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SN 2022eyw

Right ascension (α)
190.99987583 Degree
Declination (δ)
62.33008111 Degree
Distance (d)
41.86301370 Mpc Calculated from recession velocity using H₀ = 73 km/s/Mpc.
Recession velocity (vrec)
3056 Kilometres per second Virgo infall + Great Attractor corrected
Redshift (z)
0.01019372
Photometry
Yes · 288 points
Spectra
5 spectra

Measurements

Each column groups the values reported together by one source entry. Empty cells mean that source did not report that property.

Property Das et al. (2025)
Host galaxy reddening (E(B−V)host) 0.05600000 Magnitude
Milky Way reddening (E(B−V)MW) 0.01200000 Magnitude
Absolute peak magnitude — B band (MB) Johnson filter system -17.61000000 Magnitude ± 0.15000000 Magnitude
Absolute peak magnitude — r band (Mr) Sloan filter system -17.90000000 Magnitude ± 0.15000000 Magnitude
Absolute peak magnitude — V band (MV) Johnson filter system -17.79000000 Magnitude ± 0.15000000 Magnitude
Apparent peak magnitude — B band (mB) Johnson filter system 15.71000000 Magnitude ± 0.02000000 Magnitude
Apparent peak magnitude — r band (mr) Sloan filter system 15.32000000 Magnitude ± 0.01000000 Magnitude
Apparent peak magnitude — V band (mV) Johnson filter system 15.47000000 Magnitude ± 0.02000000 Magnitude
Decline over 15 days — B band (Δm15(B)) Johnson filter system 1.46000000 Magnitude
Decline over 15 days — r band (Δm15(r)) Sloan filter system 0.62000000 Magnitude
Decline over 15 days — V band (Δm15(V)) Johnson filter system 0.85000000 Magnitude
Explosion time (texp) 59658.89000000 Day
Ejecta mass (Mej) 0.79000000 Solar mass
Nickel mass (MNi) 0.11000000 Solar mass
Peak bolometric luminosity (Lbol) 5.52000000 10^42 erg per second
Rise time (trise) 18.75000000 Day

Light curve

Observed magnitude by reported observation time. Axis labels identify the displayed time and magnitude systems; brighter measurements appear at the top.

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Spectrum

Compare up to 10 selected full-resolution observed spectra on one chart. Raw flux is shown by default; normalization is an explicit display option.

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Move across the chart to inspect the nearest point in each selected spectrum.
Flux display Normalization divides each spectrum by its maximum absolute reported flux.