A 1010 Solar Mass Flow of Molecular Gas in the A1835 Brightest Cluster Galaxy
A CFH12k lensing survey of X-ray luminous galaxy clusters. II. Weak lensing analysis and global correlations
A Hubble Space Telescope Lensing Survey of X-Ray Luminous Galaxy Clusters. I. A383
A Hubble Space Telescope lensing survey of X-ray-luminous galaxy clusters - II. A search for gravitationally lensed EROs *
A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters - III. A multiply imaged extremely red galaxy at z=1.6
A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z= 0.2
A neural network gravitational arc finder based on the Mediatrix filamentation method
A New Survey for Giant Arcs
A simple prescription for simulating and characterizing gravitational arcs
A Statistical Study of Multiply Imaged Systems in the Lensing Cluster Abell 68
A Systematic Search for Gravitationally Lensed Arcs in the Hubble Space Telescope WFPC2 Archive
Constraining star formation rates in cool-core brightest cluster galaxies
Discovery of a faint R-band drop-out: A strongly reddened lensed star forming galaxy at z = 1.68
Discovery of a Transient U-Band Dropout in a Lyman Break Survey: A Tidally Disrupted Star at z=3.3?
Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters
Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
Galaxy properties in low X-ray luminosity clusters at z=0.25
Hubble Space Telescope Far-ultraviolet Observations of Brightest Cluster Galaxies: The Role of Star Formation in Cooling Flows and BCG Evolution
Intense Star Formation and Feedback at High Redshift: Spatially Resolved Properties of the z = 2.6 Submillimeter Galaxy SMM J14011+0252
ISAAC/VLT observations of a lensed galaxy at z = 10.0
Locating the Starburst in the SCUBA Galaxy SMM J14011+0252
LoCuSS: A Dynamical Analysis of X-Ray Active Galactic Nuclei in Local Clusters
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters at z = 0.2
Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton
Measuring s8 with Cluster Lensing: Biases from Unrelaxed Clusters
Molecular Gas and Dust at z=2.6 in SMM J14011+0252: A Strongly Lensed Ultraluminous Galaxy, Not a Huge Massive Disk
Near-IR search for lensed supernovae behind galaxy clusters. II. First detection and future prospects
Offset between dark matter and ordinary matter: evidence from a sample of 38 lensing clusters of galaxies
On the distribution of dark matter in clusters of galaxies
Optical and Infrared Nondetection of the z = 10 Galaxy behind Abell 1835
Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100 pc scales at 1 < z < 4
Separating Baryons and Dark Matter in Cluster Cores: A Full Two-dimensional Lensing and Dynamic Analysis of Abell 383 and MS 2137-23
Star formation histories, extinction, and dust properties of strongly lensed z ~ 1.5-3 star-forming galaxies from the Herschel Lensing Survey
Testing the Universality of the Fundamental Metallicity Relation at High Redshift Using Low-mass Gravitationally Lensed Galaxies
The Abundance of Low-Luminosity Lya Emitters at High Redshift
The Dark Matter Distribution in A383: Evidence for a Shallow Density Cusp from Improved Lensing, Stellar Kinematic, and X-ray Data
The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter
The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius
The emission line properties of gravitationally lensed 1.5 < z < 5 galaxies
The Intrinsic Properties of SMM J14011+0252
The Lensed Arc Production Efficiency of Galaxy Clusters: A Comparison of Matched Observed and Simulated Samples
Ultraviolet emission lines in young low-mass galaxies at z 2: physical properties and implications for studies at z > 7
Unveiling C II clumps in a lensed star-forming galaxy at z ~ 3.4
X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range
z ~ 7-10 Galaxies Behind Lensing Clusters: Contrast with Field Search Results
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-11-05T10:23:13Z/2000-11-20T13:19:33Z
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, KNEIB JEAN-PAUL, 2001, 'A Strong Lensing Survey of the Mass Distribution in X-ray Luminous Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-dzrkou2
