Opendata, web and dolomites

Light-Trap

A SiPM upgrade for VHE Astronomy and beyond

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 Light-Trap project word cloud

Explore the words cloud of the Light-Trap project. It provides you a very rough idea of what is the project "Light-Trap" about.

photons    reducing    scanners    shorter    inserted    direction    resolution    telescopes    pixels    hence    area    goals    overcome    drawbacks    telescope    pmts    observations    experiment    fluorescence    pms    classes    magic    universe    physics    material    cameras    larger    actual    generation    silicon    longer    electronic    uncovered    photodetectors    productive    iact    whipple    lacking    disciplinary    hess    significantly    camera    optimize    mature    threshold    reconstruct    rays    utilizing    astronomy    imaging    sub    vhe    cosmic    sipms    source    veritas    view    noise    integrating    light    technique    primary    collection    agenda    ground    standard    cluster    medical    ultra    regime    generations    cta    shifting    relatively    gamma    sipm    background    gt    wavelength    ray    array    collecting    detection    energy    interesting    incoming    replace    tested    small    pixel    upgrades    gev    efficiency    wavelengths    pet    angular    fast    cherenkov    photomultipliers    astrophysics    physical    sensitivity    atmospheric   

Project "Light-Trap" data sheet

The following table provides information about the project.

Coordinator
INSTITUTO DE FISICA DE ALTAS ENERGIAS 

Organization address
address: CAMPUS DE BELLATERRA - UNIVERSIDAD AUTONOMA DE BARCELONA
city: CERDANYOLA DEL VALLES
postcode: 8193
website: http://www.ifae.es

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Spain [ES]
 Project website http://www.ifae.es
 Total cost 158˙121 €
 EC max contribution 158˙121 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2014
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2015
 Duration (year-month-day) from 2015-04-01   to  2017-03-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    INSTITUTO DE FISICA DE ALTAS ENERGIAS ES (CERDANYOLA DEL VALLES) coordinator 158˙121.00

Map

 Project objective

Ground-based gamma-ray astronomy in the Very High Energy (VHE, E>100 GeV) regime has fast become one of the most interesting and productive sub-fields of astrophysics today. Utilizing the Imaging Atmospheric Cherenkov Technique (IACT) to reconstruct the energy and direction of incoming gamma-ray photons from the universe, several source-classes have been uncovered by previous and current generations of IACT telescopes (e.g. Whipple, MAGIC, HESS, VERITAS). The next generation IACT experiment, the Cherenkov Telescope Array (CTA) will provide increased sensitivity across a wider energy range and with better angular resolution. However, research into new and improved technology for potential upgrades of the CTA system are already being considered. Improving the light-collection efficiency (hence reducing the energy threshold) and field-of-view of CTA cameras is high on the agenda of future upgrades. One may also consider increasing the number of telescopes if the cost of the cameras could be significantly reduced. The primary path to these goals is to replace PhotoMultipliers (PMTs) with Silicon-PMs (SiPM). These new photodetectors will also find multi-disciplinary use in e.g. in fluorescence telescopes for detection of Ultra High Energy Cosmic Rays and PET scanners in medical physics. However SiPMs are not yet mature enough to replace PMTs for several reasons: sensitivity to unwanted longer wavelengths while lacking sensitivity at short wavelengths, small physical area, high cost and electronic noise. Here we propose a novel method to build relatively low-cost SiPM-based pixels utilizing wavelength-shifting material which overcome some of these drawbacks by collecting light over a larger area than standard SiPMs and improving sensitivity to shorter wavelengths while reducing background. We aim to optimize the design of such pixels, integrating them in an actual 7-pixel cluster which will be inserted into a MAGIC camera and tested during real observations.

 Publications

year authors and title journal last update
List of publications.
2016 J.E. Ward, J. Cortina, D. Guberman
Light-Trap: a SiPM upgrade for VHE astronomy and beyond
published pages: C11007-C11007, ISSN: 1748-0221, DOI: 10.1088/1748-0221/11/11/C11007
Journal of Instrumentation 11/11 2019-07-24

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "LIGHT-TRAP" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

The information about "LIGHT-TRAP" are provided by the European Opendata Portal: CORDIS opendata.

More projects from the same programme (H2020-EU.1.3.2.)

NSTree (2020)

Understanding substrate delivery for cell wall biosynthesis in plants

Read More  

ReproMech (2019)

The Molecular Mechanisms of Cell Fate Reprogramming in Vertebrate Eggs

Read More  

UQ4ORC (2020)

Uncertainty Quantification And Design Tools For Robust Organic Rankine Cycles

Read More