RA/DEC (2000)
00:42:39.280 +41:15:16.90
10.663667 +41.254694
Type
Nova
Redshift
Reporting Group
None
Discovering Data Source
None
Discovery Date
2022-07-14 05:05:35.000
TNS AT
Y
Public
Y
Host Name
M31
Discovery Mag
17.6
Filter
Clear-
Reporter/s
Filipp Romanov

Spectra

 AT_2022ouu - 2022-08-04 03:58:02 LT / SPRAT (F. D. Romanov)z=
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   Binning factor: (rounded to nearest integer >1)
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Light curves

 LT_IO-O_r
 LT_SPRAT_Clear
 Other_Other_G
 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
13145 2022-08-04 03:58:02 LT / SPRAT 1800 Robotic; requested by Filipp Romanov Reduced by Andrea Pastorello (INAF-OAPd); calibrated by Filipp Romanov F. D. Romanov tns_2022ouu_2022-08-04_03-58-02_LT_SPRAT_F._D._Romanov.txt tns_2022ouu_2022-08-04_03-58-02_LT_SPRAT_F._D._Romanov.fits Object
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
r-Sloan LT_IO-O 2022-07-19 03:30:21 - 2022-07-19 03:30:21 2459779.6460764 - 2459779.6460764 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
299035 2022-07-19 03:30:21 2459779.6460764 17.12 0.05 ABMag r-Sloan LT_IO-O 60 F. D. Romanov
Clear- LT_SPRAT 2022-08-04 03:39:53 - 2022-08-04 03:39:53 2459795.6526968 - 2459795.6526968 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
299036 2022-08-04 03:39:53 2459795.6526968 17.9 0.05 VegaMag Clear- LT_SPRAT 50 F. D. Romanov
G-Gaia Other_Other 2022-07-16 03:19:16 - 2022-07-16 03:19:16 2459776.6383796 - 2459776.6383796 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
292914 2022-07-16 03:19:16 2459776.6383796 17.1 ABMag G-Gaia Other_Other 300 F. D. Romanov 0.355-m f/6.2 Schmidt-Cassegrain telescope + CCD
Clear- Other_Other 2022-07-10 04:53:27 - 2022-07-14 05:05:35 2459770.7037847 - 2459774.7122106 2
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
292751 2022-07-14 05:05:35 2459774.7122106 17.6 VegaMag Clear- Other_Other 300 F. D. Romanov
292750 2022-07-10 04:53:27 2459770.7037847 19 VegaMag Clear- Other_Other 300 F. D. Romanov [Last non detection]
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
155325 2022-08-21 16:06:44 Filipp Romanov Filipp Romanov et al. F. D. Romanov F. D. Romanov 00:42:39.280 +41:15:16.70 2022-07-19 03:30:21.000 17.12 r-Sloan PNV M31 PNV J00423928+4115169, Romanov N1 F. D. Romanov Follow-up observations of AT 2022ouu = PNV J00423928+4115169 taken remotely using 2-m robotic Liverpool Telescope (La Palma, Spain). The combined light curve (from July 14 to August 4, 2022) is also uploaded to the TNS. The position has been updated. N
Related files
File Comments Last Modified (UT) Modified By
tns_2022ouu_atrep_155325_F._D._Romanov.jpg 60-sec. image taken remotely using 2-m robotic Liverpool Telescope (La Palma, Spain) with IO:O camera and Sloan r' filter. 2022-08-21 16:06:44 Filipp Romanov
tns_2022ouu_atrep_155325_F._D._Romanov_0.jpg Combined light curve for AT 2022ouu = PNV J00423928+4115169 from July 14 to August 4, 2022. The data was received remotely using telescopes: 0.61-m f/6.5 corrected Dall-Kirkham of Burke-Gaffney Observatory in Canada; 0.355-m f/6.2 Schmidt-Cassegrain of Abbey Ridge Observatory in Canada; 0.50-m f/6.8 reflector + f/4.5 focal reducer (T11) and 0.43-m f/6.8 reflector + f/4.5 focal reducer (T21) of iTelescope.Net in the USA; 2-m f/10 Liverpool Telescope (La Palma, Spain) - using IO:O camera and camera of the SPRAT. 2022-08-21 16:06:44 Filipp Romanov
152388 2022-07-16 19:01:34 Filipp Romanov Filipp Romanov et al. F. D. Romanov F. D. Romanov 00:42:39.300 +41:15:17.10 2022-07-16 03:19:16.000 17.1 G-Gaia PNV M31 PNV J00423928+4115169, Romanov N1 Follow-up observation of AT 2022ouu = PNV J00423928+4115169 remotely using 0.355-m f/6.2 Schmidt-Cassegrain telescope of Abbey Ridge Observatory (Lane, 2018, RTSRE, 1, 119) in Canada. N
Related files
File Comments Last Modified (UT) Modified By
tns_2022ouu_atrep_152388.jpg Stacked color image (Rc for red, V for green, B for blue) from 300-sec. photos taken remotely using 0.355-m f/6.2 Schmidt-Cassegrain telescope of Abbey Ridge Observatory, Canada. 2022-07-16 19:01:35 Filipp Romanov
152316 2022-07-14 12:22:26 Filipp Romanov Filipp Romanov et al. F. D. Romanov F. D. Romanov 00:42:39.280 +41:15:16.90 2022-07-14 05:05:35.000 17.6 Clear- PNV M31 PNV J00423928+4115169, Romanov N1 Probable nova discovered during the search for novae in M31 remotely using 0.61-m f/6.5 corrected Dall-Kirkham robotic telescope (Lane, 2018, RTSRE, 1, 119) of Burke-Gaffney Observatory (BGO) in Saint Mary's University (Halifax, Nova Scotia, Canada) with Astrodon Luminance filter. Visible in three images taken on July 14, 2022. 2022TNSTR1975....1R N
Related files
File Comments Last Modified (UT) Modified By
tns_2022ouu_atrep_152316.jpg Stacked (3x300 sec.) images from 0.61-m f/6.5 corrected Dall-Kirkham robotic telescope of Burke-Gaffney Observatory. 2022-07-14 18:26:25 Filipp Romanov
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
13073 2022-08-21 17:09:56 Filipp Romanov Filipp Romanov F. D. Romanov Nova 1 F. D. Romanov The spectrum of AT 2022ouu (PNV J00423928+4115169) was obtained at my request during 1800 seconds (PATAG proposal AZ22A01; PI: F. Romanov) on 2022-08-04, midtime 03:58:02 UT, remotely using the low resolution (approximately R = 350 = 18 Å) SPRAT spectrograph on the 2-m robotic Liverpool Telescope (La Palma, Spain) with the blue-optimised mode (grating option). The spectrum has been reduced by Andrea Pastorello (INAF-OAPd). The spectrum (calibrated by me) shows strong emission lines: Hα, Hβ, Fe II (42, 48, 49 multiplets) and Na I D (or He 5876); Fe II lines are as strong as Hβ. I measured the FWHM of the Hα line ~ 34 Å, corresponding to the velocity of ~ 1550 km/s. Based on the above, I conclude that AT 2022ouu is M31 nova of the Fe II spectroscopic type. 2022TNSCR2408....1R
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
13145 2022-08-04 03:58:02 LT / SPRAT 1800 Robotic; requested by Filipp Romanov Reduced by Andrea Pastorello (INAF-OAPd); calibrated by Filipp Romanov F. D. Romanov tns_2022ouu_2022-08-04_03-58-02_LT_SPRAT_F._D._Romanov.txt tns_2022ouu_2022-08-04_03-58-02_LT_SPRAT_F._D._Romanov.fits Object

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