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ASTROSTAT-II SIGNED

Development of Novel Statistical Tools for the Analysis of Astronomical Data

Total Cost €

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EC-Contrib. €

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Partnership

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Project "ASTROSTAT-II" data sheet

The following table provides information about the project.

Coordinator
IDRYMA TECHNOLOGIAS KAI EREVNAS 

Organization address
address: N PLASTIRA STR 100
city: IRAKLEIO
postcode: 70013
website: www.forth.gr

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 Greece [EL]
 Total cost 690˙000 €
 EC max contribution 556˙600 € (81%)
 Programme 1. H2020-EU.1.3.3. (Stimulating innovation by means of cross-fertilisation of knowledge)
 Code Call H2020-MSCA-RISE-2019
 Funding Scheme MSCA-RISE
 Starting year 2020
 Duration (year-month-day) from 2020-03-01   to  2024-02-29

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    IDRYMA TECHNOLOGIAS KAI EREVNAS EL (IRAKLEIO) coordinator 220˙800.00
2    UNIVERSITE DE GENEVE CH (GENEVE) participant 138˙000.00
3    IMPERIAL COLLEGE OF SCIENCE TECHNOLOGY AND MEDICINE UK (LONDON) participant 115˙000.00
4    THE CHANCELLOR MASTERS AND SCHOLARSOF THE UNIVERSITY OF CAMBRIDGE UK (CAMBRIDGE) participant 82˙800.00
5    CALIFORNIA INSTITUTE OF TECHNOLOGYCORP US (PASADENA) partner 0.00
6    NORTHWESTERN UNIVERSITY US (EVANSTON, ILLINOIS) partner 0.00
7    Simon Fraser University CA (BURNABY) partner 0.00
8    SMITHSONIAN INSTITUTION US (WASHINGTON DC) partner 0.00

Map

 Project objective

We propose an interdisciplinary collaboration network involving leading groups in Astrophysics (Astrophysics Group in Crete, Geneva Observatory, University of Cambridge, Smithsonian Astrophysical Observatory, Caltech, and Nortwestern University), and Statistics (Imperial College, University of Cambridge, Simon Fraser University). The goal of this project is to share expertise between the different fields and geographical areas in order to tackle key questions in observational Astrophysics, related to the nature of dark energy and dark matter, the populations of accreting binary stars in galaxies and their evolution, the morphological and activity classification of galaxies, and the identification and characterization of fast evolving, or transient, sources. To address each of these questions we will use state-of-the-art observations and theoretical models, and we will develop novel, principled tools for statistical analysis in the domains of source classification, structure detection, and fitting. The methods developed under this program will have lasting value and applications beyond the field of Astrophysics.

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

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