190 +41:16:19.60 2022-11-12 12:37:11.712 16.8 Clear- PNV M31 XM88MZ XOSS Nova candidate classified by XOSS, possible RN M31N 1984-07a. Details can be found at http://xjltp.china-vo.org/xm88mz.html 2022TNSTR3284....1Z N
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
13788 2022-11-13 11:54:20 Kenta Taguchi Kenta Taguchi (Kyoto University), Masaaki Otsuka (Kyoto University) None Nova 1 Though the signal-to-noise ratio is small, the H alpha and H beta lines of FWZI ~ 50 A are seen in our spectrum, and therefore this object is likely the recurrent outburst of M31N 1984-07a = 2004-11f = 2012-09a. Another spectrum with less noise is expected. 2022TNSCR3298....1T
Spectra
ID Obs-date (UT) Tel / Inst Exp-Time Observer/s Reducer/s Group Spectrum ascii file Spectrum fits file Spec. Type Assoc. Groups End prop. period Remarks
13862 2022-11-12 15:19:26 Other / Other 750 Kenta Taguchi, Masaaki Otsuka Kenta Taguchi None tns_2022zyr_2022-11-12_15-19-26_Other_Other.dat tns_2022zyr_2022-11-12_15-19-26_Other_Other.fits Object We performed the follow-up spectroscopic observation using the KOOLS-IFU attached to the 3.8-m Seimei telescope at Okayama Observatory. The spectral resolution is ~ 500 and the wavelength coverage is 4100-8900 A. The weather was partially cloudy.

Comments

Jozsef
Vinko

The correct discovery date

The correct discovery date for AT report #164198 is 2022-11-12 16:39:08 UT.  Sorry for the typo.