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SPIAKID SIGNED

SpectroPhotometric Imaging in Astronomy with Kinetic Inductance Detectors

Total Cost €

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EC-Contrib. €

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Partnership

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 SPIAKID project word cloud

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

science    camera    imaging    kids    sources    emission    evolution    faint    provides    imagers    red    instead    image    zero    reconstruction    few    seeing    equip    innovative    45    community    position    kinetic    diffraction    deeper    unnecessary    internal    detectors    precise    throughput    first    technological    exposures    faintness    exoplanets    galaxy    instruments    ms    mu    exposure    electromagnetic    combined    feedback    resolution    ages    spectrophotometry    single    tackle    monitoring    15    ultra    fluorescence    reconstructed    kid    galaxies    shaping    impossible    images    acquiring    microscopy    efficiency    atmospheric    simplified    environment    band    read    uses    visible    derive    unprecedented    spectral    gravitational    coherence    integration    transiting    signal    fast    astronomy    optical    telescope    paths    turbulence    inductance    full    infra    ufds    delta    spiakid    time    instrument    lambda    wave    faster    local    atmospheres    techniques    place    limited    scientists    ratio    noise    stellar    group    class    dwarf    stars    sharper    obtain    difficult    metallicities    filtering    spectrum    understand   

Project "SPIAKID" data sheet

The following table provides information about the project.

Coordinator
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS 

Organization address
address: RUE MICHEL ANGE 3
city: PARIS
postcode: 75794
website: www.cnrs.fr

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 France [FR]
 Total cost 3˙109˙215 €
 EC max contribution 3˙109˙215 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-ADG
 Funding Scheme ERC-ADG
 Starting year 2020
 Duration (year-month-day) from 2020-01-01   to  2024-12-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS FR (PARIS) coordinator 3˙109˙215.00

Map

 Project objective

The SPIAKID project will build a camera using Kinetic Inductance Detectors (KIDs) to equip an 8 m class telescope to derive ages and metallicities for stars in Ultra Faint Dwarf galaxies (UFDs) in the Local Group. UFDs are the key to understand early galaxy formation processes, including the properties of the first stars, and the role of environment and internal feedback in shaping the evolution of dwarf galaxies. A full exploitation of UFDs to understand these processes requires knowledge of their precise stellar ages and metallicities. This is difficult, in many cases impossible, to obtain with existing instruments because of the faintness of UFDs. SPIAKID will allow unprecedented efficiency in acquiring wide-band spectrophotometry, making this possible. The KID provides a low resolution spectrum (goal: λ/Δλ~15) over a wide spectral range (goal: 0.45 μm to 1.60 μm), a single exposure instead of many single-band exposures. The instrument throughput is increased as the design is simplified since filtering is unnecessary and the visible and infra-red optical paths are combined. The KIDs are read continuously with zero read-out noise so the integration is driven in real time by monitoring the signal-to-noise ratio. Finally, their response is faster (~ 30 μs) than the coherence time of atmospheric turbulence (a few ms) so diffraction-limited resolution is achieved with existing image reconstruction techniques. The reconstructed images will be sharper and deeper than can be achieved by traditional seeing-limited imagers. The SPIAKID instrument will tackle other science cases, e.g. transiting exoplanets and their atmospheres or the electromagnetic emission from gravitational wave sources, and the instrument will be offered to the community to foster other uses. Our technological developments for the KIDs will place European scientists in a position to design and build innovative instruments, in astronomy but also, for example, in fast imaging for fluorescence microscopy.

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The information about "SPIAKID" are provided by the European Opendata Portal: CORDIS opendata.

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lastchecktime (2020-10-29 22:32:57) correctly updated