DRAFT
2024-11-07 17:21:25
Type: Object/s-Discovery/Classification
ePESSTO+ spectroscopic classification of optical transients
Authors: K. Tsalapatas, Y. Hu, P. J. Pessi, A. Gangopadhyay, A. Singh, A. Gkini, J. Sollerman, S. Barmentloo (Stockholm), T. Kravtsov (Turku), G. Pignata (UTA), J. Anderson (ESO), T.-W. Chen (NCU), M. Gromadzki (Warsaw), C. Inserra (Cardiff), E. Kankare (Turku), T. Müller Bravo (Trinity), O. Yaron (Weizmann), D. Young (QUB), S. Benetti (INAF), N. Ihanec (ING,Warsaw), E. Zimmerman (Weizmann), Asaf Horowicz (Weizmann), J. Tonry, L. Denneau, H. Weiland, A. Lawrence, R. Siverd (IfA, University of Hawaii), N. Erasmus, W. Koorts (South African Astronomical Observatory), A. Jordan, V. Suc (UAI, Obstech), S. J. Smartt (Oxford/QUB), K. W. Smith, S. Srivastav, D. R. Young, M. Fulton, M. McCollum, T. Moore, M. Nicholl, J. Weston (QUB), L. Shingles (GSI/QUB), L. Rhodes (Oxford), J. Sommer (LMU/QUB), A. Rest (STScI), C. Stubbs (Harvard)
Source Group: ePESSTO+
Abstract:
This report includes classifications of 6 Type Ia SNe, 1 Type II SN, 1 AGN and 1 blue featureless transient.

ePESSTO+, the advanced Public ESO Spectroscopic Survey for Transient Objects (Smartt et al. 2015 2015A&A...579A..40S), reports the following supernova classifications.

Targets were supplied by the ATLAS survey (Smith et al. 2020 2020PASP..132h5002S), the Zwicky Transient Facility ZTF (Bellm et al. 2019 2019PASP..131a8002B) - data stream processed through the Lasair broker (Smith, Williams, Young et al. 2019 2019RNAAS...3...26S) and by the ALeRCE broker (Forster et al. 2020 2021AJ....161..242F) and by the Gravitational-wave Optical Transient Observer GOTO (see Dyer et al. 2020, SPIE, 11445 2020SPIE11445E..7GD).

Observations were performed on the ESO New Technology Telescope (NTT) at La Silla on the night of 2024 Nov 6, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution).Classifications were done using SNID (Blondin & Tonry 2007 2007ApJ...666.1024B), GELATO (Harutyunyan et al. 2008 2008A&A...488..383H) and NGSF (Next Generation SuperFit; AstroNote 2022-191, Howell et al. 2005 2005ApJ...634.1190H).

The classification spectra and additional details can be obtained from http://www.pessto.org (via WISeREP) and the IAU Transient Name Server.

The classified objects are listed in the Related Objects table below.

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2024aalt [ATLAS24pyg] 23:23:33.532 +08:18:37.92 SN Ia 0.051 WISEA J232333.68+081838.4 Redshift from SNID 23:23:33.539 +08:18:37.75 SN Ia 0.051
TNS 2024zkr [ZTF18abuxiwj] 01:54:22.956 -05:59:50.42 AGN 0.078 SDSS J015422.95-055950.7 Redshift from the host lines. The spectrum shows Bowen fluorescence lines N III and He II. Potentially a TDE-Bowen. 01:54:22.960 -05:59:50.60 AGN 0.078
TNS 2024zzh [ZTF24abpzvqo] 23:05:56.647 -10:49:49.96 SN Ia 0.08 2MASX J23055627-1049491 Redshift from SNID 23:05:56.651 -10:49:50.13 SN Ia 0.08
TNS 2024aall [ZTF24abprrom] 22:30:50.578 -21:28:52.79 SN Ia 0.07 WISEA J223050.73-212853.9 Redshift form NGSF 22:30:50.578 -21:28:52.79 SN Ia 0.07
TNS 2024aaoh [ZTF24abqxysf] 22:55:19.455 -19:28:28.45 0.08 WISEA J225519.46-192828.1 Redshift from host lines. Blue featureless transient. 22:55:19.455 -19:28:28.45 0.08
TNS 2024zvt [ATLAS24pwa] 23:14:52.957 -11:57:53.73 SN Ia 0.087 WISEA J231453.44-115741.9 0.086637 Redshift from host galaxy 23:14:52.954 -11:57:53.92 SN Ia 0.087
TNS 2024zol [GOTO24hnq] 06:45:33.700 -42:55:38.21 SN Ia 0.033 WISEA J064528.52-425554.6 0.03317 Redshift from host galaxy 06:45:33.700 -42:55:38.10 SN Ia 0.033
TNS 2024zvx [ATLAS24pwf] 10:01:05.223 -85:45:45.46 SN Ia 0.064 WISEA J100110.81-854550.3 Redshift from NGSF 10:01:05.223 -85:45:45.46 SN Ia 0.064
TNS 2024ydr [ZTF18adowxvg] 08:22:10.666 +03:16:04.71 SN II 0.014 IC 0503 0.013756 Redshift from host galaxy 08:22:10.666 +03:16:04.71 SN IIP 0.01376

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