A constrained cosmological model in f(R ,Lm) gravity
A Model-independent Test of Cosmic Isotropy with Low-z Pantheon Supernovae
Anisotropy of the Universe via the Pantheon supernovae sample revisited
Assessing the potential of cluster edges as a standard ruler on constraining dark energy models
Assessment of the cosmic distance duality relation using Gaussian process
Calibrating the effective magnitudes of type Ia supernovae with a model-independent method
Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmography?
Can late dark energy transitions raise the Hubble constant?
Constraints on a Bianchi type I spacetime extension of the standard L CDM model
Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
Cosmography in f (Q ) gravity
Cosmological constraints on Horava gravity revised in light of GW170817 and GRB170817A and the degeneracy with massive neutrinos
Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing
Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
Do the observational data favor a local void?
Effect of low anisotropy on cosmological models by using supernova data
Gamma-ray bursts, quasars, baryonic acoustic oscillations, and supernovae Ia: new statistical insights and cosmological constraints
Improving sampling and calibration of gamma-ray bursts as distance indicators
Kinematic constraints on spatial curvature from supernovae Ia and cosmic chronometers
Late-time acceleration due to a generic modification of gravity and the Hubble tension
Likelihood-free Cosmological Constraints with Artificial Neural Networks: An Application on Hubble Parameters and SNe Ia
Multipole expansion of the local expansion rate
On the impact of f(Q) gravity on the large scale structure
Planck 2018 results. VI. Cosmological parameters
Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
Pre-main-sequence Stellar Populations across Shapley Constellation III. I. Photometric Analysis and Identification
Reconstructing the weak lensing magnification distribution of type Ia supernovae
Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
Tension with the flat LCDM model from a high-redshift Hubble diagram of supernovae, quasars, and gamma-ray bursts
Testing gravity on cosmic scales: A case study of Jordan-Brans-Dicke theory
Testing interacting dark matter and dark energy model with cosmological data
Testing the Cosmic Distance Duality Relation with the Latest Strong Gravitational Lensing and Type Ia Supernovae
The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
The Pantheon+ Analysis: Cosmological Constraints
The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration Systematic Uncertainty
The Pantheon+ Analysis: The Full Data Set and Light-curve Release
The Unusual Variability of the Large Magellanic Cloud Planetary Nebula RPJ 053059-683542
The VMC Survey. XXXII. Pre-main-sequence populations in the Large Magellanic Cloud
Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics Experiments
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2007-05-08T04:50:16Z/2007-06-29T02:51:36Z
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, Rest comma Armin, 2007, 'Resolving the LMC Microlensing Puzzle: Where are the Lensing Objects?', 1.0, European Space Agency, https://doi.org/10.5270/esa-9kknzvf