DRAFT
2026-05-08 11:30:46
Type: Object/s-Discovery/Classification
NOT Spectroscopic Classification of Transients
Authors: Levente Örs Benkóczy, Alma Bergström, Suhyeon Choe, Marguerite de Sainte Marie D'agneaux, Sara Kutschbach, Emma Lundqvist, Margarida Moreira Camelo Ferreira, Neo Persson, Vlad-Stefan Serbanescu, Liv Sivet, Pontus Strand, Aditya Swamy, Konstantinos Tsalapatas, Blanka Világos, Sara Ines Zamorano Chaves, Marckie Zeender, Greta Zucchi, Yang Hu, Anjasha Gangopadhyay, Avinash Singh, Jesper Sollerman, Ragnhild Lunnan (SU)
Source Group: ZTF
Abstract:
We report the spectroscopic classification of 7 transients obtained with the Nordic Optical Telescope as part of the Observational Astrophysics II course at Stockholm University.

As part of the Observational Astrophysics II course at Stockholm University (SU) we obtained spectroscopic observations of 7 transients, using the Nordic Optical Telescope (NOT) on La Palma for remote observing on May 7th 2026. Here we report the classification obtained  through spectral matching using SNID-SAGE (Stoppa F., Smartt S.~J., 2026, arXiv.2603.28741). The observations were taken with the ALFOSC instrument mounted on the NOT using Grism#4 and a 1.0 (or 1.3) arcsec wide slit. The targets reported here were supplied by the Zwicky Transient Facility (ZTF, Bellm et al. 2019). 


Below we list the classified objects. All the spectra can be accessed through the Transient Name Server and also the WISeREP repository. 

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 2026kyp [ZTF26aatidrh] 09:07:24.047 +12:24:11.80 SN Ia 0.087 SDSS J090724.21+122410.1 Matches with a Type Ia SN2008bf around maximum using SNID-SAGE. Redshift and Phase are derived from SNID-SAGE. 09:07:24.047 +12:24:11.80 SN Ia 0.087
TNS 2026iic [ZTF26aaqdhwx] 09:31:50.563 -00:02:37.62 SN Ia-CSM 0.111 LEDA 1153285 0.111093 Matches with a Type Ia-CSM SNe 2016iks and LSQ15adm using SNID-SAGE. The light curve is rising over 45 d and currently peaks at around -20.3 mag (I-band). Redshift is the catalogued spectroscopic redshift of the host LEDA 1153285. 09:31:50.563 -00:02:37.62 SN Ia-CSM 0.111
TNS 2026lap [ZTF26aaumtdl] 16:11:49.625 -12:20:03.25 SN Ia 0.042 WISEA J161149.61-122004.0 Matches with Type Ia SN2003du 7 days before maximum. Redshift and Phase are derived from SNID-SAGE 16:11:49.622 -12:20:03.31 SN Ia 0.042
TNS 2026jms [ZTF26aasygmo] 11:30:53.180 -04:21:09.35 SN IIb 0.0369 LEDA 1059440 0.0369 Matches with Type IIb 2011dh at around maximum. Redshift is the catalogued spectroscopic redshift of the host LEDA 1059440. 11:30:53.178 -04:21:09.37 SN IIb 0.0369
TNS 2026jzl [ZTF26aatbuhc] 16:40:16.563 -10:59:34.45 SN Ib 0.067 Matches peculiar Ib 2021ukt/2019odp using SNID-SAGE. Redshift derived from SNID-SAGE. 16:40:16.563 -10:59:34.45 SN Ib 0.067
TNS 2026iha [ZTF26aarorxm] 17:06:08.619 +30:34:00.57 SN IIn 0.084 Spectrum shows Halpha/Hbeta emission lines along with He II+CIII/NIII flash features at a redshift of 0.084. The light curve peaks at around -18.7 mag (r-band) with a rise time of around 30d. SNID SAGE gives matches to a Type IIn SN 2017hcc spectrum at +48 days, consistent with discovery 46 days earlier. Due to its long-lived nature, we classify it as a Type IIn, but encourage further follow-up. 17:06:08.619 +30:34:00.57 SN IIn 0.084
TNS 2026akp [ZTF26aaqklxk] 22:51:21.878 +32:21:10.23 SN II 0.0214 UGC 12218 0.021371 Matches with a Type II SN 2 months after maximum using SNID-SAGE. Redshift is the catalogued spectroscopic redshift of the host UGC 12218. 22:51:21.888 +32:21:10.22 SN II 0.0214

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