A test of Tully-Fisher distance estimates using Cepheids and SNIa
Cepheid Distances to SNe Ia Host Galaxies Based on a Revised Photometric Zero Point of the HST WFPC2 and New PL Relations and Metallicity Corrections
Discovery of Cepheids in IC 4182: Absolute Peak Brightness of SN IA 1937C and the Value of H 0
On the Automatic Determination of Light-Curve Parameters for Cepheid Variables
Reddening, Absorption, and Decline Rate Corrections for a Complete Sample of Type Ia Supernovae Leading to a Fully Corrected Hubble Diagram to v < 30,000 km s-1
The Brightest Stars in Nearby Galaxies IX: Comparison of Ground-Based and HST Photometry of the Brightest Stars in IC 4182
The Cepheid Distance to IC 4182: Calibration of M V(max) for SN IA 1937C and the Value of H 0
The Environments of Supernovae in Archival Hubble Space Telescope Images
The Hubble Constant: A Summary of the Hubble Space Telescope Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
Instrument
WFPC/WFC
Temporal Coverage
1992-01-27T02:47:17Z/1992-03-13T06:19:57Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Sandage et al., 1993, 'CALIBRATION OF SUPERNOVAE OF TYPE I AS STANDARD CANDLES', 1.0, European Space Agency, https://doi.org/10.5270/esa-2288wue