Mario Hamuy (Carnegie Observatories) reports spectroscopic observations
made by Jose Maza (U. Chile) and Mark Phillips (Carnegie Observatories) 
on Nov. 28-29 UT with the Las Campanas Observatory Baade 6.5-m telescope and 
B&C spectrograph in the wavelength range 320-920 nm.  A spectrum of SN 2002jh
obtained on Nov. 28.23 UT shows it to be a Type-Ia supernova about 10 days 
past maximum at an approximate redshift of 0.048.  A spectrum of SN 2002jf
obtained on Nov. 28.19 UT reveals this object to be a Type Ia event 2-3 weeks 
after maximum at a redshift of 0.079 measured from the host galaxy.
A spectrum of SN 2002ib obtained on Nov. 29.10 UT shows it to be a Type Ia 
about 10 days after maximum.  Superimposed narrow emission lines yield a 
redshift of 0.068.  A spectrum of SN 2002ic obtained on Nov. 29.11 UT
reveals it to be a Type Ia with strong Fe III absorption features and a weak 
Si II 635.5 nm line, similar to the peculiar SN 1999ac near maximum light. 
Superimposed narrow emission lines yield a redshift of 0.066.  Finally, a 
spectrum of SN 2002ia obtained on Nov. 29.13 UT shows it to be a Type Ia 
about 2-3 weeks after maximum at an approximate redshift of 0.072.