中文
相关论文

相关论文: Characterizing the Dark Count Rate of a Large-Form…

200 篇论文

We report on a laboratory search for ultralight dark photon dark matter using a single-site, two-sensor scalar magnetometer array. The experiment employs two scalar optically pumped magnetometers (OPMs) operated in a differential…

In the next decades millimeter and sub-mm astronomy requires large format imaging arrays and broad-band spectrometers to complement the high spatial and spectral resolution of the Atacama Large Millimeter/sub-millimeter Array. The desired…

天体物理仪器与方法 · 物理学 2014-08-15 R. M. J. Janssen , J. J. A. Baselmans , A. Endo , L. Ferrari , S. J. C. Yates , A. M. Baryshev , T. M. Klapwijk

We have fabricated and characterized 10,000 and 20,440 pixel Microwave Kinetic Inductance Detector (MKID) arrays for the Dark-speckle Near-IR Energy-resolved Superconducting Spectrophotometer (DARKNESS) and the MKID Exoplanet Camera (MEC).…

Single-photon detectors operating on satellites for use in a quantum communications network can incur large dark count rate increases from the natural radiation environment of space. Displacement damage to the material lattice of a detector…

量子物理 · 物理学 2022-06-02 Brandon A. Wilson , Alexander Miloshevsky , David A. Hooper , Nicholas A. Peters

The dark photon, an new hypothetical light spin 1 field, constitutes a well-motivated dark matter candidate. It manifests as an oscillating electric field with a fixed direction, which can be observed in magnetometric records. In this…

宇宙学与河外天体物理 · 物理学 2015-07-27 G. Pignol , B. Clement , M. Guigue , D. Rebreyend , B. Voirin

We present the first observation by the Telescope Array Surface Detector (TASD) of the effect of thunderstorms on the development of cosmic ray single count rate intensity over a 700 km$^{2}$ area. Observations of variations in the…

高能天体物理现象 · 物理学 2022-04-06 R. U. Abbasi , T. Abu-Zayyad , M. Allen , Y. Arai , R. Arimura , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , I. Buckland , R. Cady , B. G. Cheon , J. Chiba , M. Chikawa , T. Fujii , K. Fujisue , K. Fujita , R. Fujiwara , M. Fukushima , R. Fukushima , G. Furlich , N. Globus , R. Gonzalez , W. Hanlon , M. Hayashi , N. Hayashida , K. Hibino , R. Higuchi , K. Honda , N. Husseini , D. Ikeda , T. Inadomi , N. Inoue , T. Ishii , H. Ito , D. Ivanov , H. Iwakura , A. Iwasaki , H. M. Jeong , S. Jeong , H. Johnson , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , K. Kasahara , S. Kasami , H. Kawai , S. Kawakami , S. Kawana , K. Kawata , I. Kharuk , E. Kido , H. B. Kim , J. H. Kim , J. H. Kim , M. H. Kim , S. W. Kim , Y. Kimura , S. Kishigami , Y. Kubota , S. Kurisu , V. Kuzmin , M. Kuznetsov , Y. J. Kwon , K. H. Lee , R. LeVon , B. Lubsandorzhiev , J. P. Lundquist , K. Machida , H. Matsumiya , T. Matsuyama , J. N. Matthews , R. Mayta , J. Mazich , M. Minamino , K. Mukai , I. Myers , P. Myers , S. Nagataki , K. Nakai , R. Nakamura , T. Nakamura , T. Nakamura , Y. Nakamura , A. Nakazawa , E. Nishio , T. Nonaka , K. OBrien , H. Oda , S. Ogio , M. Ohnishi , H. Ohoka , Y. Oku , T. Okuda , Y. Omura , M. Ono , R. Onogi , A. Oshima , S. Ozawa , I. H. Park , M. Potts , M. S. Pshirkov , J. Remington , D. C. Rodriguez , G. I. Rubtsov , D. Ryu , H. Sagawa , R. Sahara , Y. Saito , N. Sakaki , T. Sako , N. Sakurai , K. Sano , K. Sato , T. Seki , K. Sekino , P. D. Shah , Y. Shibasaki , F. Shibata , N. Shibata , T. Shibata , H. Shimodaira , B. K. Shin , H. S. Shin , D. Shinto , J. D. Smith , P. Sokolsky , N. Sone , B. T. Stokes , T. A. Stroman , Y. Takagi , Y. Takahashi , M. Takamura , M. Takeda , R. Takeishi , A. Taketa , M. Takita , Y. Tameda , H. Tanaka , K. Tanaka , M. Tanaka , Y. Tanoue , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , R. Tsuda , Y. Tsunesada , Y. Uchihori , S. Udo , T. Uehama , F. Urban , T. Wong , M. Yamamoto , K. Yamazaki , J. Yang , K. Yashiro , F. Yoshida , Y. Yoshioka , Y. Zhezher , Z. Zundel

One of the future instruments to resolve the origin of the unidentified 3.5 keV emission line is the Micro-X sounding rocket telescope. According to the estimate made in 2015, Micro-X will be able to detect on average about 18.2 photons…

天体物理仪器与方法 · 物理学 2019-08-28 Denys Savchenko , Dmytro Iakubovskyi

The Array Camera for Optical to Near-IR Spectrophotometry, or ARCONS, is a camera based on Microwave Kinetic Inductance Detectors (MKIDs), a new technology that has the potential for broad application in astronomy. Using an array of MKIDs,…

天体物理仪器与方法 · 物理学 2015-08-06 J. C. van Eyken , M. J. Strader , A. B. Walter , S. R. Meeker , P. Szypryt , C. Stoughton , K. O'Brien , D. Marsden , N. K. Rice , Y. Lin , B. A. Mazin

Five FBK ``NUV-HD-Cryo'' SiPMs have been characterized at 7 K and 10 K, with 405 nm and 530 nm LED light, respectively. The dark count rate (DCR) was measured to be $\sim$ 1 Hz for the $\sim$ 100 mm$^2$-size SiPMs, or 0.01 Hz/mm$^2$, which…

We report measurements of counting statistics, average and variance, of microwave photons of ill-defined frequency : bichromatic photons, i.e. photons involving two well separated frequencies, and "white" broadband photons. Our setup allows…

量子物理 · 物理学 2024-12-10 Simon Bolduc Beaudoin , Edouard Pinsolle , Bertrand Reulet

Uncovering the nature of dark matter is one of the most important goals of particle physics. Light bosonic particles, such as the dark photon, are well-motivated candidates: they are generally long-lived, weakly-interacting, and naturally…

The detection of few-photon signals in a broadband background is an extreme challenge for photon counting, requiring filtering that accepts a narrow range of optical frequencies while strongly rejecting all others. Recent work [Zarraoa et.…

量子物理 · 物理学 2026-04-10 Laura Zarraoa , Tomas Lamich , Sondos Elsehimy , Morgan W. Mitchell , Romain Veyron

Background rates in several pixel array detectors are investigated with an eye toward using them with hard, >6 keV, x-rays in very low-rate experiments - e.g. at signal rates <0.1/s/cm^2. Measured background event rates for a detector with…

仪器与探测器 · 物理学 2023-03-01 Alfred Q. R. Baron , Daisuke Ishikawa

A detailed and accurate characterisation of silicon photomultiplier detectors is required for a better understanding of the signal and noise in many applications. The collected information is a valuable feedback to the manufacturers in…

Infrared spectroscopy has been developed significantly. In particular, infrared photons can be measured with high spectral and angular resolution in state-of-art spectrographs. They are sensitive to monochromatic photons due to the decay…

高能物理 - 唯象学 · 物理学 2025-02-06 Taiki Bessho , Yuji Ikeda , Wen Yin

The technique is described of the search for dark photons with a multicathode counter. The aim of experiment is to search for diurnal variations of the effect from conversion of dark photons at the surface of the metallic cathode. The…

高能物理 - 实验 · 物理学 2023-06-29 A. V. Kopylov , I. V. Orekhov , V. V. Petukhov

We demonstrate fast counting and multiphoton detection abilities of a Silicon Photo Multiplier (SiPM). In fast counting mode we are able to detect two consecutive photons separated by only 2.3 ns corresponding to 430 MHz. The counting…

量子物理 · 物理学 2009-11-13 P. Eraerds , M. Legre , A. Rochas , H. Zbinden , N. Gisin

We present a scheme for a photon-counting detection system that can be operated at incident photon rates higher than otherwise possible by suppressing the effects of detector deadtime. The method uses an array of N detectors and a 1-by-N…

量子物理 · 物理学 2009-11-13 S. Castelletto , I. P. Degiovanni , V. Schettini , A. Migdall

We report on a new photon-counting detector possessing unprecedented spatial resolution, moderate spectral resolution and high background-rejection capability for 0.1-100 keV X-rays. It consists of an X-ray charge-coupled device (CCD) and…

天体物理学 · 物理学 2009-11-10 E. Miyata , K. Tamura