JWST spectroscopic confirmation of the Cosmic Gems arc at z = 9.625 - Insights into the small-scale structure of a post-burst system

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Volume 705 (January 2026)

A&A, 705 (2026) A173

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Table B.1.

Star cluster magnifications in different lens models.

ID	`glafic`	`Lenstool`	Ratio
A.1	$47 . 9_{- 4.0}^{+ 4.0}$ $47.9^{+4.0}_{-4.0}$	$67 . 7_{- 0.3}^{+ 9.1}$ $67.7^{+9.1}_{-0.3}$	$1 . 4_{- 0.1}^{+ 0.2}$ $1.4^{+0.2}_{-0.1}$
B.1	$92 . 3_{- 10.6}^{+ 11.7}$ $92.3^{+11.7}_{-10.6}$	$125 . 4_{- 3.2}^{+ 23.2}$ $125.4^{+23.2}_{-3.2}$	$1 . 4_{- 0.2}^{+ 0.3}$ $1.4^{+0.3}_{-0.2}$
C.1	$124 . 5_{- 16.8}^{+ 19.7}$ $124.5^{+19.7}_{-16.8}$	$160 . 6_{- 6.7}^{+ 35.1}$ $160.6^{+35.1}_{-6.7}$	$1 . 3_{- 0.2}^{+ 0.3}$ $1.3^{+0.3}_{-0.2}$
D.1	$166 . 6_{- 26.5}^{+ 31.7}$ $166.6^{+31.7}_{-26.5}$	$216 . 3_{- 13.4}^{+ 61.8}$ $216.3^{+61.8}_{-13.4}$	$1 . 3_{- 0.3}^{+ 0.4}$ $1.3^{+0.4}_{-0.3}$
E.1	$323 . 5_{- 82.4}^{+ 125.5}$ $323.5^{+125.5}_{-82.4}$	$369 . 8_{- 48.9}^{+ 198.9}$ $369.8^{+198.9}_{-48.9}$	$1 . 1_{- 0.5}^{+ 0.7}$ $1.1^{+0.7}_{-0.5}$
v A.2	$52 . 2_{- 3.2}^{+ 4.4}$ $52.2^{+4.4}_{-3.2}$	$74 . 1_{- 3.1}^{+ 8.0}$ $74.1^{+8.0}_{-3.1}$	$1 . 4_{- 0.1}^{+ 0.2}$ $1.4^{+0.2}_{-0.1}$
B.2	$90 . 3_{- 7.4}^{+ 7.3}$ $90.3^{+7.3}_{-7.4}$	$131 . 6_{- 10.2}^{+ 18.3}$ $131.6^{+18.3}_{-10.2}$	$1 . 5_{- 0.2}^{+ 0.2}$ $1.5^{+0.2}_{-0.2}$
C.2+D.2	$132 . 5_{- 14.4}^{+ 16.7}$ $132.5^{+16.7}_{-14.4}$	$200 . 6_{- 22.8}^{+ 40.6}$ $200.6^{+40.6}_{-22.8}$	$1 . 5_{- 0.3}^{+ 0.3}$ $1.5^{+0.3}_{-0.3}$

Notes. Shown is a comparison between the magnification values obtained for the five main clusters in the case of the two lens models studied (glafic and LENSTOOL). Their ratios, reported in the last column, represent the scaling factor used to convert the intrinsic masses, derived assuming one of the models, to the ones obtained by the other.

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