A contribution of star-forming clumps and accreting satellites to the mass assembly of z ~ 2 galaxies
Deciphering the Activity and Quiescence of High-redshift Cluster Environments: ALMA Observations of Cl J1449+0856 at z = 2
Feedback factory: multiple faint radio jets detected in a cluster at z = 2
Galaxy Evolution in Overdense Environments at High Redshift: Passive Early-type Galaxies in a Cluster at z ~ 2
Metal Deficiency in Cluster Star-Forming Galaxies At Z = 2
Molecular gas in distant brightest cluster galaxies
Suppressed CO emission and high G/D ratios in z = 2 galaxies with sub-solar gas-phase metallicity
The Early Early Type: Discovery of a Passive Galaxy at z spec ~ 3
The Red Sequence at Birth in the Galaxy Cluster Cl J1449+0856 at z = 2
WFC3 GRISM Confirmation of the Distant Cluster Cl J1449+0856 at langzrang = 2.00: Quiescent and Star-forming Galaxy Populations
Instrument
WFC3, WFC3/IR
Temporal Coverage
2010-06-06T05:59:59Z/2010-07-09T16:44:53Z
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, Daddi comma Emanuele, 2011, 'WFC3 spectroscopy of an X-ray luminous galaxy cluster at z>2', 1.0, European Space Agency, https://doi.org/10.5270/esa-xi5pzli
