A Calibration of NICMOS Camera 2 for Low Count Rates
Colour gradients in cluster ellipticals at z ~ 1.4: the hidden content of the galaxy central regions
Intracluster light is already abundant at redshift beyond unity
Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
Morphological evolution in situ: disc-dominated cluster red sequences at z ~ 1.25
Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39
The accelerated build-up of the red sequence in high-redshift galaxy clusters
The KMOS Cluster Survey (KCS). II. The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift 1.39 < z < 1.61
The KMOS Cluster Survey (KCS). I. The Fundamental Plane and the Formation Ages of Cluster Galaxies at Redshift 1.4 < z < 1.6
The morphological transformation of red sequence galaxies in clusters since z ~ 1
The morphological transformation of red sequence galaxies in the distant cluster XMMU J1229+0151
The resolved jet of 3C 273 at 150 MHz. Sub-arcsecond imaging with the LOFAR international baselines
Instrument
WFC3, WFC3/IR
Temporal Coverage
2010-02-09T20:47:04Z/2010-05-24T08:03:27Z
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, 2011, 'Cross Calibration of NICMOS and WFC3 in the Low-Count-Rate Regime', 1.0, European Space Agency, https://doi.org/10.5270/esa-yom1y12
