A High Merger Fraction in the Rich Cluster MS 1054-03 at Z = 0.83: Direct Evidence for Hierarchical Formation of Massive Galaxies
A Keck Spectroscopic Survey of MS 1054-03 (z = 0.83): Forming the Red Sequence
A Substantial Population of Red Galaxies at z > 2: Modeling of the Spectral Energy Distributions of an Extended Sample
Chandra X-Ray Observatory Observation of the High-Redshift Cluster MS 1054-0321
Colors of Luminous Bulges in Cluster MS 1054-03 and Field Galaxies at Redshifts z~0.83
Cosmic-Ray Rejection by Laplacian Edge Detection
Evolution since z = 1 of the Morphology-Density Relation for Galaxies
Faint Infrared Extragalactic Survey: Data and Source Catalog of the MS 1054-03 Field
Field E+A Galaxies at Intermediate Redshifts (0.3 < z < 1)
Hubble Space Telescope Photometry and Keck Spectroscopy of the Rich Cluster MS 1054-03: Morphologies, Butcher-Oemler Effect, and the Color-Magnitude Relation at Z = 0.83
Hubble Space Telescope Weak-Lensing Study of the z=0.83 Cluster MS 1054-03
Infall, the Butcher-Oemler Effect, and the Descendants of Blue Cluster Galaxies at z~0.6
IR Observations of MS 1054-03: Star Formation and Its Evolution in Rich Galaxy Clusters
Luminosity Evolution of Field Early-Type Galaxies to Z=0.55
Maximum-entropy weak lens reconstruction: improved methods and application to data
Multi-wavelength landscape of the young galaxy cluster RXJ 1257.2+4738 at z = 0.866. II. Morphological properties
Spectroscopic Confirmation of a Substantial Population of Luminous Red Galaxies at Redshifts z>~2
Spectroscopic Confirmation of Multiple Red Galaxy-Galaxy Mergers in MS 1054-03 (z = 0.83)1,
Stellar Populations and Kinematics of Red Galaxies at z > 2: Implications for the Formation of Massive Galaxies
Supernovae in deep Hubble Space Telescope galaxy cluster fields: cluster rates and field counts
The Color-Magnitude Distribution of Field Galaxies to z~3: The Evolution and Modeling of the Blue Sequence
The Detailed Fundamental Plane of Two High-Redshift Clusters: MS 2053-04 at z=0.58 and MS 1054-03 at z=0.83
The Hubble diagram of type Ia supernovae as a function of host galaxy morphology
The Nature of E+A Galaxies in Intermediate-Redshift Clusters
The Size Evolution of Galaxies since z~3: Combining SDSS, GEMS, and FIRES
The Tully-Fisher relation of cluster spirals at z= 0.83
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., 1999, 'Fundamental Plane, Morphology-Density Relation, and Lensing in the z=0.83 Cluster MS1054--03', 1.0, European Space Agency, https://doi.org/10.5270/esa-wwaju09