Hola,
¿eres nuevo aquí?

Regístrate gratis y conecta tu empresa con financiación pública, partners y proyectos.

Tengo cuenta

Regístrate

Ver video

GLIMPSE

Financiado

Cerrado

GLIMPSE Understanding the dark universe through 3D weak lensing reconstructions

Weak gravitational lensing has emerged as a powerful tool to probe the distribution and nature of the dark components of our Universe, and thus to better constrain our cosmological model. For this reason, several large projects su... ver más

28/02/2017

UNIVERSITY COLLEGE...

222K€

Presupuesto del proyecto: 222K€

Líder del proyecto

UNIVERSITY COLLEGE LONDON No se ha especificado una descripción o un objeto social para esta compañía.

Fecha límite participación Sin fecha límite de participación.

Ver 2 Participantes

Financiación concedida El organismo FP7 notifico la concesión del proyecto el día 2017-02-28 No tenemos la información de la convocatoria

0% 100% 100%

Información adicional privada

No hay información privada compartida para este proyecto. Habla con el coordinador.

2 Participantes

UNIVERSITY COLLEGE LONDON

221.61K€ | Lider

UNIVERSITY COLLEGE LONDON

Proyectos interesantes

ADULT

Applied Physics

Data Science

1M€ Cerrado

CODE

Applied Physics

Data Science

100K€ Cerrado

HALOS2020

Applied Physics

Data Science

166K€ Cerrado

WEBMAP

Applied Physics

Data Science

222K€ Cerrado

COSMIC LENS

Applied Physics

Data Science

2M€ Cerrado

Halo modelling

Applied Physics

Data Science

243K€ Cerrado

Conecta tu I+D

¿Tienes un proyecto y buscas un partner? Gracias a nuestro motor inteligente podemos recomendarte los mejores socios y ponerte en contacto con ellos. Te lo explicamos en este video

Líder del proyecto

UNIVERSITY COLLEGE LONDON No se ha especificado una descripción o un objeto social para esta compañía.

Presupuesto del proyecto 222K€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto Weak gravitational lensing has emerged as a powerful tool to probe the distribution and nature of the dark components of our Universe, and thus to better constrain our cosmological model. For this reason, several large projects such as the Dark Energy Survey and Euclid have been commissioned to study this effect. Arising from the deflection of light due to the gravitational potential of structures in the Universe, it manifests as a small, correlated elliptical distortion -- a shear -- in galaxy images. Lensing is sensitive only to the presence of matter, and not to the nature of that matter (luminous, dark, baryonic, etc.), and thus provides an ideal and unbiased probe of the structure of the cosmic web. This proposal will address the problem of mapping the dark matter distribution in three dimensions using measurements of weak gravitational lensing. This is a very complex, ill-posed problem with numerous sources of noise and signal contamination. A focus of my postdoctoral work has been in developing a multidisciplinary approach to this problem, marking a dramatic shift from earlier methods. My new algorithm -- GLIMPSE -- demonstrates an impressive improvement in the fidelity of the maps generated, thereby for the first time opening up allowing 3D mapping techniques to directly constrain the cosmological model. With this in mind, the specific aims of this proposal are to further develop the GLIMPSE algorithm to ready the software for application to survey data, and to more fully develop the applicable theory and statistical tools to allow the outputs of GLIMPSE to be used to directly constrain our cosmological model. This development will establish GLIMPSE at the forefront of the field, and will significantly further the goals of large targeted weak lensing surveys. This is essential to a better understanding of the nature and behaviour of the dark components of the Universe.

Conecta tu I+D

Entra hoy

¿Olvidé mi contraseña?

Financiación

Empresas

CTIs/Universidades

Proyectos

Investigadores