A Database of Cepheid Distance Moduli and Tip of the Red Giant Branch, Globular Cluster Luminosity Function, Planetary Nebula Luminosity Function, and Surface Brightness Fluctuation Data Useful for Distance Determinations
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 NGC 5253: Absolute Peak Brightness of SN IA 1895B and SN IA 1972E and the Value of H 0
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 Cepheid Distance to NGC 5253: Calibration of M(max) for the Type I Supernovae SN 1972E and SN 1895B
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
The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXVI. The Calibration of Population II Secondary Distance Indicators and the Value of the Hubble Constant
Instrument
WFPC/WFC
Temporal Coverage
1993-05-31T02:25:18Z/1993-07-19T14:13:56Z
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 comma Allan, 1994, 'CALIBRATION OF NEARBY GALAXY TYPE IA SUPERNOVAE AS STANDARD CANDLES: NGC 5253: CYCLE3HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-vjxrzgs