TY - JOUR
T1 - Recent developments in astrophysical and cosmological exploitation of microwave surveys
AU - Burigana, Carlo
AU - Davies, Rodney D.
AU - De Bernardis, Paolo
AU - Delabrouille, Jacques
AU - De Paolis, Francesco
AU - Douspis, Marian
AU - Khatri, Rishi
AU - Liu, Guo Chin
AU - Maris, Michele
AU - Masi, Silvia
AU - Mennella, Aniello
AU - Natoli, Paolo
AU - Norgaard-Nielsen, Hans Ulrik
AU - Pointecouteau, Etienne
AU - Rephaeli, Yoel
AU - Toffolatti, Luigi
N1 - Funding Information:
aPlanck is a project of the European Space Agency (ESA) with instruments provided by two scientific Consortia funded by ESA member states (in particular the lead countries: France and Italy) with contributions from NASA (USA), and telescope reflectors provided in a collaboration between ESA and a scientific Consortium led and funded by Denmark. bThis paper is based largely on the Planck Early Release Compact Source Catalogue (ERCSC) and publicly available publications by ESA and the Planck Collaboration, for what concerns the related aspects. Any material presented here that is not already described in Planck Collaboration papers represents the views of the authors and not necessarily those of the Planck Collaboration.
Funding Information:
We thank the Editorial Board of Astronomy and Astrophysics (European Southern Observatory; ESO) and the Editors of the Annual meeting of the French Society of Astronomy and Astrophysics for having granted us the permission to reproduce many figures originally published (or in press) in the same Journals or Proceedings. Some figures are reproduced with the permission of the American Astronomical Society (AAS). Credits are indicated when each reprinted figure is mentioned in the text for the first time. The authors that are members of the Planck Collaboration warmly thank the Planck Collaboration and, in particular, all the members of the Planck Working Groups 2, 5, 6, 7 and of the HFI and LFI Core Teams, with whom they shared the analysis and the interpretation of Planck data as for the subjects discussed here, and the members of the Planck Science Team and Editorial Board for the permission of publishing this paper. CB and PN wish to thank A. Gruppuso and N. Mandolesi, with whom they have carried out part of the work described in this paper. Some of the results in this paper have been derived using the HEALPIX77 package. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA) supported by the NASA Office of Space Science. Some of the simulations presented in this work have been performed using the computational facility of IASF Bologna and at CINECA. CB, MM, AM, PN acknowledge support by ASI through ASI/INAF Agreement I/072/09/0 for the Planck LFI Activity of Phase E2 and by MIUR through PRIN 2009 Grant No. 2009XZ54H2. EP acknowledges the support of ANR project Multiverse under grant ANR-11-BD56-015. LT acknowledges partial financial support from the Spanish Ministerio de Economía y Competitividad, under proyects AYA2010-21766-C03-01, AYA2012-39475-C02-01 and by the Consolider Ingenio-2010 Programme, project CSD2010-00064.
PY - 2013/5
Y1 - 2013/5
N2 - In this paper, we focus on the astrophysical results and the related cosmological implications derived from recent microwave surveys, with emphasis to those coming from the Planck mission. We critically discuss the impact of systematic effects and the role of methods to separate the cosmic microwave background (CMB) signal from the astrophysical emissions and each different astrophysical component from the others. We then review the state-of-the-art diffuse emissions, extragalactic sources, cosmic infrared background and galaxy clusters, addressing the information they provide to our global view of the cosmic structure evolution and for some crucial physical parameters, as the neutrino mass. Finally, we present three different kinds of scientific perspectives for fundamental physics and cosmology offered by the analysis of on-going and future CMB projects at different angular scales dedicated to anisotropies in total intensity and polarization and to absolute temperature.
AB - In this paper, we focus on the astrophysical results and the related cosmological implications derived from recent microwave surveys, with emphasis to those coming from the Planck mission. We critically discuss the impact of systematic effects and the role of methods to separate the cosmic microwave background (CMB) signal from the astrophysical emissions and each different astrophysical component from the others. We then review the state-of-the-art diffuse emissions, extragalactic sources, cosmic infrared background and galaxy clusters, addressing the information they provide to our global view of the cosmic structure evolution and for some crucial physical parameters, as the neutrino mass. Finally, we present three different kinds of scientific perspectives for fundamental physics and cosmology offered by the analysis of on-going and future CMB projects at different angular scales dedicated to anisotropies in total intensity and polarization and to absolute temperature.
KW - Cosmology
KW - Milky Way
KW - active galaxies
KW - cosmic background radiation
KW - galaxy clusters
KW - primordial galaxies
KW - zodiacal light
UR - https://www.scopus.com/pages/publications/84875359798
U2 - 10.1142/S0218271813300115
DO - 10.1142/S0218271813300115
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AN - SCOPUS:84875359798
SN - 0218-2718
VL - 22
JO - International Journal of Modern Physics D
JF - International Journal of Modern Physics D
IS - 6
M1 - 1330011
ER -