A 0.9% calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids
An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt Law
A Sub-2% Distance to M31 from Photometrically Homogeneous Near-infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
Cosmological discordances. III. More on measure properties, large-scale-structure constraints, the Hubble constant and Planck data
Interacting dark energy in a closed universe
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond LCDM
On the Color-Metallicity Relation of the Red Clump and the Reddening toward the Magellanic Clouds
Spectral energy distributions of classical Cepheids in the Magellanic Clouds
Instrument
WFC3/IR, WFC3/UVIS
Temporal Coverage
2017-11-22T14:26:04Z/2018-12-16T05:23:52Z
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, Riess comma Adam, 2019, 'A New Threshold of Precision, 30 micro-arcsecond Parallaxes and Beyond', 1.0, European Space Agency, https://doi.org/10.5270/esa-w8f6ah4
