A Hubble Space Telescope Study of Extragalactic OB Associations
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
Compact Optical Counterparts of Ultraluminous X-Ray Sources
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
`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?
Multi-Epoch Multi-Wavelength Study of an Ultraluminous X-ray Source in M101: The Nature of the Secondary
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 Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XIII. The Metallicity Dependence of the Cepheid Distance Scale
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-03-04T19:45:17Z/1995-04-17T07:57:37Z
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 - M101 CARRYOVER CYCLE 4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-drqvskd
