scholarly journals 5 Cosmology with the Planck Satellite: from quantum foam to the cosmic web

2020 ◽  
pp. 131-160
Author(s):  
François R. Bouchet
Keyword(s):  
Planck Satellite

Foreground Separation Methods for Satellite and Balloon Experiments

2005 ◽  
Vol 201 ◽  
pp. 71-74
Author(s):  
R. Belén Barreiro ◽  
Michael P. Hobson ◽  
Anthony N. Lasenby ◽  
Patricio Vielva ◽  
Enrique Martínez-González ◽  
...  
Keyword(s):  
Point Source ◽  
Maximum Entropy ◽  
Maximum Entropy Method ◽  
Entropy Method ◽  
Mexican Hat Wavelet ◽  
Mexican Hat ◽  
Balloon Experiments ◽  
Combined Technique ◽  
Physical Components ◽  
Planck Satellite

A combined technique using the maximum-entropy method (MEM) and the mexican hat wavelet (MHW) to separate and reconstruct the physical components of the microwave sky is presented. We apply this method to simulated observations by the ESA Planck satellite in small patches of the sky. The reconstructed maps of the CMB and foregrounds are improved as compared to those obtained with MEM on its own. Moreover, more accurate point source catalogues are produced at each observing frequency. This technique may also be extended to deal with other multifrequency CMB experiments, including all-sky data.

scholarly journals Multi-mode horn design and beam characteristics for the Planck satellite

2010 ◽  
Vol 5 (04) ◽  
pp. T04001-T04001 ◽  
Author(s):  
J A Murphy ◽  
T Peacocke ◽  
B Maffei ◽  
I McAuley ◽  
F Noviello ◽  
...  
Keyword(s):  
Multi Mode ◽  
Beam Characteristics ◽  
Planck Satellite

THE PLANCK MISSION: RECENT RESULTS, COSMOLOGICAL AND FUNDAMENTAL PHYSICS PERSPECTIVES

2013 ◽  
Vol 22 (14) ◽  
pp. 1330029
Author(s):  
NAZZARENO MANDOLESI ◽  
CARLO BURIGANA ◽  
ALESSANDRO GRUPPUSO ◽  
PAOLO NATOLI
Keyword(s):  
Polarization Data ◽  
Fundamental Physics ◽  
Parity Symmetry ◽  
And Performance ◽  
Observational Strategy ◽  
Planck Satellite ◽  
Key Questions

We provide a description of the latest status and performance of the Planck satellite, focusing on the final predicted sensitivity of Planck. The optimization of the observational strategy for the additional surveys following the nominal 15 months of integration (about two surveys) originally allocated and the limitation represented by astrophysical foreground emissions are presented. An outline of early and intermediate astrophysical results from the Planck Collaboration is provided. A concise view of some fundamental cosmological results that will be achieved by exploiting Planck's full set of temperature and polarization data are presented. Finally, the perspectives opened by Planck in answering some key questions in fundamental physics, with particular attention to parity symmetry analyses, are described.

THE PLANCK SATELLITE: STATUS & PERSPECTIVES

2007 ◽  
Vol 22 (25n28) ◽  
pp. 1857-1863 ◽  
Author(s):  
◽  
F. R. BOUCHET
Keyword(s):  
Cosmic Microwave Background ◽  
Current Knowledge ◽  
Fast Rate ◽  
Microwave Background ◽  
The Status ◽  
Scientific Results ◽  
To Come ◽  
Planck Satellite

I review the status of development of the PLANCK project which is slated for launch mid-2008. In particular, I illustrate the type of scientific results to expect in light of the current knowledge of the two on-board instruments. Indeed both instruments have now been delivered to industry for integration and they have been fully tested. This leads us to anticipate that the steady and fast rate of progress enjoyed by cosmology, in particular through the constraints given by the analysis of the Cosmic Microwave background (CMB) will continue unabated in the years to come.

Planck satellite 70 GHz receiver noise tests

2001 ◽  
Vol 16 (12) ◽  
pp. 19-23 ◽  
Author(s):  
P. Sjoman ◽  
T. Ruokokoski ◽  
P. Jukkala ◽  
P. Eskelinen
Keyword(s):  
Receiver Noise ◽  
Planck Satellite

scholarly journals Far-IR to Submm SEDs for local galaxies: Herschel, Planck and the HRS

2011 ◽  
Vol 7 (S284) ◽  
pp. 279-282
Author(s):  
David L Clements ◽  
Keyword(s):  
Reference Sample ◽  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Space Observatory ◽  
Energy Distributions ◽  
Herschel Space Observatory ◽  
Fitting Procedure ◽  
Nearby Galaxies ◽  
New Generation ◽  
Planck Satellite

AbstractThe Herschel Space Observatory and the Planck satellite are providing radical improvements to our knowledge of the spectral energy distributions of galaxies in the far-IR and submm. We here present the results of the first combination of Herschel and Planck fluxes of local galaxies from the Herschel Reference Sample (HRS) survey, covering galaxies at distances between 15 and 25 Mpc. This combination provides information on SEDs in eight bands from 60μm, using IRAS, to 1.4mm using Planck. We apply a similar fitting procedure to this data as applied to the Planck ERCSC-detected nearby galaxies and confirm the result that dust significantly colder than 20K is common in local galaxies. It is early days for this kind of study, but it is clear that the new generation of satellites are already adding considerably to our knowledge of the far-IR/submm properties of galaxies.

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