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Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time
Jacques Delabrouille,Jacques Delabrouille,Maximilian H. Abitbol,Nabila Aghanim,Yacine Ali-Haïmoud,David Alonso,David Alonso,Marcelo A. Alvarez,Marcelo A. Alvarez,A. J. Banday,James G. Bartlett,James G. Bartlett,Jochem J. A. Baselmans,Jochem J. A. Baselmans,Kaustuv Basu,Nicholas Battaglia,Jose Ramon Bermejo Climent,José Luis Bernal,Matthieu Béthermin,Boris Bolliet,Matteo Bonato,François R. Bouchet,Patrick C. Breysse,Carlo Burigana,Zhen-Yi Cai,Zhen-Yi Cai,Jens Chluba,Eugene Churazov,Helmut Dannerbauer,Paolo de Bernardis,Gianfranco De Zotti,Eleonora Di Valentino,Emanuela Dimastrogiovanni,Akira Endo,Akira Endo,Jens Erler,Simone Ferraro,Simone Ferraro,Fabio Finelli,Dale J. Fixsen,Shaul Hanany,Luke Hart,Carlos Hernández-Monteagudo,J. Colin Hill,Selim C. Hotinli,K. Karatsu,K. Karatsu,Kirit Karkare,Garrett K. Keating,I. Khabibullin,Alan J. Kogut,Kazunori Kohri,Ely D. Kovetz,Guilaine Lagache,Julien Lesgourgues,Mathew S. Madhavacheril,Bruno Maffei,N. Mandolesi,N. Mandolesi,Carlos Martins,Silvia Masi,John C. Mather,Jean-Baptiste Melin,Azadeh Moradinezhad Dizgah,Azadeh Moradinezhad Dizgah,Tony Mroczkowski,Suvodip Mukherjee,Daisuke Nagai,Mattia Negrello,Nathalie Palanque-Delabrouille,Daniela Paoletti,Subodh P. Patil,F. Piacentini,Srinivasan Raghunathan,Andrea Ravenni,Mathieu Remazeilles,V. Reveret,L. Rodriguez,Aditya Rotti,Jose Alberto Rubino Martin,Jack Sayers,Douglas Scott,Joseph Silk,Joseph Silk,Marta B. Silva,Tarun Souradeep,Naonori Sugiyama,R. A. Sunyaev,Eric R. Switzer,Andrea Tartari,Tiziana Trombetti,Íñigo Zubeldia +91 more
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TLDR
In this article, the authors proposed a spectro-polarimetric survey of the microwave sky using a broadband polarised imager and a moderate resolution spectroimager at the focus of a 3.5m aperture telescope actively cooled to about 8K.Abstract:
This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-dimensional distribution of hot gas, velocity flows, early metals, dust, and mass distribution in the entire Hubble volume, exploit CMB temperature and polarisation anisotropies down to fundamental limits, and track energy injection and absorption into the radiation background across cosmic times by measuring spectral distortions of the CMB blackbody emission. In addition to its exceptional capability for cosmology and fundamental physics, such a survey would provide an unprecedented view of microwave emissions at sub-arcminute to few-arcminute angular resolution in hundreds of frequency channels, a data set that would be of immense legacy value for many branches of astrophysics. We propose that this survey be carried-out with a large space mission featuring a broad-band polarised imager and a moderate resolution spectro-imager at the focus of a 3.5m aperture telescope actively cooled to about 8K, complemented with absolutely-calibrated Fourier Transform Spectrometer modules observing at degree-scale angular resolution in the 10-2000 GHz frequency range. We propose two observing modes: a survey mode to map the entire sky as well as a few selected wide fields, and an observatory mode for deeper observations of regions of specific interest.read more
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The optical system of the Tenerife Microwave Spectrometer: a window for observing the 10-20 GHz sky spectra
TL;DR: The TMS optical system is based on a decentered dual-reflector system in a Gregorian configuration to observe with an angular resolution of less than $2^\circ$. The primary goal of as mentioned in this paper is to evaluate the final design and verify that it satisfies the design requirements.
Posted Content
Reconstructing simulated CMB polarization power spectra with the Analytical Blind Separation method
TL;DR: In this article, the authors apply the ABS method to simulated polarization sky maps in order to test its ability in the recovery of the CMB $E$- and $B$-mode power spectra.
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ESO Staff Publications (2021)
TL;DR: The ESO Library maintains the ESO Telescope Bibliography (telbib) and is responsible for providing paper-based statistics as mentioned in this paper . But these statistics do not include papers that use data from non-ESO telescopes or observations obtained with hosted telescopes.
Proceedings ArticleDOI
BISOU: a balloon project for spectral observations of the early universe
Bruno Maffei,Nabila Aghanim,J. Aumont,Elia S. Battistelli,Jens Chluba,X. Coulon,P. de Bernardis,Marian Douspis,Julien Grain,J. C. Hill,Alan J. Kogut,Joseph Kuruvilla,Guilaine Lagache,J. F. Macías-Pérez,Silvia Masi,Tomotake Matsumura,L. Mele,Alessandro Monfardini,Créidhe O'Sullivan,L. Pagano,Giampaolo Pisano,N. Ponthieu,Mathieu Remazeilles,A. Ritacco,Aditya Rotti,Giorgio Savini,Valentin Sauvage,Alexey Shitvov,S. Stever,Andrea Tartari,Leander Thiele,Neil Trappe,Jean-François Aubrun,André Laurens,D. Pheav,F. Vacher +35 more
TL;DR: In this paper , a balloon-borne spectrometer, based on a Fourier Transform Spectrometer (FTS), is proposed for the measurement of the CMB spectral distortions.
Journal ArticleDOI
Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
Mattia Negrello,Matteo Bonato,Zhen-Yi Cai,Helmut Dannerbauer,Gianfranco De Zotti,Jacques Delabrouille,Douglas Scott +6 more
TL;DR: In this paper, a far-IR/submm all-sky spectroscopic survey with a 3m-class space telescope is presented, which provides a 3D view of the universe and allows us to take full advantage of the sensitivity of present-day instrumentation.
References
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The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
Joop Schaye,Robert A. Crain,Richard G. Bower,Michelle Furlong,Matthieu Schaller,Tom Theuns,Tom Theuns,Claudio Dalla Vecchia,Claudio Dalla Vecchia,Carlos S. Frenk,Ian G. McCarthy,John C. Helly,Adrian Jenkins,Yetli Rosas-Guevara,Simon D. M. White,Maarten Baes,C. M. Booth,C. M. Booth,Peter Camps,Julio F. Navarro,Yan Qu,Alireza Rahmati,Till Sawala,Peter A. Thomas,James W. Trayford +24 more
TL;DR: The Virgo Consortium's EAGLE project as discussed by the authors is a suite of hydrodynamical simulations that follow the formation of galaxies and black holes in representative volumes, where thermal energy is injected into the gas, allowing winds to develop without predetermined speed or mass loading factors.
Journal ArticleDOI
Results from a Search for Dark Matter in the Complete LUX Exposure
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,R. Bramante,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon experiment are reported.
Journal ArticleDOI
Dark Matter Results from 225 Live Days of XENON100 Data
Elena Aprile,M. Alfonsi,K. Arisaka,F. Arneodo,C. Balan,Laura Baudis,Boris Bauermeister,A. Behrens,P. Beltrame,K. Bokeloh,Ethan Brown,Giacomo Bruno,Ran Budnik,João Cardoso,W. T. Chen,B. Choi,David B. Cline,Auke-Pieter Colijn,H. Contreras,Jean-Pierre Cussonneau,M. P. Decowski,Ehud Duchovni,S. Fattori,A. D. Ferella,W. Fulgione,F. Gao,M. Garbini,C. Ghag,K. L. Giboni,Luke Goetzke,C. Grignon,Eilam Gross,W. Hampel,Florian Kaether,A. Kish,J. Lamblin,H. Landsman,R. F. Lang,R. F. Lang,M. Le Calloch,C. Levy,K. E. Lim,Qing Lin,Sebastian Lindemann,Manfred Lindner,J. A. M. Lopes,K. Lung,T. Marrodán Undagoitia,F. V. Massoli,A. J. Melgarejo Fernandez,Y. Meng,A. Molinario,E. Nativ,Kaixuan Ni,Uwe Oberlack,Uwe Oberlack,S. E. A. Orrigo,E. Pantic,R. Persiani,G. Plante,N. Priel,A. Rizzo,S. Rosendahl,J.M.F. dos Santos,G. Sartorelli,Jochen Schreiner,Marc Schumann,L. Scotto Lavina,P. R. Scovell,M. Selvi,P. Shagin,Hardy Simgen,A. Teymourian,D. Thers,O. Vitells,Hui Wang,M. Weber,Ch. Weinheimer +77 more
TL;DR: A search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012, has yielded no evidence for dark matter interactions.
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