First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA - II. Spectral analysis and X-ray luminosity function

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Table A.1

Spectral fit parameters

MCSNR	N_H [10²² cm^-2]	kT [keV]	O	Ne	Mg	Si	S	Ar	Ca	Fe	τ [10¹¹ s cm³]	F_X [10^-13 erg s^-1 cm^-2]
J0505–6753
Comp1	${0.07}_{- 0.02}^{+ 0.04}$ $Mathematical equation: $0.07^{+0.04}_{-0.02}$$	${0.46}_{- 0.15}^{+ 0.04}$ $Mathematical equation: $0.46^{+0.04}_{-0.15}$$	0.26	0.40	0.49	0.0	0.0	0.5	0.5	0.0	${0.48}_{- 0.07}^{+ 1.11}$ $Mathematical equation: $0.48^{+1.11}_{-0.07}$$	73.0 ±0.7
Comp2		${0.72}_{- 0.01}^{+ 0.02}$ $Mathematical equation: $0.72^{+0.02}_{-0.01}$$	0.0	0.0	0.0	1.03	1.27	0.0	0.0	1.21	$282_{- 177}^{+ 130}$ $Mathematical equation: $282^{+130}_{-177}$$	64.6 ±0.6
Comp3		${0.08}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.08^{+0.01}_{-0.01}$$	0.0	0.0	0.0	1.03	1.27	0.0	0.0	1.21	${0.01}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.01^{+0.01}_{-0.01}$$	8.3 ± 0.7

J0505–6802
Comp1	${0.16}_{- 0.01}^{+ 0.02}$ $Mathematical equation: $0.16^{+0.02}_{-0.01}$$	${0.80}_{- 0.06}^{+ 0.05}$ $Mathematical equation: $0.80^{+0.05}_{-0.06}$$	0.50	0.50	0.50	0.50	0.50	0.50	0.50	0.50	${0.78}_{- 0.07}^{+ 0.13}$ $Mathematical equation: $0.78^{+0.13}_{-0.07}$$	44.1 ± 0.9
Comp2		${0.21}_{- 0.02}^{+ 0.01}$ $Mathematical equation: $0.21^{+0.01}_{-0.02}$$	0.11	0.16	0.18	0.37	0.50	0.50	0.50	0.20	${11.0}_{- 1.64}^{+ 126}$ $Mathematical equation: $11.0^{+126}_{-1.64}$$	42.7 ±0.8

J0509–6731
Comp1	${0.14}_{- 0.02}^{+ 0.02}$ $Mathematical equation: $0.14^{+0.02}_{-0.02}$$	${0.72}_{- 0.04}^{+ 0.05}$ $Mathematical equation: $0.72^{+0.05}_{-0.04}$$	0.0	0.0	0.0	${7.47}_{- 0.90}^{+ 1.18}$ $Mathematical equation: $7.47^{+1.18}_{-0.90}$$	${12.3}_{- 2.0}^{+ 2.5}$ $Mathematical equation: $12.3^{+2.5}_{-2.0}$$	0.0	0.0	${0.68}_{- 0.08}^{+ 0.10}$ $Mathematical equation: $0.68^{+0.10}_{-0.08}$$	${0.15}_{- 0.03}^{+ 0.02}$ $Mathematical equation: $0.15^{+0.02}_{-0.03}$$	31.4 ±0.6
Comp2		${0.23}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.23^{+0.01}_{-0.01}$$	0.50	0.50	0.50	0.50	0.50	0.50	0.50	0.50	356	14.4 ±0.6

J0509–6844
Comp1	${0.33}_{- 0.02}^{+ 0.03}$ $Mathematical equation: $0.33^{+0.03}_{-0.02}$$	${0.87}_{- 0.02}^{+ 0.02}$ $Mathematical equation: $0.87^{+0.02}_{-0.02}$$	0.25	1.71	0.33	2.84	3.48	5.26	9.51	1.10	${3.95}_{- 0.44}^{+ 0.84}$ $Mathematical equation: $3.95^{+0.84}_{-0.44}$$	118.5 ±1.2
Comp2		${1.33}_{- 0.13}^{+ 0.19}$ $Mathematical equation: $1.33^{+0.19}_{-0.13}$$	0.25	1.71	0.33	2.84	3.48	5.26	9.51	1.10	$364_{- 262}^{+ 78}$ $Mathematical equation: $364^{+78}_{-262}$$	29.5 ±1.5
Comp3		${0.30}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.30^{+0.01}_{-0.01}$$	0.5	0.5	0.5	0.5	0.5	0.5	0.5	0.5	$471_{- 407}^{+ 14}$ $Mathematical equation: $471^{+14}_{-407}$$	38.4 ±0.8

J0519–6902
Comp1	${0.16}_{- 0.01}^{+ 0.02}$ $Mathematical equation: $0.16^{+0.02}_{-0.01}$$	${1.13}_{- 0.08}^{+ 0.08}$ $Mathematical equation: $1.13^{+0.08}_{-0.08}$$	0.0	0.0	0.0	0.0	0.0	0.0	0.0	Pure	${0.75}_{- 0.11}^{+ 0.14}$ $Mathematical equation: $0.75^{+0.14}_{-0.11}$$	54.5 ±1.1
Comp2		${0.54}_{- 0.04}^{+ 0.03}$ $Mathematical equation: $0.54^{+0.03}_{-0.04}$$	0.50	0.50	0.50	0.50	0.50	0.50	0.50	0.50	$489_{- 67}^{+ 9}$ $Mathematical equation: $489^{+9}_{-67}$$	25.8 ±1.0
Comp3		${1.11}_{- 0.08}^{+ 0.09}$ $Mathematical equation: $1.11^{+0.09}_{-0.08}$$	0.0	0.0	0.0	0.0	0.0	0.0	0.0	Pure	${1.06}_{- 0.19}^{+ 0.11}$ $Mathematical equation: $1.06^{+0.11}_{-0.19}$$	22.5 ±0.9
Comp4		${0.45}_{- 0.10}^{+ 0.06}$ $Mathematical equation: $0.45^{+0.06}_{-0.10}$$	0.0	0.0	0.0	0.0	0.0	0.0	0.0	Pure	$298_{- 37}^{+ 54}$ $Mathematical equation: $298^{+54}_{-37}$$	11.4 ±0.7
Comp5		${0.40}_{- 0.05}^{+ 0.05}$ $Mathematical equation: $0.40^{+0.05}_{-0.05}$$	Pure	0.0	0.0	0.0	0.0	0.0	0.0	0.0	${0.63}_{- 0.16}^{+ 0.14}$ $Mathematical equation: $0.63^{+0.14}_{-0.16}$$	6.1 ±0.4
Comp6		${0.08}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.08^{+0.01}_{-0.01}$$	0.0	0.0	0.0	0.0	0.0	1.33	1.33	0.0	$148_{- 27}^{+ 19}$ $Mathematical equation: $148^{+19}_{-27}$$	2.3 ±0.3

J0525–6559
Comp1	${0.27}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.27^{+0.01}_{-0.01}$$	${0.51}_{- 0.03}^{+ 0.02}$ $Mathematical equation: $0.51^{+0.02}_{-0.03}$$	0.07	0.27	0.43	0.34	0.50	0.50	0.50	0.10	${1.49}_{- 0.13}^{+ 0.23}$ $Mathematical equation: $1.49^{+0.23}_{-0.13}$$	74.2 ±0.7
Comp2		${0.21}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.21^{+0.01}_{-0.01}$$	0.50	0.50	0.50	0.50	0.50	0.50	0.50	0.50	$344_{- 287}^{+ 129}$ $Mathematical equation: $344^{+129}_{-287}$$	52.5 ±0.5

J0525–6938
Comp1	${0.03}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.03^{+0.01}_{-0.01}$$	${0.85}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.85^{+0.01}_{-0.01}$$	0.05	0.46	0.19	0.39	0.5	0.5	0.5	0.28	${2.73}_{- 0.07}^{+ 0.17}$ $Mathematical equation: $2.73^{+0.17}_{-0.07}$$	763.4 ±3.0
Comp2		${0.25}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.25^{+0.01}_{-0.01}$$	9.03	0.25	2.59	1.37	1.03	0.5	0.5	0.15	$481_{- 422}^{+ 7}$ $Mathematical equation: $481^{+7}_{-422}$$	219.0 ±1.7
Comp3		${0.43}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.43^{+0.01}_{-0.01}$$	0.0	0.0	0.0	0.0	0.0	5.29	2.20	1.0	$500_{- 405}^{+ 2.16}$ $Mathematical equation: $500^{+2.16}_{-405}$$	92.8 ± 2.0

J0526–6605
Comp1	${0.35}_{- 0.01}^{+ 0.20}$ $Mathematical equation: $0.35^{+0.20}_{-0.01}$$	${0.85}_{- 0.02}^{+ 0.02}$ $Mathematical equation: $0.85^{+0.02}_{-0.02}$$	0.30	0.42	0.52	1.00	0.50	0.50	0.50	0.41	${2.21}_{- 0.58}^{+ 0.38}$ $Mathematical equation: $2.21^{+0.38}_{-0.58}$$	106.0 ±0.9
Comp2		${0.23}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.23^{+0.01}_{-0.01}$$	0.30	${0.22}_{- 0.02}^{+ 0.02}$ $Mathematical equation: $0.22^{+0.02}_{-0.02}$$	0.52	1.00	0.50	0.50	0.50	0.41	${25.8}_{- 0.09}^{+ 0.12}$ $Mathematical equation: $25.8^{+0.12}_{-0.09}$$	93.8±0.8

J0535–6602
Comp1	${0.22}_{- 0.03}^{+ 0.01}$ $Mathematical equation: $0.22^{+0.01}_{-0.03}$$	${0.70}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.70^{+0.01}_{-0.01}$$	${0.70}_{- 0.27}^{+ 0.10}$ $Mathematical equation: $0.70^{+0.10}_{-0.27}$$	${1.98}_{- 0.11}^{+ 0.02}$ $Mathematical equation: $1.98^{+0.02}_{-0.11}$$	0.85	0.76	0.48	0.14	0.50	${0.40}_{- 0.02}^{+ 0.01}$ $Mathematical equation: $0.40^{+0.01}_{-0.02}$$	$373_{- 252}^{+ 91}$ $Mathematical equation: $373^{+91}_{-252}$$	534.9 ±1.6
Comp2	${0.08}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.08^{+0.01}_{-0.01}$$	${0.25}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.25^{+0.01}_{-0.01}$$	${0.37}_{- 0.01}^{+ 0.07}$ $Mathematical equation: $0.37^{+0.07}_{-0.01}$$	0.57	0.12	0.13	0.50	0.50	0.50	0.28	${13.7}_{- 1.33}^{+ 16.2}$ $Mathematical equation: $13.7^{+16.2}_{-1.33}$$	161.3±1.1

J0535–6916
Comp1	${0.18}_{- 0.01}^{+ 0.01}$ $Mathematical equation: $0.18^{+0.01}_{-0.01}$$	${2.09}_{- 0.17}^{+ 0.39}$ $Mathematical equation: $2.09^{+0.39}_{-0.17}$$	0.23	0.76	0.68	0.90	0.65	0.50	0.50	0.31	$328_{- 285}^{+ 145}$ $Mathematical equation: $328^{+145}_{-285}$$	34.6 ±1.0
Comp2		1.15									$440_{- 415}^{+ 38}$ $Mathematical equation: $440^{+38}_{-415}$$	16.7 ±0.7
Comp3		${0.71}_{- 0.06}^{+ 0.04}$ $Mathematical equation: $0.71^{+0.04}_{-0.06}$$									${1.43}_{- 0.19}^{+ 0.28}$ $Mathematical equation: $1.43^{+0.28}_{-0.19}$$	20.9±0.6

J0540–6920^a
Comp1	${0.67}_{- 0.02}^{+ 0.04}$ $Mathematical equation: $0.67^{+0.04}_{-0.02}$$	${0.55}_{- 0.26}^{+ 0.07}$ $Mathematical equation: $0.55^{+0.07}_{-0.26}$$	0.50	0.50	0.50	0.50	0.50	0.50	0.50	0.50	$316_{- 280}^{+ 155}$ $Mathematical equation: $316^{+155}_{-280}$$	3.0 ±0.5

J0540–6944^b
Comp1	${1.26}_{- 0.26}^{+ 0.09}$ $Mathematical equation: $1.26^{+0.09}_{-0.26}$$	${0.21}_{- 0.05}^{+ 0.02}$ $Mathematical equation: $0.21^{+0.02}_{-0.05}$$	0.50	0.50	0.50	0.50	0.50	0.50	0.50	0.50	${1.27}_{- 0.03}^{+ 471}$ $Mathematical equation: $1.27^{+471}_{-0.03}$$	1.3 ± 0.1

Notes. The flux from the single component are not absorbed. ^(a)To account for the pulsar PSR 0540-69 a power-law model was also used with a PhotonIndex= ${1.99}_{- 0.03}^{+ 0.05}$ $Mathematical equation: $1.99^{+0.05}_{-0.03}$$ , yielding an unabsorbed flux of F_X = (269.5 ± 1.6) × 10⁻¹³ ergs⁻¹ cm⁻². ^(b)The model include a powerlaw with PhotonIndex= ${2.43}_{- 0.19}^{+ 0.10}$ $Mathematical equation: $2.43^{+0.10}_{-0.19}$$ , F_X = (18.3 ± 0.7) × 10⁻¹³ ergs⁻¹ cm⁻². In this case the power-law accounts for the straight light contribution from the nearby high mass X-ray binary LMC X-1.

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