A BayeSN distance ladder: H0 from a consistent modelling of Type Ia supernovae from the optical to the near-infrared
A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s-1 Mpc-1 Uncertainty from the Hubble Space Telescope and the SH0ES Team
Crowded No More: The Accuracy of the Hubble Constant Tested with High-resolution Observations of Cepheids by JWST
Hubble Space Telescope Observations of Mira Variables in the SN Ia Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8s Confidence
Measurements of the Hubble Constant with a Two-rung Distance Ladder: Two Out of Three Aint Bad
Relative Intrinsic Scatter in Hierarchical Type Ia Supernova Sibling Analyses: Application to SNe 2021hpr, 1997bq, and 2008fv in NGC 3147
Spherical symmetry in the kilonova AT2017gfo/GW170817
The Early Light Curve of the Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model
The Galaxy Activity, Torus, and Outflow Survey (GATOS). I. ALMA images of dusty molecular tori in Seyfert galaxies
The Hubble Tension Revisited: Additional Local Distance Ladder Uncertainties
The impact of satellite trails on Hubble Space Telescope observations
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2017-09-09T02:55:35Z/2019-02-16T21:50:18Z
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, 'The Hubble Constant to 1%: Physics beyond LambdaCDM', 1.0, European Space Agency, https://doi.org/10.5270/esa-q7y7qs1