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GALSIZE SIGNED

Galaxy Sizes as Tracers of Dark Matter

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 GALSIZE project word cloud

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

forefront    supervised    experimental    resolved    outgoing    hosts    structural    s01    world    provides    model    sizes    spain    acquired    group    paradigm    dagal    relations    canada    s03    ir    telescopes    esr    complete    astrof    de    assembling    simulations    return    spectroscopic    theory    iac    led    s02    astrophysics    definitive    iacute    physics    models    complement    catalogue    former    goals    tackled    incoming    capitalize    photometric    class    tenerife    kingston    country    components    nature    tracers    beneficiary    comparisons    prof    supercomputers    gf    empirical    data    queen    detections    experts    observational    laureate    wp3    aid    optical    cold    courteau    uncharted    galaxies    mass    instituto    near    experiences    galaxy    realm    numerical    university    mcdonald    knapen    galsize    msca    dynamical    host    inferences    coupling    training    expand    observatory    nobel    itn    wp2    sica    disk    astroparticle    unprecedentedly    characterization    2015    dark    scientific    luminous    canarias    efforts    scaling   

Project "GALSIZE" data sheet

The following table provides information about the project.

Coordinator
INSTITUTO DE ASTROFISICA DE CANARIAS 

Organization address
address: CALLE VIA LACTEA
city: SAN CRISTOBAL DE LA LAGUNA
postcode: 38205
website: www.iac.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]
 Total cost 250˙497 €
 EC max contribution 250˙497 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2019
 Funding Scheme MSCA-IF-GF
 Starting year 2020
 Duration (year-month-day) from 2020-09-01   to  2023-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    INSTITUTO DE ASTROFISICA DE CANARIAS ES (SAN CRISTOBAL DE LA LAGUNA) coordinator 250˙497.00
2    Queen's University at Kingston CA (Kingston) partner 0.00

Map

 Project objective

I propose the project Galaxy Sizes as Tracers of Dark Matter (GALSIZE) to be supervised by Prof. Courteau at Queen’s University in Kingston (Canada, Third Country for the outgoing phase) and by Prof. Knapen at the Instituto de Astrofísica de Canarias (IAC, Tenerife, Spain, beneficiary institution and host for the incoming phase). The main scientific goals are to (S01) establish a new paradigm of galaxy data-model comparisons, developing a definitive theory of disk formation based on galaxy sizes; (S02) characterize the nature of, and coupling between, dark and luminous matter in galaxies, with the aid of scaling relations, mass tracers, and numerical simulations; and (S03) expand model inferences into the uncharted realm of low-mass galaxies. These objectives will be tackled by assembling the largest and most complete catalogue of spatially resolved structural and dynamical properties (WP2) of galaxies to characterize in a novel way their luminous and dark components (WP3). Queen's University is a world-leading institution for the study of dark matter. The Queen’s Astrophysics Group includes many experts in the observational and numerical characterization of luminous and dark matter in galaxies. The Queen’s Astroparticle group, led by 2015 Physics Nobel Laureate Prof. Art McDonald, is also at the forefront of experimental cold dark matter detections. The return phase institution, the IAC, hosts world experts in both the empirical analysis and numerical modelling of galaxies. It provides access to supercomputers and world-class telescopes (best optical/near-IR observatory in Europe). Through this MSCA-IF-GF, my training in Canada would capitalize upon my past experiences (former MSCA ESR in DAGAL ITN) by coupling photometric and spectroscopic properties of unprecedentedly large sets of galaxies and simulations to constrain in a novel way models of galaxy formation. Dissemination of the knowledge acquired in Canada would greatly complement related European efforts.

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

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