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SN 2008ae

Right ascension (α)
149.01333333 Degree
Declination (δ)
10.49966667 Degree
Distance (d)
127.63013699 Mpc Calculated from recession velocity using H₀ = 73 km/s/Mpc.
Recession velocity (vrec)
9317 Kilometres per second Virgo infall + Great Attractor corrected
Redshift (z)
0.03107817
Photometry
Yes · 172 points
Spectra
16 spectra

Measurements

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

Property Foley et al. (2013) Hicken et al. (2012)
Milky Way reddening (E(B−V)MW) 0.02400000 Magnitude
Absolute peak magnitude — B band (MB) Johnson filter system -17.10000000 Magnitude ± 0.15000000 Magnitude
Absolute peak magnitude — r band (Mr) Sloan filter system -17.76000000 Magnitude ± 0.16000000 Magnitude
Absolute peak magnitude — V band (MV) Johnson filter system -17.53000000 Magnitude ± 0.15000000 Magnitude
Apparent peak magnitude — B band (mB) Johnson filter system 18.62000000 Magnitude ± 0.03000000 Magnitude
Apparent peak magnitude — r band (mr) Sloan filter system 17.93000000 Magnitude ± 0.05000000 Magnitude
Apparent peak magnitude — V band (mV) Johnson filter system 18.17000000 Magnitude ± 0.02000000 Magnitude
Decline over 15 days — B band (Δm15(B)) Johnson filter system 1.35000000 Magnitude
Decline over 15 days — r band (Δm15(r)) Sloan filter system 0.71000000 Magnitude
Decline over 15 days — V band (Δm15(V)) Johnson filter system 0.94000000 Magnitude
Photometric blueshift (vph) -9000 Kilometres per second
Spectral-line blueshift — Si II (vSi II) -6100 Kilometres per second

Light curve

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

Chart data loads when this section becomes visible.

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.

Spectrum choices load when this section becomes visible.

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.