UC Berkeley

Because Type Ia supernovae (SNe Ia) are not perfect standard candles, it is important to be able to use distance–independent observables (DIOs) to define subsets of SNe Ia that are “nearly standard candles” or to correct SN Ia absolute magnitudes to make them nearly homogeneous (“standardized candles”). This is not cruci al for the measurement of Ho but it is for the measurement of qo and of parent–galaxy peculi ar velocities. We discuss the use of various photometric and spectroscopic SN Ia DIOs, and a parent–galaxy DIO, for this purpose. We also discuss the status of the absolute–magnitude calibration of SNe Ia. We find that SNe Ia, whether calibrated by means of (1) Cepheids in their parent g al axies, (2) fitting their optical –ultraviolet spectra with detailed non-LTE model atmosphere calculations, or (3) by considering that the light curve is powered by the decay of radioactive 56Ni, firmly indicate that the value of Ho is low, less than or about 60 km s-1 Mpc-1. Some issues regarding the determination of qo by means of SNe Ia are discussed briefly. Finally, we conjecture that even if qo=0.5, there probably is no cosmic age problem.