We used the Nordic Optical Telescope (NOT), equipped with ALFOSC, to observe SN 2026naq, which had been identified as a rapidly fading transient at 100 Mpc by Srivastav et al. 2026 (AN 2026-149).
Observations started on 2026-05-22 at 21:31 UT and consisted of 2 x 1800 sec exposures with grism #4 and a 1.0 arcsec slit (wavelength coverage 3200 - 9600 Å, nominal resolution R = 360). We produced a prompt reduction of the data based on archival calibrations.
Template comparison with SNID-SAGE (Stoppa & Smartt 2026, arXiv:2603.28741) reveals that SN 2026naq is a Type II SN, with Type IIb being the preferred subtype. This classification is consistent with an early shock-cooling phase, seen in many Type IIb supernovae.
SNe IIb are a common contaminant in searches for kilonovae (Ackley et al. 2026, arXiv:2605.02639; the ENGRAVE collaboration).
| 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 | 2026naq | 12:51:56.470 | +16:16:53.47 | SN IIb | 0.021 | 12:51:56.463 | +16:16:53.32 | SN IIb | 0.021 |


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