Can standard cosmological models explain the observed Abell cluster bulk flow? |
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CLASH: complete lensing analysis of the largest cosmic lens MACS J0717.5+3745 and surrounding structures |
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CLASH: extreme emission-line galaxies and their implication on selection of high-redshift galaxies |
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CLASH: mass distribution in and around MACS J1206.2-0847 from a full cluster lensing analysis |
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CLASH: PRECISE NEW CONSTRAINTS ON THE MASS PROFILE OF THE GALAXY CLUSTER A2261 |
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CLASH: three strongly lensed images of a candidate z {approx} 11 galaxy |
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CLASH-x: a comparison of lensing and X-ray techniques for measuring the mass profiles of galaxy clusters |
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Classifying the high energy universe with ClassX |
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The Cluster Lensing And Supernova survey with Hubble: an overview |
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The Cluster Mass Function from Early Sloan Digital Sky Survey Data: Cosmological Implications |
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Clustering at High Redshift: Precise Constraints from a Deep, Wide‐Area Survey |
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Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-Ray, SZ, and Lensing Data |
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The contribution of halos with different mass ratios to the overall growth of cluster-sized halos |
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Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters |
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A Definitive Optical Detection of a Supercluster at z approximately 0.91. |
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Detecting Clusters of Galaxies in the Sloan Digital Sky Survey. I. Monte Carlo Comparison of Cluster Detection Algorithms |
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The detection and statistics of giant arcs behind CLASH clusters |
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Direct imaging and spectroscopy of habitable planets using JWST and a starshade |
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Discovery of a New Fundamental Plane Dictating Galaxy Cluster Evolution from Gravitational Lensing |
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Distant Cluster Hunting: A Comparison Between the Optical and X-Ray Luminosity Functions from an Optical/X-Ray Joint Survey |
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The distribution of nearby rich clusters of galaxies |
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Early-type galaxies at z = 1.3. I. The Lynx supercluster: cluster and groups at z = 1.3. Morphology and color-magnitude relation |
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Evidence for Cluster Evolution from an Improved Measurement of the Velocity Dispersion and Morphological Fraction of Cluster 1324+3011 at [CLC][ITAL]z[/ITAL][/CLC] = 0.76 |
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Evidence for X-Ray Emission from a Large-Scale Filament of Galaxies? |
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The Evolution of Early-Type Field Galaxies Selected from a NICMOS Map of the Hubble Deep Field North |
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Evolution of the color-magnitude relation in galaxy clusters at z ~ 1 from the ACS intermediate redshift cluster survey |
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The Far‐Field Hubble Constant |
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Galaxies with a Central Minimum in Stellar Luminosity Density |
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Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847 |
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The genus curve of the Abell clusters |
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A Group-Group Merger at a Redshift of [ITAL]z[/ITAL] = 0.84? |
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A high-definition space telescope for the 2030s |
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The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry |
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The Hubble Deep Field South: Formulation of the Observing Campaign |
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Hubble Space Telescope combined strong and weak lensing analysis of the CLASH sample: mass and magnification models and systematic uncertainties |
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Improving dark energy constraints with high-redshift Type Ia supernovae from CANDELS and CLASH |
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The infrared properties of quasars and radio galaxies - Testing the unification schemes |
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The Infrared Surface Brightness Fluctuation Hubble Constant |
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IRAS galaxies and the large-scale structure in the CfA slice |
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Is there structure on the scale of 300/h MPC ? |
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[ITAL]Hubble Space Telescope[/ITAL] Imaging of Brightest Cluster Galaxies |
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A Keck Spectroscopic Survey of MS 1054−03 (z= 0.83): Forming the Red Sequence |
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A large population of 'Lyman-break' galaxies in a protocluster at redshift z approximately 4.1. |
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The Large UV/Optical/Infrared (LUVOIR) Surveyor: Decadal Mission concept design update |
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The Luminosity Function of Galaxies in SDSS Commissioning Data |
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Luminosity Functions of the Galaxy Cluster MS 1054−0321 atz = 0.83 based on ACS Photometry |
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The Lumpy Cluster Abell 1185 |
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A magnified young galaxy from about 500 million years after the Big Bang |
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The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes |
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Modular assembled space telescope |
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The morphologies and alignments of gas, mass, and the central galaxies of CLASH clusters of galaxies |
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The motion of the Local Group with respect to the 15,000 kilometer per second Abell cluster inertial frame |
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A new paradigm for space astrophysics mission design |
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Observational Constraints on Higher Order Clustering up toz≃ 1 |
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Observations of Lyαand O vi: Signatures of Cooling and Star Formation in a Massive Central Cluster Galaxy |
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Optical photometry of the emission-line M star PC 0025 + 0447 |
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Overview of the Advanced Camera for Surveys on-orbit performance |
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The Palomar Distant Clusters Survey. I. The Cluster Catalog |
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A precise cluster mass profile averaged from the highest-quality lensing data |
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Profiles of dark matter velocity anisotropy in simulated clusters |
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The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters |
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A Radio Relic and a Search for the Central Black Hole in the Abell 2261 Brightest Cluster Galaxy |
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Science drivers and requirements for an Advanced Technology Large Aperture Space Telescope (ATLAST): implications for technology development and synergies with other future facilities |
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Science with an 8-meter to 16-meter optical/UV space telescope |
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SDSS-RASS: Next Generation of Cluster-Finding Algorithms |
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Shellflow. I. The Convergence of the Velocity Field at 6000 Kilometers per Second |
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Space Telescopes in the Ultraviolet, Optical, and Infrared (UV/O/IR) |
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Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample |
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The Spiderweb Galaxy: A Forming Massive Cluster Galaxy atz~ 2 |
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Stellar Mass and 3.4 μm M/L Ratio Evolution of Brightest Cluster Galaxies in COSMOS since z ∼ 1.0 |
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Stellar populations and morphology on the red sequence at z≈1 |
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Strong‐Lensing Analysis of A1689 from Deep Advanced Camera Images |
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A Study of Nine High-Redshift Clusters of Galaxies. IV. Photometry and Spectra of Clusters 1324+3011 and 1604+4321 |
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Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate |
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Ultraviolet morphology and unobscured UV star formation rates of CLASH brightest cluster galaxies |
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