Anisotropy in the Hubble constant as observed in the HST extragalactic distance scale key project results
Calibration of the distance scale from galactic Cepheids. I. Calibration based on the GFG sample
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
Global Properties of the Globular Cluster Systems of Four Spiral Galaxies
`Hyper-parameters approach to joint estimation: applications to Cepheid-calibrated distances and X-ray clusters
Measurement of Hubble constant: were differences in secondary distance indicators apparent as early as the HST Key Project?
Non-Gaussianity and direction-dependent systematics in HST Key Project data
Planetary Nebulae as Standard Candles. XII. Connecting the Population I and Population II Distance Scales
Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
Reconstructing a Cepheid Light Curve with Fourier Techniques. I. The Fourier Expansion and Interrelations
The dispersion in the Cepheid period-luminosity relation and the consequences for the extragalactic distance scale
The extragalactic Cepheid bias: significant influence on the cosmic distance scale
The Hubble Space Telescope Extragalactic Distance Scale Key Project. X. The Cepheid Distance to NGC 7331
The opacity of spiral galaxy disks: IX. Dust and gas surface densities
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-06-19T13:31:17Z/1995-08-17T09:49:17Z
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, Mould comma Jeremy R., 1996, 'DETERMINATION OF THE EXTRAGALACTIC DISTANCE SCALE - N7331 HOPR', 1.0, European Space Agency, https://doi.org/10.5270/esa-fe85yzb
