RA/DEC (2000)
00:42:36.173 +41:17:18.08
10.6507211111 +41.2883566667
Type
Nova
Redshift
0
Discovery ReportClassification Report
Reporting Group
None
Discovering Data Source
None
Discovery Date
2023-09-29 08:36:23.040
TNS AT
Y
Public
Y
Host Name
M31
Discovery Mag
16.4
Filter
L-
Reporter/s
Yuqing Ren, Jingyuan Zhao
NEDSIMBADDECaLSPanSTARRS-1SkyMapperVizieRWISEDSSADS

Spectra

 ▌AT_2023ttu - 2023-09-29 22:40:00 Other / Other (None)z=
 ▌AT_2023ttu - 2023-09-29 15:46:14 Other / Other (None)z=
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),

Light curves

 ▌ATLAS-HKO_ATLAS-02_orange_
 ▌Other_Other_L_
 ▌Other_Other_R_
 ▌Other_Other_V_
   
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
15758 2023-09-29 22:40:00 Other / Other 5400 Claudio Balcon Claudio Balcon None tns_2023ttu_2023-09-29_22-40-00_Other_Other.dat tns_2023ttu_2023-09-29_22-40-00_Other_Other.fit Object We obtained the low-resolution spectrum using the FOSC-ES32 spectrograph attached to a 0.41m telescope, in the course of Italian Supernovae Search Project.
15760 2023-09-29 15:46:14 Other / Other 2700 Kenta Taguchi Kenta Taguchi None tns_2023ttu_2023-09-29_15-46-14_Other_Other.dat tns_2023ttu_2023-09-29_15-46-14_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, Kyoto University. The spectral resolution is ~ 500, and the wavelength coverage is 4100-8500 A.
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
orange-ATLAS ATLAS-HKO_ATLAS-02 2023-09-28 13:03:42 - 2023-09-29 11:27:14 2460216.04424 - 2460216.97725 2
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
365959 2023-09-29 11:27:14 2460216.97725 16.147 0.04 18.18 ABMag orange-ATLAS ATLAS-HKO_ATLAS-02 30 Robot
365958 2023-09-28 13:03:42 2460216.04424 18.71 ABMag orange-ATLAS ATLAS-HKO_ATLAS-02 30 Robot [Last non detection]
L- Other_Other 2023-08-27 00:00:00 - 2023-09-29 08:36:23 2460183.5 - 2460216.8586 2
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
365934 2023-09-29 08:36:23 2460216.8586 16.4 21 VegaMag L- Other_Other 360 Yuqing Ren, Jingyuan Zhao Image taken by the 0.61-m f/6.5 calibrated Dall-Kirkham Robotic Telescope (Lane, 2018, RTSRE, 1, 119) at the Burke-Gaffney Observatory (BGO) at St. Mary's University (Halifax, Nova Scotia, Canada), with a 360-second exposure using a LUM filter.
365933 2023-08-27 00:00:00 2460183.5 21 VegaMag L- Other_Other 360 Yuqing Ren [Last non detection] Image taken by the 0.61-m f/6.5 calibrated Dall-Kirkham Robotic Telescope (Lane, 2018, RTSRE, 1, 119) at the Burke-Gaffney Observatory (BGO) at St. Mary's University (Halifax, Nova Scotia, Canada), with a 360-second exposure using a LUM filter[Last non detection]
R-Cousins Other_Other 2023-09-28 16:57:40 - 2023-09-29 17:06:14 2460216.20671 - 2460217.21266 2
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
365987 2023-09-29 17:06:14 2460217.21266 16.1 VegaMag R-Cousins Other_Other 600 Jingyuan Zhao, Weihao Wang The image from the 0.5-m f/6.8 Lulin-ASIAA Telescope for Transients and Education (LATTE) at Lulin Observatory (D35).
365985 2023-09-28 16:57:40 2460216.20671 20.5 VegaMag R-Cousins Other_Other 600 Jingyuan Zhao, Weihao Wang [Last non detection] The image from the 0.5-m f/6.8 Lulin-ASIAA Telescope for Transients and Education (LATTE) at Lulin Observatory (D35).
V-Johnson Other_Other 2023-09-29 16:55:39 - 2023-09-29 16:55:39 2460217.20531 - 2460217.20531 1
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
365986 2023-09-29 16:55:39 2460217.20531 16.4 20.5 VegaMag V-Johnson Other_Other 600 Jingyuan Zhao, Weihao Wang The image from the 0.5-m f/6.8 Lulin-ASIAA Telescope for Transients and Education (LATTE) at Lulin Observatory (D35).
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 Bibcode Unreal Auto classification
189360 2023-09-30 02:43:36 Jingyuan Zhao Wenjie Zhou,Mi Zhang,Jingyuan Zhao and Weihao Wang et al. 00:42:36.200 +41:17:17.90 2023-09-29 16:55:38.784 16.4 V-Johnson PNV M31 We report following-up photometry and outburst upper limit for AT 2023ttu=PNV J00423617+4117178. The nova is visible on V-filter image, exposured 600-s, obtained by 0.5-m f/6.8 Lulin-ASIAA Telescope for Transients and Education (LATTE) at Lulin Observatory (D35) around 2023 Sept. 29.70531 UT, mag=16.4 V. The nova is also visible on another R-filter image taken by the same instrument (2023 Sept. 29.71266, mag = 16.1 R), but nothing is visible at this position on archival images taken on 2023 Sept. 28.69936 UT (limiting mag 20.5 V) and 2023 Sept. 28.70671 UT (limiting mag 20.5 R). N
189340 2023-09-29 14:26:10 ATLAS_Bot1 J. Tonry,L. Denneau,H. Weiland et al. ATLAS ATLAS 00:42:36.173 +41:17:18.08 2023-09-29 11:27:14.400 16.147 orange-ATLAS PSN ATLAS23tik ATLAS N
189326 2023-09-29 11:19:03 Yuqing Ren Yuqing Ren,Jingyuan Zhao et al. 00:42:36.170 +41:17:18.10 2023-09-29 08:36:23.040 16.4 L- 1 PNV M31 Image taken by the 0.61-m f/6.5 calibrated Dall-Kirkham Robotic Telescope (Lane, 2018, RTSRE, 1, 119) at the Burke-Gaffney Observatory (BGO) at St. Mary's University (Halifax, Nova Scotia, Canada), with a 360-second exposure using a LUM filter. The target is clearly visible. 2023TNSTR2437....1R N
Related files
File Comments Last Modified (UT) Modified By
tns_2023ttu_atrep_189326.jpg 2023-09-29 11:19:04 Yuqing Ren
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
15675 2023-09-30 09:48:30 Kenta Taguchi Kenta Taguchi (Kyoto University) None Nova 1 The overall spectral feature is consistent with the result reported by Claudio Balcon. Possible absorption absorption component of H alpha is seen at -3,300 km/s. 2023TNSCR2450....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
15760 2023-09-29 15:46:14 Other / Other 2700 Kenta Taguchi Kenta Taguchi None tns_2023ttu_2023-09-29_15-46-14_Other_Other.dat tns_2023ttu_2023-09-29_15-46-14_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, Kyoto University. The spectral resolution is ~ 500, and the wavelength coverage is 4100-8500 A.
15673 2023-09-29 23:52:49 Claudio Balcon Claudio Balcon (Belluno A.O. ISSP) None Nova 0 1 The low-resolution spectrum presents a strong broad emission likely associated with H-alpha. The spectrum resembles that of a Nova. 2023TNSCR2443....1B
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
15758 2023-09-29 22:40:00 Other / Other 5400 Claudio Balcon Claudio Balcon None tns_2023ttu_2023-09-29_22-40-00_Other_Other.dat tns_2023ttu_2023-09-29_22-40-00_Other_Other.fit Object We obtained the low-resolution spectrum using the FOSC-ES32 spectrograph attached to a 0.41m telescope, in the course of Italian Supernovae Search Project.

Comments

Yuqing
Ren

Fri, 09/29/2023 - 15:11

Corrected data

last undetected on 2023-08-27 08:30:53(UTC). Limit magnitude is 19.5 Mag.

TNS
System

Fri, 09/29/2023 - 13:30

Object coordinates updated

Object coordinates updated according to AT-report 189340 of Group ATLAS
Previous RA, DEC: 00:42:36.170, +41:17:18.10 (10.650708, +41.288361)
Updated RA, DEC: 00:42:36.173, +41:17:18.08 (10.6507211111, 41.2883566667)