Table 2.
Results of the experiments performed in Sect. 3.4.
Cusp_l | Cusp_s | Fold | Cross | ||||||
---|---|---|---|---|---|---|---|---|---|
χ2 | 1.00 | 1.02 | 1.02 | 1.04 | |||||
IN: composite, no multipole | H0 |
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MOD: free slope | Slope | 1.94 | 1.96 | 1.97 | 1.96 | ||||
Boxy | Discy | Boxy | Discy | Boxy | Discy | Boxy | Discy | ||
IN: composite, MOD: fixed slope | χ2 | 1.46 | 1.24 | 1.61 | 1.43 | 1.45 | 1.28 | 1.42 | 1.29 |
H0 |
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IN: composite, MOD: free slope | χ2 | 1.44 | 1.18 | 1.52 | 1.35 | 1.43 | 1.25 | 1.38 | 1.22 |
H0 |
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Notes. The mock systems follow the base case with γext = 0.05, q = 0.8, 5400 s exposure time, and a very bright source (⟨mQSO⟩ = 18.5 mag), but differ by the main lens mass profile which is a composite mass profile made of a baryonic component and a dark matter component, instead of being a SIE. The case represented in the first row is multipole free while the two bottom rows display a multipole a4 = 0.01, either in discy or boxy orientation. The mock images are fitted with a power-law model (hence the bold characters to differentiate it from the base SIE modelling, following the conventions of Table 1) with either a free slope or a fixed slope. In the latter case, the fixed value is the value retrieved in the no multipole case for each configuration.
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