Gravitational lensing imprints distinctive non-gaussianities on the total intensity CMB map. Computation of the four-point correlation function over the map provides estimation of the integrated mass distribution along given lines of sight.
Moreover, it is remarkable to notice that measurements of CMB lensing are complementary to optical ones because they probe bigger volumes and have the advantage of a precisely known source redshift.
This is a bi-lingual blog of the members of the ADAMIS team at Laboratoire APC and invited guests. We comment on selected papers and events exploring, or relevant to, the interface between physics, cosmology, applied math, statistics, and numerical algorithms and which we have found interesting.
The opinions expressed in this blog reflect those of their authors and neither that of the ADAMIS group as a whole nor of Laboratoire APC.
The opinions expressed in this blog reflect those of their authors and neither that of the ADAMIS group as a whole nor of Laboratoire APC.
Showing posts with label CMB experiments. Show all posts
Showing posts with label CMB experiments. Show all posts
Sunday, May 1, 2011
Wednesday, February 16, 2011
First Planck science papers are out ... but CMB-free ... [arXiv:1101.2048, ..., arXiv:1101.1721]
First science results from Planck are finally available. At last ... Well they have been out since January, 11, but let's not be picky about these few weeks ... What is that after all, when compared to more than 15 years of sweating and toiling it took to get the instrument designed, built, tested, launched, and operating ... And moreover so well, as these recent results seem to demonstrate so convincingly.
Monday, January 17, 2011
A first step to reconstruct lensing potential [arXiv:1012.1600]
Somebody has already mentioned on this blog post the importance of gravitational lensing effect on CMB and the necessity somehow to get rid of its signature in a, hopefully soon, measured B-mode spectum to estimate signal due to inflationary processes.
Labels:
CMB,
CMB experiments,
Cosmology,
lensing,
non-Gaussianities,
Statistics,
weak lensing,
WMAP
Wednesday, December 22, 2010
First season QUIET observations [1012.3191]
L'expérience QUIET a observé le fond diffus cosmologique entre octobre 2008 et décembre 2010, utilisant un télescope dédié et des récepteurs à 43 et 95 GHz, depuis le désert d'Atacama au Chili (cf. photo ci-contre).L'article que vous trouverez ici présente les résultats obtenus avec les 19 détecteurs fonctionnant à 43 GHz, d'une sensibilité de 69 uK/sqrt(Hz) pour l'ensemble du plan focal (durée d'observation : 3458 heures).
Le but scientifique de QUIET est la détection des modes B primordiaux, entre l=25 et l=475.
Labels:
CMB,
CMB experiments,
CMB polarization,
quiet,
systematic errors
Sunday, October 17, 2010
WMAP is no more ...
Quietly, and almost unnoticeably (though check this New York Times editorial), Wilkinson Microwave Anisotropy Probe has lived up its science days. First on Aug, 19, 2010, the satellite stopped taking scientific data, and then on Oct, 09, 2010 left its anchor point at Sun-Earth Lagrange 2 (L2) point, which it was orbiting around since 2001, to join a stable orbit around the Sun. The satellite's mission has been therefore concluded. Its thrusters will ignite no more ...
Labels:
CMB,
CMB experiments,
Cosmology,
satellite missions
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