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@article{bib:paper23, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, date-added = {2023-04-22 10:26:31 +0200}, date-modified = {2023-04-22 10:26:44 +0200}, doi = {10.1103/PhysRevLett.130.161001}, issue = {16}, journal = {Phys. Rev. Lett.}, month = {Apr}, numpages = {11}, pages = {161001}, publisher = {American Physical Society}, title = {Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.130.161001}, volume = {130}, year = {2023}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.130.161001}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.130.161001}}
@article{bib:POX, adsnote = {Provided by the SAO/NASA Astrophysics Data System}, adsurl = {https://ui.adsabs.harvard.edu/abs/2022MmSAI..93b.256D}, author = {{D'Urso}, D. and {...} and {M. Duranti} and {et al.}}, date-modified = {2023-03-17 08:24:54 +0100}, doi = {10.36116/MEMSAIT_93N2_3.2022.31/2022MemSAIT}, journal = {Memorie della Societ{`a} Astronomica Italiana}, keywords = {Particle detector, silicon tracker, gamma-ray, cosmic rays}, month = nov, number = {2-3}, pages = {256}, title = {{POX - PANGU Optimization and eXperimental verification: design and perfor- mance}}, volume = {93}, year = 2022, bdsk-url-1 = {https://doi.org/10.36116/MEMSAIT_93N2_3.2022.31/2022MemSAIT}}
@article{bib:TIC_proceeding2, abstract = {A space-based detector dedicated to measurements of γ-rays and charged particles has to achieve a balance between different instrumental requirements. A good angular resolution is necessary for the γ-rays, whereas an excellent geometric factor is needed for the charged particles. The tracking reference technique of γ-ray physics is based on a pair-conversion telescope made of passive material (e.g., tungsten) coupled with sensitive layers (e.g., silicon microstrip). However, this kind of detector has a limited acceptance because of the large lever arm between the active layers, needed to improve the track reconstruction capability. Moreover, the passive material can induce fragmentation of nuclei, thus worsening charge reconstruction performances. The Tracker-In-Calorimeter (TIC) project aims to solve all these drawbacks. In the TIC proposal, the silicon sensors are moved inside a highly-segmented isotropic calorimeter with a couple of external scintillators dedicated to charge reconstruction. In principle, this configuration has a good geometrical factor, and the angle of the γ-rays can be precisely reconstructed from the lateral profile of the electromagnetic shower sampled, at different depths in the calorimeter, by silicon strips. The effectiveness of this approach has been studied with Monte Carlo simulations and validated with beam test data of a small prototype.}, article-number = {52}, author = {Bigongiari, Gabriele and {...} and {M. Duranti} and {et al.}}, date-added = {2023-03-12 08:25:29 +0100}, date-modified = {2023-03-12 08:25:51 +0100}, doi = {10.3390/instruments6040052}, issn = {2410-390X}, journal = {Instruments}, number = {4}, title = {Tracker-in-Calorimeter (TIC) Project: A Calorimetric New Solution for Space Experiments}, url = {https://www.mdpi.com/2410-390X/6/4/52}, volume = {6}, year = {2022}, bdsk-url-1 = {https://www.mdpi.com/2410-390X/6/4/52}, bdsk-url-2 = {https://doi.org/10.3390/instruments6040052}}
@article{bib:HVO, archiveprefix = {arXiv}, author = {Pelosi, David and {...} and {M. Duranti} and {et al.}}, date-added = {2022-03-23 19:50:13 +0100}, date-modified = {2022-03-23 19:50:24 +0100}, doi = {10.1393/ncc/i2021-21097-2}, eprint = {2101.09366}, journal = {Nuovo Cim. C}, number = {2-3-3}, pages = {97}, primaryclass = {physics.space-ph}, title = {{Development of a web application for monitoring solar activity and cosmic radiation}}, volume = {44}, year = {2021}, bdsk-url-1 = {https://doi.org/10.1393/ncc/i2021-21097-2}}
@article{bib:HVO2, author = {Pelosi, David and {...} and {M. Duranti} and {et al.}}, date-added = {2022-03-23 19:49:41 +0100}, date-modified = {2022-03-23 19:49:56 +0100}, doi = {10.22323/1.395.1259}, journal = {PoS}, pages = {1259}, title = {{A web application for monitoring cosmic rays and solar activity}}, volume = {ICRC2021}, year = {2021}, bdsk-url-1 = {https://doi.org/10.22323/1.395.1259}}
@article{bib:paper22, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, date-modified = {2022-12-05 16:23:15 +0100}, doi = {10.1103/PhysRevLett.128.231102}, issue = {23}, journal = {Phys. Rev. Lett.}, month = {Jun}, numpages = {10}, pages = {231102}, publisher = {American Physical Society}, title = {Properties of Daily Helium Fluxes}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.128.231102}, volume = {128}, year = {2022}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.128.231102}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.128.231102}}
@article{bib:paper21, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, date-modified = {2022-12-05 16:22:35 +0100}, doi = {10.1103/PhysRevLett.127.271102}, issue = {27}, journal = {Phys. Rev. Lett.}, month = {Dec}, numpages = {8}, pages = {271102}, publisher = {American Physical Society}, title = {Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.127.271102}, volume = {127}, year = {2021}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.127.271102}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.127.271102}}
@article{bib:paper20, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, date-modified = {2022-12-05 16:23:10 +0100}, doi = {10.1103/PhysRevLett.127.021101}, issue = {2}, journal = {Phys. Rev. Lett.}, month = {Jul}, numpages = {9}, pages = {021101}, publisher = {American Physical Society}, title = {Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.127.021101}, volume = {127}, year = {2021}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.127.021101}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.127.021101}}
@article{bib:ALADInO2, abstract = {A new generation magnetic spectrometer in space will open the opportunity to investigate the frontiers in direct high-energy cosmic ray measurements and to precisely measure the amount of the rare antimatter component in cosmic rays beyond the reach of current missions. We propose the concept for an Antimatter Large Acceptance Detector In Orbit (ALADInO), designed to take over the legacy of direct measurements of cosmic rays in space performed by PAMELA and AMS-02. ALADInO features technological solutions conceived to overcome the current limitations of magnetic spectrometers in space with a layout that provides an acceptance larger than 10 m2 sr. A superconducting magnet coupled to precision tracking and time-of-flight systems can provide the required matter–antimatter separation capabilities and rigidity measurement resolution with a Maximum Detectable Rigidity better than 20 TV. The inner 3D-imaging deep calorimeter, designed to maximize the isotropic acceptance of particles, allows for the measurement of cosmic rays up to PeV energies with accurate energy resolution to precisely measure features in the cosmic ray spectra. The operations of ALADInO in the Sun–Earth L2 Lagrangian point for at least 5 years would enable unique revolutionary observations with groundbreaking discovery potentials in the field of astroparticle physics by precision measurements of electrons, positrons, and antiprotons up to 10 TeV and of nuclear cosmic rays up to PeV energies, and by the possible unambiguous detection and measurement of low-energy antideuteron and antihelium components in cosmic rays.}, article-number = {19}, author = {Adriani, Oscar and {...} and {M. Duranti} and {et al.}}, doi = {10.3390/instruments6020019}, issn = {2410-390X}, journal = {Instruments}, number = {2}, title = {Design of an Antimatter Large Acceptance Detector In Orbit (ALADInO)}, url = {https://www.mdpi.com/2410-390X/6/2/19}, volume = {6}, year = {2022}, bdsk-url-1 = {https://www.mdpi.com/2410-390X/6/2/19}, bdsk-url-2 = {https://doi.org/10.3390/instruments6020019}}
@article{bib:ALADInO, abstract = {Multimessenger astrophysics is based on the detection, with the highest possible accuracy, of the cosmic radiation. During the last 20 years, the advent space-borne magnetic spectrometers in space (AMS-01, Pamela, AMS-02), able to measure the charged cosmic radiation separating matter from antimatter, and to provide accurate measurement of the rarest components of Cosmic Rays (CRs) to the highest possible energies, have become possible, together with the ultra-precise measurement of ordinary CRs. These developments started the era of precision Cosmic Ray physics providing access to a rich program of high-energy astrophysics addressing fundamental questions like matter-antimatter asymmetry, indirect detection for Dark Matter and the detailed study of origin, acceleration and propagation of CRs and their interactions with the interstellar medium.}, author = {Battiston, R. and {...} and {M. Duranti} and {et al.}}, da = {2021/05/19}, date-added = {2021-06-07 10:13:17 +0200}, date-modified = {2021-06-07 10:14:05 +0200}, doi = {10.1007/s10686-021-09708-w}, id = {Battiston2021}, isbn = {1572-9508}, journal = {Experimental Astronomy}, title = {High precision particle astrophysics as a new window on the universe with an Antimatter Large Acceptance Detector In Orbit (ALADInO)}, ty = {JOUR}, url = {https://doi.org/10.1007/s10686-021-09708-w}, year = {2021}, bdsk-url-1 = {https://doi.org/10.1007/s10686-021-09708-w}}
@article{bib:SLA, abstract = {Low Gain Avalanche Diode (LGAD) is a consolidated technology developed for particle detectors at colliders which allows for simultaneous and accurate time (<100 ps) and position (tens of μm) resolutions. It is a candidate technology that could enable for the first time 5D tracking in space using LGAD Si-microstrip tracking systems. The intrinsic gain of LGAD sensors may also allow to decrease the sensor thickness while achieving signal yields similar to those of Si-microstrips currently operated in Space. In this document we discuss the possible applications and breakthrough opportunities in next generation large area cosmic ray detectors and sub-GeV gamma-ray detectors that could be enabled by LGAD Si-microstrip tracking detectors in Space. We propose the design of a cost-effective instrument demonstrator on a CubeSat platform to enable and qualify the operations of LGAD Si-microstrip detectors in space.}, author = {Matteo Duranti and {et al.}}, doi = {10.1088/1742-6596/2374/1/012046}, journal = {Journal of Physics: Conference Series}, month = {nov}, number = {1}, pages = {012046}, publisher = {IOP Publishing}, title = {Opportunities of Si-microstrip LGAD for next-generation space detectors}, url = {https://dx.doi.org/10.1088/1742-6596/2374/1/012046}, volume = {2374}, year = {2022}, bdsk-url-1 = {https://dx.doi.org/10.1088/1742-6596/2374/1/012046}}
@article{bib:Timing, author = {Duranti, Matteo and {et al.}}, date-modified = {2022-03-23 19:48:36 +0100}, doi = {10.3390/instruments5020020}, issn = {2410-390X}, journal = {Instruments}, month = {May}, number = {2}, pages = {20}, publisher = {MDPI AG}, title = {Advantages and Requirements in Time Resolving Tracking for Astroparticle Experiments in Space}, url = {http://dx.doi.org/10.3390/instruments5020020}, volume = {5}, year = {2021}, bdsk-url-1 = {http://dx.doi.org/10.3390/instruments5020020}}
@article{bib:DAMPENature, abstract = {A direct measurement of cosmic-ray electrons and positrons with unprecedentedly high energy resolution reveals a spectral break at about 0.9 teraelectronvolts, confirming the evidence found by previous indirect measurements.}, author = {Ambrosi, G. and {...} and {M. Duranti} and {et al.}}, da = {2017/12/01}, date-added = {2021-05-06 17:20:07 +0200}, date-modified = {2021-05-06 17:21:03 +0200}, doi = {10.1038/nature24475}, id = {Ambrosi2017}, isbn = {1476-4687}, journal = {Nature}, number = {7683}, pages = {63--66}, title = {Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons}, ty = {JOUR}, url = {https://doi.org/10.1038/nature24475}, volume = {552}, year = {2017}, bdsk-url-1 = {https://doi.org/10.1038/nature24475}}
@article{bib:paper18, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.126.081102}, issue = {8}, journal = {Phys. Rev. Lett.}, month = {Feb}, numpages = {8}, pages = {081102}, publisher = {American Physical Society}, title = {Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.126.081102}, volume = {126}, year = {2021}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.126.081102}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.126.081102}}
@article{bib:paper19, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.126.041104}, issue = {4}, journal = {Phys. Rev. Lett.}, month = {Jan}, numpages = {8}, pages = {041104}, publisher = {American Physical Society}, title = {Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.126.041104}, volume = {126}, year = {2021}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.126.041104}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.126.041104}}
@article{bib:AMSPR2, abstract = {The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on the International Space Station (ISS) conducting a unique, long-duration mission of fundamental physics research in space. The physics objectives include the precise studies of the origin of dark matter, antimatter, and cosmic rays as well as the exploration of new phenomena. Following a 16-year period of construction and testing, and a precursor flight on the Space Shuttle, AMS was installed on the ISS on May 19, 2011. In this report we present results based on 120 billion charged cosmic ray events up to multi-TeV energies. This includes the fluxes of positrons, electrons, antiprotons, protons, and nuclei. These results provide unexpected information, which cannot be explained by the current theoretical models. The accuracy and characteristics of the data, simultaneously from many different types of cosmic rays, provide unique input to the understanding of origins, acceleration, and propagation of cosmic rays.}, author = {M. Aguilar and {...} and {M. Duranti} and {et al.}}, date-added = {2021-01-16 17:11:48 +0100}, date-modified = {2021-01-16 17:11:48 +0100}, doi = {https://doi.org/10.1016/j.physrep.2020.09.003}, issn = {0370-1573}, journal = {Physics Reports}, keywords = {Cosmic ray composition & spectra, Cosmic ray acceleration, Cosmic ray propagation, Cosmic ray sources, Particle astrophysics, Particle dark matter, Cosmic ray detectors, Alpha Magnetic Spectrometer, International space station}, note = {The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part II - Results from the First Seven Years}, pages = {1 - 116}, title = {The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II --- Results from the first seven years}, url = {http://www.sciencedirect.com/science/article/pii/S0370157320303434}, volume = {894}, year = {2021}, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S0370157320303434}, bdsk-url-2 = {https://doi.org/10.1016/j.physrep.2020.09.003}}
@article{bib:TIC_JoI, abstract = {A multi-messenger, space-based cosmic ray detector for gamma rays and charged particles poses several design challenges due to the different instrumental requirements for the two kind of particles. Gamma-ray detection requires layers of high Z materials for photon conversion and a tracking device with a long lever arm to achieve the necessary angular resolution to separate point sources; on the contrary, charge measurements for atomic nuclei requires a thin detector in order to avoid unwanted fragmentation, and a shallow instrument so to maximize the geometric factor. In this paper, a novel tracking approach for gamma rays which tries to reconcile these two conflicting requirements is presented. The proposal is based on the Tracker-In-Calorimeter (TIC) design that relies on a highly-segmented calorimeter to track the incident gamma ray by sampling the lateral development of the electromagnetic shower at different depths. The effectiveness of this approach has been studied with Monte Carlo simulations and has been validated with test beam data of a detector prototype.}, author = {O. Adriani and {...} and {M. Duranti} and {et al.}}, doi = {10.1088/1748-0221/15/09/p09034}, journal = {Journal of Instrumentation}, month = {sep}, number = {09}, pages = {P09034--P09034}, publisher = {{IOP} Publishing}, title = {Tracker-In-Calorimeter ({TIC}): a calorimetric approach to tracking gamma rays in space experiments}, url = {https://doi.org/10.1088%2F1748-0221%2F15%2F09%2Fp09034}, volume = {15}, year = 2020, bdsk-url-1 = {https://doi.org/10.1088%2F1748-0221%2F15%2F09%2Fp09034}, bdsk-url-2 = {https://doi.org/10.1088/1748-0221/15/09/p09034}}
@inproceedings{bib:PAN_IEEE, author = {Ambrosi, Giovanni and {...} and {M. Duranti} and {et al.}}, booktitle = {{2019 IEEE Nuclear Science Symposium (NSS) and Medical Imaging Conference (MIC)}}, date-modified = {2021-01-10 14:30:46 +0100}, doi = {10.1109/NSS/MIC42101.2019.9059946}, journal = {Advances in Space Research}, pages = {2672--2682}, publisher = {IEEE}, title = {{The Penetrating particle ANalyzer (PAN) instrument for measurements of low energy cosmic rays}}, volume = {63}, year = {2019}, bdsk-url-1 = {https://doi.org/10.1109/NSS/MIC42101.2019.9059946}}
@article{bib:PAN, archiveprefix = {arXiv}, author = {Wu, X. and {...} and {M. Duranti} and {et al.}}, doi = {10.1016/j.asr.2019.01.012}, eprint = {1901.04351}, journal = {Adv. Space Res.}, pages = {2672--2682}, primaryclass = {physics.space-ph}, title = {{Penetrating particle ANalyzer (PAN)}}, volume = {63}, year = {2019}, bdsk-url-1 = {https://doi.org/10.1016/j.asr.2019.01.012}}
@article{bib:PreselDB, author = {M. Duranti and {et al.}}, doi = {10.1051/epjconf/201921404030}, journal = {EPJ Web Conf.}, pages = {04030}, title = {Dynamic and on demand data streams}, url = {https://doi.org/10.1051/epjconf/201921404030}, volume = 214, year = 2019, bdsk-url-1 = {https://doi.org/10.1051/epjconf/201921404030}}
@article{bib:DODAS, author = {D. Spiga and {...} and {M. Duranti} and {et al.}}, booktitle = {{International Symposium on Grids and Clouds 2018 in conjunction with Frontiers in Computational Drug Discovery (ISGC 2018 & FCDD) - Infrastructure Clouds and Virtualisation}}, doi = {10.22323/1.327.0024}, journal = {PoS}, title = {DODAS: How to effectively exploit heterogeneous clouds for scientific computations}, volume = {327}, year = {2018}, bdsk-url-1 = {https://doi.org/10.22323/1.327.0024}}
@article{bib:OpenStackSSDC, author = {M. Mariotti and {...} and {M. Duranti} and {et al.}}, booktitle = {{International Symposium on Grids and Clouds 2018 in conjunction with Frontiers in Computational Drug Discovery (ISGC 2018 & FCDD) - Infrastructure Clouds and Virtualisation}}, doi = {10.22323/1.327.0009}, journal = {PoS}, title = {Harvesting dispersed computational resources with OpenStack: a Cloud infrastructure for the Computational Science community}, volume = {327}, year = {2018}, bdsk-url-1 = {https://doi.org/10.22323/1.327.0009}}
@article{bib:DAMPECharge, abstract = {The DArk Matter Particle Explorer (DAMPE) can detect electrons and photons from 5 GeV to 10 TeV and charged nuclei from a few tens of GeV to 100 TeV. The silicon--tungstentracker (STK), which is composed of 768 singled-sided silicon microstrip detectors, is one of four subdetectors in DAMPE providing photon conversion, track reconstruction, and charge identification for relativistic charged particles. This paper focuses on the charge identification performance of the STK detector. The charge response depends mainly on the incident angle and the impact position of the incoming particle. To improve the charge resolution, a reconstruction algorithm to correct for these parameters was tested during a test beam campaign conducted with a high-intensity ion beam at CERN. This algorithm was successfully applied to the ion test beam and the ion charge of Z=4∼10 and was successfully reconstructed for both normal and 9$\,^{\circ}$incident beams.}, author = {Rui Qiao and {...} and {M. Duranti} and {et al.}}, doi = {https://doi.org/10.1016/j.nima.2019.04.036}, issn = {0168-9002}, journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, keywords = {DAMPE, STK, Silicon microstrip detector, Charge reconstruction, Charge sharing}, pages = {24 - 29}, title = {A charge reconstruction algorithm for DAMPE silicon microstrip detectors}, url = {http://www.sciencedirect.com/science/article/pii/S016890021930484X}, volume = {935}, year = {2019}, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S016890021930484X}, bdsk-url-2 = {https://doi.org/10.1016/j.nima.2019.04.036}}
@article{bib:AMS100, abstract = {The next generation magnetic spectrometer in space, AMS-100, is designed to have a geometrical acceptance of 100 m 2 sr and to be operated for at least ten years at the Sun--Earth Lagrange Point 2. Compared to existing experiments, it will improve the sensitivity for the observation of new phenomena in cosmic rays, and in particular in cosmic antimatter, by at least a factor of 1000. The magnet design is based on high temperature superconductor tapes, which allow the construction of a thin solenoid with a homogeneous magnetic field of 1 Tesla inside. The inner volume is instrumented with a silicon tracker reaching a maximum detectable rigidity of 100 TV and a calorimeter system that is 70 radiation lengths deep, equivalent to four nuclear interaction lengths, which extends the energy reach for cosmic-ray nuclei up to the PeV scale, i.e. beyond the cosmic-ray knee. Covering most of the sky continuously, AMS-100 will detect high-energy gamma-rays in the calorimeter system and by pair conversion in the thin solenoid, reconstructed with excellent angular resolution in the silicon tracker.}, author = {S. Schael and {...} and {M. Duranti} and {et al.}}, doi = {https://doi.org/10.1016/j.nima.2019.162561}, issn = {0168-9002}, journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, keywords = {Cosmic rays, Dark matter, Antimatter, Cosmic-ray knee, High-energy gamma-rays, Multi-messenger astrophysics}, pages = {162561}, title = {AMS-100: The next generation magnetic spectrometer in space -- An international science platform for physics and astrophysics at Lagrange point 2}, url = {http://www.sciencedirect.com/science/article/pii/S0168900219310848}, volume = {944}, year = {2019}, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900219310848}, bdsk-url-2 = {https://doi.org/10.1016/j.nima.2019.162561}}
@article{bib:paper17, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS}, doi = {10.1103/PhysRevLett.124.211102}, journal = {Physical Review Letters}, number = {21}, pages = {211102}, title = {Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer}, volume = {124}, year = {2020}, bdsk-url-1 = {https://doi.org/10.1103/PhysRevLett.124.211102}}
@article{bib:paper16, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.123.181102}, issue = {18}, journal = {Phys. Rev. Lett.}, month = {Nov}, numpages = {8}, pages = {181102}, publisher = {American Physical Society}, title = {Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.123.181102}, volume = {123}, year = {2019}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.123.181102}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.123.181102}}
@article{bib:paper15, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.122.101101}, issue = {10}, journal = {Phys. Rev. Lett.}, month = {Mar}, numpages = {9}, pages = {101101}, publisher = {American Physical Society}, title = {Towards Understanding the Origin of Cosmic-Ray Electrons}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.122.101101}, volume = {122}, year = {2019}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.122.101101}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.122.101101}}
@article{bib:CaloCube_proceeding, abstract = {Given the good performances in terms of geometrical acceptance and energy resolution, calorimeters are the best suited detectors to measure high energy cosmic rays directly in space. However, in order to exploit this potential, the design of calorimeters must be carefully optimized to take into account all limitations related to space missions, due mainly to the mass of the experimental apparatus. CaloCube is a three years R&D project, approved and financed by INFN in 2014, aiming to optimize the design of a space-borne calorimeter by the use of a cubic, homogeneous and isotropic geometry. In order to maximize detector performances with respect to the total mass of the apparatus, comparative studies on different scintillating materials, different sizes of crystals and different spacings among them have been performed making use of Monte Carlo simulations. In parallel to this activity, several prototypes instrumented with CsI:Tl cubic crystals have been constructed and tested with particle beams (muons, electrons, protons and ions). Both simulations and prototypes showed that the CaloCube design leads to a good particle energy resolution ( 3:5 m2 sr for electromagnetic showers, > 2:5 m2 sr for hadronic showers). Thanks to these performances, in 5 years of operation it would be possible to measure the ux of electrons+positrons up to some tens of TeV and the uxes of protons and nuclei up to some units of PeV/nucleon, hence extending these measurements by at least one order of magnitude in energy compared to the experiments currently operating in space.}, author = {E Berti and {...} and {M. Duranti} and {et al.}}, date-added = {2019-05-17 12:27:13 +0200}, date-modified = {2019-05-17 12:29:18 +0200}, doi = {10.1088/1742-6596/1162/1/012042}, journal = {Journal of Physics: Conference Series}, month = {jan}, pages = {012042}, publisher = {{IOP} Publishing}, title = {{CaloCube}: a new concept calorimeter for the detection of high energy cosmic rays in space}, url = {https://doi.org/10.1088%2F1742-6596%2F1162%2F1%2F012042}, volume = {1162}, year = 2019, bdsk-url-1 = {https://doi.org/10.1088%2F1742-6596%2F1162%2F1%2F012042}, bdsk-url-2 = {https://doi.org/10.1088/1742-6596/1162/1/012042}}
@article{bib:RICAP2018, author = {M. Duranti}, date-added = {2019-05-17 11:31:43 +0200}, date-modified = {2019-05-17 11:32:01 +0200}, doi = {10.1051/epjconf/201920901014}, journal = {EPJ Web Conf.}, pages = {01014}, title = {The AMS-02 detector on the ISS - Status and highlights, after the first 7 years on orbit}, url = {https://doi.org/10.1051/epjconf/201920901014}, volume = 209, year = 2019, bdsk-url-1 = {https://doi.org/10.1051/epjconf/201920901014}}
@article{bib:paper14, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.122.041102}, issue = {4}, journal = {Phys. Rev. Lett.}, month = {Jan}, numpages = {9}, pages = {041102}, publisher = {American Physical Society}, title = {Towards Understanding the Origin of Cosmic-Ray Positrons}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.122.041102}, volume = {122}, year = {2019}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.122.041102}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.122.041102}}
@article{bib:TIC_proceeding, author = {Bigongiari, Gabriele and {...} and {M. Duranti} and {et al.}}, date-modified = {2019-05-17 12:29:26 +0200}, doi = {10.3390/universe5030072}, journal = {Universe}, month = {03}, pages = {72}, title = {A New Approach to Calorimetry in Space-Based Experiments for High-Energy Cosmic Rays}, volume = {5}, year = {2019}, bdsk-url-1 = {https://doi.org/10.3390/universe5030072}}
@article{bib:DAMPETrackerAlignment, abstract = {The DArk Matter Particle Explorer (DAMPE) is a space-borne particle detector designed to probe electrons and gamma-rays in the few GeV to 10 TeV energy range, as well as cosmic-ray proton and nuclei components between 10 GeV and 100 TeV. The silicon--tungsten tracker--converter is a crucial component of DAMPE. It allows the direction of incoming photons converting into electron--positron pairs to be estimated, and the trajectory and charge (Z) of cosmic-ray particles to be identified. It consists of 768 silicon micro-strip sensors assembled in 6 double layers with a total active area of 6.6 m2. Silicon planes are interleaved with three layers of tungsten plates, resulting in about one radiation length of material in the tracker. Internal alignment parameters of the tracker have been determined on orbit, with non-showering protons and helium nuclei. We describe the alignment procedure and present the position resolution and alignment stability measurements.}, author = {A. Tykhonov and {...} and {M. Duranti} and {et al.}}, doi = {https://doi.org/10.1016/j.nima.2018.02.105}, issn = {0168-9002}, journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, keywords = {Cosmic-ray detectors, Gamma-ray telescopes, Alignment, Silicon-strip detectors}, pages = {43 - 56}, title = {Internal alignment and position resolution of the silicon tracker of DAMPE determined with orbit data}, url = {http://www.sciencedirect.com/science/article/pii/S0168900218302936}, volume = {893}, year = {2018}, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900218302936}, bdsk-url-2 = {https://doi.org/10.1016/j.nima.2018.02.105}}
@article{bib:DAMPETrackerNIM, author = {A. Tykhonov and {...} and {M. Duranti} and {et al.}}, date-modified = {2021-01-10 14:22:39 +0100}, doi = {https://doi.org/10.1016/j.nima.2018.06.036}, issn = {0168-9002}, journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment}, keywords = {Spaceborne experiment, Dark matter, Cosmic rays, Gamma rays, Silicon tracker}, pages = {309-315}, title = {In-flight performance of the DAMPE silicon tracker}, url = {http://www.sciencedirect.com/science/article/pii/S0168900218307575}, volume = {924}, year = {2019}, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900218307575}, bdsk-url-2 = {https://doi.org/10.1016/j.nima.2018.06.036}}
@article{bib:paper13, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.121.051103}, issue = {5}, journal = {Phys. Rev. Lett.}, month = {Jul}, numpages = {8}, pages = {051103}, publisher = {American Physical Society}, title = {Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.121.051103}, volume = {121}, year = {2018}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.121.051103}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.121.051103}}
@article{bib:paper12, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.121.051101}, issue = {5}, journal = {Phys. Rev. Lett.}, month = {Jul}, numpages = {7}, pages = {051101}, publisher = {American Physical Society}, title = {Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.121.051101}, volume = {121}, year = {2018}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.121.051101}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.121.051101}}
@article{bib:paper11, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.121.051102}, issue = {5}, journal = {Phys. Rev. Lett.}, month = {Jul}, numpages = {8}, pages = {051102}, publisher = {American Physical Society}, title = {Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.121.051102}, volume = {121}, year = {2018}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.121.051102}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.121.051102}}
@article{bib:paper10, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.120.021101}, issue = {2}, journal = {Phys. Rev. Lett.}, month = {Jan}, numpages = {8}, pages = {021101}, publisher = {American Physical Society}, title = {Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.120.021101}, volume = {120}, year = {2018}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.120.021101}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.120.021101}}
@article{bib:paper9, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.119.251101}, issue = {25}, journal = {Phys. Rev. Lett.}, month = {Dec}, numpages = {8}, pages = {251101}, publisher = {American Physical Society}, title = {Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.119.251101}, volume = {119}, year = {2017}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.119.251101}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.119.251101}}
@article{bib:HERDICRC2, author = {Dong, Yongwei and {...} and {M. Duranti} and {et al.}}, booktitle = {{The Fluorescence detector Array of Single-pixel Telescopes: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)}}, date-modified = {2021-01-10 14:24:34 +0100}, doi = {10.22323/1.301.0253}, journal = {PoS}, pages = {253}, slaccitation = {%%CITATION = POSCI,ICRC2017,253;%%}, title = {{A novel 3-D calorimeter for the High Energy cosmic-Radiation Detection (HERD) Facility onboard China's Future Space Station}}, volume = {301 - ICRC2017}, year = {2018}, bdsk-url-1 = {https://doi.org/10.22323/1.301.0253}}
@article{bib:HERDICRC1, author = {Zhang, Shuang-Nan and {...} and {M. Duranti} and {et al.}}, booktitle = {{The Fluorescence detector Array of Single-pixel Telescopes: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)}}, date-modified = {2021-01-10 14:24:51 +0100}, doi = {10.22323/1.301.1077}, journal = {PoS}, pages = {1077}, slaccitation = {%%CITATION = POSCI,ICRC2017,1077;%%}, title = {{Introduction to the High Energy cosmic-Radiation Detection (HERD) Facility onboard China's Future Space Station}}, volume = {301 - ICRC2017}, year = {2018}, bdsk-url-1 = {https://doi.org/10.22323/1.301.1077}}
@article{bib:paper8, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, date-added = {2017-01-13 16:10:24 +0000}, date-modified = {2017-01-13 16:10:33 +0000}, doi = {10.1103/PhysRevLett.117.231102}, issue = {23}, journal = {Phys. Rev. Lett.}, month = {Nov}, numpages = {8}, pages = {231102}, publisher = {American Physical Society}, title = {Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station}, url = {http://link.aps.org/doi/10.1103/PhysRevLett.117.231102}, volume = {117}, year = {2016}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.117.231102}, bdsk-url-2 = {http://dx.doi.org/10.1103/PhysRevLett.117.231102}}
@inproceedings{bib:HERDBT, abstract = { The High Energy cosmic-Radiation Detection (HERD) facility is one of several space astronomy payloads of the cosmic light house program onboard China's Space Station, which is planned for operation starting around 2020 for about 10 years. Beam test with a HERD prototype, to verify the HERD specifications and the reading out method of wavelength shifting fiber and image intensified CCD, was taken at CERN SPS in November, 2015. The prototype is composed of an array of 5510 LYSO crystals, which is 1/40th of the scale of HERD calorimeter. Experimental results on the performances of the calorimeter are discussed. }, author = {Dong, Yongwei and {...} and {M. Duranti} and {et al.}}, booktitle = {{Proc. SPIE 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray}}, doi = {10.1117/12.2231804}, journal = {Proc. SPIE}, pages = {99056D-99056D-8}, title = {Experimental verification of the HERD prototype at CERN SPS}, url = {http://dx.doi.org/10.1117/12.2231804}, volume = {9905}, year = {2016}, bdsk-url-1 = {http://dx.doi.org/10.1117/12.2231804}}
@article{bib:DAMPEmission, author = {J. Chang and {...} and {M. Duranti} and {et al.}}, doi = {https://doi.org/10.1016/j.astropartphys.2017.08.005}, issn = {0927-6505}, journal = {Astroparticle Physics}, number = {Supplement C}, pages = {6 - 24}, title = {The DArk Matter Particle Explorer mission}, url = {http://www.sciencedirect.com/science/article/pii/S0927650517300841}, volume = {95}, year = {2017}, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S0927650517300841}, bdsk-url-2 = {https://doi.org/10.1016/j.astropartphys.2017.08.005}}
@article{bib:DAMPETracker2, author = {Gallo, Valentina and {...} and {M. Duranti} and {et al.}}, booktitle = {{Proceedings, 25th International Workshop on Vertex Detectors (Vertex 2016): La Biodola, Elba Island, Livorno, Italy, September 26-30, 2016}}, date-modified = {2021-01-10 14:27:02 +0100}, doi = {https://doi.org/10.22323/1.287.0010}, journal = {PoS}, pages = {010}, slaccitation = {%%CITATION = POSCI,Vertex2016,010;%%}, title = {{The DAMPE silicon tungsten tracker}}, volume = {287 - Vertex2016}, year = {2017}, bdsk-url-1 = {https://doi.org/10.22323/1.287.0010}}
@article{bib:DAMPETracker, author = {P. Azzarello and {...} and {M. Duranti} and {et al.}}, date-modified = {2021-01-10 14:27:57 +0100}, doi = {10.1016/j.nima.2016.02.077}, journal = {Nucl. Instrum. Meth.}, reportnumber = {DAMPE-2016-001}, slaccitation = {%%CITATION = DAMPE-2016-001;%%}, title = {{The DAMPE silicon--tungsten tracker}}, url = {http://dx.doi.org/10.1016/j.nima.2016.02.077}, volume = {831}, year = {2016}, bdsk-url-1 = {http://dx.doi.org/10.1016/j.nima.2016.02.077}}
@article{bib:ICRC2015_DAMPETrackerWu, author = {Wu, X. and {...} and {M. Duranti} and {et al.}}, booktitle = {Proceedings of The 34th International Cosmic Ray Conference {\textemdash} PoS(ICRC2015)}, document_type = {Conference Paper}, doi = {10.22323/1.236.1192}, journal = {Proceedings of Science}, pages = {1192}, title = {The silicon-tungsten tracker of the DAMPE mission}, url = {https://pos.sissa.it/236/1192/}, volume = {236}, year = 2016, bdsk-url-1 = {https://pos.sissa.it/236/1192/}, bdsk-url-2 = {https://doi.org/10.22323/1.236.1192}}
@article{bib:ICRC2015_DAMPETrackerGallo, author = {Gallo, V. and {...} and {M. Duranti} and {et al.}}, booktitle = {Proceedings of The 34th International Cosmic Ray Conference {\textemdash} PoS(ICRC2015)}, document_type = {Conference Paper}, doi = {10.22323/1.236.1199}, journal = {Proceedings of Science}, pages = {1199}, title = {The test results of the silicon tungsten tracker of DAMPE}, url = {https://pos.sissa.it/236/1199/}, volume = {236}, year = 2016, bdsk-url-1 = {https://pos.sissa.it/236/1199/}, bdsk-url-2 = {https://doi.org/10.22323/1.236.1199}}
@article{bib:paper7, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.117.091103}, issue = {9}, journal = {Phys. Rev. Lett.}, month = {Aug}, numpages = {10}, pages = {091103}, publisher = {American Physical Society}, title = {Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station}, url = {https://link.aps.org/doi/10.1103/PhysRevLett.117.091103}, volume = {117}, year = {2016}, bdsk-url-1 = {https://link.aps.org/doi/10.1103/PhysRevLett.117.091103}, bdsk-url-2 = {https://doi.org/10.1103/PhysRevLett.117.091103}}
@article{bib:paper6, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.115.211101}, issue = {21}, journal = {Phys. Rev. Lett.}, month = {Nov}, numpages = {9}, pages = {211101}, publisher = {American Physical Society}, title = {Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with the Alpha Magnetic Spectrometer on the International Space Station}, url = {http://link.aps.org/doi/10.1103/PhysRevLett.115.211101}, volume = {115}, year = {2015}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.115.211101}, bdsk-url-2 = {http://dx.doi.org/10.1103/PhysRevLett.115.211101}}
@article{bib:paper5, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, doi = {10.1103/PhysRevLett.114.171103}, issue = {17}, journal = {Phys. Rev. Lett.}, month = {Apr}, numpages = {9}, pages = {171103}, publisher = {American Physical Society}, title = {Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station}, url = {http://link.aps.org/doi/10.1103/PhysRevLett.114.171103}, volume = {114}, year = {2015}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.114.171103}, bdsk-url-2 = {http://dx.doi.org/10.1103/PhysRevLett.114.171103}}
@article{bib:paper4, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {(AMS Collaboration)}, doi = {10.1103/PhysRevLett.113.221102}, issue = {22}, journal = {Phys. Rev. Lett.}, month = {Nov}, numpages = {7}, pages = {221102}, publisher = {American Physical Society}, title = {Precision Measurement of the $({e}^{+}+{e}^{-})$ Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station}, url = {http://link.aps.org/doi/10.1103/PhysRevLett.113.221102}, volume = {113}, year = {2014}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.113.221102}, bdsk-url-2 = {http://dx.doi.org/10.1103/PhysRevLett.113.221102}}
@article{bib:paper3, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {(AMS Collaboration)}, doi = {10.1103/PhysRevLett.113.121102}, issue = {12}, journal = {Phys. Rev. Lett.}, month = {Sep}, numpages = {9}, pages = {121102}, publisher = {American Physical Society}, title = {Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station}, url = {http://link.aps.org/doi/10.1103/PhysRevLett.113.121102}, volume = {113}, year = {2014}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.113.121102}, bdsk-url-2 = {http://dx.doi.org/10.1103/PhysRevLett.113.121102}}
@article{bib:paper2, author = {Accardo, L. and {...} and {M. Duranti} and {et al.}}, collaboration = {(AMS Collaboration)}, doi = {10.1103/PhysRevLett.113.121101}, issue = {12}, journal = {Phys. Rev. Lett.}, month = {Sep}, numpages = {9}, pages = {121101}, publisher = {American Physical Society}, title = {High Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5\char21{}500 GeV with the Alpha Magnetic Spectrometer on the International Space Station}, url = {http://link.aps.org/doi/10.1103/PhysRevLett.113.121101}, volume = {113}, year = {2014}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.113.121101}, bdsk-url-2 = {http://dx.doi.org/10.1103/PhysRevLett.113.121101}}
@article{bib:paper1, author = {Aguilar, M. and {...} and {M. Duranti} and {et al.}}, collaboration = {AMS Collaboration}, date-modified = {2014-07-30 13:30:08 +0000}, doi = {10.1103/PhysRevLett.110.141102}, issue = {14}, journal = {Phys. Rev. Lett.}, month = {Apr}, numpages = {10}, pages = {141102}, publisher = {American Physical Society}, title = {First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5--350 GeV}, url = {http://dx.doi.org/10.1103/PhysRevLett.110.141102}, volume = {110}, year = {2013}, bdsk-url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.110.141102}}
@unpublished{bib:note1, author = {M. Duranti and {et al.}}, month = 7, note = {\textbf{AMS Note 2014-06-09}}, title = {AMS-02 $e^+$ + $e^-$ flux measurement: part 1 - signal selection}, url = {http://ams.cern.ch/AMS/Reports/AMSnotes2014/AMSnote-2014_0609(1).pdf}, year = 2014, bdsk-url-1 = {http://ams.cern.ch/AMS/Reports/AMSnotes2014/AMSnote-2014_0609(1).pdf}}
@unpublished{bib:note2, author = {M. Duranti and {et al.}}, month = 7, note = {\textbf{AMS Note 2014-06-09}}, title = {AMS-02 $e^+$ + $e^-$ flux measurement: part 2 - detector acceptance and efficiencies}, url = {http://ams.cern.ch/AMS/Reports/AMSnotes2014/AMSnote-2014_0609(2).pdf}, year = 2014, bdsk-url-1 = {http://ams.cern.ch/AMS/Reports/AMSnotes2014/AMSnote-2014_0609(2).pdf}}
@unpublished{bib:note3, author = {M. Duranti and {et al.}}, month = 7, note = {\textbf{AMS Note 2014-06-09}}, title = {AMS-02 $e^+$ + $e^-$ flux measurement: part 3 - flux evaluation}, url = {http://ams.cern.ch/AMS/Reports/AMSnotes2014/AMSnote-2014_0609(3).pdf}, year = 2014, bdsk-url-1 = {http://ams.cern.ch/AMS/Reports/AMSnotes2014/AMSnote-2014_0609(3).pdf}}
@article{bib:IsotopicComposition, author = {M. Aguilar and {...} and {M. Duranti} and {et al.}}, date-modified = {2014-07-30 13:29:54 +0000}, doi = {10.1088/0004-637X/736/2/105}, issn = {0004-637X}, journal = {ApJ}, pages = 105, title = {Isotopic Composition Of Light Nuclei In Cosmic Rays: Results From AMS-01}, url = {http://dx.doi.org/10.1088/0004-637X/736/2/105}, volume = 736, year = 2011, bdsk-url-1 = {http://dx.medra.org/10.1088/0004-637X/736/2/105}}
@article{bib:RelativeComposition, author = {M. Aguilar and {...} and {M. Duranti} and {et al.}}, date-modified = {2014-07-30 13:29:43 +0000}, doi = {10.1088/0004-637X/724/1/329}, issn = {0004-637X}, journal = {ApJ}, pages = {329--340}, title = {Relative Composition and Energy Spectra Of Light Nuclei In Cosmic Rays: Results From AMS-01}, url = {http://dx.doi.org/10.1088/0004-637X/724/1/329}, volume = {724 and Number 1}, year = 2010, bdsk-url-1 = {http://dx.medra.org/10.1088/0004-637X/724/1/329}}
@article{bib:TrackerAlignment, author = {B. Alpat and {...} and {M. Duranti} and {et al.}}, date-modified = {2014-07-30 13:27:50 +0000}, doi = {10.1016/j.nima.2009.11.065}, issn = {0168-9002}, journal = {Nucl. Instr. Meth. Phys. Res. A}, pages = {207--217}, title = {The internal alignment and position resolution of the AMS-02 silicon tracker determined with cosmic-ray muons}, url = {http://dx.doi.org/10.1016/j.nima.2009.11.065}, volume = {613 and Issue 2}, year = 2010, bdsk-url-1 = {http://dx.medra.org/10.1016/j.nima.2009.11.065}}
@article{bib:TrackerUpgrade, author = {K. L{\"u}belsmeyer and {...} and {M. Duranti} and {et al.}}, date-added = {2013-02-13 16:28:16 +0000}, date-modified = {2014-07-30 13:29:29 +0000}, doi = {10.1016/j.nima.2011.06.051}, issn = {0168-9002}, journal = {Nucl. Instr. Meth. Phys. Res. A}, pages = {639-648}, title = {Upgrade of the Alpha Magnetic Spectrometer (AMS-02) for long term operation on the International Space Station (ISS)}, url = {http://dx.doi.org/10.1016/j.nima.2011.06.051}, volume = 654, year = 2011, bdsk-url-1 = {http://www.sciencedirect.com/science/article/pii/S0168900211011752}}
@inproceedings{bib:RICAP2016, author = {Duranti, Matteo}, booktitle = {{RICAP2016}}, doi = {10.1051/epjconf/201713602004}, journal = {EPJ Web Conf.}, pages = {02004}, title = {{The AMS-02 detector on the International Space Station - The status after the first 5 years on orbit}}, url = {https://doi.org/10.1051/epjconf/201713602004}, volume = 136, year = 2017, bdsk-url-1 = {https://doi.org/10.1051/epjconf/201713602004}}
@inproceedings{bib:Moriond2014, author = {Duranti, M.}, booktitle = {{Proceedings, 49th Rencontres de Moriond on Electroweak Interactions and Unified Theories}}, pages = {169-176}, slaccitation = {%%CITATION = INSPIRE-1338142;%%}, title = {{The AMS-02 detector after 1000 days on the international space station}}, url = {http://inspirehep.net/record/1338142/files/Pages_from_C14-03-15--1_169.pdf}, year = {2014}, bdsk-url-1 = {http://inspirehep.net/record/1338142/files/Pages_from_C14-03-15--1_169.pdf}}
@inproceedings{bib:IFAE13, author = {Duranti, M.}, booktitle = {IFAE2013 (C037)}, collaboration = {AMS}, date-modified = {2014-07-30 13:52:09 +0000}, doi = {10.1393/ncc/i2014-11682-9}, journal = {Nuovo Cim.}, number = {01}, pages = {161-166}, title = {{AMS-02 - Status and first results}}, url = {http://dx.doi.org/10.1393/ncc/i2014-11682-9}, year = {2014}, bdsk-url-1 = {http://dx.doi.org/10.1393/ncc/i2014-11682-9}}
@inproceedings{bib:RD11, author = {Duranti, Matteo}, booktitle = {RD11}, collaboration = {AMS-02 Collaboration}, date-modified = {2014-07-30 13:28:44 +0000}, journal = {PoS}, pages = {011}, title = {{The AMS-02 Silicon Tracker status}}, url = {http://inspirehep.net/record/1206749/files/RD11_011.pdf}, year = {2011}, bdsk-url-1 = {http://inspirehep.net/record/1206749/files/RD11_011.pdf}}
@inproceedings{bib:Vertex2012, author = {Duranti, Matteo}, booktitle = {Vertex2012}, collaboration = {AMS-02 Tracker}, date-modified = {2014-07-30 13:28:55 +0000}, journal = {PoS}, pages = {052}, title = {{The AMS-02 Silicon Tracker after 500 days in space}}, url = {http://inspirehep.net/record/1247108/files/Vertex\%202012_052.pdf}, year = {2013}, bdsk-url-1 = {http://inspirehep.net/record/1247108/files/Vertex%5C%202012_052.pdf}}
@inproceedings{bib:ICRC2013TrackerAlignment, adsnote = {Provided by the SAO/NASA Astrophysics Data System}, adsurl = {https://ui.adsabs.harvard.edu/abs/2013ICRC...33..570A}, author = {{Ambrosi}, G. and {...} and {M. Duranti} and {et al.}}, booktitle = {International Cosmic Ray Conference}, keywords = {Silicon Tracker, Cosmic Ray Detector, Alignment}, month = jan, pages = {570}, series = {International Cosmic Ray Conference}, title = {{Alignment of the AMS-02 Silicon Tracker}}, volume = {33}, year = 2013}
@inproceedings{bib:ICRC2013TrackerCharge, adsnote = {Provided by the SAO/NASA Astrophysics Data System}, adsurl = {https://ui.adsabs.harvard.edu/abs/2013ICRC...33.2102A}, author = {{Ambrosi}, G. and {...} and {M. Duranti} and {et al.}}, booktitle = {International Cosmic Ray Conference}, keywords = {Charged Particles, Cosmic Ray Detector, Silicon Tracker.}, month = jan, pages = {2102}, series = {International Cosmic Ray Conference}, title = {{Nuclear Charge Measurement with the AMS-02 Silicon Tracker}}, volume = {33}, year = 2013}
@inproceedings{bib:ICRC2013TrackerOperations, adsnote = {Provided by the SAO/NASA Astrophysics Data System}, adsurl = {https://ui.adsabs.harvard.edu/abs/2013ICRC...33.2121A}, author = {{Ambrosi}, G. and {...} and {M. Duranti} and {et al.}}, booktitle = {International Cosmic Ray Conference}, keywords = {AMS-02, silicon Tracker, calibration, performance.}, month = jan, pages = {2121}, series = {International Cosmic Ray Conference}, title = {{In-flight Operations and Efficiency of the AMS-02 Silicon Tracker}}, volume = {33}, year = 2013}
@inproceedings{bib:ICRC2013TrackerReconstruction, adsnote = {Provided by the SAO/NASA Astrophysics Data System}, adsurl = {https://ui.adsabs.harvard.edu/abs/2013ICRC...33.2306A}, author = {{Ambrosi}, G. and {...} and {M. Duranti} and {et al.}}, booktitle = {International Cosmic Ray Conference}, keywords = {AMS, silicon tracker, resolution}, month = jan, pages = {2306}, series = {International Cosmic Ray Conference}, title = {{AMS-02 Track Reconstruction and Rigidity Measurement}}, volume = {33}, year = 2013}
@inproceedings{bib:ICRC2015, author = {Duranti, Matteo}, booktitle = {ICRC2015}, collaboration = {AMS-02 Collaboration}, date-modified = {2021-01-10 14:35:13 +0100}, journal = {PoS}, pages = {273}, title = {{Precision measurement of the fluxes of electrons and positrons in Primary Cosmic Rays up to the TeV with the Alpha Magnetic Spectrometer}}, url = {http://pos.sissa.it/archive/conferences/236/273/ICRC2015_273.pdf}, volume = {ICRC2015}, year = {2015}, bdsk-url-1 = {http://pos.sissa.it/archive/conferences/236/273/ICRC2015%5C_273.pdf}}
@inproceedings{bib:ICRC2015Fiandra, author = {E. Fiandrini and {...} and {M. Duranti} and {et al.}}, booktitle = {ICRC2015}, date-modified = {2021-01-10 14:35:21 +0100}, journal = {PoS}, pages = {095}, title = {{Time dependent Geomagnetic Cutoff estimation along the ISS orbit}}, url = {http://pos.sissa.it/archive/conferences/236/095/ICRC2015_095.pdf}, volume = {ICRC2015}, year = {2015}, bdsk-url-1 = {http://pos.sissa.it/archive/conferences/236/095/ICRC2015%5C_095.pdf}}
@inproceedings{bib:ICRC2015Grandi, author = {D. Grandi and {...} and {M. Duranti} and {et al.}}, booktitle = {ICRC2015}, date-modified = {2021-01-10 14:35:28 +0100}, journal = {PoS}, pages = {116}, title = {{Trajectory reconstruction in the Earth Magnetosphere using TS05 model and evaluation of geomagnetic cutoff in AMS-02 data}}, url = {http://pos.sissa.it/archive/conferences/236/116/ICRC2015_116.pdf}, volume = {ICRC2015}, year = {2015}, bdsk-url-1 = {http://pos.sissa.it/archive/conferences/236/116/ICRC2015%5C_116.pdf}}
@inproceedings{bib:ICRC2015Vitillo, author = {G. Ambrosi and {...} and {M. Duranti} and {et al.}}, booktitle = {ICRC2015}, date-modified = {2021-01-10 14:35:35 +0100}, journal = {PoS}, pages = {429}, title = {{Nuclei Charge measurement with the AMS-02 Silicon Tracker}}, url = {http://pos.sissa.it/archive/conferences/236/429/ICRC2015_429.pdf}, volume = {ICRC2015}, year = {2015}, bdsk-url-1 = {http://pos.sissa.it/archive/conferences/236/429/ICRC2015%5C_429.pdf}}
@inproceedings{bib:ICRC2015Qin, author = {G. Ambrosi and {...} and {M. Duranti} and {et al.}}, booktitle = {ICRC2015}, date-modified = {2021-01-10 14:35:40 +0100}, journal = {PoS}, pages = {690}, title = {{In-flight operations and status of the AMS-02 silicon tracker}}, url = {http://pos.sissa.it/archive/conferences/236/690/ICRC2015_690.pdf}, volume = {ICRC2015}, year = {2015}, bdsk-url-1 = {http://pos.sissa.it/archive/conferences/236/690/ICRC2015%5C_690.pdf}}
@inproceedings{bib:CHEP2015, author = {D'Urso, Domenico and {...} and {M. Duranti} and {et al.}}, booktitle = {{Proceedings, 21st International Conference on Computing in High Energy and Nuclear Physics (CHEP 2015)}}, doi = {10.1088/1742-6596/664/7/072016}, journal = {J. Phys. Conf. Ser.}, pages = {072016}, slaccitation = {%%CITATION = 00462,664,072016;%%}, title = {{A flexible and modular data format ROOT-based implementation for HEP}}, url = {http://dx.doi.org/10.1088/1742-6596/664/7/072016}, volume = {664}, year = {2015}, bdsk-url-1 = {http://dx.doi.org/10.1088/1742-6596/664/7/072016}}
@inproceedings{bib:CHEP2015Sapunenko, abstract = {Data management constitutes one of the major challenges that a geographically- distributed e-Infrastructure has to face, especially when remote data access is involved. We discuss an integrated solution which enables transparent and efficient access to on-line and near-line data through high latency networks. The solution is based on the joint use of the General Parallel File System (GPFS) and of the Tivoli Storage Manager (TSM). Both products, developed by IBM, are well known and extensively used in the HEP computing community. Owing to a new feature introduced in GPFS 3.5, so-called Active File Management (AFM), the definition of a single, geographically-distributed namespace, characterised by automated data flow management between different locations, becomes possible. As a practical example, we present the implementation of AFM-based remote data access between two data centres located in Bologna and Rome, demonstrating the validity of the solution for the use case of the AMS experiment, an astro-particle experiment supported by the INFN CNAF data centre with the large disk space requirements (more than 1.5 PB).}, author = {Vladimir Sapunenko and {...} and {M. Duranti} and {et al.}}, booktitle = {{Proceedings, 21st International Conference on Computing in High Energy and Nuclear Physics (CHEP 2015)}}, date-modified = {2021-01-10 14:41:13 +0100}, journal = {J. Phys. Conf. Ser.}, pages = {042047}, title = {An integrated solution for remote data access}, url = {http://stacks.iop.org/1742-6596/664/i=4/a=042047}, volume = {664}, year = {2015}, bdsk-url-1 = {http://stacks.iop.org/1742-6596/664/i=4/a=042047}}
@article{bib:MultipleVolumeReflection, author = {W. Scandale and {...} and {M. Duranti} and {et al.}}, date-modified = {2014-07-30 13:30:35 +0000}, doi = {10.1103/PhysRevLett.102.084801}, issn = {0031-9007}, journal = {Phys. Rev. Lett.}, title = {Observation of Multiple Volume Reflection of Ultrarelativistic Protons by a Sequence of Several Bent Silicon Crystals}, url = {http://dx.doi.org/10.1103/PhysRevLett.102.084801}, volume = 102, year = 2009, bdsk-url-1 = {http://dx.medra.org/10.1103/PhysRevLett.102.084801}}
@article{bib:RadiationFromVolumeReflection, author = {W. Scandale and {...} and {M. Duranti} and {et al.}}, date-modified = {2014-07-30 13:30:55 +0000}, doi = {10.1103/PhysRevA.79.012903}, issn = {1050-2947}, journal = {Phys. Rev. A}, title = {Experimental study of the radiation emitted by 180 GeV/c electrons and positrons volume-reflected in a bent crystal}, url = {http://dx.doi.org/10.1103/PhysRevA.79.012903}, volume = 79, year = 2009, bdsk-url-1 = {http://dx.medra.org/10.1103/PhysRevA.79.012903}}
@article{bib:VolumeReflection, author = {W. Scandale and {...} and {M. Duranti} and {et al.}}, date-modified = {2014-07-30 13:30:18 +0000}, doi = {10.1103/PhysRevLett.101.234801}, issn = {0031-9007}, journal = {Phys. Rev. Lett.}, title = {Volume Reflection Dependence of 400 GeV/c Protons on the Bent Crystal Curvature}, url = {http://dx.doi.org/10.1103/PhysRevLett.101.234801}, volume = 101, year = 2008, bdsk-url-1 = {http://dx.medra.org/10.1103/PhysRevLett.101.234801}}