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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.

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

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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