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This project explores the design and development of a transition edge sensor (TES) spectrometer for resonant soft X- ray scattering (RSXS) measurements developed in collaboration between Argonne National Laboratory (ANL) and the National…

The Cadmium Zinc Telluride Imager (CZTI) onboard AstroSat is designed for hard X-ray imaging and spectroscopy in the energy range of 20 - 100 keV. The CZT detectors are of 5 mm thickness and hence have good efficiency for Compton…

Instrumentation and Methods for Astrophysics · Physics 2021-03-01 Abhay Kumar , Tanmoy Chattopadhyay , Santosh V Vadawale , A. R. Rao , Soumya Gupta , Mithun N. P. S. , Varun Bhalerao , Dipankar Bhattacharya

This paper discusses the latest progress in the development of GRAPE (Gamma-Ray Polarimeter Experiment), a hard X-ray Compton Polarimeter. The purpose of GRAPE is to measure the polarization of hard X-rays in the 50-300 keV energy range. We…

Astrophysics · Physics 2017-08-23 J. S. Legere , P. Bloser , J. R. Macri , M. L. McConnell , T. Narita , J. M. Ryan

In the past decade, Resonant Inelastic X-ray Scattering (RIXS) has made remarkable progress as a spectroscopic technique. This is a direct result of the availability of high-brilliance synchrotron X-ray radiation sources and of advanced…

Strongly Correlated Electrons · Physics 2012-12-03 Luuk J. P. Ament , Michel van Veenendaal , Thomas P. Devereaux , John P. Hill , Jeroen van den Brink

We are presenting a detailed parameter study of the time-dependent electron injection and kinematics and the self-consistent radiation transport in jets of intermediate and low-frequency peaked BL Lac objects. Using a time-dependent,…

Astrophysics · Physics 2009-11-07 M. Boettcher , J. Chiang

We propose PET scanners using low atomic number media that undergo a persistent local change of state along the paths of the Compton recoil electrons. Measurement of the individual scattering locations and angles, deposited energies, and…

X-ray observations of the binary pulsar GX 1+4 made using the Rossi X-ray Timing Explorer (RXTE) satellite between February 1996 and May 1997 were analysed to quantify source spectral variation with luminosity. Mean Proportional Counter…

Astrophysics · Physics 2007-05-23 D. K. Galloway

X-ray polarimetry promises to give qualitatively new information about high-energy astrophysical sources, such as binary black hole systems, micro-quasars, active galactic nuclei, and gamma-ray bursts. We designed, built and tested a hard…

The elastic and inelastic high--energy small--angle electron--positron scattering is considered. All radiative corrections to the cross--section with the relative accuracy $\delta\sigma/ \sigma = 0.1 \% $ are explicitly taken into account.…

High Energy Physics - Phenomenology · Physics 2009-10-28 A. B. Arbuzov , V. S. Fadin , E. A. Kuraev , L. N. Lipatov , N. P. Merenkov , L. G. Trentadue

Understanding the excitations of quantum materials is essential for unraveling how their microscopic constituents interact. Among these, particle-hole excitations form a particularly important class, as they govern fundamental processes…

Cryogenic calorimeters for low-mass dark matter searches have achieved sub-eV energy resolutions, driving advances in both low-energy calibration techniques and our understanding of detector physics. The energy deposition spectrum of gamma…

Instrumentation and Detectors · Physics 2025-12-11 SuperCDMS Collaboration , M. F. Albakry , I. Alkhatib , D. Alonso-Gonźalez , D. W. P. Amaral , J. Anczarski , T. Aralis , T. Aramaki , I. Ataee Langroudy , C. Bathurst , R. Bhattacharyya , A. J. Biffl , P. L. Brink , M. Buchanan , R. Bunker , B. Cabrera , R. Calkins , R. A. Cameron , C. Cartaro , D. G. Cerdeño , Y. -Y. Chang , M. Chaudhuri , J. -H. Chen , R. Chen , N. Chott , J. Cooley , H. Coombes , P. Cushman , R. Cyna , S. Das , S. Dharani , M. L. di Vacri , M. D. Diamond , M. Elwan , S. Fallows , E. Fascione , E. Figueroa-Feliciano , S. L. Franzen , A. Gevorgian , M. Ghaith , G. Godden , J. Golatkar , S. R. Golwala , R. Gualtieri , J. Hall , S. A. S. Harms , C. Hays , B. A. Hines , Z. Hong , L. Hsu , M. E. Huber , V. Iyer , V. K. S. Kashyap , S. T. D. Keller , M. H. Kelsey , K. T. Kennard , Z. Kromer , A. Kubik , N. A. Kurinsky , M. Lee , J. Leyva , B. Lichtenberg , J. Liu , Y. Liu , E. Lopez Asamar , P. Lukens , R. López Noé , D. B. MacFarlane , R. Mahapatra , J. S. Mammo , N. Mast , A. J. Mayer , P. C. McNamara , H. Meyer zu Theenhausen , É. Michaud , E. Michielin , K. Mickelson , N. Mirabolfathi , M. Mirzakhani , B. Mohanty , D. Mondal , D. Monteiro , J. Nelson , H. Neog , V. Novati , J. L. Orrell , M. D. Osborne , S. M. Oser , L. Pandey , S. Pandey , R. Partridge , P. K. Patel , D. S. Pedreros , W. Peng , W. L. Perry , R. Podviianiuk , M. Potts , S. S. Poudel , A. Pradeep , M. Pyle , W. Rau , E. Reid , R. Ren , T. Reynolds , M. Rios , A. Roberts , A. E. Robinson , L. Rosado Del Rio , J. L. Ryan , T. Saab , D. Sadek , B. Sadoulet , S. P. Sahoo , I. Saikia , S. Salehi , J. Sander , B. Sandoval , A. Sattari , B. Schmidt , R. W. Schnee , B. Serfass , A. E. Sharbaugh , R. S. Shenoy , A. Simchony , P. Sinervo , Z. J. Smith , R. Soni , K. Stifter , J. Street , M. Stukel , H. Sun , E. Tanner , N. Tenpas , D. Toback , A. N. Villano , J. Viol , B. von Krosigk , Y. Wang , O. Wen , Z. Williams , M. J. Wilson , J. Winchell , S. Yellin , B. A. Young , B. Zatschler , S. Zatschler , A. Zaytsev , E. Zhang , L. Zheng , A. Zuniga , M. J. Zurowski

The Cu K-edge resonant inelastic x-ray scattering (RIXS) spectrum in one-dimensional insulating cuprates is theoretically examined by using the exact diagonalization technique for the extended one-dimensional Hubbard model with nearest…

Strongly Correlated Electrons · Physics 2016-08-31 K. Tsutsui , T. Tohyama , S. Maekawa

The possibility to study elastic and diffractive physics in pp collisions at LHC is investigated. For this purpose we have considered detectors close to the beam in conjunction with the magnetic elements of the accelerator to provide a high…

High Energy Physics - Phenomenology · Physics 2009-10-30 M. Arneodo , S. Maselli , C. Peroni

We present the previously unanalysed high quality XMM-Newton spectrum of an ultraluminous X-ray source candidate in NGC 4517. As with other high quality ULX spectra, a downturn in the spectrum is observed at ~6 keV. Both of the recent disc…

High Energy Astrophysical Phenomena · Physics 2015-05-27 D. J. Walton , J. C. Gladstone , T. P. Roberts , A. C. Fabian , M. D. Caballero-Garcia , C. Done , M. J. Middleton

We present an exhaustive methodology for fitting Compton-thick X-ray reprocessor models to obscured AGNs and for interpreting the results. We focus on the MYTORUS model but also utilize other models. We apply the techniques to Suzaku,…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Tahir Yaqoob

In a recent publication Larson \textit{et al.} reported remarkably clear $d$-$d$ excitations for NiO and CoO measured with x-ray energies well below the transition metal $K$ edge. In this letter we demonstrate that we can obtain an accurate…

Strongly Correlated Electrons · Physics 2008-01-09 M. W. Haverkort , A. Tanaka , L. H. Tjeng , G. A. Sawatzky

Spectral analysis is one of the most powerful technologies for studying and understanding matter. As the devices for spectral analysis, spectrometers are widely used in material detection, isotope analysis, trace gas detection, and the…

A new method for the determination of the real part of the elastic scattering amplitude is examined for high energy proton-proton and proton-nuclei elastic scattering at small momentum transfer. This method allows to decrease the number of…

High Energy Physics - Phenomenology · Physics 2007-05-23 B. Nicolescu , O. V. Selyugin

When matter is exposed to a high-intensity x-ray free-electron-laser pulse, the x rays excite inner-shell electrons leading to the ionization of the electrons through various atomic processes and creating high-energy-density plasma, i.e.,…

Atomic and Molecular Clusters · Physics 2017-08-24 Malik Muhammad Abdullah , Anurag , Zoltan Jurek , Sang-Kil Son , Robin Santra

The synchrotron-self Compton (SSC) radiation process is widely held to provide a close representation of the double peaked spectral energy distributions from BL Lac Objects (BL Lacs), which are marked by non-thermal beamed radiations,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 A. Paggi , F. Massaro , V. Vittorini , A. Cavaliere , F. D'Ammando , F. Vagnetti , M. Tavani