Proceedings Article10.1117/12.461140
Planck data processing centers
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TL;DR: The success of the Planck mission heavily relies on careful planning, design and implementation of its ground segment facilities as discussed by the authors, including two Data Processing Centres (DPCs), which are operated by the consortia responsible for building the instruments forming the scientific payload of Planck.
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Abstract: The success of the Planck mission heavily relies on careful planning, design and implementation of its ground segment facilities. Among these, two Data Processing Centres (DPCs) are being implemented, which are operated by the consortia responsible for building the instruments forming the scientific payload of Planck. The two DPCs, together with the Mission Operations Centre (MOC) and the Herschel Science Centre (HSC), are the major elements of the Herschel/Planck scientific ground segment.
The Planck DPCs are responsible for the operation of the instruments, and for the production, delivery and archiving of the scientific data products, which can be considered as the final results of the mission:
· Calibrated time series data, for each receiver, after removal of systematic features and attitude reconstruction.
· Photometrically and astrometrically calibrated maps of the sky in the observed bands.
· Sky maps of the main astrophysical components.
· Catalogs of sources detected in the sky maps of the main astrophysical components.
· CMB power spectrum coefficients.
During the development phase, the DPCs are furthermore responsible for the production of data simulating realistically the behaviour of the instruments in flight, and for the support to instrument testing activities.
In this paper, some aspects related to the control of the Planck instruments, to the data flow and to the data processing for Planck are described, and an overview of the activities being carried out is provided.
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Citations
A simulation pipeline for the Planck mission
TL;DR: Tauber et al. as mentioned in this paper describe an assembly of numerical tools to model the output data of the Planck satellite, including data handling, data integrity checking, calibration, map making, physical component separation, and power spectrum estimation.
Foreground separation methods for satellite observations of the cosmic microwave background
TL;DR: In this article, a maximum entropy method (MEM) is presented for separating the emission due to different foreground components from simulated satellite observations of the cosmic microwave background radiation (CMBR), in particular, the method is applied to simulated observations by the proposed Planck Surveyor satellite.
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Davide Maino,A. Farusi,Carlo Baccigalupi,Francesca Perrotta,A. J. Banday,L. Bedini,Carlo Burigana,G. de Zotti,Krzysztof M. Gorski,Krzysztof M. Gorski,Emanuele Salerno +10 more
TL;DR: In this article, an independent component analysis (ICA) technique is proposed to recover the spatial pattern and the frequency scalings of the emissions from statistically independent astrophysical processes, present along the line-of-sight, from multi-frequency observations, without any a priori assumption on properties of the components to be separated, except that all of them, but at most one, must have non-Gaussian distributions.
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Combining maximum-entropy and the Mexican hat wavelet to reconstruct the microwave sky
P. Vielva,P. Vielva,R. B. Barreiro,Michael P. Hobson,Enrique Martínez-González,Anthony Lasenby,J. L. Sanz,L. Toffolatti +7 more
TL;DR: In this paper, a maximum entropy method (MEM) and Mexican Hat wavelet (MHW) joint analysis is presented to recover the different components of the microwave sky from simulated observations by the ESA Planck satellite in a small patch of the sky.
PLANCK LFI: Comparison between Galaxy Straylight Contamination and other systematic effects
Carlo Burigana,Davide Maino,Krzysztof M. Gorski,Krzysztof M. Gorski,N. Mandolesi,Marco Bersanelli,Fabrizio Villa,Luca Valenziano,Benjamin D. Wandelt,Michele Maltoni,Eric Hivon +10 more
TL;DR: In this paper, the authors evaluate the impact of the straylight contamination due to the Galactic emission (GSC, Galaxy Straylight Contamination) entering at large angles from the antenna center direction.
COBRAS/SAMBA. A mission dedicated to imaging the anisotropies of the cosmic microwave background. Report on the phase A study.
M. Bersanelli,F. R. Bouchet,George Efstathiou,Matthew Joseph Griffin,J.-M. Lamarre,N. Mandolesi,H. U. Norgaard-Nielsen,O. Pace,J. Polny,J. L. Puget,J. A. Tauber,Nicola Vittorio,Sergio Volonte +12 more
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Sharing data, information, and software for the ESA Planck mission: the IDIS prototype
K. Bennett,Fabio Pasian,Jean-Francois Sygnet,A. J. Banday,Matthias Bartelmann,Richard Gispert,Adam Hazell,William O'Mullane,Claudio Vuerli +8 more
TL;DR: An Integrated Data and Information System (IDIS) will be developed to allow proper intra-Consortium and inter-Consortia information exchange and a set of tools will be provided, maximizing use of Commercial Off-The-Shelf or reliable public domain software, to allow distributed collaborative research to be carried out.
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