Are Hubble Deep Field Galaxy Counts Whole Numbers?
Candidate primeval galaxies in the Hubble Deep Field.
Cloning Dropouts: Implications for Galaxy Evolution at High Redshift
Faint galaxy counts as a function of morphological type in a hierarchical merger model
Galaxy morphology to I=25 mag in the Hubble Deep Field
High-resolution studies of radio sources in the Hubble Deep and Flanking Fields
Hubble Deep Field Constraint on Baryonic Dark Matter
Lyman alpha emitting galaxies at high redshift: Direct detection of young galaxies in a young universe
Optical Rotation Curves of Distant Field Galaxies: Sub-L* Systems
The Axis Ratio Distribution of Local and Distant Galaxies
The Relative Star Formation Histories of Spiral Bulges and Elliptical Galaxies in the Hubble Deep Fields
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-12-18T03:07:17Z/1995-12-30T23:21:16Z
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, Williams comma Robert E., 1996, 'THE HDF EXPERIMENTS: FLANKING FIELDS', 1.0, European Space Agency, https://doi.org/10.5270/esa-leovr9x