DRAFT
2025-08-09 18:03:00
Type: Object/s-Discovery/Classification
Bibcode: 2025TNSAN.248....1D
ePESSTO+ spectroscopic classification of optical transients
Authors: J. N. D. van Dalen (Radboud), D. B. Malesani (DAWN/NBI Radboud), G. Corcoran (UCD) , L. Cotter (UCD), A. Martin-Carrillo (UCD), L. Galbany (IEEC-CSIC), T. Petrushevska (Nova Gorica), S. Srivastav (Oxford), O. Yaron (Weizmann), C. Gutiérrez (IEEC-CSIC), J. Anderson (ESO), T. Müller Bravo (Southampton), T.-W. Chen (NCU), M. Gromadzki (Warsaw), C. Inserra (Cardiff), E. Kankare (Turku), M. Nicholl (QUB), D. Young (QUB), J. Tonry, L. Denneau, H. Weiland, R. Siverd (IfA, University of Hawaii), N. Erasmus, W. Koorts (South African Astronomical Observatory), A. Jordan, V. Suc (UAI, Obstech), S. J. Smartt, K. W. Smith (Oxford/QUB), H. Stevance (Oxford), M. Fulton, M. McCollum, T. Moore, J. Weston (QUB), L. Shingles (GSI/QUB), L. Rhodes (Oxford), J. Sommer (LMU/QUB), A. Rest (STScI), C. Stubbs (Harvard)
Source Group: ePESSTO+
Keywords: Transient, Supernova, Optical, Spectroscopy
Abstract:
This report includes classifications of 3 Type Ia's, two Type II's and a featureless continuum.

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), the All Sky Automated Survey for SuperNovae ASAS-SN (see Shappee et al. 2014 2014ApJ...788...48S), and 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 2025 August 8, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution). Classifications were done using SNID (Blondin & Tonry 2007 2007ApJ...666.1024B) 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 2025svw 15:59:09.659 +26:35:19.31 SN Ia 0.088 Redshift from SNID 15:59:09.652 +26:35:19.34 SN Ia 0.088
TNS 2025spw 21:32:12.672 +21:30:49.02 SN II 0.021 21:32:12.672 +21:30:49.02 SN II 0.021
TNS 2025tfy 01:55:03.397 -81:37:19.20 SN Ia 0.072 Redshift from SNID 01:55:03.397 -81:37:19.20 SN Ia 0.072
TNS 2025sok 04:48:38.182 -37:17:03.07 SN Ia 0.077 Redshift from SNID 04:48:38.182 -37:17:03.07 SN Ia 0.077
TNS 2025ruw 20:45:09.312 +23:23:53.20 NA/Unknown 0.072 Featureless continuum with a strong H-alpha used to derive redshift. 20:45:09.312 +23:23:53.20 SN IIn 0.072
TNS 2025rjo 13:26:35.754 -30:59:35.59 SN II 0.048 13:26:35.754 -30:59:35.59 SN II 0.048

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