A Test of Galaxy Evolutionary Models via Angular Sizes
Cosmic Gravitational Shear from the Hubble Space Telescope Medium Deep Survey
High-Resolution V, I, and K-Band Imaging of Faint Field Galaxies from the HST Medium-Deep Survey
Hubble Space Telescope Counts of Elliptical Galaxies: Constraints on Cosmological Models?
Luminosity Functions of Elliptical Galaxies at Z <1.2
Structural Parameters of Faint Galaxies from Prerefurbishment Hubble Space Telescope Medium Deep Survey Observations
The Axis Ratio Distribution of Faint Galaxies: Evidence for a Population of Dwarf Galaxies at I approximately 20.5
The Contribution of Late-Type/Irregulars to the Faint Galaxy Counts from Hubble Space Telescope Medium-Deep Survey Images
The Hubble Space Telescope Medium Deep Survey Cluster Sample: Methodology and Data
The Hubble Space Telescope Medium Deep Survey with the Wide Field and Planetary Camera. I. Methodology and Results on the Field near 3C 273
The Morphologically Divided Redshift Distribution of Faint Galaxies
The Morphologies of Distant Galaxies. II. Classifications from the Hubble Space Telescope Medium Deep Survey
The physical parameters of the evolving population of faint galaxies
Weak gravitational lensing around field galaxies in Hubble Space Telescope survey images
Instrument
WFPC/PC
Temporal Coverage
1993-05-23T15:07:18Z/1993-12-01T10:35:17Z
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, Griffiths comma Richard E., 1994, 'HST MEDIUM-DEEP SURVEY - PART 2: LO-LAT - CYC3HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-kcijypm