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The last years have seen a revolution in ground-based gamma-ray detectors. We can now detect the spectra of nearby TeV blazars like Mrk 421 and 501 out to approximately 20 TeV, and during the strongest flares, we can now follow fluctuations…

Astrophysics · Physics 2009-10-31 Paolo S. Coppi , Felix A. Aharonian

A new, compact beam position monitor based on segmented a toroidal coil surrounding the charged particle beam has been investigated. It makes use of the induced voltages in the windings instead of the induced charge imbalance on capacitor…

We present a summary of the in-orbit performance of the soft X-ray imaging telescope Xtend onboard the XRISM mission, based on in-flight observation data, including first-light celestial objects, calibration sources, and results from the…

The detector for imaging of explosions (DIMEX) is in operation at the synchrotron radiation (SR) beam-line at VEPP-3 electron ring at Budker INP since 2002. DIMEX is based on one-coordinate gas ionization chamber filled with Xe-CO2(3:1)…

Instrumentation and Detectors · Physics 2008-11-26 V. M. Aulchenko , O. V. Evdokov , L. I. Shekhtman , K. A. Ten , B. P. Tolochko , I. L. Zhogin , V. V. Zhulanov

Highly directional millimeter wave (mmWave) radios need to perform beam management to establish and maintain reliable links. To do so, existing solutions mostly rely on explicit coordination between the transmitter (TX) and the receiver…

Networking and Internet Architecture · Computer Science 2021-06-09 Michele Polese , Francesco Restuccia , Tommaso Melodia

Measurements of the intensity of the cosmic X-ray background (XRB) carried out over small solid angles are subject to spatial variations due to the discrete nature of the XRB. This cosmic variance can account for the dispersion of XRB…

Astrophysics · Physics 2009-10-31 X. Barcons , S. Mateos , M. T. Ceballos

For some synchrotron light source beamline applications, a round beam is preferable to a flat one. A conventional method of obtaining round beam in an electron storage ring is to shift its tune close to a linear difference resonance. The…

Accelerator Physics · Physics 2026-03-09 Yongjun Li , Robert Rainer

Cen X-3 is a well-studied high-mass accreting X-ray binary and a variable source of high energy gamma rays from 100 MeV to 1 TeV. The object has been extensively monitored with the University of Durham Mark 6 telescope. Results of…

Vector vortex beams, featuring independent spatial modes in orthogonal polarization components, offer an increase in information density for emerging applications in both classical and quantum communication technology. Recent advances in…

A real-time beam profile monitoring system is proposed for GeV photon beams at the BM4 beamline of the Mikamine site, Research Center for Accelerator and Radioisotope Science (RARiS; previously known as ELPH) at Tohoku University. This…

Precise and accurate mass and radius measurements of evolved stars are crucial to calibrating stellar models. Stars in detached eclipsing binaries (EBs) are excellent potential calibrators because their stellar parameters can be measured…

The High Energy X-ray telescope (HE) on-board the Hard X-ray Modulation Telescope (\textit{Insight}-HXMT) can serve as a wide Field of View (FOV) gamma-ray monitor with high time resolution ($\mu$s) and large effective area (up to thousands…

The Gamma-Ray Burst Monitor (GBM) will significantly augment the science return from the Fermi Observatory in the study of Gamma-Ray Bursts (GRBs). The primary objective of GBM is to extend the energy range over which bursts are observed…

Transmission electron microscopy and spectroscopy currently enable the acquisition of spatially resolved spectral information from a specimen by focusing electron beams down to a sub-Angstrom spot and then analyzing the energy of the…

Materials Science · Physics 2022-09-12 Andrea Konečná , Fadil Iyikanat , F. Javier García de Abajo

We report the development of an instrument combining an ultrafast, high-repetition-rate, polarization-tunable monochromatic extreme ultraviolet (XUV, 21.6 eV) beamline and a next-generation momentum microscope endstation. This setup enables…

High-Mass X-ray Binaries (HMXBs) serve as useful laboratories for exploring the behaviour of accreted matter onto compact objects and for probing the complex wind environments of massive stars. These investigations are essential for…

High Energy Astrophysical Phenomena · Physics 2025-11-05 C. M. Diez , S. Dupourqué , M. Zhou , E. Quintin , G. A. Matzeu , F. Fürst , P. Kretschmar , R. Amato , C. Malacaria

A beam-energy-spread monitor is under development in order to control and stabilize the energy spread of high-current single-bunch electron beams for producing a sufficient number of positrons. The author has proposed a new monitor using…

Accelerator Physics · Physics 2009-10-05 Tsuyoshi Suwada

This paper presents the beam dynamics systematic corrections and their uncertainties for the Run-1 data set of the Fermilab Muon g-2 Experiment. Two corrections to the measured muon precession frequency $\omega_a^m$ are associated with…

Accelerator Physics · Physics 2021-04-29 T. Albahri , A. Anastasi , K. Badgley , S. Baeßler , I. Bailey , V. A. Baranov , E. Barlas-Yucel , T. Barrett , F. Bedeschi , M. Berz , M. Bhattacharya , H. P. Binney , P. Bloom , J. Bono , E. Bottalico , T. Bowcock , G. Cantatore , R. M. Carey , B. C. K. Casey , D. Cauz , R. Chakraborty , S. P. Chang , A. Chapelain , S. Charity , R. Chislett , J. Choi , Z. Chu , T. E. Chupp , S. Corrodi , L. Cotrozzi , J. D. Crnkovic , S. Dabagov , P. T. Debevec , S. Di Falco , P. Di Meo , G. Di Sciascio , R. Di Stefano , A. Driutti , V. N. Duginov , M. Eads , J. Esquivel , M. Farooq , R. Fatemi , C. Ferrari , M. Fertl , A. Fiedler , A. T. Fienberg , A. Fioretti , D. Flay , E. Frlež , N. S. Froemming , J. Fry , C. Gabbanini , M. D. Galati , S. Ganguly , A. Garcia , J. George , L. K. Gibbons , A. Gioiosa , K. L. Giovanetti , P. Girotti , W. Gohn , T. Gorringe , J. Grange , S. Grant , F. Gray , S. Haciomeroglu , T. Halewood-Leagas , D. Hampai , F. Han , J. Hempstead , A. T. Herrod , D. W. Hertzog , G. Hesketh , A. Hibbert , Z. Hodge , J. L. Holzbauer , K. W. Hong , R. Hong , M. Iacovacci , M. Incagli , P. Kammel , M. Kargiantoulakis , M. Karuza , J. Kaspar , D. Kawall , L. Kelton , A. Keshavarzi , D. Kessler , K. S. Khaw , Z. Khechadoorian , N. V. Khomutov , B. Kiburg , M. Kiburg , O. Kim , Y. I. Kim , B. King , N. Kinnaird , M. Korostelev , E. Kraegeloh , N. A. Kuchinskiy , K. R. Labe , J. LaBounty , M. Lancaster , M. J. Lee , S. Lee , B. Li , D. Li , L. Li , I. Logashenko , A. Lorente Campos , A. Lucà , G. Lukicov , A. Lusiani , A. L. Lyon , B. MacCoy , R. Madrak , K. Makino , F. Marignetti , S. Mastroianni , J. P. Miller , S. Miozzi , W. M. Morse , J. Mott , A. Nath , D. Newton , H. Nguyen , R. Osofsky , S. Park , G. Pauletta , G. M. Piacentino , R. N. Pilato , K. T. Pitts , B. Plaster , D. Počanić , N. Pohlman , C. C. Polly , J. Price , B. Quinn , N. Raha , S. Ramachandran , E. Ramberg , J. L. Ritchie , B. L. Roberts , D. L. Rubin , L. Santi , D. Sathyan , C. Schlesier , A. Schreckenberger , Y. K. Semertzidis , M. W. Smith , M. Sorbara , D. Stöckinger , J. Stapleton , C. Stoughton , D. Stratakis , T. Stuttard , H. E. Swanson , G. Sweetmore , D. A. Sweigart , M. J. Syphers , D. A. Tarazona , T. Teubner , A. E. Tewsley-Booth , K. Thomson , V. Tishchenko , N. H. Tran , W. Turner , E. Valetov , D. Vasilkova , G. Venanzoni , T. Walton , A. Weisskopf , L. Welty-Rieger , P. Winter , A. Wolski , W. Wu

The paper reports the results of measuring the total dose of X-ray bremsstrahlung from a powerful X-ray source based on the high-current pulsed direct-action electron accelerator Temp-B. The parameters of the high-current, tubular…

Future strategic X-ray satellite telescopes, such as the probe-class Advanced X-ray Imaging Satellite (AXIS), will require excellent soft energy response in their imaging detectors to enable maximum discovery potential. In order to…

Instrumentation and Methods for Astrophysics · Physics 2024-07-25 Haley R. Stueber , Tanmoy Chattopadhyay , Sven C. Herrmann , Peter Orel , Tsion Gebre , Aanand Joshi , Steven W. Allen , Glenn Morris , Artem Poliszczuk