Three hot Jupiters transiting K-dwarfs with significant heavy element masses

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Table F.2

Fitted photometric instrumental parameters for the companions presented in this paper.

		TOI-2969 b	TOI-2989 b	TOI-5300 b
γ_TESS	[×10⁻⁶]	$- 33_{- 27}^{+ 26}$ $-33_{-27}^{+26}$	$- 26_{- 31}^{+ 28}$ $-26_{-31}^{+28}$	−30 ± 39
σ_TESS	[ppm]	${4.5}_{- 4.0}^{+ 33.3}$ $4.5_{-4.0}^{+33.3}$	${3.9}_{- 3.6}^{+ 33.3}$ $3.9_{-3.6}^{+33.3}$	${3.5}_{- 3.1}^{+ 33.1}$ $3.5_{-3.1}^{+33.1}$
γ_QLP	[×10⁻⁶]	$- 135_{- 19}^{+ 20}$ $-135_{-19}^{+20}$
σ_QLP	[ppm]	$81_{- 75}^{+ 167}$ $81_{-75}^{+167}$
γ_R₁	[×10⁻³]	$- 53_{- 8}^{+ 9}$ $-53_{-8}^{+9}$	−11 ± 2
σ_R₁	[ppm]	$849_{- 245}^{+ 110}$ $849_{-245}^{+110}$	$172_{- 171}^{+ 728}$ $172_{-171}^{+728}$
θ₀,R₁	[×10⁻³]	$- 47_{- 7}^{+ 8}$ $-47_{-7}^{+8}$	4 ± 2
γ_R₂	[×10⁻³]	2 ± 1
σ_R₂	[ppm]	$18_{- 16}^{+ 183}$ $18_{-16}^{+183}$
θ₀,R₂	[×10⁻³]	${1.3}_{- 0.7}^{+ 0.8}$ $1.3_{-0.7}^{+0.8}$
γ_R₃	[×10⁻³]			2.8 ± 1.0
σ_R₃	[ppm]			$9_{- 9}^{+ 200}$ $9_{-9}^{+200}$
θ₀,R₃	[×10⁻³]			1.7 ± 0.5
γ_i′₁	[×10⁻³]	22 ± 4
σ_i′₁	[ppm]	$800_{- 696}^{+ 160}$ $800_{-696}^{+160}$
θ_0,i′₁	[×10⁻³]	15 ± 2
γ_g′₁	[×10⁻³]			$37_{- 8}^{+ 7}$ $37_{-8}^{+7}$
σ_g′₁	[ppm]			$16_{- 15}^{+ 238}$ $16_{-15}^{+238}$
θ₀,g′₁	[×10⁻³]			$21_{- 5}^{+ 4}$ $21_{-5}^{+4}$
γ_i′₂	[×10⁻³]			1 ± 2
σ_i′₂	[ppm]			$20_{- 19}^{+ 580}$ $20_{-19}^{+580}$
θ_0,i′₂	[×10⁻³]			$1_{- 1}^{+ 2}$ $1_{-1}^{+2}$
γ_g′₂	[×10⁻³]			24 ± 6
σ_g′₂	[ppm]			$689_{- 684}^{+ 257}$ $689_{-684}^{+257}$
θ_0,g′₂	[×10⁻³]			29 ± 5
γ_g′₃	[×10⁻³]	21 ± 5
σ_g′₃	[ppm]	$13_{- 12}^{+ 147}$ $13_{-12}^{+147}$
θ_0,g′₃	[×10⁻³]	14 ± 3
γ_z′	[×10⁻³]	25 ± 1
σ_z′	[ppm]	$704_{- 698}^{+ 237}$ $704_{-698}^{+237}$
θ_0,z′	[×10⁻³]	14.6 ± 0.6
γ_I+z	[×10⁻³]		$- 9_{- 1}^{+ 2}$ $-9_{-1}^{+2}$
σ_I+z	[ppm]		$875_{- 521}^{+ 97}$ $875_{-521}^{+97}$
θ_0,I+z	[×10⁻³]		${4.2}_{- 0.8}^{+ 0.9}$ $4.2_{-0.8}^{+0.9}$
γ_V	[×10⁻³]			$- 26_{- 8}^{+ 9}$ $-26_{-8}^{+9}$
σ_V	[ppm]			$5_{- 5}^{+ 93}$ $5_{-5}^{+93}$
θ_0,V	[×10⁻³]			−23 ± 7
γ_B₁	[×10⁻³]	$32_{- 1}^{+ 2}$ $32_{-1}^{+2}$	3 ± 8
σ_B₁	[ppm]	$3_{- 3}^{+ 77}$ $3_{-3}^{+77}$	$9_{- 9}^{+ 185}$ $9_{-9}^{+185}$
θ_0,B₁	[×10⁻³]	19.5 ± 0.5	13 ± 7
γ_B₂	[×10⁻³]	2 ± 2
σ_B₂	[ppm]	$28_{- 26}^{+ 207}$ $28_{-26}^{+207}$
θ_0,B₂	[×10⁻³]	${1.5}_{- 0.9}^{+ 1.0}$ $1.5_{-0.9}^{+1.0}$

Notes. Where γ is the offset relative flux, σ the jitter, and θ₀ the linear regressor. The filter subscripts correspond to the instruments specified for the limb darkening coefficients in Table F.1.

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