A Test of Galaxy Evolutionary Models via Angular Sizes
Calibration of HST Wide Field Camera for Quantitative Analysis of Faint Galaxy Images
Constraints on thick disc and halo parameters from HST photometry of field stars in the Galaxy
Cosmic Gravitational Shear from the Hubble Space Telescope Medium Deep Survey
Detection, Photometry, and Completeness of FOCAS Catalogs for the HST Medium-Deep Survey
Flatfielding and Photometric Accuracy of The First Hubble Space Telescope Wide Field Camera
Galaxy Clustering Statistics of Hubble Space Telescope Medium Deep Survey WF/PC Images
GOYA Survey: U and B Number Counts in the Groth-Westphal Strip
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?
Ks Number Counts in the Groth and Coppi Fields
Luminosity Functions of Elliptical Galaxies at Z <1.2
Removing Cosmic-Ray Hits from Multi-Orbit HST Wide Field Camera Images
Structure and Photometry of an I < 20.5 Galaxy Sample from the Hubble Space Telescope Medium Deep Survey
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 HST Medium Deep Survey: Light Profiles and Redshifts for Field Galaxies with z<~0.6
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 Morphological Content of 10 EDisCS Clusters at 0.5 < z < 0.8
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
What can you Gain From Deconvolution? Observing Faint Galaxies With the Hubble Space Telescope Wide Field Camera
Instrument
WFPC/WFC
Temporal Coverage
1992-01-06T14:26:17Z/1992-01-08T20:01:17Z
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., 1993, 'HST MEDIUM-DEEP SURVEY: CYCLE 1', 1.0, European Space Agency, https://doi.org/10.5270/esa-f5x420c