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
Asteroid Trails in Hubble Space TelescopeWFPC2 Images: First Results
A test of Tully-Fisher distance estimates using Cepheids and SNIa
Determination of the Hubble constant from observations of Cepheid variables in the galaxy M96
Gone without a bang: an archival HST survey for disappearing massive stars
Nuclear star clusters in 228 spiral galaxies in the HST/WFPC2 archive: catalogue and comparison to other stellar systems
The Cepheid distance to M96 and the Hubble constant
The dispersion in the Cepheid period-luminosity relation and the consequences for the extragalactic distance scale
The extra-galactic Cepheid distance scale from LMC and Galactic period-luminosity relations
The Extragalactic Distance Scale Without Cepheids. II. Surface Brightness Fluctuations
The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXV. A Recalibration of Cepheid Distances to Type IA Supernovae and the Value of the Hubble Constant
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
WFPC2, WFPC2/PC
Temporal Coverage
1994-03-29T18:23:17Z/1995-04-06T12:59:17Z
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, TANVIR NIAL R., 1996, 'THE DISTANCE TO THE M96 GALAXY GROUP: CYCLE4 MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-19ixocy