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Measurement of the largest angular scale ($\ell < 30$) features of the cosmic microwave background (CMB) polarization is a powerful way to constrain the optical depth to reionization and search for the signature of inflation through the…

This paper investigates the impact of mutual coupling on MIMO systems with densely deployed antennas. Leveraging multiport communication theory, we analyze both coherent and noncoherent detection approaches in a single-user uplink scenario…

Signal Processing · Electrical Eng. & Systems 2026-01-08 Aniol Martí , Luca Sanguinetti , Jaume Riba , Meritxell Lamarca

We consider reflector imaging in a weakly random waveguide. We address the situation in which the source is farther from the reflector to be imaged than the energy equipartition distance, but the receiver array is closer to the reflector to…

Analysis of PDEs · Mathematics 2013-04-17 Habib Ammari , Josselin Garnier , Wenjia Jing

We show that the epoch(s) of reionization when the ionization fraction of the universe is about half can be determined by correlating Cosmic Microwave Background (CMB) temperature maps with 21-cm line maps at degree scales ($l\sim 100$).…

Astrophysics · Physics 2009-11-13 Marcelo A. Alvarez , Eiichiro Komatsu , Olivier Doré , Paul R. Shapiro

A new pixel detector for the CMS experiment was built in order to cope with the instantaneous luminosities anticipated for the Phase~I Upgrade of the LHC. The new CMS pixel detector provides four-hit tracking with a reduced material budget…

Instrumentation and Detectors · Physics 2017-06-02 M. Dragicevic , M. Friedl , J. Hrubec , H. Steininger , A. Gädda , J. Härkönen , T. Lampén , P. Luukka , T. Peltola , E. Tuominen , E. Tuovinen , A. Winkler , P. Eerola , T. Tuuva , G. Baulieu , G. Boudoul , L. Caponetto , C. Combaret , D. Contardo , T. Dupasquier , G. Gallbit , N. Lumb , L. Mirabito , S. Perries , M. Vander Donckt , S. Viret , C. Bonnin , L. Charles , L. Gross , J. Hosselet , D. Tromson , L. Feld , W. Karpinski , K. Klein , M. Lipinski , G. Pierschel , M. Preuten , M. Rauch , M. Wlochal , M. Aldaya , C. Asawatangtrakuldee , K. Beernaert , D. Bertsche , C. Contreras-Campana , G. Eckerlin , D. Eckstein , T. Eichhorn , E. Gallo , J. Garay Garcia , K. Hansen , M. Haranko , A. Harb , J. Hauk , J. Keaveney , A. Kalogeropoulos , C. Kleinwort , W. Lohmann , R. Mankel , H. Maser , G. Mittag , C. Muhl , A. Mussgiller , D. Pitzl , O. Reichelt , M. Savitskyi , P. Schütze , V. Sola , S. Spannagel , R. Walsh , A. Zuber , H. Biskop , P. Buhmann , M. Centis-Vignali , E. Garutti , J. Haller , M. Hoffmann , R. Klanner , T. Lapsien , M. Matysek , A. Perieanu , Ch. Scharf , P. Schleper , A. Schmidt , J. Schwandt , J. Sonneveld , G. Steinbrück , B. Vormwald , J. Wellhausen , M. Abbas , C. Amstutz , T. Barvich , Ch. Barth , F. Boegelspacher , W. De Boer , E. Butz , M. Casele , F. Colombo , A. Dierlamm , B. Freund , F. Hartmann , S. Heindl , U. Husemann , A. Kornmeyer , S. Kudella , Th. Muller , H. J. Simonis , P. Steck , M. Weber , Th. Weiler , T. Kiss , F. Siklér , T. Tölyhi , V. Veszprémi , P. Cariola , D. Creanza , M. De Palma , G. De Robertis , L. Fiore , M. Franco , F. Loddo , G. Sala , L. Silvestris , G. Maggi , S. My , G. Selvaggi , S. Albergo , G. Cappello , S. Costa , A. Di Mattia , F. Giordano , R. Potenza , M. A. Saizu , A. Tricomi , C. Tuve , E. Focardi , M. E. Dinardo , S. Fiorendi , S. Gennai , S. Malvezzi , R. A. Manzoni , D. Menasce , L. Moroni , D. Pedrini , P. Azzi , N. Bacchetta , D. Bisello , M. Dall'Osso , N. Pozzobon , M. Tosi , L. Alunni Solestizi , M. Biasini , G. M. Bilei , C. Cecchi , B. Checcucci , D. Ciangottini , L. Fanò , C. Gentsos , M. Ionica , R. Leonardi , E. Manoni , G. Mantovani , S. Marconi , V. Mariani , M. Menichelli , A. Modak , A. Morozzi , F. Moscatelli , D. Passeri , P. Placidi , V. Postolache , A. Rossi , A. Saha , A. Santocchia , L. Storchi , D. Spiga , K. Androsov , P. Azzurri , G. Bagliesi , A. Basti , T. Boccali , L. Borrello , F. Bosi , R. Castaldi , M. Ceccanti , M. A. Ciocci , R. Dell'Orso , S. Donato , G. Fedi , A. Giassi , M. T. Grippo , F. Ligabue , G. Magazzu , P. Mammini , F. Mariani , E. Mazzoni , A. Messineo , A. Moggi , F. Morsani , F. Palla , F. Palmonari , A. Profeti , F. Raffaelli , A. Ragonesi , A. Rizzi , A. Soldani , P. Spagnolo , R. Tenchini , G. Tonelli , A. Venturi , P. G. Verdini , D. Abbaneo , I. Ahmed , E. Albert , G. Auzinger , G. Berruti , J. Bonnaud , J. Daguin , A. D'Auria , S. Detraz , O. Dondelewski , B. Engegaard , F. Faccio , N. Frank , K. Gill , A. Honma , A. Kornmayer , A. Labaza , F. Manolescu , I. McGill , S. Mersi , S. Michelis , A. Onnela , M. Ostrega , S. Pavis , A. Peisert , J. -F. Pernot , P. Petagna , H. Postema , K. Rapacz , C. Sigaud , P. Tropea , J. Troska , A. Tsirou , F. Vasey , B. Verlaat , P. Vichoudis , L. Zwalinski , F. Bachmair , R. Becker , D. di Calafiori , B. Casal , P. Berger , L. Djambazov , M. Donega , C. Grab , D. Hits , J. Hoss , G. Kasieczka , W. Lustermann , B. Mangano , M. Marionneau , P. Martinez Ruiz del Arbol , M. Masciovecchio , M. Meinhard , L. Perozzi , U. Roeser , A. Starodumov , V. Tavolaro , R. Wallny , D. Zhu , K. Bösiger , L. Caminada , F. Canelli , V. Chiochia , A. de Cosa , C. Galloni , T. Hreus , B. Kilminster , C. Lange , R. Maier , J. Ngadiuba , D. Pinna , P. Robmann , S. Taroni , Y. Yang , W. Bertl , K. Deiters , W. Erdmann , R. Horisberger , H. -C. Kaestli , D. Kotlinski , U. Langenegger , B. Meier , T. Rohe , S. Streuli , P. -H. Chen , C. Dietz , F. Fiori , U. Grundler , W. -S. Hou , R. -S. Lu , M. Moya , J. -F. Tsai , Y. M. Tzeng , D. Cussans , J. Goldstein , M. Grimes , D. Newbold , P. Hobson , I. D. Reid , G. Auzinger , R. Bainbridge , P. Dauncey , G. Hall , T. James , A. -M. Magnan , M. Pesaresi , D. M. Raymond , K. Uchida , T. Durkin , K. Harder , C. Shepherd-Themistocleous , M. Chertok , J. Conway , R. Conway , C. Flores , R. Lander , D. Pellett , F. Ricci-Tam , M. Squires , J. Thomson , R. Yohay , K. Burt , J. Ellison , G. Hanson , M. Olmedo , W. Si , B. R. Yates , A. Dominguez , R. Bartek , B. Bentele , J. P. Cumalat , W. T. Ford , F. Jensen , A. Johnson , M. Krohn , S. Leontsinis , T. Mulholland , K. Stenson , S. R. Wagner , A. Apresyan , G. Bolla , K. Burkett , J. N. Butler , A. Canepa , H. W. K. Cheung , D. Christian , W. E. Cooper , G. Deptuch , G. Derylo , C. Gingu , S. Grünendahl , S. Hasegawa , J. Hoff , J. Howell , M. Hrycyk , S. Jindariani , M. Johnson , F. Kahlid , S. Kwan , C. M. Lei , R. Lipton , R. Lopes De Sá , T. Liu , S. Los , M. Matulik , P. Merkel , S. Nahn , A. Prosser , R. Rivera , B. Schneider , G. Sellberg , A. Shenai , K. Siehl , L. Spiegel , N. Tran , L. Uplegger , E. Voirin , D. R. Berry , X. Chen , L. Ennesser , A. Evdokimov , C. E. Gerber , S. Makauda , C. Mills , I. D. Sandoval Gonzalez , J. Alimena , L. J. Antonelli , B. Francis , A. Hart , C. S. Hill , N. Parashar , J. Stupak , D. Bortoletto , M. Bubna , N. Hinton , M. Jones , D. H. Miller , X. Shi , P. Baringer , A. Bean , S. Khalil , A. Kropivnitskaya , D. Majumder , E. Schmitz , G. Wilson , A. Ivanov , R. Mendis , T. Mitchell , N. Skhirtladze , R. Taylor , I. Anderson , D. Fehling , A. Gritsan , P. Maksimovic , C. Martin , K. Nash , M. Osherson , M. Swartz , M. Xiao , J. G. Acosta , L. M. Cremaldi , S. Oliveros , L. Perera , D. Summers , K. Bloom , D. R. Claes , C. Fangmeier , R. Gonzalez Suarez , J. Monroy , J. Siado , E. Bartz , Y. Gershtein , E. Halkiadakis , S. Kyriacou , A. Lath , K. Nash , M. Osherson , S. Schnetzer , R. Stone , M. Walker , S. Malik , S. Norberg , J. E. Ramirez Vargas , M. Alyari , J. Dolen , A. Godshalk , C. Harrington , I. Iashvili , A. Kharchilava , D. Nguyen , A. Parker , S. Rappoccio , B. Roozbahani , J. Alexander , J. Chaves , J. Chu , S. Dittmer , K. McDermott , N. Mirman , A. Rinkevicius , A. Ryd , E. Salvati , L. Skinnari , L. Soffi , Z. Tao , J. Thom , J. Tucker , M. Zientek , B. Akgün , K. M. Ecklund , M. Kilpatrick , T. Nussbaum , J. Zabel , P. D'Angelo , W. Johns , K. Rose

Multichroic polarization sensitive detectors enable increased sensitivity and spectral coverage for observations of the Cosmic Microwave Background (CMB). An array optimized for dual frequency detectors can provide 1.7 times gain in…

The Simons Observatory (SO) will make precise temperature and polarization measurements of the cosmic microwave background (CMB) using a set of telescopes which will cover angular scales between 1 arcminute and tens of degrees, contain over…

We present a novel algorithm for high resolution coherent imaging of sound sources in random scattering media using time resolved measurements of the acoustic pressure at an array of receivers. The sound waves travel a long distance between…

Numerical Analysis · Mathematics 2017-12-15 Liliana Borcea , Ilker Kocyigit

We show that the sensitivity of antenna-coupled field-effect transistors (FETs) to terahertz (THz) radiation improves continuously with decreasing temperature. The noise-equivalent power (NEP) of 540 GHz patch-antenna-coupled FETs decreases…

BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad…

We are developing multi-chroic antenna-coupled TES detectors for CMB polarimetry. Multi-chroic detectors increase the mapping speed per focal plane area and provide greater discrimination of polarized galactic foregrounds with no increase…

The DEPFET collaboration develops highly granular, ultra-transparent active pixel detectors for high-performance vertex reconstruction at future collider experiments. The characterization of detector prototypes has proven that the key…

We report a measurement of the E-mode polarization power spectrum of the cosmic microwave background (CMB) using 150 GHz data taken from July 2014 to December 2016 with the POLARBEAR experiment. We reach an effective polarization map noise…

High order modulation formats constitute the most prominent way for increasing spectral efficiency in transmission systems. Coherent transceivers that support such higher order formats require heavy digital signal processing (DSP), which…

We developed a method based on crossed polarizers to observe high-contrast coherent population trapping (CPT) resonance. Since crossed polarizers have a simple optical system, our method is suitable for chip-scale atomic clocks (CSACs). We…

Atomic Physics · Physics 2014-12-16 Yuichiro Yano , Shigeyoshi Goka

Using analytical methods and Monte Carlo simulations, we analyze a new statistic designed to detect isolated step-like discontinuities which are coherent over large areas of Cosmic Microwave Background (CMB) pixel maps. Such coherent…

Astrophysics · Physics 2007-05-23 Leandros Perivolaropoulos

We analyse the feasibility of detecting the polarization of the CMB caused by scattering of the remote temperature quadrupole by galaxy clusters with forthcoming CMB polarization surveys. For low-redshift clusters, the signal is strongly…

Cosmology and Nongalactic Astrophysics · Physics 2014-09-24 Alex Hall , Anthony Challinor

Present cosmic microwave background (CMB) observations have significantly advanced our understanding of the universe's origin, especially with primordial gravitational waves (PGWs). Currently, ground-based CMB telescopes are mainly located…

Cosmology and Nongalactic Astrophysics · Physics 2024-08-02 Dongdong Zhang , Bo Wang , Jia-Rui Li , Yi-Fu Cai , Chang Feng