We report the observation of 7 transients using the Kast Double Spectrograph on the 3.05 meter C. Donald Shane telescope at the Lick observatory. Observations were obtained between MJD 60699.10 and MJD 60700.51.
On the red side detector the 300/7500 grating was used, which has a dispersion of 2.55 Å/pixel. On the blue side the 600/4310 grism was used, which has a dispersion of 1.02 Å/pixel. A slit width of 1.5" was used for all observations. Part of 2024abpg/ZTF24abtejwy's observation sequence was mistakenly observed with a 0.5" slit width before we switched back to 1.5". Spectra were reduced using the UCSC Spectral Pipeline (Siebert et al. 2019). A spectral range of approximately 3470-10590 Å was obtained for the reduced spectra.
Of these 14 transients new classifications were found for 10 events, which includes 1 infant SN II, 2 SLSN-I, 6 SN Ia and 1 SN Ia-CSM. Our observations also support pre-existing classifications of 1 SN Ic, 1 SN Ia and 2 SN II. Classifications were performed by fitting observations to template spectra from previously classified transients using Next Generation Superfit (NGSF, Goldwasser et al. 2022) and manual inspection of line profiles.
Details of each observed transient are summarised in the "Related Objects" table. Our NGSF fits, plots of spectra which we classified manually, and spectral files for transients which we have not classified submitted a classification report for on TNS have been included in this Astronote.
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 |
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TNS | 2025adj [ATLAS25awc] | 14:59:44.474 | +51:27:46.98 | SN II | 0.011389 | KUG 1458+516 | 0.011389 | First discovered by the ATLAS survey on MJD 60699.61 and reported as a candidate supernova in AstroNote #2025-35. We observed a blue, mostly featureless spectrum consistent with it being a young SN II. Redshift of z = 0.011389 ± 0.000023 from SDSS DR13. | 14:59:44.465 | +51:27:47.06 | SN II | 0.011389 |
TNS | 2024aezo [ATLAS24rwd] | 13:24:17.079 | +27:43:01.10 | SLSN-I | 0.4227 | SSTSL2 J132417.09+274301.7 | 0.4227 | ZTF internal name = ZTF24abwsvtj. Spectrum is well-fit to template spectra of the SLSN-I events iPTF13ajg, PTF12dam, PTF10aagc and PTF09cnd. Its lightcurve appears to be at a peak of g~19.1 in ZTF, which corresponds to a rest-frame peak absolute magnitude of M_u ~ -22.4 when applying a 2.5log10(1+z) K-correction. Reported as a hostless transient candidate by ELEPHANT in AstroNote #2025-6. We note that the host was imaged within the Subaru Deep Field. MMT/Hectospec and Keck/DEIMOS spectroscopic observations were taken by Chun Ly et at. 2016 between April 11 2008 and March 17 2015, in which they measure a redshift of z = 0.4227. | 13:24:17.066 | +27:43:01.14 | SLSN-I | 0.4227 |
TNS | 2024xsk [ZTF24ablestl] | 11:18:11.786 | +26:03:23.40 | SLSN-I | 0.1686 | RCS 04200003884 | Spectrum is well-fit to template spectra of the SLSN-I events SN2011ke, LSQ14an, SN2015bn, SN2003jd and SN2010md. Redshift obtained using host galaxy H-alpha and [OIII] emission lines. | 11:18:11.786 | +26:03:23.40 | SLSN-I | 0.1686 | |
TNS | 2024abpg [ZTF24abtejwy] | 00:14:17.798 | +03:25:49.24 | SN Ia-CSM | 0.154 | WISEA J001417.80+032551.3 | Reported as a ZTF superluminous supernova candidate in AstroNote #2025-34. Spectrum is well-fit to template spectra of the SN Ia events SN2012Z, PTF10ops, SN2005hk and SN2002cx. Its lightcurve rises slowly in ZTF, with a ~40 observed day rise time to peak from first detection. These factors, combined with visible broad wings to its H-alpha profile, motivate us to classify this event as an SN Ia-CSM. Redshift obtained using H-alpha emission in observed spectrum. | 00:14:17.798 | +03:25:49.24 | SN Ia-CSM | 0.154 | |
TNS | 2025li [ZTF25aabegog] | 12:45:55.093 | +17:29:35.35 | SN Ia | 0.079202 | WISEA J124555.09+172932.3 | 0.079202 | Spectrum is well-fit to the template spectra of the SN Ia-norm events SN2011by, SN2011fe and SN2012ht. Redshift of z = 0.079202 ± 0.000008 from SDSS DR13 | 12:45:55.093 | +17:29:35.35 | SN Ia | 0.079202 |
TNS | 2024aglr [ZTF25aaaalin] | 23:07:57.896 | +25:03:40.97 | SN Ia | 0.0414 | WISEA J230758.02+250343.3 | Spectrum is well-fit to template spectra to the SN Ia-norm events SN2012cg, SN2012fr, SN2012ht and SN2015N. Redshift from host galaxy H-alpha emission. | 23:07:57.908 | +25:03:40.95 | SN Ia | 0.0414 | |
TNS | 2025kl [ZTF25aabowed] | 01:11:52.757 | +20:23:57.13 | SN Ia | 0.058 | SDSS J011152.60+202358.9 | Spectrum is well-fit to template spectra of the SN Ia-norm events SN2012cg, SN2011by, SN2011fe and SN2012fr. Redshift of z = 0.058 ± 0.003 found from NGSF template fits. | 01:11:52.757 | +20:23:57.13 | SN Ia | 0.058 | |
TNS | 2025jx [ZTF25aabovpf] | 03:03:50.453 | -00:12:13.25 | SN Ia | 0.027605 | IC 0283 | 0.027605 | Spectrum is well-fit to template spectra of the SN Ia-norm events SN2012ht, SN2011fe, SN2011by, SN1994D and SN2012cg. Redshift of z = 0.027605 ± 0.000012 from SDSS DR13. | 03:03:50.453 | -00:12:13.25 | SN Ia | 0.027605 |
TNS | 2025hf [ZTF25aabmhdd] | 12:29:16.826 | +05:04:04.41 | SN Ia | 0.0718 | SDSS J122916.88+050404.2 | Spectrum is well-fit to template spectra of the SN Ia events SN2011by, SN2013dy, SN1999aa, SN2012cg and SN2011fe. Our classification is in agreement with the ePESSTO+ SN Ia classification from AstroNote #2025-39. Redshift obtained using host galaxy H-alpha emission. | 12:29:16.826 | +05:04:04.41 | SN Ia | 0.07 | |
TNS | 2025kd [ZTF25aabpoxz] | 05:45:53.157 | -25:53:17.05 | SN Ia | 0.0425 | 2MASS J05455310-2553158 | Spectrum is well-fit to template spectra of the SN Ia events SN2015ac, SN2012ht, SN2012cg, SN2015N and PTF10ops. Redshift found using host-galaxy Na D absorption. | 05:45:53.157 | -25:53:17.05 | SN Ia | 0.0425 | |
TNS | 2025iv [GOTO25ft] | 02:07:27.256 | +19:11:36.88 | SN Ic | 0.0173 | CGCG 461-046 | ZTF internal name = ZTF25aabobjw. Spectrum is well-fit to SN Ic template spectra from the SN Ic events SN2007gr, SN1994I and SN2007ce. We also find good fits to the Ca-Ia SN2019ofm and the Ia 91bg-like SN2016ije. Our classification and redshift broadly agree with the SN Ic classification from ePESSTO+ in AstroNote #2025-30. | 02:07:27.256 | +19:11:36.88 | SN Ic | 0.0173 | |
TNS | 2025dc [ZTF25aaapkzn] | 09:53:46.435 | -08:18:09.09 | SN II | 0.047 | WISEA J095346.29-081821.6 | Spectrum displays a broad H-alpha P-Cygni profile characteristic of a SN II, with narrow host H-alpha emission at z = 0.047. Our classification and redshift agree with those found by ePESSTO+ in AstroNote #2025-36 | 09:53:46.435 | -08:18:09.09 | SN II | 0.047 | |
TNS | 2025ei [ATLAS25agn] | 11:44:47.403 | +19:46:24.38 | SN II | 0.028247 | NGC 3860B | 0.028247 | ZTF internal name = ZTF25aabskal. Spectrum shows H-alpha and H-beta P-cygni features characteristic of a SN II. Our classification agrees with with pre-existing TNS classification from SCAT, and ePESSTO+ in AstroNote #2025-8. Host redshift of 0.028247 ± 0.000008 from SDSS DR13. | 11:44:47.404 | +19:46:24.36 | SN II | 0.03 |
TNS | 2025ky [ZTF22ablqzpz] | 10:02:49.869 | -05:51:12.65 | SN Ia | 0.0828 | WISEA J100249.83-055112.0 | Spectrum is low S/N due to high altitude clouds present during observation. We find tentative fits to template spectra from the SN Ia events SN2013dy, SN1999aa, PTF10ops and SN2009dc. We also find a tentative fit to the SN Ic-BL SN1998bw. Our fits are in broad agreement with the SN Ia classification found by ePESSTO+ in AstroNote #2025-39. Host redshift of z = 0.0828 ± 0.0004 from The 2dF Galaxy Redshift Survey: Final Data Release. | 10:02:49.869 | -05:51:12.65 | SN Ia | 0.0828 |
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