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The Gamma-Ray Infrastructure For Fundamental Investigations of Nuclei, GRIFFIN, is a new experimental facility for radioactive decay studies at the TRIUMF-ISAC laboratory. The performance of the 16 high-purity germanium (HPGe) clover…

We describe the development of a noise-temperature testing capability for phased-array antennas operating in receive mode from 0.7 GHz to 1.8 GHz. Sampled voltages from each array port were recorded digitally as the zenith-pointing array…

Instrumentation and Methods for Astrophysics · Physics 2014-04-04 Aaron Chippendale , Douglas Hayman , Stuart Hay

Raman spectroscopy enables broadband, multi-species gas analysis by providing access to an entire vibrational spectrum in a single measurement. However, the sensitivity of gas-phase Raman sensing is often limited by weak signals and…

Large-size hybrid and pixelized GEM-Micromegas gaseous detectors (40x40 cm$^2$ active area) were developed and installed in 2014 and 2015 for the COMPASS2 physics program which started at the same time. That program involved in particular…

A second monolithic silicon pixel prototype was produced for the MONOLITH project. The ASIC contains a matrix of hexagonal pixels with 100 {\mu}m pitch, readout by a low-noise and very fast SiGe HBT frontend electronics. Wafers with 50…

In MicroPattern Gas Detectors (MPGD) when the pixel size is below 100 micron and the number of pixels is large (above 1000) it is virtually impossible to use the conventional PCB read-out approach to bring the signal charge from the…

Instrumentation and Detectors · Physics 2015-06-26 R. Bellazzini , F. Angelini , L. Baldini , F. Bitti , A. Brez , L. Latronico , M. M. Massai , M. Minuti , N. Omodei , M. Razzano , C. Sgro , G. Spandre , E. Costa , P. Soffitta

Separate absorption charge multiplication germanium tin on silicon avalanche photodiode offers a viable solution to achieve CMOS compatible, high sensitivity detection technology in SWIR or extended SWIR range, leveraging the excellent…

The performance of hybrid GaAs pixel detectors as X-ray imaging sensors were investigated at room temperature. These hybrids consist of 300 mu-m thick GaAs pixel detectors, flip-chip bonded to a CMOS Single Photon Counting Chip (PCC). This…

A new type of gaseous micropattern particle detector based on a closed-cell microcavity plasma panel sensor is reported. The first device was fabricated with 1 x 1 x 2 mm cells. It has shown very clean signals of 0.6 to 2.5 volt amplitude,…

Optical transition-edge sensors have shown energy resolution for resolving the number of incident photons at the telecommunication wavelength. Higher energy resolution is required for biological imaging and microscope spectroscopy. In this…

Instrumentation and Detectors · Physics 2022-07-27 Kaori Hattori , Toshio Konno , Yoshitaka Miura , Sachiko Takasu , Daiji Fukuda

Prototype of gamma ray detector based on Micro Pixel Avalanche Photodiodes (MAPD) with high pixel density 15000 pixel/$mm^2$, optically coupled to Lutetium Fine Silicate (LFS) scintillator has been developed. The detection performance…

Instrumentation and Detectors · Physics 2013-02-11 E. Guliyev , F. Ahmadov , G. Ahmadov , A. Sadigov , Z. Sadigov , N. Anfimov , Z. Krumshtein , A. Olshevski , V. Shvetsov , V. Zhezher , R. Madatov

The new beam profile measurement for the Antiproton Decelerator (AD) at CERN is based on a single Gas Electron Multiplier (GEM) with a 2D readout structure. This detector is very light (~0.4% X0), and measures horizontal and vertical…

Instrumentation and Detectors · Physics 2012-03-20 Serge Duarte Pinto , Rhodri Jones , Leszek Ropelewski , Jens Spanggaard , Gerard Tranquille

We show that polar materials are excellent targets for direct detection of sub-GeV dark matter due to the presence of gapped optical phonons as well as acoustic phonons with high sound speed. We take the example of Gallium Arsenide (GaAs),…

High Energy Physics - Phenomenology · Physics 2018-11-02 Simon Knapen , Tongyan Lin , Matt Pyle , Kathryn M. Zurek

Whispering gallery modes in GaAs disk resonators reach half a million of optical quality factor. These high Qs remain still well below the ultimate design limit set by bending losses. Here we investigate the origin of residual optical…

A novel approach for designing the next generation of vertex detectors foresees to employ wafer-scale sensors that can be bent to truly cylindrical geometries after thinning them to thicknesses of 20-40$\mu$m. To solidify this concept, the…

Instrumentation and Detectors · Physics 2021-08-18 ALICE ITS project , : , G. Aglieri Rinella , M. Agnello , B. Alessandro , F. Agnese , R. S. Akram , J. Alme , E. Anderssen , D. Andreou , F. Antinori , N. Apadula , P. Atkinson , R. Baccomi , A. Badalà , A. Balbino , C. Bartels , R. Barthel , F. Baruffaldi , I. Belikov , S. Beole , P. Becht , A. Bhatti , M. Bhopal , N. Bianchi , M. B. Blidaru , G. Boca , J. Bok , G. Bonomi , M. Bonora , M. Borri , V. Borshchov , E. Botta , G. E. Bruno , M. Buckland , S. Bufalino , M. Cai , P. Camerini , P. Cariola , F. Catalano , C. Ceballos Sanchez , I. Chakaberia , M. Chartier , F. Colamaria , D. Colella , A. Collu , M. Concas , G. Contin , S. Costanza , P. Cui , A. Dainese , J. B. Dainton , L. De Cilladi , C. De Martin , G. De Robertis , W. Deng , A. Di Mauro , Y. Ding , M. Durkac , D. Elia , M. R. Ersdal , M. Faggin , F. Fan , A. Fantoni , P. Fecchio , A. Feliciello , G. Feofilov , A. Ferk , J. Ferencei , G. Fiorenza , A. N. Flores , E. Fragiacomo , D. Gajanana , A. Gal , C. Gao , C. Gargiulo , P. Gianotti , P. Giubilato , A. Grant , L. Greiner , A. Grelli , O. S. Groettvik , F. Grosa , C. Guo Hu , R. Hannigan , J. A. Hasenbichler , H. Helstrup , H. Hillemanns , C. Hills , P. Hindley , B. Hippolyte , B. Hofman , G. H. Hong , G. Huang , J. P. Iddon , H. Ilyas , M. A. Imhoff , A. Isakov , A. Jadlovska , S. Jadlovska , J. Jadlovsky , S. Jaelani , T. Johnson , A. Junique , P. Kalinak , A. Kalweit , M. Keil , Z. Khabanova , H. Khan , B. Kim , C. Kim , J. Kim , J. Kim , T. Kim , J. Klein , A. Kluge , C. Kobdaj , A. Kotliarov , I. Králik , F. Krizek , T. Kugathasan , C. Kuhn , P. G. Kuijer , S. Kushpil , M. J. Kweon , J. Y. Kwon , Y. Kwon , P. La Rocca , A. Lakrathok , R. Langoy , P. Larionov , E. Laudi , T. Lazareva , R. Lea , R. C. Lemmon , X. L. Li , J. Lien , B. Lim , S. H. Lim , S. Lindsay , A. Liu , J. Liu , J. Liu , M. Lunardon , G. Luparello , M. Lupi , M. Mager , A. Maire , Q. W. Malik , G. Mandaglio , V. Manzari , Y. Mao , G. V. Margagliotti , C. Markert , D. Marras , P. Martinengo , S. Masciocchi , M. Masera , A. Masoni , A. Mastroserio , P. F. T. Matuoka , G. Mazza , F. Mazzaschi , M. A. Mazzoni , F Morel , V. Muccifora , A. Mulliri , L. Musa , S. V. Nesbo , D. Nesterov , J. Norman , J. Park , R. N Patra , C. Pastore , H. Pei , X. Peng , S. Piano , C. Pinto , S. Pisano , S. Politano , E. Prakasa , F. Prino , M. Protsenko , M. Puccio , A. Rachevski , L. Ramello , F. Rami , I. Ravasenga , A. Rehman , F. Reidt , F. Riggi , K. Røed , D. Röhrich , F. Ronchetti , A. Rosano , M. J. Rossewij , A. Rossi , R. Rui , R. Russo , R. Sadikin , V. Sarritzu , J. Schambach , S. Senyukov , J. J. Seo , R. Shahoyan , S. Shaukat , S. Siddhanta , M. Sitta , R. J. M. Snellings , W. Snoeys , A. Songmoolnak , J. Sonneveld , F. Soramel , M. Suljic , S. Sumowidagdo , D. Sun , X. Sun , G. J. Tambave , G. Tersimonov , M. Tkacik , M. Toppi , A. Trifiró , S. Trogolo , V. Trubnikov , R. Turrisi , T. S. Tveter , I. Tymchuck , K. Ullaland , M. Urioni , G. L. Usai , N. Valle , L. V. R. van Doremalen , T. Vanat , J. W. Van Hoorne , M. Varga-Kofarago , A. Velure , D. Wang , Y. Wang , J. Wikne , J. R. Wright , R. Xu , P. Yang , Z. Yin , I. -K. Yoo , J. H. Yoon , S. Yuan , V. Zaccolo , E. Zhang , X. Zhang , V. Zherebchevskii , D. Zhou , J. Zhu , Y. Zhu , G. Zinovjev , N. Zurlo

We present in this paper the results of a comprehensive GEANT simulation of the Gamma-Ray Imaging Detector (GRID) being developed for the AGILE space astrophysics mission. The GRID is designed to be sensitive in the 30 MeV - 50 GeV energy…

Astrophysics · Physics 2015-06-24 Francesco Longo , Veronica Cocco , Marco Tavani

The Bayesian gravitational shear estimation algorithm developed by Bernstein and Armstrong (2014) can potentially be used to overcome multiplicative noise bias and recover shear using very low signal-to-noise ratio (S/N) galaxy images. In…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-19 Erin S. Sheldon

The Spherical Proportional Counter is a novel type of radiation detector, with a low energy threshold (typically below 100 eV) and good energy resolution. This detector is being developed by the network NEWS, which includes several…

Instrumentation and Detectors · Physics 2015-01-09 F. J. Iguaz , A. Rodriguez , J. F. Castel , I. G. Irastorza

A photodiode with 0.55$\pm$0.1 A/W responsivity at a wavelength of 1176.9 nm has been fabricated in a 45 nm microelectronics silicon-on-insulator foundry process. The resonant waveguide photodetector exploits carrier generation in…

Optics · Physics 2016-02-17 Luca Alloatti , Rajeev Jagga Ram

The GLAST Burst Monitor (GBM) will augment the capabilities of GLAST for the detection of cosmic gamma-ray bursts by extending the energy range (20 MeV to > 300 GeV) of the Large Area Telescope (LAT) towards lower energies by 2…