
New observation and firstime supernova for me ! A light coming from 20 millons Ly !
At V mag nearly 10.5, this SN is in the range of both low and high resolution amateur spectroscopy. Cause of the doppler broadening effect, the spectral lines are very large and oversize my spectral domain, here around HeII 4686A.
But tiny lines in the spectrum maybe insterstellar and intergalactic (!) absorption useful to calculate the extinction of the supernova and then the true brightness and distance (Diffuse interstellar bands (DIB): co-planar...
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