scholarly article | Q13442814 |
P819 | ADS bibcode | 2011ApJ...742..117Z |
P818 | arXiv ID | 1103.5618 |
P356 | DOI | 10.1088/0004-637X/742/2/117 |
P953 | full work available at URL | https://iopscience.iop.org/article/10.1088/0004-637X/742/2/117/pdf |
P50 | author | Adam Riess | Q106454 |
Matthias Bartelmann | Q1909702 | ||
Megan Donahue | Q1917100 | ||
Ofer Lahav | Q3349501 | ||
Rychard Bouwens | Q7384802 | ||
Peter Melchior | Q56473983 | ||
Massimo Meneghetti | Q56482079 | ||
Mario Nonino | Q56482086 | ||
Larry Bradley | Q56482092 | ||
Keiichi Umetsu | Q56482098 | ||
Anton Koekemoer | Q56482119 | ||
Steven Rodney | Q56515166 | ||
Or Graur | Q56527817 | ||
Yolanda Jiménez-Teja | Q57901739 | ||
Dan Coe | Q58483706 | ||
Ruth Lazkoz | Q58483869 | ||
Elinor Medezinski | Q58484631 | ||
Leopoldo Infante | Q63231232 | ||
P2093 | author name string | G. Graves | |
H. Ford | |||
C. McCully | |||
D. Maoz | |||
M. Postman | |||
P. Rosati | |||
W. Zheng | |||
D. Kelson | |||
N. Benítez | |||
B. Patel | |||
S. Seitz | |||
L. A. Moustakas | |||
T. Broadhurst | |||
A. Molino | |||
A. Zitrin | |||
D. Lemze | |||
J. Merten | |||
O. Host | |||
S. Jouvel | |||
S. Ogaz | |||
S. Jha | |||
A. Van der Wel | |||
E. Regoes | |||
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Discovery of a possibly old galaxy at z= 6.027, multiply imaged by the massive cluster Abell 383 | Q58489758 | ||
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Optimal filter systems for photometric redshift estimation | Q58982582 | ||
Comparison of an X-ray-selected sample of massive lensing clusters with the MareNostrum Universe ΛCDM simulation | Q59320601 | ||
Combining weak and strong cluster lensing: applications to simulations and MS 2137 | Q59320655 | ||
cD galaxy contribution to the strong lensing cross-sections of galaxy clusters | Q59320827 | ||
Dynamical effects of the cosmological constant | Q59629216 | ||
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Weighing simulated galaxy clusters using lensing and X-ray | Q59747072 | ||
A precise cluster mass profile averaged from the highest-quality lensing data | Q59764418 | ||
Triaxiality and non-thermal gas pressure in Abell 1689 | Q59782793 | ||
A weak lensing detection of the cosmological distance-redshift relation behind three massive clusters★ | Q59782799 | ||
Strong-lensing analysis of MS 1358.4+6245: New multiple images and implications for the well-resolved z= 4.92 galaxy | Q59782801 | ||
Cluster mass profiles from a bayesian analysis of weak-lensing distortion and magnification measurements: applications to Subaru data | Q59782805 | ||
Full lensing analysis of Abell 1703: comparison of independent lens-modelling techniques | Q59782814 | ||
Detailed cluster mass and light profiles of A1703, A370 and RXJ1347−11 from deep Subaru imaging | Q59782827 | ||
LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters | Q59782829 | ||
The mass structure of the galaxy cluster Cl0024+1654 from a full lensing analysis of joint Subaru and ACS/NIC3 observations | Q59782833 | ||
New multiply-lensed galaxies identified in ACS/NIC3 observations of Cl0024+1654 using an improved mass model | Q59782845 | ||
Combining Lens Distortion and Depletion to Map the Mass Distribution of A1689 | Q59782859 | ||
Comparison of Cluster Lensing Profiles with ΛCDM Predictions | Q59782860 | ||
The Surprisingly Steep Mass Profile of A1689, from a Lensing Analysis of Subaru Images | Q59782888 | ||
A weak-lensing analysis of the Abell 383 cluster | Q59924650 | ||
The dark matter distribution in A383: evidence for a shallow density cusp from improved lensing, stellar kinematic, and X-ray data | Q59969801 | ||
The distribution of dark matter over three decades in radius in the lensing cluster Abell 611 | Q59969813 | ||
Hubble space telescope weak-lensing study of the galaxy cluster XMMU J2235.3 - 2557 at z ~ 1.4: a surprisingly massive galaxy cluster when the universe is one-third of its current age | Q60663402 | ||
Multi-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1 | Q60663404 | ||
Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North | Q60737367 | ||
Galaxies in the Hubble Ultra Deep Field. I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology | Q62623157 | ||
The density profiles of the dark matter halo are not universal | Q68264347 | ||
Mass and redshift dependence of dark halo structure | Q68364111 | ||
The dark matter distribution in the central regions of galaxy clusters: implications for cold dark matter | Q68372431 | ||
Characterizing the cluster lens population | Q68465805 | ||
Subaru weak lensing measurements of four strong lensing clusters: are lensing clusters overconcentrated? | Q68488297 | ||
Discovery of the largest known lensed images formed by a critically convergent lensing cluster | Q68489545 | ||
Accurate universal models for the mass accretion histories and concentrations of dark matter halos | Q68490816 | ||
A radial mass profile analysis of the lensing cluster MS 2137.3-2353 | Q68523332 | ||
Analytical models for galactic nuclei | Q68628168 | ||
Profiles of dark haloes: evolution, scatter and environment | Q68696041 | ||
Stellar population synthesis at the resolution of 2003 | Q68703757 | ||
A genetic algorithm for the non-parametric inversion of strong lensing systems | Q68712533 | ||
Parametric strong gravitational lensing analysis of Abell 1689 | Q68715052 | ||
The dark matter haloes of massive, relaxed galaxy clusters observed with Chandra | Q68717941 | ||
Non-parametric inversion of gravitational lensing systems with few images using a multi-objective genetic algorithm | Q68718692 | ||
The probability distribution of cluster formation times and implied Einstein radii | Q68722310 | ||
What is the largest Einstein radius in the universe ? | Q68723876 | ||
Cosmology with the cluster mass function: mass estimators and shape systematics in large weak lensing surveys | Q68725876 | ||
Cluster contribution to the X-ray background as a cosmological probe | Q68726919 | ||
Bayesian photometric redshift estimation | Q68875783 | ||
Shape, spin, and baryon fraction of clusters in the MareNostrum universe | Q68896699 | ||
Non-parametric strong lens inversion of SDSS J1004+4112 | Q68965800 | ||
The largest gravitational lens: MACS J0717.5+3745 (z = 0.546) | Q68978663 | ||
On the overconcentration problem of strong lensing clusters | Q68990628 | ||
An empirical pixel-based correction for imperfect CTE. I. HST's advanced camera for surveys | Q68995692 | ||
Strong-lensing analysis of a complete sample of 12 MACS clusters at {\em z} > 0.5: mass models and EINSTEIN radii | Q69015587 | ||
P433 | issue | 2 | |
P407 | language of work or name | English | Q1860 |
P304 | page(s) | 117 | |
P577 | publication date | 2011-11-15 | |
P1433 | published in | The Astrophysical Journal | Q598789 |
P1476 | title | The cluster lensing and supernova survey with Hubble (CLASH): strong-lensing analysis of A383 from 16-band HST/WFC3/ACS imaging | |
P478 | volume | 742 |
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Q57686691 | CLASH: Photometric redshifts with 16 HST bands in galaxy cluster fields |
Q59320356 | CLASH: accurate photometric redshifts with 14 HST bands in massive galaxy cluster cores |
Q58474366 | CLASH: new multiple images constraining the inner mass profile of MACS J1206.2-0847 |
Q58908313 | Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members |
Q58474362 | Cosmological simulations with self-interacting dark matter – I. Constant-density cores and substructure |
Q59320509 | Miscentring in galaxy clusters: dark matter to brightest cluster galaxy offsets in 10 000 Sloan Digital Sky Survey clusters |
Q56933559 | Observational Status of Dark Matter |
Q57686673 | Three gravitationally lensed supernovae behind CLASH galaxy clusters |
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