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The selection of low-radioactive construction materials is of the utmost importance for rare-event searches and thus critical to the XENONnT experiment. Results of an extensive radioassay program are reported, in which material samples have…

Instrumentation and Detectors · Physics 2023-01-27 E. Aprile , K. Abe , F. Agostini , S. Ahmed Maouloud , M. Alfonsi , L. Althueser , E. Angelino , J. R. Angevaare , V. C. Antochi , D. Antón Martin , F. Arneodo , L. Baudis , A. L. Baxter , L. Bellagamba , R. Biondi , A. Bismark , A. Brown , S. Bruenner , G. Bruno , R. Budnik , C. Capelli , J. M. R. Cardoso , D. Cichon , B. Cimmino , M. Clark , A. P. Colijn , J. Conrad , J. J. Cuenca-García , J. P. Cussonneau , V. D'Andrea , M. P. Decowski , P. Di Gangi , S. Di Pede , A. Di Giovanni , R. Di Stefano , S. Diglio , A. Elykov , S. Farrell , A. D. Ferella , H. Fischer , W. Fulgione , P. Gaemers , R. Gaior , M. Galloway , F. Gao , R. Glade-Beucke , L. Grandi , J. Grigat , A. Higuera , C. Hils , K. Hiraide , L. Hoetzsch , J. Howlett , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , N. Kato , P. Kavrigin , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Liang , S. Lindemann , M. Lindner , K. Liu , F. Lombardi , J. Long , J. A. M. Lopes , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , A. Manfredini , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , K. Ni , U. Oberlack , J. Palacio , R. Peres , J. Pienaar , M. Pierre , V. Pizzella , G. Plante , J. Qi , J. Qin , D. Ramírez García , S. Reichard , A. Rocchetti , N. Rupp , L. Sanchez , J. M. F. dos Santos , G. Sartorelli , J. Schreiner , D. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , E. Shockley , M. Silva , H. Simgen , A. Takeda , P. -L. Tan , A. Terliuk , C. Therreau , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , F. Tönnies , K. Valerius , G. Volta , Y. Wei , C. Weinheimer , M. Weiss , D. Wenz , J. Westermann , C. Wittweg , T. Wolf , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , Y. Zhang , M. Zhong , T. Zhu , J. P. Zopounidis , M. Laubenstein , S. Nisi

We present high angular resolution radio snap-shot observations of seven nearby low-luminosity active galaxies (LLAGN) from the NUclei of GAlaxies (NUGA) survey. The observations were conducted with MERLIN and EVN/VLBI at 18cm and 6cm. At…

Neutron sources can play a variety of roles in warhead verification. For transmission radiography, a source of directed high energy neutrons is required, while for applications to detect fissile isotopes, sub-MeV neutrons are preferred. The…

Instrumentation and Detectors · Physics 2025-03-19 Jihye Jeon , Erik P. Gilson , Michael Hepler , Alexander Glaser , Robert J. Goldston

Calibration of X-ray detectors is very important to understand the performance characteristics of the detectors and their variation with time and changing operational conditions. This enables the most accurate translation of the…

Instrumentation and Methods for Astrophysics · Physics 2010-03-30 A. R. Rao , Sachindra Naik , Milind Patil , J. P. Malkar , R. P. S. Kalyan Kumar

Nuclear resonant excitation of the 29.19-keV level in $^{229}$Th with high-brilliance synchrotron- radiation and detection of its decay signal, are proposed with the aim of populating the extremely low-energy isomeric state of…

We consider predictions for the MeV gamma-ray spectrum emitted by the $\beta$ decays of freshly synthesized isotopes from a neutron star merger at timescales of relevance for post-merger (days) and remnant (years) emission. We develop a…

High Energy Astrophysical Phenomena · Physics 2026-05-19 Maude Lariviere , Nicole Vassh , Yanwen Deng , Xilu Wang , Rebecca Surman

$^{222}$Rn is a noble radioactive gas produced along the $^{238}$U decay chain, which is present in the majority of soils and rocks. As $^{222}$Rn is the most relevant source of natural background radiation, understanding its distribution…

We customized a laser calibration system and four radioactive $\gamma$-ray calibration sources for the Jiangmen Underground Neutrino Observatory (JUNO), a 20-kton liquid scintillator-based neutrino detector. The laser source system was…

At present, a two-phase argon detector is being developed in our laboratory for dark matter search and low-energy neutrino experiments. To calibrate its energy scale a $^{109}$Cd gamma-ray source was used. In this work a detailed emission…

Instrumentation and Detectors · Physics 2018-06-01 A. Bondar , A. Buzulutskov , A. Dolgov , A. Legkodymov , V. Nosov , V. Oleynikov , V. Porosev , E. Shemyakina , A. Sokolov

In this paper a new version of Li6-based neutron spectrometer for high flux environments is described. The new spectrometer was built with commercial single crystal Chemical Vapour Deposition diamonds of electronic grade. These crystals…

Instrumentation and Detectors · Physics 2018-03-14 M. Osipenko , A. Bellucci , V. Ceriale , D. Corsini , G. Gariano , F. Gatti , M. Girolami , S. Minutoli , F. Panza , M. Pillon , M. Ripani , D. M. Trucchi

We present a sample of twenty-one ROSAT bright active galactic nuclei (AGN), representing a range of spectral classes, and selected for follow-up snap-shot observations with XMM-Newton. The typical exposure was between 5-10 ks. The objects…

Astrophysics · Physics 2009-11-13 L. C. Gallo , I. Lehmann , W. Pietsch , Th. Boller , W. Brinkmann , P. Friedrich , D. Grupe

Noble gas radiation detectors with optical readout are gaining popularity in fields like astrophysics and particle physics due to their ability to produce both ionization and scintillation signals in response to ionizing radiation…

Instrumentation and Detectors · Physics 2024-10-31 J. M. R. Teixeira , C. A. O. Henriques , P. A. O. C. Silva , R. D. P. Mano , J. M. F. Dos Santos , C. M. B. Monteiro

One of the major goals of the NEXT-White (NEW) detector is to demonstrate the energy resolution that an electroluminescent high pressure xenon TPC can achieve for high energy tracks. For this purpose, energy calibrations with 137Cs and…

We present multi-epoch global VLBI observations at 2 cm, 3.6 cm and 6 cm of the compact radio sources in Arp220. We resolve many sources and estimate sizes, expansion velocities and source classes. We find most source properties are…

Cosmology and Nongalactic Astrophysics · Physics 2010-11-19 Fabien Batejat , John E. Conway , Philip J. Diamond , Rodrigo Parra , Colin J. Lonsdale , Carol J. Lonsdale

We test the standardizability of a homogeneous sample of 41 lower-redshift ($0.00415\leq z \leq 0.474$) active galactic nuclei (AGNs) reverberation-mapped (RM) using the broad H$\alpha$ and H$\beta$ emission lines. We find that these…

Astrophysics of Galaxies · Physics 2025-04-07 Shulei Cao , Amit Kumar Mandal , Michal Zajaček , Bożena Czerny , Bharat Ratra

We present ASCA results on four prototype powerful far-infrared galaxies, Mrk231, Mrk273, Arp220 and NGC6240. The soft X-ray spectra show signatures of thermal emission with temperatures of (0.5-1) keV, which is probably produced in…

Astrophysics · Physics 2009-10-30 K. Iwasawa

(Abridged) We present the results of the photometric and spectroscopic identification of 110 hard X-ray selected sources (6e-15<F(2-10 keV)<4e-14 cgs) from 5 additional XMM-Newton fields, nearly doubling the original HELLAS2XMM sample. We…

Long-lived radon daughters are a critical background source in experiments searching for low-energy rare events. Originating from radon in ambient air, radioactive polonium, bismuth and lead isotopes plate-out on materials that are later…

Instrumentation and Detectors · Physics 2021-05-05 S. Bruenner , D. Cichon , G. Eurin , P. Herrero Gómez , F. Jörg , T. Marrodán Undagoitia , H. Simgen , N. Rupp

We present the first results from 60ks of observations of Arp 220 using the ACIS-S instrument on Chandra. We report the detection of several sources near the galaxy's nucleus, including a point source with a hard spectrum that is coincident…

Astrophysics · Physics 2009-11-07 D. L. Clements , J. C. McDowell , S. Shaked , A. C. Baker , K. Borne , L. Colina , S. Lamb , C. Mundell