A Binary Offset Effect in CCD Readout and Its Impact on Astronomical Data
A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry
ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments
An Assessment of the In Situ Growth of the Intracluster Light in the High-redshift Galaxy Cluster SpARCS1049+56
An Extreme Starburst in the Core of a Rich Galaxy Cluster at z = 1.7
Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z = 1.71 with Infrared Weak Lensing
Detection of a Substantial Molecular Gas Reservoir in a Brightest Cluster Galaxy at z = 1.7
Environmental processing in cluster core galaxies at z = 1.7
Evidence for the Existence of Abundant Intracluster Light at z = 1.24
First Weak-lensing Results from See Change: Quantifying Dark Matter in the Two z 1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
Galaxy Merger Candidates in High-redshift Cluster Environments
Low surface brightness galaxies in z > 1 galaxy clusters: HST approaching the progenitors of local ultra diffuse galaxies
Mass assembly and active galactic nucleus activity at z 1.5 in the dense environment of XDCP J0044.0-2033
Multiple AGN activity during the BCG assembly of XDCPJ0044.0-2033 at z ~ 1.6
Multiwavelength view of SPT-CL J2106-5844. The radio galaxies and the thermal and relativistic plasmas in a massive galaxy cluster merger at z 1.13
Resolving CO (2-1) in z ~ 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping
See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
The delay time distribution of Type-Ia supernovae in galaxy clusters: the impact of extended star-formation histories
The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22
The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries
The H a star formation main sequence in cluster and field galaxies at z ~ 1.6
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75
The Star Formation History of BCGs to z = 1.8 from the SpARCS/SWIRE Survey: Evidence for Significant In Situ Star Formation at High Redshift
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2014-09-15T01:19:25Z/2015-10-14T10:37:59Z
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, Perlmutter comma Saul, 2015, 'See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts', 1.0, European Space Agency, https://doi.org/10.5270/esa-ou6ivq0
