A Multi-wavelength Mass Analysis of RCS2 J232727.6-020437, A ~3 x 1015 M Galaxy Cluster at z = 0.7
Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks
Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
Evolution of the Ultraviolet Upturn at 0.3 < z < 1: Exploring Helium-rich Stellar Populations
Precise weak lensing constraints from deep high-resolution Ks images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2 J 232727.7-020437 at z = 0.70
RCS2 J232727.6-020437: An Efficient Cosmic Telescope at z=0.6986
Spitzer Ultra Faint SUrvey Program (SURFS UP). I. An Overview
Spitzer UltRa Faint SUrvey Program (SURFS UP). II. IRAC-detected Lyman-Break Galaxies at 6 z 10 behind Strong-lensing Clusters
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC3
Temporal Coverage
2006-07-26T07:29:43Z/2006-09-14T03:21:58Z
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, Gladders comma Michael D., 2007, 'The Halo Structure of RCS2-2327.4-0204', 1.0, European Space Agency, https://doi.org/10.5270/esa-fu9wbfm