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Table 3.

SN type at initial classification (e.g., on TNS) and if different, our classification.

SN name Our TNS MJD of TNS Phase (a) (days) of Reference for initial classification
classification classification classification spectrum TNS
classification
spectrum
SN 2023ljf Ib Ib 60118.40 −14.5 Pellegrino et al. (2023)

SN 2022nyo IIb -> Ib (b) Ib 59761.03 −15.9 Pearson et al. (2022b)

SN 2021ukt IIn -> Ib (c) IIn 59427.58 −14.1 Hinkle (2021)

SN 2021njk Ib Ib-pec 59364.41 −11.3 Hiramatsu et al. (2021)

SN 2021hen Ib I 59303.54 −8.2 Pellegrino et al. (2021)
Ib 59306.00 −5.7 Sollerman (2022)

SN 2020hvp Ib Ib 58962.74 −13.2 Burke et al. (2020)
Ib 58964.35 −11.6 Dahiwale & Fremling (2020)

SN 2019odp Ic-bl -> Ib (d) Ic-bl 58718.22 −17.0 Brennan et al. (2019)
Ic-bl 58719.89 −15.3 Fremling et al. (2019)
Ib 58759.93 24.7 Schweyer et al. (2024a)

SN 2016bau Ib Ib 57461.97 −16.2 Benetti et al. (2016)

Notes.

(a)

Phases are calculated with reference to the V-band maximum light.

(b)

Based on our spectra, SN 2022nyo transitioned from a SN IIb to a SN Ib between tVmax = −13.8 and −4.1 days (see Table B.1).

(c)

Based on our spectra, SNID identified SN 2021ukt as a SN IIn at tVmax = −12.2 days, but as a SN Ib for the subsequent spectrum at tVmax = −9.1 days (see Table B.1). Nevertheless, we note that for many of its spectra, SN 2021ukt seems to have simultaneous SNe Ib- and SN IIn-like features, which has never been seen before-see Section 4.3.

(d)

Based on our spectra, SN 2019odp transitioned between a SN Ic-bl and a SN Ib between tVmax = −2.7 and 1.4 days (see Table B.1).

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