A Measurement of Weak Lensing by Large‐Scale Structure in Red‐Sequence Cluster Survey Fields

2002 ◽  
Vol 572 (1) ◽  
pp. 55-65 ◽  
Author(s):  
Henk Hoekstra ◽  
Howard K. C. Yee ◽  
Michael D. Gladders ◽  
L. Felipe Barrientos ◽  
Patrick B. Hall ◽  
...  
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Weak Lensing ◽  
Sequence Cluster ◽  
Cluster Survey ◽  
Red Sequence

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

Probing the Large-Scale Structure with the REFLEX Cluster Survey

2006 ◽  
pp. 157-163
Author(s):  
H. Böhringer ◽  
L. Guzzo ◽  
C. A. Collins ◽  
P. Schuecker ◽  
S. Schindler ◽  
...  
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Cluster Survey

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 Constraints on Ωmand σ8from Weak Lensing in Red‐Sequence Cluster Survey Fields

2002 ◽  
Vol 577 (2) ◽  
pp. 595-603 ◽  
Author(s):  
Henk Hoekstra ◽  
Howard K. C. Yee ◽  
Michael D. Gladders
Keyword(s):  
Weak Lensing ◽  
Sequence Cluster ◽  
Cluster Survey ◽  
Red Sequence

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: 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
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