scholarly journals Weak Lensing by Large‐Scale Structure and the Polarization Properties of Distant Radio Sources

1999 ◽  
Vol 515 (2) ◽  
pp. 455-464 ◽  
Author(s):  
Gabriela C. Surpi ◽  
Diego D. Harari
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Weak Lensing ◽  
Radio Sources

scholarly journals Weak lensing of large scale structure in the presence of screening

2015 ◽  
Vol 2015 (10) ◽  
pp. 036-036 ◽  
Author(s):  
Nicolas Tessore ◽  
Hans A. Winther ◽  
R. Benton Metcalf ◽  
Pedro G. Ferreira ◽  
Carlo Giocoli
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Weak Lensing

scholarly journals Weak Lensing by Large‐Scale Structure with the FIRST Radio Survey

2004 ◽  
Vol 617 (2) ◽  
pp. 794-810 ◽  
Author(s):  
Tzu‐Ching Chang ◽  
Alexandre Refregier ◽  
David J. Helfand
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Weak Lensing ◽  
Radio Survey

scholarly journals The large-scale structure of FR-II radio sources

1998 ◽  
Vol 297 (4) ◽  
pp. 1087-1108 ◽  
Author(s):  
S. S. Komissarov ◽  
S. A. E. G. Falle
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Radio Sources

scholarly journals Weak Lensing of the CMB by Large Scale Structure

2004 ◽  
Vol 2004 (IAUS225) ◽  
pp. 105-109 ◽  
Author(s):  
A. Amblard ◽  
C. Vale ◽  
M. White
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Weak Lensing

scholarly journals DO WE HAVE EVIDENCE FOR NEW PHYSICS IN THE SKY?

2006 ◽  
Vol 21 (01) ◽  
pp. 1-21 ◽  
Author(s):  
LAURA MERSINI-HOUGHTON
Keyword(s):  
String Theory ◽  
Large Scale ◽  
Recent Progress ◽  
Large Scale Structure ◽  
New Physics ◽  
Scale Structure ◽  
Weak Lensing ◽  
Source Terms ◽  
Crucial Importance

Predicting signatures of string theory on cosmological observables is not sufficient. Often the observable effects string theory may impact upon the cosmological arena which may equally be predicted by features of inflationary physics. The question: what observable signatures are unique to new physics, is thus of crucial importance for claiming evidence for the theory. Here we discuss recent progress in addressing the above question. The evidence relies on identifying discrepancies between the source terms that give rise to large scale structure (LSS) and CMB, by cross-correlating the weak lensing potential that maps LSS with the CMB spectra.

Weak Lensing by Large-Scale Structure

2018 ◽  
pp. 209-232
Author(s):  
Arthur B. Congdon ◽  
Charles R. Keeton
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Weak Lensing

Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach

2000 ◽  
Vol 535 (1) ◽  
pp. L9-L12 ◽  
Author(s):  
Asantha Cooray ◽  
Wayne Hu ◽  
Jordi Miralda-Escudé
Keyword(s):  
Dark Matter ◽  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Dark Matter Halo ◽  
Weak Lensing

Commission 47: Cosmology (Cosmologie)

1988 ◽  
Vol 20 (1) ◽  
pp. 653-655
Author(s):  
G. Setti ◽  
K. Satco ◽  
J. Audouze ◽  
G. de Vaucouleurs ◽  
J. E. Gunn ◽  
...  
Keyword(s):  
Large Scale ◽  
Research Work ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Radio Sources ◽  
Clusters Of Galaxies ◽  
Extragalactic Radio Sources ◽  
Vast Amount ◽  
Wide Range ◽  
Commission Report

The number of pages allocated to the commission report has been very limited and certainly not sufficient to cover in any exhaustive manner the wide range of topics relevant to cosmology and to provide also extensive bibliographies. Because of the vast amount of material to be covered, the report is based on a number of contributions from different colleagues who have been asked to highlight the main trends in the triennium (mid 1984 - mid 1987), together with a list of references sufficiently comprehensive to serve as a guideline for further reading. Unfortunately, two of the expected contributions did not reach me in time for inclusion in the report, and consequently topics such as the large scale structure and streaming motions, the clusters of galaxies and the counts of extragalactic radio sources are not included. However, it is my understanding that a large portion, if not all, of these topics will be covered in the reports of Commissions 28 and 40, and if true, this will at least avoid unnecessary overlaps. It should also be mentioned here that several proceedings of very recent IAU conferences provide excellent, updated and exhaustive reviews of the research work relevant to cosmology.

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