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High space-bandwidth product with high spatial phase sensitivity is indispensable for a single-shot quantitative phase microscopy (QPM) system. It opens avenue for widespread applications of QPM in the field of biomedical imaging.…

Complex periodic variables (CPVs) are stars that exhibit highly structured and periodic optical light curves. Previous studies have indicated that these stars are typically disk-free pre-main-sequence M dwarfs with rotation periods ranging…

The VST Optical Imaging of the CDFS and ES1 Fields (VOICE) Survey is a Guaranteed Time program carried out with the ESO/VST telescope to provide deep optical imaging over two 4 deg$^2$ patches of the sky centred on the CDFS and ES1…

In the last years, high-resolution time tagging has emerged as the tool to tackle the problem of high-track density in the detectors of the next generation of experiments at particle colliders. Time resolutions below 50ps and event average…

High-cadence multi-band imaging and polarimetry have important scientific applications in astronomy. Observations of transits of exoplanets are a particular application that requires robust data reduction and analysis. We present the SPARC4…

This paper addresses simultaneous, high-precision measurement and analysis of generic reference signals by using inexpensive commercial off-the-shelf Software Defined Radio hardware. Sine reference signals are digitally down-converted to…

Signal Processing · Electrical Eng. & Systems 2018-04-12 Carsten Andrich , Alexander Ihlow , Julia Bauer , Niklas Beuster , Giovanni Del Galdo

Multicolor Panoramic Photometer-Polarimeter (MPPP) with a time resolution of 1 microsecond has been built based on a PSD and used at the 6-meter telescope in SAO (Russia). The device allows registration of the photon fluxes in four…

Astrophysics · Physics 2015-06-24 V. Plokhotnichenko , G. Beskin , V. Debur , A. Panferov , I. Panferova

Data from the Transiting Exoplanet Survey Satellite (TESS) has produced of order one million light curves at cadences of 120 s and especially 1800 s for every ~27-day observing sector during its two-year nominal mission. These data…

We present -- and make publicly available -- accurate and precise photometric redshifts in the ACS footprint from the COSMOS field for objects with $i_{\mathrm{AB}}\leq 23$. The redshifts are computed using a combination of narrow band…

Precision pulsar timing can be used for a variety of astrophysical tests from the detection of gravitational waves to probing the properties of the interstellar medium (ISM). Here we present analyses of the noise contributions to pulsar…

High Energy Astrophysical Phenomena · Physics 2020-02-20 Brent J. Shapiro-Albert , Maura A. McLaughlin , Michael T. Lam , James M. Cordes , Joe K. Swiggum

Stellar oscillations appear all across the Hertzsprung-Russell diagram. Recent theoretical studies support their existence also in the atmospheres of M dwarfs. These studies predict for them short periodicities ranging from 20~min to 3~h.…

3I/ATLAS is the third known interstellar object to pass through our Solar System. NASA's Transiting Exoplanet Survey Satellite (TESS) made dedicated observations of 3I/ATLAS between 15 -- 22 January 2026 (Sector 1751), capturing…

Earth and Planetary Astrophysics · Physics 2026-02-16 Jorge Martinez-Palomera , Amy Tuson , TESS Science Support Center

Maps of the sky in millimeter wavelengths contain rich information on cosmology through anisotropies of the cosmic microwave background (CMB). Creating multifrequency sky maps of anisotropies in the $I$, $Q$, and $U$ Stokes parameters is…

Photomultiplier tubes (PMTs) are widely deployed at neutrino and dark matter experiments for photon counting. When multiple photons hit a PMT consecutively, their photo-electron (PE) pulses pile up to hinder the precise measurements of the…

High Energy Physics - Experiment · Physics 2025-09-12 Yuyi Wang , Aiqiang Zhang , Yiyang Wu , Benda Xu , Xuewei Liu , Jiajie Chen , Zhe Wang , Shaomin Chen

We present MESS, a fully automated algorithm for identifying and characterizing double-lined spectroscopic binaries (SB2) in large databases of multi-epoch spectra. MESS extends the two-dimensional TODCOR approach to a global multi-epoch…

Solar and Stellar Astrophysics · Physics 2026-02-06 Gil Nachmani , Simchon Faigler , Tsevi Mazeh

We describe an ongoing search for pulsars and dispersed pulses of radio emission, such as those from rotating radio transients (RRATs) and fast radio bursts (FRBs), at 350 MHz using the Green Bank Telescope. With the Green Bank Ultimate…

Exclusive $J/\psi$ and $\psi(2S)$ vector meson production has been observed in the dimuon channel using the LHCb detector. The cross-section times branching fractions to two muons with pseudorapidities between 2.0 and 4.5 are measured to be…

High Energy Physics - Experiment · Physics 2013-03-04 LHCb collaboration , R. Aaij , C. Abellan Beteta , A. Adametz , B. Adeva , M. Adinolfi , C. Adrover , A. Affolder , Z. Ajaltouni , J. Albrecht , F. Alessio , M. Alexander , S. Ali , G. Alkhazov , P. Alvarez Cartelle , A. A. Alves , S. Amato , Y. Amhis , L. Anderlini , J. Anderson , R. Andreassen , R. B. Appleby , O. Aquines Gutierrez , F. Archilli , A. Artamonov , M. Artuso , E. Aslanides , G. Auriemma , S. Bachmann , J. J. Back , C. Baesso , V. Balagura , W. Baldini , R. J. Barlow , C. Barschel , S. Barsuk , W. Barter , Th. Bauer , A. Bay , J. Beddow , I. Bediaga , S. Belogurov , K. Belous , I. Belyaev , E. Ben-Haim , M. Benayoun , G. Bencivenni , S. Benson , J. Benton , A. Berezhnoy , R. Bernet , M. -O. Bettler , M. van Beuzekom , A. Bien , S. Bifani , T. Bird , A. Bizzeti , P. M. Bjørnstad , T. Blake , F. Blanc , C. Blanks , J. Blouw , S. Blusk , A. Bobrov , V. Bocci , A. Bondar , N. Bondar , W. Bonivento , S. Borghi , A. Borgia , T. J. V. Bowcock , E. Bowen , C. Bozzi , T. Brambach , J. van den Brand , J. Bressieux , D. Brett , M. Britsch , T. Britton , N. H. Brook , H. Brown , I. Burducea , A. Bursche , J. Buytaert , S. Cadeddu , O. Callot , M. Calvi , M. Calvo Gomez , A. Camboni , P. Campana , A. Carbone , G. Carboni , R. Cardinale , A. Cardini , H. Carranza-Mejia , L. Carson , K. Carvalho Akiba , G. Casse , M. Cattaneo , Ch. Cauet , M. Charles , Ph. Charpentier , P. Chen , N. Chiapolini , M. Chrzaszcz , K. Ciba , X. Cid Vidal , G. Ciezarek , P. E. L. Clarke , M. Clemencic , H. V. Cliff , J. Closier , C. Coca , V. Coco , J. Cogan , E. Cogneras , P. Collins , A. Comerma-Montells , A. Contu , A. Cook , M. Coombes , G. Corti , B. Couturier , G. A. Cowan , D. Craik , S. Cunliffe , R. Currie , C. D'Ambrosio , P. David , P. N. Y. David , I. De Bonis , K. De Bruyn , S. De Capua , M. De Cian , J. M. De Miranda , L. De Paula , W. De Silva , P. De Simone , D. Decamp , M. Deckenhoff , H. Degaudenzi , L. Del Buono , C. Deplano , D. Derkach , O. Deschamps , F. Dettori , A. Di Canto , J. Dickens , H. Dijkstra , P. Diniz Batista , M. Dogaru , F. Domingo Bonal , S. Donleavy , F. Dordei , A. Dosil Suárez , D. Dossett , A. Dovbnya , F. Dupertuis , R. Dzhelyadin , A. Dziurda , A. Dzyuba , S. Easo , U. Egede , V. Egorychev , S. Eidelman , D. van Eijk , S. Eisenhardt , U. Eitschberger , R. Ekelhof , L. Eklund , I. El Rifai , Ch. Elsasser , D. Elsby , A. Falabella , C. Färber , G. Fardell , C. Farinelli , S. Farry , V. Fave , D. Ferguson , V. Fernandez Albor , F. Ferreira Rodrigues , M. Ferro-Luzzi , S. Filippov , C. Fitzpatrick , M. Fontana , F. Fontanelli , R. Forty , O. Francisco , M. Frank , C. Frei , M. Frosini , S. Furcas , E. Furfaro , A. Gallas Torreira , D. Galli , M. Gandelman , P. Gandini , Y. Gao , J. Garofoli , P. Garosi , J. Garra Tico , L. Garrido , C. Gaspar , R. Gauld , E. Gersabeck , M. Gersabeck , T. Gershon , Ph. Ghez , V. Gibson , V. V. Gligorov , C. Göbel , D. Golubkov , A. Golutvin , A. Gomes , H. Gordon , M. Grabalosa Gándara , R. Graciani Diaz , L. A. Granado Cardoso , E. Graugés , G. Graziani , A. Grecu , E. Greening , S. Gregson , O. Grünberg , B. Gui , E. Gushchin , Yu. Guz , T. Gys , C. Hadjivasiliou , G. Haefeli , C. Haen , S. C. Haines , S. Hall , T. Hampson , S. Hansmann-Menzemer , N. Harnew , S. T. Harnew , J. Harrison , P. F. Harrison , T. Hartmann , J. He , V. Heijne , K. Hennessy , P. Henrard , J. A. Hernando Morata , E. van Herwijnen , E. Hicks , D. Hill , M. Hoballah , C. Hombach , P. Hopchev , W. Hulsbergen , P. Hunt , T. Huse , N. Hussain , D. Hutchcroft , D. Hynds , V. Iakovenko , P. Ilten , R. Jacobsson , A. Jaeger , E. Jans , F. Jansen , P. Jaton , F. Jing , M. John , D. Johnson , C. R. Jones , B. Jost , M. Kaballo , S. Kandybei , M. Karacson , T. M. Karbach , I. R. Kenyon , U. Kerzel , T. Ketel , A. Keune , B. Khanji , O. Kochebina , I. Komarov , R. F. Koopman , P. Koppenburg , M. Korolev , A. Kozlinskiy , L. Kravchuk , K. Kreplin , M. Kreps , G. Krocker , P. Krokovny , F. Kruse , M. Kucharczyk , V. Kudryavtsev , T. Kvaratskheliya , V. N. La Thi , D. Lacarrere , G. Lafferty , A. Lai , D. Lambert , R. W. Lambert , E. Lanciotti , G. Lanfranchi , C. Langenbruch , T. Latham , C. Lazzeroni , R. Le Gac , J. van Leerdam , J. -P. Lees , R. Lefèvre , A. Leflat , J. Lefrançois , O. Leroy , Y. Li , L. Li Gioi , M. Liles , R. Lindner , C. Linn , B. Liu , G. Liu , J. von Loeben , J. H. Lopes , E. Lopez Asamar , N. Lopez-March , H. Lu , J. Luisier , H. Luo , F. Machefert , I. V. Machikhiliyan , F. Maciuc , O. Maev , S. Malde , G. Manca , G. Mancinelli , N. Mangiafave , U. Marconi , R. Märki , J. Marks , G. Martellotti , A. Martens , L. Martin , A. Martín Sánchez , M. Martinelli , D. Martinez Santos , D. Martins Tostes , A. Massafferri , R. Matev , Z. Mathe , C. Matteuzzi , M. Matveev , E. Maurice , A. Mazurov , J. McCarthy , R. McNulty , B. Meadows , F. Meier , M. Meissner , M. Merk , D. A. Milanes , M. -N. Minard , J. Molina Rodriguez , S. Monteil , D. Moran , P. Morawski , R. Mountain , I. Mous , F. Muheim , K. Müller , R. Muresan , B. Muryn , B. Muster , P. Naik , T. Nakada , R. Nandakumar , I. Nasteva , M. Needham , N. Neufeld , A. D. Nguyen , T. D. Nguyen , C. Nguyen-Mau , M. Nicol , V. Niess , R. Niet , N. Nikitin , T. Nikodem , S. Nisar , A. Nomerotski , A. Novoselov , A. Oblakowska-Mucha , V. Obraztsov , S. Oggero , S. Ogilvy , O. Okhrimenko , R. Oldeman , M. Orlandea , J. M. Otalora Goicochea , P. Owen , B. K. Pal , A. Palano , M. Palutan , J. Panman , A. Papanestis , M. Pappagallo , C. Parkes , C. J. Parkinson , G. Passaleva , G. D. Patel , M. Patel , G. N. Patrick , C. Patrignani , C. Pavel-Nicorescu , A. Pazos Alvarez , A. Pellegrino , G. Penso , M. Pepe Altarelli , S. Perazzini , D. L. Perego , E. Perez Trigo , A. Pérez-Calero Yzquierdo , P. Perret , M. Perrin-Terrin , G. Pessina , K. Petridis , A. Petrolini , A. Phan , E. Picatoste Olloqui , B. Pietrzyk , T. Pilař , D. Pinci , S. Playfer , M. Plo Casasus , F. Polci , G. Polok , A. Poluektov , E. Polycarpo , D. Popov , B. Popovici , C. Potterat , A. Powell , J. Prisciandaro , V. Pugatch , A. Puig Navarro , W. Qian , J. H. Rademacker , B. Rakotomiaramanana , M. S. Rangel , I. Raniuk , N. Rauschmayr , G. Raven , S. Redford , M. M. Reid , A. C. dos Reis , S. Ricciardi , A. Richards , K. Rinnert , V. Rives Molina , D. A. Roa Romero , P. Robbe , E. Rodrigues , P. Rodriguez Perez , G. J. Rogers , S. Roiser , V. Romanovsky , A. Romero Vidal , J. Rouvinet , T. Ruf , H. Ruiz , G. Sabatino , J. J. Saborido Silva , N. Sagidova , P. Sail , B. Saitta , C. Salzmann , B. Sanmartin Sedes , M. Sannino , R. Santacesaria , C. Santamarina Rios , E. Santovetti , M. Sapunov , A. Sarti , C. Satriano , A. Satta , M. Savrie , D. Savrina , P. Schaack , M. Schiller , H. Schindler , S. Schleich , M. Schlupp , M. Schmelling , B. Schmidt , O. Schneider , A. Schopper , M. -H. Schune , R. Schwemmer , B. Sciascia , A. Sciubba , M. Seco , A. Semennikov , K. Senderowska , I. Sepp , N. Serra , J. Serrano , P. Seyfert , M. Shapkin , I. Shapoval , P. Shatalov , Y. Shcheglov , T. Shears , L. Shekhtman , O. Shevchenko , V. Shevchenko , A. Shires , R. Silva Coutinho , T. Skwarnicki , N. A. Smith , E. Smith , M. Smith , K. Sobczak , M. D. Sokoloff , F. J. P. Soler , F. Soomro , D. Souza , B. Souza De Paula , B. Spaan , A. Sparkes , P. Spradlin , F. Stagni , S. Stahl , O. Steinkamp , S. Stoica , S. Stone , B. Storaci , M. Straticiuc , U. Straumann , V. K. Subbiah , S. Swientek , V. Syropoulos , M. Szczekowski , P. Szczypka , T. Szumlak , S. T'Jampens , M. Teklishyn , E. Teodorescu , F. Teubert , C. Thomas , E. Thomas , J. van Tilburg , V. Tisserand , M. Tobin , S. Tolk , D. Tonelli , S. Topp-Joergensen , N. Torr , E. Tournefier , S. Tourneur , M. T. Tran , M. Tresch , A. Tsaregorodtsev , P. Tsopelas , N. Tuning , M. Ubeda Garcia , A. Ukleja , D. Urner , U. Uwer , V. Vagnoni , G. Valenti , R. Vazquez Gomez , P. Vazquez Regueiro , S. Vecchi , J. J. Velthuis , M. Veltri , G. Veneziano , M. Vesterinen , B. Viaud , D. Vieira , X. Vilasis-Cardona , A. Vollhardt , D. Volyanskyy , D. Voong , A. Vorobyev , V. Vorobyev , C. Voß , H. Voss , R. Waldi , R. Wallace , S. Wandernoth , J. Wang , D. R. Ward , N. K. Watson , A. D. Webber , D. Websdale , M. Whitehead , J. Wicht , J. Wiechczynski , D. Wiedner , L. Wiggers , G. Wilkinson , M. P. Williams , M. Williams , F. F. Wilson , J. Wishahi , M. Witek , S. A. Wotton , S. Wright , S. Wu , K. Wyllie , Y. Xie , F. Xing , Z. Xing , Z. Yang , R. Young , X. Yuan , O. Yushchenko , M. Zangoli , M. Zavertyaev , F. Zhang , L. Zhang , W. C. Zhang , Y. Zhang , A. Zhelezov , A. Zhokhov , L. Zhong , A. Zvyagin

The Simons Observatory (SO) will perform ground-based observations of the cosmic microwave background (CMB) with several small and large aperture telescopes, each outfitted with thousands to tens of thousands of superconducting aluminum…