A multi-frequency, multi-epoch radio continuum study of the Arches cluster with the Very Large Array

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Table 4

Clumping ratios.

ID	${(f_{c l}^{C} / f_{c l}^{X})}_{18}$ $\[\left(f_{\mathrm{cl}}^{C} / f_{\mathrm{cl}}^{X}\right)_{18}\]$	${(f_{c l}^{C} / f_{c l}^{X})}_{22}$ $\[\left(f_{\mathrm{cl}}^{C} / f_{\mathrm{cl}}^{X}\right)_{22}{ }\]$ ^(a)	$(f_{c l}^{C} / f_{c l}^{K})$ $\[\left(f_{\mathrm{cl}}^{C} / f_{\mathrm{cl}}^{K}\right)\]$ ^(b)	$(f_{c l}^{X} / f_{c l}^{K})$ $\[\left(f_{\mathrm{cl}}^{X} / f_{\mathrm{cl}}^{K}\right)\]$ ^(b)
F7	0.9 ± 0.2	0.8 ± 0.1	0.9 ± 0.3	1.2 ± 0.3
F3	1.0 ± 0.1	0.8 ± 0.1	0.6 ± 0.1	0.6 ± 0.2
Dong19	0.9 ± 0.1	0.9 ± 0.1	−	−
F4	0.7 ± 0.1	0.8 ± 0.1	−	−
F5	1.0 ± 0.1	0.8 ± 0.1	0.6 ± 0.2	0.7 ± 0.2
F8	1.1 ± 0.4	0.9 ± 0.4	0.3 ± 0.1	0.4 ± 0.1
Dong96	0.9 ± 0.1	0.9 ± 0.1	−	−
F1	0.7 ± 0.2	0.8 ± 0.2	−	−
F2	1.0 ± 0.2	1.1 ± 0.3	−	−
F9	0.6 ± 0.2	0.7 ± 0.2	−	−
B1	0.8 ± 0.3	0.9 ± 0.4	−	−
F14	−	0.9 ± 0.4	−	−

Notes. ^(a)2022 clumping ratios were computed using the contemporaneous set of C- and X-band data from 4 July. ^(b)We used the fluxes from the deep C- and X-band images to compute clumping ratios with Lang et al. (2005) K-band data.

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