A high stellar velocity dispersion for a compact massive galaxy at redshift z = 2.186
Comparing Dynamical and Photometric Mass Estimates of Low- and High-Redshift Galaxies: Random and Systematic Uncertainties
Faint Infrared Extragalactic Survey: Data and Source Catalog of the MS 1054-03 Field
Hubble Space Telescope and Spitzer Imaging of Red and Blue Galaxies at z ~ 2.5: A Correlation between Size and Star Formation Activity from Compact Quiescent Galaxies to Extended Star-forming Galaxies
Is NGC 300 a pure exponential disk galaxy?
Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters. II. Physical Properties of dE Progenitor Candidates
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC3
Temporal Coverage
2005-01-09T13:45:31Z/2005-02-15T01:18:10Z
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, Franx et al., 2006, 'Morphologies of a new class of rest-frame optical selected high redshift galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-l9kaznf