相关论文: Archeops In-flight Performance, Data Processing an…

The Low Frequency Instrument in the ESA Planck mission

Measurements of the cosmic microwave background (CMB) allow high precision observation of the cosmic plasma at redshift z~1100. After the success of the NASA satellite COBE, that in 1992 provided the first detection of the CMB anisotropy,…

天体物理学 · 物理学 2009-11-10 A. Mennella , M. Bersanelli , B. Cappellini , D. Maino , P. Platania , S. Garavaglia , R. C. Butler , N. Mandolesi F. Pasian , O. D'arcangelo , A. Simonetto , C. Sozzi

A Map of the Cosmic Microwave Background from the BEAST Experiment

We present the first sky maps from the BEAST (Background Emission Anisotropy Scanning Telescope) experiment. BEAST consists of a 2.2 meter off axis Gregorian telescope fed by a cryogenic millimeter wavelength focal plane currently…

天体物理学 · 物理学 2007-05-23 Peter R. Meinhold , Marco Bersanelli , Jeffrey Childers , Newton Figueiredo , Todd C. Gaier , Doron Halevi , Charles R. Lawrence , Miikka Kangas , Alan Levy , Philip M. Lubin , Marco Malaspina , Nazzareno Mandolesi , Joshua Marvil , Jorge Mejia , Paolo Natoli , Ian O'Dwyer , Hugh O'Neill , Shane Parendo , Agenor Pina , Michael D. Seiffert , Nathan C. Stebor , Camilo Tello , Fabrizio Villa , Thyrso Villela , Benjamin D. Wandelt , Brian Williams , Carlos Alexandre Wuensche

Preparation to the CMB Planck analysis : contamination due to the polarized galactic emission

The Planck satellite experiment, which was launched the 14th of may 2009, will give an accurate measurement of the anisotropies of the Cosmic Microwave Background (CMB) in temperature and polarization. This measurement is polluted by the…

宇宙学与河外天体物理 · 物理学 2010-07-20 L. Fauvet , J. F. Macias-Perez

Imaging the first light: experimental challenges and future perspectives in the observation of the Cosmic Microwave Background Anisotropy

Measurements of the cosmic microwave background (CMB) allow high precision observation of the Last Scattering Surface at redshift $z\sim$1100. After the success of the NASA satellite COBE, that in 1992 provided the first detection of the…

天体物理学 · 物理学 2007-05-23 A. Mennella , C. Baccigalupi , A. Balbi , M. Bersanelli , C. Burigana , C. Butler , B. Cappellini , G. De Gasperis , F. Hansen , D. Maino , N. Mandolesi , M. Maris , G. Morgante , P. Natoli , F. Pasian , F. Perrotta , P. Platania , L. Valenziano , F. Villa , A. Zacchei

The Scientific Programme of Planck

For 40 years, the cosmic microwave background (CMB) has been the most important source of information about the geometry and contents of the Universe. Even so, only a small fraction of the information available in the CMB has been extracted…

天体物理学 · 物理学 2012-08-27 The Planck Collaboration

MAXIMA: A Balloon-Borne Cosmic Microwave Background Anisotropy Experiment

We describe the Millimeter wave Anisotropy eXperiment IMaging Array (MAXIMA), a balloon-borne experiment designed to measure the temperature anisotropy of the Cosmic Microwave Background (CMB) on angular scales of 10' to 5 degrees . MAXIMA…

天体物理学 · 物理学 2015-06-24 B. Rabii , C. D. Winant , M. E. Abroe , P. Ade , A. Balbi , J. J. Bock , J. Borrill , A. Boscaleri , P. de Bernardis , J. S. Collins , P. G. Ferreira , S. Hanany , V. V. Hristov , A. H. Jaffe , B. R. Johnson , A. E. Lange , A. T. Lee , C. B. Netterfield , E. Pascale , P. L. Richards , G. F. Smoot , R. Stompor , J. H. P. Wu

Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG

We present the BOOMERanG-03 experiment and maps of the Stokes parameters I, Q, U of the microwave sky obtained during a 14 day balloon flight in 2003. Three regions of the southern sky were surveyed: a deep survey (~ 90 square degrees) and…

天体物理学 · 物理学 2009-11-11 S Masi , P Ade , J Bock , J Bond , J Borrill , A Boscaleri , P Cabella , C Contaldi , B Crill , P de Bernardis , G De Gasperis , A de Oliveira-Costa , G De Troia , G Di Stefano , P Ehlers , E Hivon , V Hristov , A Iacoangeli , A Jaffe , W Jones , T Kisner , A Lange , C MacTavish , C Marini-Bettolo , P Mason , P Mauskopf , T Montroy , F Nati , L Nati , P Natoli , C Netterfield , E Pascale , F Piacentini , D Pogosyan , G Polenta , S Prunet , S Ricciardi , G Romeo , J Ruhl , P Santini , M Tegmark , E Torbet , M Veneziani , N Vittorio

Planck early results: first assessment of the High Frequency Instrument in-flight performance

The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six wide bands centered at 100, 143, 217, 353, 545 and 857 GHz at…

天体物理仪器与方法 · 物理学 2015-05-27 Planck HFI Core Team , P. A. R. Ade , N. Aghanim , R. Ansari , M. Arnaud , M. Ashdown , J. Aumont , A. J. Banday , M. Bartelmann , J. G. Bartlett , E. Battaner , K. Benabed , A. Benot , J. -P. Bernard , M. Bersanelli , R. Bhatia , J. J. Bock , J. R. Bond , J. Borrill , F. R. Bouchet , F. Boulanger , T. Bradshaw , E. Brelle , M. Bucher , P. Camus , J. -F. Cardoso , A. Catalano , A. Challinor , A. Chamballu , J. Charra , M. Charra , R. -R. Chary , C. Chiang , S. Church , D. L. Clements , S. Colombi , F. Couchot , A. Coulais , C. Cressiot , B. P. Crill , M. Crook , P. de Bernardis , J. Delabrouille , J. -M. Delouis , F. -X. Désert , K. Dolag , H. Dole , O. Doré , M. Douspis , G. Efstathiou , P. Eng , C. Filliard , O. Forni , P. Fosalba , J. -J. Fourmond , K. Ganga , M. Giard , D. Girard , Y. Giraud-Héraud , R. Gispert , K. M. Gorski , S. Gratton , M. Griffin , G. Guyot , J. Haissinski , D. Harrison , G. Helou , S. Henrot-Versillé , C. Hernandez-Monteagudo , S. R. Hildebrandt , R. Hills , E. Hivon , M. Hobson , W. A. Holmes , K. M. Huenberger , A. H. Jae , W. C. Jones , J. Kaplan , R. Kneissl , L. Knox , G. Lagache , J. -M. Lamarre , P. Lami , A. E. Lange , A. Lasenby , A. Lavabre , C. R. Lawrence , B. Leriche , C. Leroy , Y. Longval , J. F. Macas-Perez , T. Maciaszek , C. J. MacTavish , B. Maei , N. Mandolesi , R. Mann , B. Mansoux , S. Masi , T. Matsumura , P. McGehee , J. -B. Melin , C. Mercier , M. -A. Miville-Deschnes , A. Moneti , L. Montier , D. Mortlock , A. Murphy , F. Nati , C. B. Nettereld , H. U. Norgaard-Nielsen , C. North , F. Noviello , D. Novikov , S. Osborne , C. Paine , F. Pajot , G. Patanchon , T. Peacocke , T. J. Pearson , O. Perdereau , L. Perotto , F. Piacentini , M. Piat , S. Plaszczynski , E. Pointecouteau , R. Pons , N. Ponthieu , G. Prezeau , S. Prunet , J. -L. Puget , W. T. Reach , C. Renault , I. Ristorcelli , G. Rocha , C. Rosset , G. Roudier , M. Rowan-Robinson , B. Rusholme , D. Santos , G. Savini , B. M. Schaefer , P. Shellard , L. Spencer , J. -L. Starck , P. Stassi , V. Stolyarov , R. Stompor , R. Sudiwala , R. Sunyaev , J. -F. Sygnet , J. A. Tauber , C. Thum , J. -P. Torre , F. Touze , M. Tristram , F. Van Leeuwen , L. Vibert , D. Vibert , L. A. Wade , B. D. Wandelt , S. D. M. White , H. Wiesemeyer , A. Woodcraft , V. Yurchenko , D. Yvon , A. Zacchei

MAXIMA: Observations of CMB Anisotropy

This document describes the Millimeter Anisotropy eXperiment IMaging Array (MAXIMA), a balloon-borne experiment measuring the temperature anisotropy of the Cosmic Microwave Background (CMB) on angular scales of 10 arcminutes to 5 degrees.…

天体物理学 · 物理学 2011-11-09 Bahman Rabii

The Microwave Anisotropy Probe (MAP) Mission

The purpose of the MAP mission is to determine the geometry, content, and evolution of the universe via a 13 arcmin full-width-half-max (FWHM) resolution full sky map of the temperature anisotropy of the cosmic microwave background…

天体物理学 · 物理学 2008-11-26 C. L. Bennett , M. Bay , M. Halpern , G. Hinshaw , C. Jackson , N. Jarosik , A. Kogut , M. Limon , S. S. Meyer , L. Page , D. N. Spergel , G. S. Tucker , D. T. Wilkinson , E. Wollack , E. L. Wright

Current Status and Perspectives of Cosmic Microwave Background Observations

Measurements of the cosmic microwave background (CMB) radiation provide a unique opportunity for a direct study of the primordial cosmic plasma at redshift z ~1000. The angular power spectra of temperature and polarisation fluctuations are…

天体物理学 · 物理学 2009-11-10 Marco Bersanelli , Davide Maino , Aniello Mennella

Model of the polarized foreground diffuse Galactic emissions from 33 to 353 GHz

We present 3D models of the Galactic magnetic field including regular and turbulent components, and of the distribution of matter in the Galaxy including relativistic electrons and dust grains. By integrating along the line of sight, we…

星系天体物理 · 物理学 2013-03-26 L. Fauvet , J. F. Macías-Pérez , F. X. Désert

BOOMERanG: a scanning telescope for 10 arcminutes resolution CMB maps

The BOOMERanG experiment is a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and ten arcminutes. The experiment features a wide focal plane with 16…

天体物理学 · 物理学 2009-10-31 S. Masi , P. A. R. Ade , R. Artusa , J. J. Bock , A. Boscaleri , B. P. Crill , P. de Bernardis , G. De Troia , P. C. Farese , M. Giacometti , V. V. Hristov , A. Iacoangeli , A. E. Lange , A. T. Lee , L. Martinis , P. V. Mason , P. D. Mauskopf , F. Melchiorri , L. Miglio , T. Montroy , C. B. Netterfield , E. Pascale , F. Piacentini , P. L. Richards , G. Romeo , J. E. Ruhl , F. Scaramuzzi

Cosmic Microwave Background Observations in the Post-Planck Era

The Microwave Anisotropy Probe and Planck missions will provide low noise maps of the temperature of the cosmic microwave background (CMB). These maps will allow measurement of the power spectrum of the CMB with measurement noise below…

天体物理学 · 物理学 2007-05-23 J. B. Peterson , J. E. Carlstrom , E. S. Cheng , M. Kamionkowski , A. E. Lange , M. Seiffert , D. N. Spergel , A. Stebbins

MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

We present a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of MAXIMA. MAXIMA is a balloon-borne experiment with an array of 16 bolometric photometers operated at 100 mK.…

天体物理学 · 物理学 2009-10-31 S. Hanany , P. Ade , A. Balbi , J. Bock , J. Borrill , A. Boscaleri , P. de Bernardis , P. G. Ferreira , V. V. Hristov , A. H. Jaffe , A. E. Lange , A. T. Lee , P. D. Mauskopf , C. B. Netterfield , S. Oh , E. Pascale , B. Rabii , P. L. Richards , G. F. Smoot , R. Stompor , C. D. Winant , J. H. P. Wu

A Constraint on Primordial $B$-Modes from the First Flight of the SPIDER Balloon-Borne Telescope

We present the first linear polarization measurements from the 2015 long-duration balloon flight of SPIDER, an experiment designed to map the polarization of the cosmic microwave background (CMB) on degree angular scales. Results from these…

宇宙学与河外天体物理 · 物理学 2021-03-25 SPIDER Collaboration , P. A. R. Ade , M. Amiri , S. J. Benton , A. S. Bergman , R. Bihary , J. J. Bock , J. R. Bond , J. A. Bonetti , S. A. Bryan , H. C. Chiang , C. R. Contaldi , O. Doré , A. J. Duivenvoorden , H. K. Eriksen , M. Farhang , J. P. Filippini , A. A. Fraisse , K. Freese , M. Galloway , A. E. Gambrel , N. N. Gandilo , K. Ganga , R. Gualtieri , J. E. Gudmundsson , M. Halpern , J. Hartley , M. Hasselfield , G. Hilton , W. Holmes , V. V. Hristov , Z. Huang , K. D. Irwin , W. C. Jones , A. Karakci , C. L. Kuo , Z. D. Kermish , J. S. -Y. Leung , S. Li , D. S. Y. Mak , P. V. Mason , K. Megerian , L. Moncelsi , T. A. Morford , J. M. Nagy , C. B. Netterfield , M. Nolta , R. O'Brient , B. Osherson , I. L. Padilla , B. Racine , A. S. Rahlin , C. Reintsema , J. E. Ruhl , M. C. Runyan , T. M. Ruud , J. A. Shariff , E. C. Shaw , C. Shiu , J. D. Soler , X. Song , A. Trangsrud , C. Tucker , R. S. Tucker , A. D. Turner , J. F. van der List , A. C. Weber , I. K. Wehus , S. Wen , D. V. Wiebe , E. Y. Young

Mapping the CMB III: combined analysis of QMAP flights

We present results from the QMAP balloon experiment, which maps the Cosmic Microwave Background (CMB) and probes its angular power spectrum on degree scales. In two separate flights, data were taken in six channels at two frequency bands…

天体物理学 · 物理学 2009-10-30 Angelica de Oliveira-Costa , Mark Devlin , Tom Herbig , Amber Miller , Barth Netterfield , Lyman Page , Max Tegmark

MAXIPOL: A Balloon-borne Experiment for Measuring the Polarization Anisotropy of the Cosmic Microwave Background Radiation

We discuss MAXIPOL, a bolometric balloon-borne experiment designed to measure the E-mode polarization anisotropy of the cosmic microwave background radiation (CMB) on angular scales of 10 arcmin to 2 degrees. MAXIPOL is the first CMB…

天体物理学 · 物理学 2015-06-24 B. R. Johnson , M. E. Abroe , P. Ade , J. Bock , J. Borrill , J. S. Collins , P. Ferreira , S. Hanany , A. H. Jaffe , T. Jones , A. T. Lee , L. Levinson , T. Matsumura , B. Rabii , T. Renbarger , P. L. Richards , G. F. Smoot , R. Stompor , H. T. Tran , C. D. Winant

Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American test flight of BOOMERANG

We describe a measurement of the angular power spectrum of anisotropies in the Cosmic Microwave Background (CMB) from 0.3 degrees to ~10 degrees from the North American test flight of the BOOMERANG experiment. BOOMERANG is a balloon-borne…

天体物理学 · 物理学 2009-10-31 P. D. Mauskopf , P. A. R. Ade , P. de Bernardis , J. J. Bock , J. Borrill , A. Boscaleri , B. P. Crill , G. DeGasperis , G. De Troia , P. Farese , P. G. Ferreira , K. Ganga , M. Giacometti , S. Hanany , V. V. Hristov , A. Iacoangeli , A. H. Jaffe , A. E. Lange , A. T. Lee , S. Masi , A. Melchiorri , F. Melchiorri , L. Miglio , T. Montroy , C. B. Netterfield , E. Pascale , F. Piacentini , P. L. Richards , G. Romeo , J. E. Ruhl , E. Scannapieco , F. Scaramuzzi , R. Stompor , N. Vittorio

Observational Scan Induced Artificial CMB Anisotropy

To reliably detect the cosmic microwave background (CMB) anisotropy is of great importance in understanding the birth and evolution of the Universe. One of the difficulties in CMB experiments is the domination of measured CMB anisotropy…

宇宙学与河外天体物理 · 物理学 2011-04-28 Hao Liu , Ti-Pei Li