Hubble Asteroid Hunter. I. Identifying asteroid trails in Hubble Space Telescope images
Hubble Asteroid Hunter. III. Physical properties of newly found asteroids
Project Dinos I: A joint lensing-dynamics constraint on the deviation from the power law in the mass profile of massive ellipticals
RINGFINDER: Automated Detection of Galaxy-scale Gravitational Lenses in Ground-based Multi-filter Imaging Data
Testing dark energy models with a new sample of strong-lensing systems
Testing the cosmic curvature at high redshifts: the combination of LSST strong lensing systems and quasars as new standard candles
The impact of satellite trails on Hubble Space Telescope observations
The SL2S Galaxy-scale Gravitational Lens Sample. I. The Alignment of Mass and Light in Massive Early-type Galaxies at z = 0.2-0.9
The SL2S Galaxy-scale Lens Sample. II. Cosmic Evolution of Dark and Luminous Mass in Early-type Galaxies
The SL2S Galaxy-scale Lens Sample. III. Lens Models, Surface Photometry, and Stellar Masses for the Final Sample
The SL2S Galaxy-scale Lens Sample. IV. The Dependence of the Total Mass Density Profile of Early-type Galaxies on Redshift, Stellar Mass, and Size
The SL2S Galaxy-scale Lens Sample. V. Dark Matter Halos and Stellar IMF of Massive Early-type Galaxies Out to Redshift 0.8
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2009-09-12T09:06:25Z/2010-09-05T23:23:00Z
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, Gavazzi et al., 2011, 'Galaxy-Scale Strong Lenses from the CFHTLS survey', 1.0, European Space Agency, https://doi.org/10.5270/esa-od0s1dr