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HiRISE SIGNED

High-Resolution Imaging and Spectroscopy of Exoplanets

Total Cost €

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EC-Contrib. €

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Partnership

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 HiRISE project word cloud

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

crires    optical    axes    oxygen    detection    atmospheres    interconnected    relay    near    structure    comprehension    internal    imagers    doppler    generation    exoplanets    instruments    observe    absolutely    lt    young    breakthrough    carbon    testbed    pick    resolution    block    instrumental    imager    1000    ambitions    composition    flagship    telescope    eso    questions    imaged    markers    time    resolutions    answering    variability    astrophysical    components    evolution    exoplanet    data    temporal    planets    injection    mechanism    characterization    spectral    demonstrator    extraction    explore    module    transverse    astrophysics    validation    photosphere    instrumentation    giant    imaging    signal    spectrograph    sphere    accurate    abundances    dynamical    fundamental    resolved    laboratory    feed    atmospheric    spectroscopy    obtain    designed    contrast    provides    clouds    installed    fiber    modeling    companions    simulations    map    light    infrared    combine    combination   

Project "HiRISE" 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 1˙496˙730 €
 EC max contribution 1˙496˙730 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2017-STG
 Funding Scheme ERC-STG
 Starting year 2017
 Duration (year-month-day) from 2017-12-01   to  2022-11-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS FR (PARIS) coordinator 1˙496˙730.00

Map

 Project objective

Atmospheric composition provides essential markers of the most fundamental properties of exoplanets, such as their formation mechanism or internal structure. New-generation exoplanet imagers have been designed to achieve high contrast for the detection of young giant planets in the near-infrared, but they only provide very low spectral resolutions (R<100) for their characterization. For a major breakthrough in the comprehension of young exoplanets and their atmospheres, an increase of a factor 100 to 1000 in spectral resolution is absolutely required.

This proposal ambitions to develop a novel demonstrator that will combine the capabilities of two flagship instruments installed on the ESO Very Large Telescope, the high-contrast exoplanet imager SPHERE and the high-resolution spectrograph CRIRES, with the goal of answering fundamental questions on the formation, composition and evolution of young planets.

The work will be organized along two axes interconnected with transverse activities: (i) the astrophysics block will investigate signal extraction from high-resolution data and atmospheric modeling, and (ii) the instrumentation block will develop a demonstrator designed to pick up the near-infrared light in SPHERE and feed CRIRES via a dedicated injection module and optical fiber relay. We will explore all the key aspects of the project using a combination of instrumental and astrophysical simulations, as well as laboratory validation of components and methods on our high-contrast imaging testbed.

We will use the demonstrator to observe a sample of directly imaged companions and obtain high-resolution spectroscopy of their atmospheres. From the data we will (1) determine their formation mechanism through an accurate determination of the carbon and oxygen abundances in their atmospheres, and (2) map the temporal variability of their photosphere through time-resolved Doppler imaging to study dynamical processes related to the formation and evolution of clouds.

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

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