General information
SN 2026kid (ZTF26aatswhm) is reported as a Type II supernova with optical follow-up starting ~2.2 days after first detection, using small-aperture telescopes in China and Spain. The SN is detected in Luminance and Red filters and associated with the nearby galaxy NGC 5907 (distance 16.5 Mpc).
Wavelength coverage
- Optical: Luminance and Red-band imaging with reported photometry from ~2.15 to ~7.30 days after first detection.
No observations were mentioned in radio, millimeter/sub-mm, infrared, ultraviolet, X-rays, gamma-rays, or neutrinos.
Lightcurve and spectrum
Redshift
What’s special vs typical