Mario Hamuy, Carnegie Observatories, reports that a spectrum (range 380-730 nm)
of SN 2002eq, obtained on Sept. 12.17 UT with the Las Campanas Dupont 2.5-m
telescope (+ Modular Spectrograph), shows it to be a type-Ia supernova.
The spectrum bears strong resemblance to SN 1994D 20 days past maximum.
By comparison to SN 1994D an approximate redshift of 0.088 is derived.

I obtained a spectrum of SN 2002ez with the same instrument on Sep. 12.27
which bears resemblance to the type-Ia SN 1994D 18 days past maximum.
By comparison to SN 1994D an approximate redshift of 0.043 is derived.

I obtained a spectrum of SN 2002fa with the same instrument on Sep. 12.08.
This supernova is of Type II with a broad H alpha line exhibiting a P-Cyg
profile. The minimum of the absorption component yields an expansion
velocity of 8100 km/s. A spectrum of the nucleus of the host galaxy
yields a redshift of 0.060.