Mario Hamuy, Carnegie Observatories, reports that a spectrum (range 360-900 nm)
of SN 2002fi, obtained on Sept. 26.29 UT with the Las Campanas Baade 6.5-m
telescope (+ LDSS-2), shows it to be a type-Ia supernova.
The spectrum bears strong resemblance to SN 1994D 20 days past maximum.

I obtained a spectrum of SN 2002fj with the same instrument on Sep. 26.39.
This supernova is of Type II-n. The spectrum is dominated by a strong
H alpha emission line of intermediate (700 km/s) width without appreciable
Doppler shift relative to the host galaxy. This emission is
superposed on a broad component. No signs of He I lines are present.