Forward fitting STIX visibilities | Astronomy & Astrophysics (A&A)

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Table 5.

Reduced χ² values associated with the reconstructions provided by VIS_FWDFIT and VIS_FWDFIT_PSO and shown in Figs. 4 and 5.

Configuration	Method	χ²
C1	VIS_FWDFIT	11.3	7.0
	VIS_FWDFIT_PSO	1.2	1.2
C2	VIS_FWDFIT	32.2	17.1
	VIS_FWDFIT_PSO	1.1	1.1
C3	VIS_FWDFIT	11.3	1.2
	VIS_FWDFIT_PSO	1.2	1.2
C4	VIS_FWDFIT	3.2	3.1
	VIS_FWDFIT_PSO	3.2	3.1
C5	VIS_FWDFIT	1.2	1.8
	VIS_FWDFIT_PSO	1.2	1.2
C6	VIS_FWDFIT	1.5	1.5
	VIS_FWDFIT_PSO	1.5	1.5

Notes. First column: considered configurations (C1–C6); second column: adopted reconstruction method; third column: reduced χ² values associated with the reconstructions of the second and fourth rows (left) and of the third and fifth rows (right) of Figs. 4 and 5.

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