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 Gravitational-wave Optical Transient Observer GOTO (see Dyer et al. 2020, SPIE, 11445 2020SPIE11445E..7GD) and by BlackGEM (Groot et al. 2024, arXiv:2405.18923).
Observations were performed on the ESO New Technology Telescope (NTT) at La Silla on the night of 2024 July 12, 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.
| 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 | 2024iub [ZTF24aanppvy] | 15:33:01.189 | -06:33:05.49 | SN II | 0.027 | WISEA J153301.08-063305.5 | > +20 | Redshift from the galaxy narrow emission lines. | 15:33:01.189 | -06:33:05.49 | SN II | 0.027 | ||
| TNS | 2024knu [ZTF24aaotlsk] | 15:18:04.642 | +14:23:38.61 | SN Ia-CSM | 0.15 | > +20 | Redshift from the galaxy narrow emission lines. | 15:18:04.648 | +14:23:38.54 | SN Ia-CSM | 0.15 | |||
| TNS | 2024lxq [ZTF24aasfxgh] | 15:28:12.124 | -27:28:29.21 | SN Ia | 0.08 | WISEA J152812.15-272829.0 | +11 to +20 | Redshift from the galaxy narrow emission lines. | 15:28:12.124 | -27:28:29.21 | SN Ia | 0.08 | ||
| TNS | 2024msu [ATLAS24jpj] | 21:24:24.274 | -80:59:04.04 | SN Ia | 0.06 | +11 to +20 | Redshift from spectral matching. | 21:24:24.274 | -80:59:04.04 | SN Ia | 0.06 | |||
| TNS | 2024ncd [ZTF24aatchko] | 17:02:56.209 | +29:33:12.08 | SN | SDSS J170256.23+293312.3 | 17:02:56.209 | +29:33:12.08 | SN | ||||||
| TNS | 2024nos [GOTO24dhk] | 12:51:47.022 | -38:22:51.89 | SN Ia | 0.08 | +4 to +7 | Redshift from spectral matching. | 12:51:47.022 | -38:22:51.89 | SN Ia | 0.08 | |||
| TNS | 2024num [ATLAS24klq] | 14:12:42.703 | +28:46:49.02 | SN Ia-91T-like | 0.06 | SDSS J141242.73+284647.3 | -7 to -4 | Redshift from spectral matching. | 14:12:42.710 | +28:46:48.47 | SN Ia-91T-like | 0.06 | ||
| TNS | 2024nzf [ZTF24aauerna] | 16:39:53.018 | +29:47:14.11 | SN Ia | 0.12 | SDSS J163952.93+294714.6 | -7 to -4 | Redshift from spectral matching. | 16:39:53.018 | +29:47:14.11 | SN Ia | 0.12 | ||
| TNS | 2024nzg [ZTF24aaumgko] | 15:56:22.839 | +21:35:13.28 | SN Ia | 0.1 | SDSS J155622.80+213512.3 | -7 to -4 | Redshift from spectral matching. | 15:56:22.839 | +21:35:13.28 | SN Ia | 0.1 | ||
| TNS | 2024nzk [GOTO24djx] | 01:29:03.993 | -10:32:36.00 | SN Ia | 0.12 | SDSS J012904.00-103237.2 | +4 to +7 | Redshift from spectral matching. | 01:29:03.958 | -10:32:35.96 | SN Ia | 0.12 | ||
| TNS | 2024pbb [ATLAS24kuk] | 22:42:42.127 | -16:44:57.42 | SN Ia | 0.07 | 2MASSJ22424227-1644574 | -7 to -4 | Redshift from spectral matching. | 22:42:42.120 | -16:44:57.73 | SN Ia | 0.07 | ||
| TNS | 2024pco [GOTO24dkw] | 01:57:55.737 | +13:21:38.36 | SN Ibn | 0.0443 | 2MASX J01575584+1321295 | 0.044325 | Around peak | Redshift from the host galaxy. | 01:57:55.700 | +13:21:38.92 | SN Ib-pec | 0.0443 | |
| TNS | 2024pgk [ZTF24aavapoe] | 20:34:40.358 | -04:20:40.89 | SN Ia | 0.09 | SDSS J203439.8-042034.7 | Around peak | Redshift from spectral matching. | 20:34:40.358 | -04:20:40.89 | SN Ia | 0.09 | ||
| TNS | 2024pgs [ZTF24aaupcqg] | 21:41:24.785 | -05:15:22.76 | SN Ia | 0.11 | SDSS J214124.70-051523.8 | -7 to -4 | Redshift from spectral matching. | 21:41:24.785 | -05:15:22.76 | SN Ia | 0.11 | ||
| TNS | 2024phr [ZTF24aavhvho] | 21:03:36.874 | +11:50:18.96 | SN II | 0.097 | WISEA J210337.12+115018.7 | Redshift from the galaxy narrow emission lines. | 21:03:36.874 | +11:50:18.96 | SN II | 0.097 | |||
| TNS | 2024pid [BGEM J004734.42-251926.3] | 00:47:34.420 | -25:19:26.35 | Nova | 0.0008 | NGC 0253 | 0.0008 | Redshift from the host galaxy (NGC 253). The current absolute magnitude of the transient is around -8 mag. | 00:47:34.420 | -25:19:26.35 | Nova | 0.0008 | ||
| TNS | 2024pii [ZTF24aauuybw] | 20:59:06.144 | -03:13:48.02 | SN Ia | 0.1 | SDSS J205906.12-031348.4 | +4 to +7 | Redshift from spectral matching. | 20:59:06.144 | -03:13:48.02 | SN Ia | 0.1 | ||
| TNS | 2023zkd [ZTF23aasnwva] | 15:48:47.536 | +09:12:00.28 | SN Ibn | 0.056 | SDSS J154847.49+091200.8 | Redshift from SN emission lines. Long lived light curve. The spectrum shows prominent Balmer lines. | 15:48:47.546 | +09:12:00.14 | SN Ibn | 0.056 |


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