DRAFT
2025-01-08 16:24:28
Type: Object/s-Discovery/Classification
Bibcode: 2025TNSAN...7....1R
ePESSTO+ spectroscopic classification of optical transients
Authors: F. Ragosta, I. Salmaso, S. Benetti, R. Carini, A. Melandri (INAF), C. Gutierrez (ICE-CSIC), A. Kumar (RHUL/Warwick), K. Tsalapatas (Stockholm Univ.), J. Anderson (ESO), T.-W. Chen (NCU), M. Gromadzki (Warsaw), C. Inserra (Cardiff), E. Kankare (Turku), T. Müller Bravo (Trinity), M. Nicholl (QUB), O. Yaron (Weizmann), D. Young (QUB), P. Pessi (Stockholm), 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, M. McCollum, T. Moore, J. Weston (QUB), L. Shingles (GSI/QUB), L. Rhodes (Oxford), J. Sommer (LMU/QUB), A. Rest (STScI), C. Stubbs (Harvard), X. Sheng, A. Aamer, C. R. Angus, D. Magill (QUB), P. Ramsden (QUB/Birmingham)
Source Group: ePESSTO+
Keywords: Transient, Supernova, Optical, Spectroscopy
Abstract:
This report includes classifications of 6 Type Ia's. We encourage follow-up observations.

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 Pan-STARRS Survey for Transients (Chambers et al. 2016 2016arXiv161205560C), 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 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 January 07, using EFOSC2 and Grism 13 (3985-9315A, 18A resolution). Classifications were done using SNID (Blondin & Tonry 2007 2007ApJ...666.1024B), and GELATO (Harutyunyan et al. 2008 2008A&A...488..383H).

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 Source Phase (days) Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2024aeyp [ATLAS24rut] 02:06:57.636 -46:03:01.13 SN Ia 0.065 close to max Redshift from NED 02:06:57.636 -46:03:01.13 SN Ia 0.065
TNS 2024afxa [ATLAS24sae] 03:23:50.382 -51:14:19.00 SN Ia 0.08 close to max Redshift from SNID 03:23:50.382 -51:14:19.00 SN Ia 0.08
TNS 2024aexl [ATLAS24rub] 06:01:06.690 -27:55:15.14 SN Ia 0.0925 ~ a week after max Object already classified (TNS Classification Report No. 20045) 06:01:06.690 -27:55:15.14 SN Ia 0.0925
TNS 2024afnp [GOTO24jpx] 07:51:48.517 +01:02:48.10 SN Ia 0.09 pre-max Redshift from SNID 07:51:48.517 +01:02:48.10 SN Ia 0.09
TNS 2024afox [ZTF24abztbsc] 08:47:05.084 -05:24:04.52 SN Ia 0.09 Halpha from host ~ a week after max Redshift from the Host 08:47:05.084 -05:24:04.52 SN Ia 0.09
TNS 2025L [PS25e] 02:31:34.366 -23:00:40.20 SN Ia 0.05 close to max Redshift from SNID 02:31:34.366 -23:00:40.20 SN Ia 0.05

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