eprintid: 1520027
rev_number: 23
eprint_status: archive
userid: 608
dir: disk0/01/52/00/27
datestamp: 2016-10-08 20:26:44
lastmod: 2020-02-12 20:46:40
status_changed: 2017-06-01 10:23:48
type: proceedings_section
metadata_visibility: show
creators_name: Rivi, M
creators_name: Miller, L
creators_name: Makhathini, S
creators_name: Abdalla, FB
title: RadioLensfit: Bayesian weak lensing measurement in the visibility domain
ispublished: pub
divisions: UCL
divisions: A01
divisions: B04
divisions: C06
divisions: F60
note: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
abstract: Observationally, weak lensing has been served so far by optical surveys due to the much larger number densities of background galaxies achieved, which is typically by two to three orders of magnitude larger compared to radio. However, the high sensitivity of the new generation of radio telescopes such as the Square Kilometre Array†(SKA) will provide a density of detected galaxies that is comparable to that found at optical wavelengths, and with significant source shape measurements to make large area radio surveys competitive for weak lensing studies. This will lead weak lensing to become one of the primary science drivers in radio surveys too, with the advantage that they will access the largest scales in the Universe going beyond optical surveys, like LSST‡and Euclid§, in terms of redshifts that are probed. RadioLensfit is an adaptation to radio data of lensfit, a model-fitting approach for galaxy shear measurement, originally developed for optical weak lensing surveys. Its key advantage is working directly in the visibility domain, which is the natural approach to adopt with radio data, avoiding systematics due to the imaging process. We present results on galaxy shear measurements, including investigation of sensitivity to instrumental parameters such as the visibilities gridding size, based on simulations of individual galaxy visibilities performed by using SKA1-MID baseline configuration. We get an amplitude of the shear bias in the method comparable with SKA1 requirements for a population of galaxies with realistic flux and scalelength distributions estimated from the VLA SWIRE catalog.
date: 2015-10-23
date_type: published
publisher: Proceedings of Science (PoS)
official_url: https://pos.sissa.it/archive/conferences/267/033/EXTRA-RADSUR2015_033.pdf
oa_status: gold
full_text_type: pub
primo: open
verified: verified_manual
elements_id: 1113500
lyricists_name: Abdalla, Filipe
lyricists_name: Rivi, Marzia
lyricists_id: FBABD21
lyricists_id: MRIVI22
full_text_status: public
series: EXTRA-RADSUR
publication: Proceedings of Science
place_of_pub: Bologna, Italy
event_title: EXTRA-RADSUR2015
issn: 1824-8039
book_title: Proceedings of EXTRA-RADSUR2015 - The many facets of extragalactic radio surveys: towards new scientific challenges
editors_name: Prandoni, I
editors_name: Morganti, R
editors_name: Best, P
editors_name: Bonafede, A
citation:        Rivi, M;    Miller, L;    Makhathini, S;    Abdalla, FB;      (2015)    RadioLensfit: Bayesian weak lensing measurement in the visibility domain.                     In: Prandoni, I and Morganti, R and Best, P and Bonafede, A, (eds.) Proceedings of EXTRA-RADSUR2015 - The many facets of extragalactic radio surveys: towards new scientific challenges.    Proceedings of Science (PoS): Bologna, Italy.       Gold open access   
 
document_url: https://discovery.ucl.ac.uk/id/eprint/1520027/1/Rivi_RadioLensfit.pdf