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In this paper we report on the characterization of the Hamamatsu VUV4 (S/N: S13370-6152) Vacuum Ultra-Violet (VUV) sensitive Silicon Photo-Multipliers (SiPMs) as part of the development of a solution for the detection of liquid xenon…

Instrumentation and Methods for Astrophysics · Physics 2019-07-24 G. Gallina , P. Giampa , F. Retiere , J. Kroeger , G. Zhang , M. Ward , P. Margetak , G. Lic , T. Tsang , L. Doria , S. Al Kharusi , M. Alfaris , G. Anton , I. J. Arnquist , I. Badhrees , P. S. Barbeau , D. Beck , V. Belov , T. Bhatta , J. Blatchford , J. P. Brodsky , E. Brown , T. Brunner , G. F. Cao , L. Cao , W. R. Cen , C. Chambers , S. A. Charlebois , M. Chiu , B. Cleveland , M. Coon , A. Craycraft , J. Dalmasson , T. Daniels , L. Darroch , S. J. Daugherty , A. De St. Croix , A. Der Mesrobian-Kabakian , R. DeVoe , J. Dilling , Y. Y. Ding , M. J. Dolinski , A. Dragone , J. Echevers , M. Elbeltagi , L. Fabris , D. Fairbank , W. Fairbank , J. Farine , S. Feyzbakhsh , R. Fontaine , P. Gautam , G. Giacomini , R. Gornea , G. Gratta , E. V. Hansen , M. Heffner , E. W. Hoppe , J. Hoßl , A. House , M. Hughes , Y. Ito , A. Iverson , A. Jamil , M. J. Jewell , X. S. Jiang , A. Karelin , L. J. Kaufman , D. Kodroff , T. Koffas , R. Krucken , A. Kuchenkov , K. S. Kumar , Y. Lana , A. Larson , B. G. Lenardo , D. S. Leonarda , S. Lik , Z. Li , C. Licciardi , Y. H. Linw , P. Lv , R. MacLellan , T. McElroy , M. Medina-Peregrina , T. Michel , B. Mong , D. C. Moore , K. Murray , P. Nakarmi , R. J. Newby , Z. Ning , O. Njoya , F. Nolet , O. Nusair , K. Odgers , A. Odian , M. Oriunno , J. L. Orrell , G. S. Ortega , I. Ostrovskiy , C. T. Overman , S. Parent , A. Piepkez , A. Pocar , J. -F. Pratte , D. Qiu , V. Radeka , E. Raguzin , S. Rescia , M. Richman , A. Robinson , T. Rossignol , P. C. Rowson , N. Roy , R. Saldanha , S. Sangiorgio , K. Skarpaas VIII , A. K. Soma , G. St-Hilaire , V. Stekhanov , T. Stiegler , X. L. Sun , M. Tarka , J. Todd , T. Tolba , T. I. Totev , R. Tsang , F. Vachon , V. Veeraraghavan , G. Visser , J. -L. Vuilleumier , M. Wagenpfeil , M. Walent , Q. Wang , J. Watkins , M. Weber , W. Wei , L. J. Wen , U. Wichoski , S. X. Wu , W. H. Wu , X. Wu , Q. Xia , H. Yang , L. Yang , Y. -R. Yen , O. Zeldovich , J. Zhao , Y. Zhou , T. Ziegler

A search has been performed, using the full 20.3 fb$^{-1}$ data sample of 8 TeV proton--proton collisions collected in 2012 with the ATLAS detector at the LHC, for photons originating from a displaced vertex due to the decay of a neutral…

High Energy Physics - Experiment · Physics 2014-12-17 ATLAS Collaboration

To cope with the challenging environment of the planned high luminosity upgrade of the Large Hadron Collider (HL-LHC), scheduled to start operation in 2029, CMS will replace its entire tracking system. The requirements for the tracker are…

Instrumentation and Detectors · Physics 2022-12-12 The Tracker Group of the CMS Collaboration

The next-generation ALICE 3 experiment at the High-Luminosity LHC (HL-LHC) requires detector technologies that combine fine spatial resolution, fast timing, and an extremely low material budget. This paper presents the design,…

Instrumentation and Detectors · Physics 2026-01-07 Umberto Follo

Silicon photomultipliers (SiPMs) are highly-sensitive photodetectors emerging as the technology of choice for many applications, including large high-energy physics experiments where they often are exposed to high radiation fluences. In…

Instrumentation and Detectors · Physics 2022-08-17 A. R. Altamura , F. Acerbi , C. Nociforo , V. Regazzoni , A. Mazzi , A. Gola

PSR J1023+0038 is the first millisecond pulsar that was ever observed as an optical and UV pulsar. So far, it is the only optical transitional millisecond pulsar. The rotation- and accretion-powered emission mechanisms hardly individually…

A recent report on the over saturation in SiPMs is puzzling. The measurements, using a variety of SiPMs, show an excess in signal far beyond the physical limit of the number of SiPM microcells without indication of an ultimate saturation.…

Instrumentation and Methods for Astrophysics · Physics 2015-07-06 Max Ludwig Ahnen

There are currently intense efforts being directed towards extending the range and energy of long distance nonlinear pulse propagation in the atmosphere by moving to longer infrared wavelengths, with the purpose of mitigating the effects of…

With the High-Luminosity Large Hadron Collider (HL-LHC) the number of collisions per bunch crossing increases. To cope with these high rates in the pixel trackers, per-pixel time measurements are required, which implies the need for fast…

Instrumentation and Detectors · Physics 2025-11-18 Daan Oppenhuis

The ATLAS Forward Physics (AFP) project plans to install 3D silicon pixel detectors about 210 m away from the interaction point and very close to the beamline (2-3 mm). This implies the need of slim edges of about 100-200 $\mu$m width for…

Instrumentation and Detectors · Physics 2015-11-09 Jörn Lange , Emanuele Cavallaro , Sebastian Grinstein , Ivan Lopez Paz

We report the observation of a phonon bottleneck effect impacting the thermal depopulation of photoexcited shallow defects in high-resistivity silicon. Using time-resolved terahertz (THz) spectroscopy, near-band-gap excitation produces a…

Materials Science · Physics 2025-11-25 Sergio Revuelta , Hai I. Wang , Mischa Bonn , Enrique Canovas

The low gain avalanche detectors (LGADs) are thin sensors with fast charge collection which in combination with internal gain deliver an outstanding time resolution of about 30 ps. High collision rates and consequent large particle rates…

Single photon detectors have dark count rates that depend strongly on the bias level for detector operation. In the case of weak light sources such as novel lasers or single-photon emitters, the rate of counts due to the light source can be…

Optics · Physics 2023-01-16 Nicole Menkart , Joseph D. Hart , Thomas E. Murphy , Rajarshi Roy

We have developed an avalanche transistor-based pulse generator for driving the photocathode of an image intensifier, which comprises a mainly capacitive load on the order of 100 pF. The circuit produces flat-top pulses with rise time of 2…

Instrumentation and Detectors · Physics 2017-12-15 N. Beev , J. Keller , T. E. Mehlstäubler

We present multi-wavelength observations of an M-class flare (M3.9) that occurred on 2014 June 11. Our observations were conducted with the Dunn Solar Telescope (DST), adaptive optics, the multi-camera system ROSA (Rapid Oscillations in…

Solar and Stellar Astrophysics · Physics 2019-07-24 Damian J. Christian , David Kuridze , David B. Jess , Menoa Yousefi , Mihalis Mathioudakis

The existing ATLAS Tracker will be at its functional limit for particle fluences of 10^15 neq/cm^2 (LHC). Thus for the upgrades at smaller radii like in the case of the planned Insertable B-Layer (IBL) and for increased LHC luminosities…

Physical principles of performance and main characteristics of a novel avalanche photodetector developed on the basis of MOS(metal-oxide-silicon) technology is presented. The photodetector contains a semitransparent gate electrode and a…

High Energy Physics - Experiment · Physics 2007-05-23 Z. Ya. Sadygov , M. K. Suleimanov , T. Yu. Bokova

Photoionization as a half-scattering process is not instantaneous. Usually, time delays in photoionization are of the order of few tens of attoseconds (1 as = 10$^{-18}$ s). While going from a single atom to a nano-object, one can expect…

High-time-resolution counters based on plastic scintillator with silicon photomultiplier (SiPM) readout have been developed for applications to high energy physics experiments for which relatively large-sized counters are required. We have…

Instrumentation and Detectors · Physics 2014-10-17 Paolo W. Cattaneo , Matteo De Gerone , Flavio Gatti , Miki Nishimura , Wataru Ootani , Massimo Rossella , Yusuke Uchiyama

The measurement of the spin frequency in accreting millisecond X-ray pulsars (AMXPs) is strongly affected by the presence of an unmodeled component in the pulse arrival times called 'timing noise'. We show that it is possible to attribute…

High Energy Astrophysical Phenomena · Physics 2011-02-11 Alessandro Patruno , Rudy Wijnands , Michiel van der Klis
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