The CFHTLS Strong Lensing Legacy Survey: I. Survey overview and T0002 release sample

TL;DR

This paper introduces the CFHTLS Strong Lensing Legacy Survey, presenting an automated method to identify strong gravitational lenses, and reports a preliminary sample of 40 candidates spanning galaxy to cluster mass scales, demonstrating the survey's potential.

Contribution

It develops automated procedures for detecting strong lenses in CFHTLS images and provides the first large sample of lenses including galaxy groups, expanding the scope of gravitational lens studies.

Findings

Discovered ~40 strong lensing candidates in 28 deg² of CFHTLS data.

Demonstrated the feasibility of uncovering galaxy group-scale lenses.

Established a foundation for future large-scale lens surveys.

Abstract

AIMS: We present data from the CFHTLS Strong Lensing Legacy Survey (SL2S). Due to the unsurpassed combined depth, area and image quality of the Canada-France-Hawaii Legacy Survey it is becoming possible to uncover a large, statistically well-defined sample of strong gravitational lenses which spans the dark halo mass spectrum predicted by the concordance model from galaxy to cluster haloes. METHODS: We describe the development of several automated procedures to find strong lenses of various mass regimes in CFHTLS images. RESULTS: The preliminary sample of about 40 strong lensing candidates discovered in the CFHTLS T0002 release, covering an effective field of view of 28 deg$^2$ is presented. These strong lensing systems were discovered using an automated search and consist mainly of gravitational arc systems with splitting angles between 2 and 15 arcsec. This sample shows for the first time that it is possible to uncover a large population of strong lenses from galaxy groups with typical halo masses of about $10^{13}h^{-1}M_\odot$. We discuss the future evolution of the SL2S project and its main scientific aims for the next 3 years, in particular our observational strategy to extract the hundreds of gravitational rings also present in these fields.