2024MNRAS.531.1823A


Query : 2024MNRAS.531.1823A

2024MNRAS.531.1823A - Mon. Not. R. Astron. Soc., 531, 1823-1840 (2024/June-2)

A general method to reconstruct strong gravitational lenses based on the singular perturbative approach.

ALARD C.

Abstract (from CDS):

The number of gravitational arcs systems detected is increasing quickly and should even increase at a faster rate in the near future. This wealth of new gravitational arcs requires the development of a purely automated method to reconstruct the lens and source. A general reconstruction method based on the singular perturbative approach is proposed in this paper. This method generates a lens and source reconstruction directly from the gravitational arc image. The method is fully automated and works in two steps. The first step is to generate a guess solution based on the circular solution in the singular perturbative approach. The second step is to break the sign degeneracy and to refine the solution by using a general source model. The refinement of the solution is conducted step-by-step to avoid the source-lens degeneracy issue. One important asset of this automated method is that the lens solution is written in universal terms which allows the computation of statistics. Considering the large number of lenses which should be available in the near future this ability to compute unbiased statistics is an important asset.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): gravitational lensing: strong - dark matter

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 CSWA 1 gLS 11 48 33.10 +19 30 03.2           ~ 90 0

Query : 2024MNRAS.531.1823A

Basic data :
CSWA 1 -- Gravitational Lens System (lens+images)
Other object types:
otypes_help
G ([DAA2009]), gLS (CSWA)
ICRS coord. (ep=J2000) :
11 48 33.10 +19 30 03.2 (Optical) [ ] D 2009MNRAS.392..104B
FK4 coord. (ep=B1950 eq=1950) :
11 45 58.02 +19 46 43.8 [ ]
Gal coord. (ep=J2000) :
237.47808 +73.69230 [ ]
Fluxes (2) :
g 20.8 [~] D 2009MNRAS.392..104B
i 18.2 [~] D 2009MNRAS.392..104B
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Identifiers (3) :
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CSWA 1 NAME Cosmic Horseshoe [DAA2009] SDSS J114833.14+193003.2

References (90 between 1850 and 2026) (Total 90)
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