An Assessment of the In Situ Growth of the Intracluster Light in the High-redshift Galaxy Cluster SpARCS1049+56
Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z = 1.71 with Infrared Weak Lensing
Galaxy Merger Candidates in High-redshift Cluster Environments
See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2015-02-07T10:50:01Z/2015-05-23T18:34:48Z
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, Webb comma Tracy, 2016, 'Understanding the In-Situ Star Formation in a z=1.7 Cluster Core Galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-dvcor5k