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EWC SIGNED

Enabling Weak lensing Cosmology

Total Cost €

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EC-Contrib. €

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Partnership

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 EWC project word cloud

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

narrow    intervening    calibrate    select    fundamental    telescope    distant    scheduled    our    photometric    compromised    quality    observations    survey    technique    spectroscopic    resolution    euclid    experiments    progress    launch    ing    standard    tidal    morphology    pipeline    corrected    light    origin    systematics    motivated    instrumental    space    challenged    obtain    lensing    vision    science    gravitational    magnitude    simulation    phenomenon    interactions    esa    perform    cosmological    alignments    astrophysical    universe    galaxies    fronts    cosmology    model    archival    return    mission    constituents    rays    intrinsic    deflection    quantity    structures    contaminate    otherwise    designed    precision    differential    matched    data    integrate    continues    imaging    improvement    signal    describes    hubble    unable    cosmic    billion    quantify    minimize    energy    accurately    carry    hst    maximise    tremendous    2020    precise    physics    constraints    redshift    dark    critical    band    arise    observational   

Project "EWC" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITY COLLEGE LONDON 

Organization address
address: GOWER STREET
city: LONDON
postcode: WC1E 6BT
website: n.a.

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 United Kingdom [UK]
 Project website https://weaklensing-cosmology.org/
 Total cost 1˙587˙154 €
 EC max contribution 1˙587˙153 € (100%)
 Programme 1. H2020-EU.2.1.6.3. (Enabling exploitation of space data)
 Code Call H2020-COMPET-2017
 Funding Scheme RIA
 Starting year 2018
 Duration (year-month-day) from 2018-04-01   to  2022-03-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITY COLLEGE LONDON UK (LONDON) coordinator 234˙090.00
2    AGENCIA ESTATAL CONSEJO SUPERIOR DEINVESTIGACIONES CIENTIFICAS ES (MADRID) participant 267˙742.00
3    CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS FR (PARIS) participant 190˙490.00
4    UNIVERSITY OF DURHAM UK (DURHAM) participant 180˙885.00
5    CENTRO DE INVESTIGACIONES ENERGETICAS, MEDIOAMBIENTALES Y TECNOLOGICAS-CIEMAT ES (MADRID) participant 163˙167.00
6    INSTITUTO DE FISICA DE ALTAS ENERGIAS ES (CERDANYOLA DEL VALLES) participant 163˙167.00
7    ISTITUTO NAZIONALE DI ASTROFISICA IT (ROMA) participant 145˙875.00
8    RHEINISCHE FRIEDRICH-WILHELMS-UNIVERSITAT BONN DE (BONN) participant 134˙706.00
9    MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV DE (MUENCHEN) participant 49˙061.00
10    FCIENCIAS.ID - ASSOCIACAO PARA A INVESTIGACAO E DESENVOLVIMENTO DE CIENCIAS PT (LISBON) participant 29˙218.00
11    UNIVERSITEIT LEIDEN NL (LEIDEN) participant 28˙750.00

Map

 Project objective

Our understanding of cosmology and fundamental physics continues to be challenged by ever more precise experiments. The resulting “standard” model of cosmology describes the data well, but is unable to explain the origin of the main constituents of our Universe, namely dark matter and dark energy. More than an order of magnitude improvement in the quality and quantity of observational data is needed. This has motivated ESA to select Euclid as the second mission of its cosmic vision program, with a scheduled launch in 2020. It is designed to accurately measure the alignments of distant galaxies due to the differential deflection of light-rays by intervening structures, a phenomenon called gravitational lensing. Euclid will measure this signal by imaging 1.5 billion galaxies with a resolution similar to that of the Hubble Space Telescope. Although Euclid is designed to minimize observational systematics the observations are still compromised by two factors. Various instrumental effects need to be corrected for, and the tremendous improvement in precision has to be matched with comparable advances in the modelling of astrophysical effects that affect the signal. The objective of this proposal is to make significant progress on both fronts. To do so, we will (i) quantify the morphology of galaxies using archival HST observations; (ii) carry out a unique narrow-band photometric redshift survey to obtain state-of-the-art constraints on the intrinsic alignments of galaxies that arise due to tidal interactions, and would otherwise contaminate the cosmological signal; (iii) integrate these results into the end-to-end simulation pipeline; (iv) perform a spectroscopic redshift survey to calibrate the photometric redshift technique. The Euclid Consortium has identified these as critical issues, which need to be addressed before launch, in order to maximise the science return of this exciting mission, and enable the dark energy science objectives of Europe.

 Deliverables

List of deliverables.
Data Management Plan Open Research Data Pilot 2019-07-23 16:42:50
Data Challenges run and report. Version 1. Other 2019-07-23 16:14:38
Creation and management of the consortium committees, set up of impact mechanisms Other 2019-07-23 16:42:47
Data Challenges run and report. Version 2 Other 2019-07-23 17:31:41
Mock catalogues with PAUCam filter set Other 2019-07-23 16:42:46
Advisory Report 1 Documents, reports 2019-07-23 16:42:47
Distribution of data acquired for the survey. Version 1. Other 2019-07-23 16:42:47
Quality Management Plan Documents, reports 2019-07-23 16:42:47
Catalogue Production Other 2019-07-23 16:42:49

Take a look to the deliverables list in detail:  detailed list of EWC deliverables.

 Publications

year authors and title journal last update
List of publications.
2018 L Cabayol, I Sevilla-Noarbe, E Fernández, J Carretero, M Eriksen, S Serrano, A Alarcón, A Amara, R Casas, F J Castander, J de Vicente, M Folger, J García-Bellido, E Gaztanaga, H Hoekstra, R Miquel, C Padilla, E Sánchez, L Stothert, P Tallada, L Tortorelli
The PAU survey: star–galaxy classification with multi narrow-band data
published pages: 529-539, ISSN: 0035-8711, DOI: 10.1093/mnras/sty3129
Monthly Notices of the Royal Astronomical Society 483/1 2019-08-05
2019 N. Tonello, P. Tallada, S. Serrano, J. Carretero, M. Eriksen, M. Folger, C. Neissner, I. Sevilla-Noarbe, F.J. Castander, M. Delfino, J. De Vicente, E. Fernandez, J. Garcia-Bellido, E. Gaztanaga, C. Padilla, E. Sanchez, L. Tortorelli
The PAU Survey: Operation and orchestration of multi-band survey data
published pages: 171-188, ISSN: 2213-1337, DOI: 10.1016/j.ascom.2019.04.002
Astronomy and Computing 27 2019-08-05
2019 M Eriksen, A Alarcon, E Gaztanaga, A Amara, L Cabayol, J Carretero, F J Castander, M Crocce, M Delfino, J De Vicente, E Fernandez, P Fosalba, J Garcia-Bellido, H Hildebrandt, H Hoekstra, B Joachimi, P Norberg, R Miquel, C Padilla, A Refregier, E Sanchez, S Serrano, I Sevilla-Noarbe, P Tallada, N Tonello, L Tortorelli
The PAU Survey: early demonstration of photometric redshift performance in the COSMOS field
published pages: 4200-4215, ISSN: 0035-8711, DOI: 10.1093/mnras/stz204
Monthly Notices of the Royal Astronomical Society 484/3 2019-08-05
2019 Thomas D. Kitching, Peter L. Taylor, Peter Capak, Daniel Masters, Henk Hoekstra
Rainbow cosmic shear: Optimization of tomographic bins
published pages: 63536, ISSN: 2470-0010, DOI: 10.1103/physrevd.99.063536
Physical Review D 99/6 2019-08-05
2018 L Stothert, P Norberg, C M Baugh, A Alarcon, A Amara, J Carretero, F J Castander, M Eriksen, E Fernandez, P Fosalba, J Garcia-Bellido, E Gaztanaga, H Hoekstra, C Padilla, A Refregier, E Sanchez, L Tortorelli
The PAU Survey: spectral features and galaxy clustering using simulated narrow-band photometry
published pages: 4221-4235, ISSN: 0035-8711, DOI: 10.1093/mnras/sty2491
Monthly Notices of the Royal Astronomical Society 481/3 2019-08-05
2018 Luca Tortorelli, Lorenza Della Bruna, Jörg Herbel, Adam Amara, Alexandre Refregier, Alex Alarcon, Jorge Carretero, Francisco J. Castander, Juan De Vicente, Martin Eriksen, Enrique Fernandez, Martin Folger, Juan García-Bellido, Enrique Gaztanaga, Ramon Miquel, Cristobal Padilla, Eusebio Sanchez, Santiago Serrano, Lee Stothert, Pau Tallada, Nadia Tonello
The PAU Survey: a forward modeling approach for narrow-band imaging
published pages: 035-035, ISSN: 1475-7516, DOI: 10.1088/1475-7516/2018/11/035
Journal of Cosmology and Astroparticle Physics 2018/11 2019-08-05

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