Key points are not available for this paper at this time.
Cepheid variables with periods from 2 to more than 50 days have been found in IC 4182 from observations with the Hubble Space Telescope over a time interval of 47 days, comprised of 20 epochs. The period-luminosity relation from photometry of 27 Cepheids in the F555W HST magnitude system gives an apparent V distance modulus of (m - M) AV_ = 28. 47 +/- 0. 08. The absolute magnitude of the type Ia supernova 1937C is MV_ (max) = - 19. 92 +/- 0. 13 from these data. Combining this with the Hubble diagram for SN Ia gives a Hubble constant of H₀_= 45 +/- 9 km s^-1^ Mpc^-1.
Sandage et al. (Tue,) studied this question.