All good things come in threes: the third image of the lensed quasar PKS 1830−211

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Table B.2.

Parameters of the Sérsic intensity profiles used for the ALMA and VLA source models (Figs. 3a and b, respectively).

		(X,Y) ^(a)	r₀^(b)	I₀^(c)	n^(d)
		(mas)	(mas)
ALMA model	S₁	( − 386, −325)	1	1	1
	S₂	( − 333, −341)	1	0.005	1
VLA model	S₁	( − 386, −325)	1	1	1
		( − 333, −341)	55	0.5	1

Notes.

^(a)

Positions are given with respect to image A;

^(b)

half-light radius;

^(c)

intensity;

^(d)

Sérsic index.

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