Results from AMS-02 on the ISS after 6 years in space

AMS-02 is a cosmic-ray detector which has been operating on the International Space Station since May 2011 to conduct a unique mission of fundamental research in space. More than 100 billion cosmic rays have been collected by AMS-02 after 6 years of operations, providing a detailed insight into the features of different species of cosmic rays. This contribution reviews the recent AMS-02 results based on 6 years of operations in space and their contribution to the advances in the understanding of cosmic-ray origin, acceleration and propagation physics

SiPM and front-end electronics development for Cherenkov light detection

The Italian Institute of Nuclear Physics (INFN) is involved in the development of a demonstrator for a SiPM-based camera for the Cherenkov Telescope Array (CTA) experiment, with a pixel size of 6$\times$6 mm$^2$. The camera houses about two thousands electronics channels and is both light and compact. In this framework, a R&D program for the development of SiPMs suitable for Cherenkov light detection (so called NUV SiPMs) is ongoing. Different photosensors have been produced at Fondazione Bruno Kessler (FBK), with different micro-cell dimensions and fill factors, in different geometrical arrangements. At the same time, INFN is developing front-end electronics based on the waveform sampling technique optimized for the new NUV SiPM. Measurements on 1$\times$1 mm$^2$, 3$\times$3 mm$^2$, and 6$\times$6 mm$^2$ NUV SiPMs coupled to the front-end electronics are presentedComment: In Proceedings of the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. All CTA contributions at arXiv:1508.0589

Characterization and possible astrophysics applications of UV sensitive SiPM devices

The National Institute of Nuclear Physics (INFN) is involved in the R&D of Silicon Photomultiplier (SiPM) sensors optimized to detect near-UV (NUV) photon radiation in low-intensity photons and high-precision time mesaurements, in collaboration with the Bruno Kessler Foundation (FBK). The performances of 6×6 mm2 NUV-HD SiPMs with 30×30 μm2 microcell area and the possible prospects for production and packaging of multi-sensor modules for astrophysical applications are discussed in this paper

ps8 161 the disease burden in patients with longstanding systemic lupus erythematosus focus on health resource use and costs

Introduction As a consequence of increased SLE patients survival, patients with long disease duration represent a significant proportion of our cohorts. This study aims to evaluate health resource use and the 6 months costs in patients with SLE with long disease duration. Methods The economic evaluation was performed in terms of cost-of-illness analysis as part of a larger study enrolling SLE patients with at least 15 years of disease duration regularly followed at our unit. At enrollment, the following information were collected: disease activity (SLEDAI), organ damage (SLICC-DI score), comorbidities, treatment patterns; in addition to clinical data, patients were required to complete an ad-hoc questionnaire for the collection of facts relevant for the estimation of the economic dimension and covering the previous six-months. Such a time frame was considered to be appropriate as recall period. Direct health (drugs, hospitalizations, emergency visits, specialists visits, laboratory tests and instrumental examination) and non-health costs (transportation and accommodation) as well as indirect costs because of productivity loss were estimated. Results 51 adult patients with long disease duration were recruited (98% female, mean age 49±11 years, median disease duration 17 years, IQR 15–23). Median (IQR) SLEDAI score was 2 (0–4), median SLICC-DI was 1 (0–2). The median (IQR) direct health costs per patients over the previous 6 months resulted 410€ (201–1687); indirect costs because of productivity lost were 130€ (0–356). The median overall cost to the Society was 473€ (327–2148); the presence of comorbid conditions resulted associated with higher overall cost for the Society (552€ [327–1807] vs 264€ [94–1164] p=0.046); disease activity and damage at enrollment were not associated with costs increase in this cohort. Conclusions This cohort of patients with long lasting disease is characterised by low disease activity and mild organ damage; in this setting, the disease burden on the single patient and family is significant and the costs to the Society are influenced by the presence of comorbidities

Internal alignment and position resolution of the silicon tracker of DAMPE determined with orbit data

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 m$^2$. 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

INFN Camera demonstrator for the Cherenkov Telescope Array

The Cherenkov Telescope Array is a world-wide project for a new generation of ground-based Cherenkov telescopes of the Imaging class with the aim of exploring the highest energy region of the electromagnetic spectrum. With two planned arrays, one for each hemisphere, it will guarantee a good sky coverage in the energy range from a few tens of GeV to hundreds of TeV, with improved angular resolution and a sensitivity in the TeV energy region better by one order of magnitude than the currently operating arrays. In order to cover this wide energy range, three different telescope types are envisaged, with different mirror sizes and focal plane features. In particular, for the highest energies a possible design is a dual-mirror Schwarzschild-Couder optical scheme, with a compact focal plane. A silicon photomultiplier (SiPM) based camera is being proposed as a solution to match the dimensions of the pixel (angular size of ~ 0.17 degrees). INFN is developing a camera demonstrator made by 9 Photo Sensor Modules (PSMs, 64 pixels each, with total coverage 1/4 of the focal plane) equipped with FBK (Fondazione Bruno Kessler, Italy) Near UltraViolet High Fill factor SiPMs and Front-End Electronics (FEE) based on a Target 7 ASIC, a 16 channels fast sampler (up to 2GS/s) with deep buffer, self-trigger and on-demand digitization capabilities specifically developed for this purpose. The pixel dimensions of $6\times6$ mm$^2$ lead to a very compact design with challenging problems of thermal dissipation. A modular structure, made by copper frames hosting one PSM and the corresponding FEE, has been conceived, with a water cooling system to keep the required working temperature. The actual design, the adopted technical solutions and the achieved results for this demonstrator are presented and discussed.Comment: In Proceedings of the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. All CTA contributions at arXiv:1508.0589