The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) - II. The radial structure of debris discs

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Table C.4

Stellar fluxes for HD 197481.

Date	ARKS Fitting		Disc + Ring		Fiducial
	Best Fit	Median	Best Fit	Median	Best Fit	Median
March 26, 2014	327	$343_{- 19}^{+ 18}$ $343_{-19}^{+18}$	370	$390_{20}^{+ 20}$ $390_{20}^{+20}$	400	$390_{- 20}^{+ 20}$ $390_{-20}^{+20}$
August 18, 2014	130	$140_{- 20}^{+ 30}$ $140_{-20}^{+30}$	140	$150_{- 30}^{+ 20}$ $150_{-30}^{+20}$	170	$160_{- 30}^{+ 20}$ $160_{-30}^{+20}$
June 24, 2015	196	$205_{- 18}^{+ 18}$ $205_{-18}^{+18}$	210	$220_{- 20}^{+ 20}$ $220_{-20}^{+20}$	240	$240_{- 20}^{+ 20}$ $240_{-20}^{+20}$

Notes. ARKS fitting results are from the best parametric model for HD 197481, a triple power law with one gap. Disc + ring and fiducial model results are from Daley et al. (2019). All fluxes are in units of μJy.

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