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
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
H 0 Tension and the Phantom Regime: A Case Study in Terms of an Infrared f(T) Gravity
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
Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant
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
Vetting Galactic Leavitt Law Calibrators Using Radial Velocities: On the Variability, Binarity, and Possible Parallax Error of 19 Long-period Cepheids
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2016-08-09T09:12:04Z/2017-07-16T05:07:14Z
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 et al., 2018, 'A New Threshold of Precision, 30 micro-arcsecond Parallaxes and Beyond', 1.0, European Space Agency, https://doi.org/10.5270/esa-6fujryc
