A Chandra view of SPT-CL J0217–5014: A massive galaxy cluster at a cosmic intersection at z = 0.53

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Table A.1.

Spectral fitting results within $1 \overset{'}{.} 5$ $1{{\overset{\prime}{.}}}5$ using different background files.

Background	Temperature	Abundance	C-stat/dof
	(keV)	(Z_⊙)
stowed	$5 . 76_{- 1.89}^{+ 1.20}$ $5.76_{-1.89}^{+1.20}$	$0 . 50_{- 0.27}^{+ 0.22}$ $0.50_{-0.27}^{+0.22}$	1139.43/1202
lbkg_an	$5 . 92_{- 0.81}^{+ 1.00}$ $5.92_{-0.81}^{+1.00}$	$0 . 44_{- 0.24}^{+ 0.26}$ $0.44_{-0.24}^{+0.26}$	1097.36/1208
lbkg_box	$5 . 54_{- 0.78}^{+ 0.94}$ $5.54_{-0.78}^{+0.94}$	$0 . 36_{- 0.24}^{+ 0.26}$ $0.36_{-0.24}^{+0.26}$	1088.00/1208

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