Table 2: The parameters resulting from the fits to the spectra of XMMU J004215.8+411924 and SWIFT J004217.4+411532.
Power-law Disc black-body Bremsstrahlung

Obs L₃₆ $\Gamma$ $N_{\rm H,21}$ $\chi^2_\nu$ L₃₆ $T_{\rm in}$ $N_{\rm H,21}$ $\chi^2_\nu$ L₃₆ $T_{\rm b}$ $N_{\rm H,21}$ $\chi^2_\nu$

XMMU J004215.8+411924

2 <0.4 (1.57) (4.2) - <3.5 (1.92) (2.2) - <3.8 (12.2) (3.6) -

3 $110\pm30$ $1.77\pm0.33$ 6.2 $\pm$ 3.7 0.98 $86\pm44$ 1.55 $\pm$ 0.35 2.5 $\pm$ 2.3 1.05 $100\pm50$ 6.5 $\pm$ 4.0 5.2 $\pm$ 2.7 0.98

4 $76\pm12$ $1.57\pm0.08$ 4.2 $\pm$ 0.5 0.84 $67\pm11$ 1.92 $\pm$ 0.14 2.2 $\pm$ 0.3 0.87 $73\pm12$ 12.2 $\pm$ 4.0 3.6 $\pm$ 0.4 0.80

5 21 $\pm$ 1 (1.57) (4.2) - $19\pm1$ (1.92) (2.2) - 20 $\pm$ 1 (12.2) (3.6) -

6 <5.8 (1.57) (4.2) - <5.1 (1.92) (2.2) - <5.6 (12.2) (3.6) -

7 <0.8 (1.57) (4.2) - <0.7 (1.92) (2.2) - <0.6 (12.2) (3.6) -

SWIFT J004217.4+411532

4 <2.1 (3.5) (4.0) - <0.9 (0.50) (0.67) - <0.9 (1.0) (1.5) -

5 $580\pm70$ $3.12\pm0.35$ $4.4\pm1.3$ 1.35 $270\pm30$ $0.61\pm0.05$ (0.67) 1.26 $350\pm70$ $1.26\pm0.26$ $2.18\pm0.91$ 1.28

6 $450\pm70$ $3.55\pm0.49$ $4.0\pm1.7$ 0.99 $180\pm30$ $0.50\pm0.06$ (0.67) 0.96 $230\pm70$ $1.07\pm0.27$ $1.13\pm1.13$ 0.86

7 $260\pm60$ $3.47\pm0.31$ $5.1\pm1.3$ 0.87 $97\pm7$ $0.57\pm0.04$ (0.67) 0.97 $130\pm20$ $1.15\pm0.11$ $2.0\pm0.9$ 0.88

8 $290\pm10$ (3.5) (4.0) - $140\pm10$ (0.50) (0.67) - $122\pm4$ (1.0) (1.5) -

9 $163\pm7$ (3.5) (4.0) - $80\pm4$ (0.50) (0.67) - $69\pm3$ (1.0) (1.5) -

10 $81\pm29$ $4.50\pm0.65$ $5.1\pm2.2$ 1.26 $20\pm2$ $0.35\pm0.03$ (0.67) 1.01 $28\pm15$ 0.58 $\pm0.12$ 1.91 $\pm1.33$ 1.10

11 $36\pm4$ $4.34\pm0.33$ $3.3\pm0.5$ 1.56 $15\pm3$ $0.27\pm0.02$ (0.67) 1.67 $18\pm4$ 0.49 $\pm$ 0.06 $1.49\pm0.27$ 1.52

12 $20\pm3$ $4.51\pm0.57$ $3.2\pm0.8$ 1.10 $8.2\pm2.2$ $0.25\pm0.03$ (0.67) 1.44 10 $\pm$ 4 0.42 $\pm$ 0.08 $1.50\pm0.43$ 1.29

13 <0.9 (3.5) (4.0) - <0.5 (0.50) (0.67) - <0.4 (1.0) (1.5) -

**Table 2:** The parameters resulting from the fits to the spectra of XMMU J004215.8+411924 and SWIFT J004217.4+411532.
	Power-law	Disc black-body	Bremsstrahlung
Obs	L₃₆	$\Gamma$	$N_{\rm H,21}$	$\chi^2_\nu$	L₃₆	$T_{\rm in}$	$N_{\rm H,21}$	$\chi^2_\nu$	L₃₆	$T_{\rm b}$	$N_{\rm H,21}$	$\chi^2_\nu$
XMMU J004215.8+411924
2	<0.4	(1.57)	(4.2)	-	<3.5	(1.92)	(2.2)	-	<3.8	(12.2)	(3.6)	-
3	$110\pm30$	$1.77\pm0.33$	6.2 $\pm$ 3.7	0.98	$86\pm44$	1.55 $\pm$ 0.35	2.5 $\pm$ 2.3	1.05	$100\pm50$	6.5 $\pm$ 4.0	5.2 $\pm$ 2.7	0.98
4	$76\pm12$	$1.57\pm0.08$	4.2 $\pm$ 0.5	0.84	$67\pm11$	1.92 $\pm$ 0.14	2.2 $\pm$ 0.3	0.87	$73\pm12$	12.2 $\pm$ 4.0	3.6 $\pm$ 0.4	0.80
5	21 $\pm$ 1	(1.57)	(4.2)	-	$19\pm1$	(1.92)	(2.2)	-	20 $\pm$ 1	(12.2)	(3.6)	-
6	<5.8	(1.57)	(4.2)	-	<5.1	(1.92)	(2.2)	-	<5.6	(12.2)	(3.6)	-
7	<0.8	(1.57)	(4.2)	-	<0.7	(1.92)	(2.2)	-	<0.6	(12.2)	(3.6)	-
SWIFT J004217.4+411532
4	<2.1	(3.5)	(4.0)	-	<0.9	(0.50)	(0.67)	-	<0.9	(1.0)	(1.5)	-
5	$580\pm70$	$3.12\pm0.35$	$4.4\pm1.3$	1.35	$270\pm30$	$0.61\pm0.05$	(0.67)	1.26	$350\pm70$	$1.26\pm0.26$	$2.18\pm0.91$	1.28
6	$450\pm70$	$3.55\pm0.49$	$4.0\pm1.7$	0.99	$180\pm30$	$0.50\pm0.06$	(0.67)	0.96	$230\pm70$	$1.07\pm0.27$	$1.13\pm1.13$	0.86
7	$260\pm60$	$3.47\pm0.31$	$5.1\pm1.3$	0.87	$97\pm7$	$0.57\pm0.04$	(0.67)	0.97	$130\pm20$	$1.15\pm0.11$	$2.0\pm0.9$	0.88
8	$290\pm10$	(3.5)	(4.0)	-	$140\pm10$	(0.50)	(0.67)	-	$122\pm4$	(1.0)	(1.5)	-
9	$163\pm7$	(3.5)	(4.0)	-	$80\pm4$	(0.50)	(0.67)	-	$69\pm3$	(1.0)	(1.5)	-
10	$81\pm29$	$4.50\pm0.65$	$5.1\pm2.2$	1.26	$20\pm2$	$0.35\pm0.03$	(0.67)	1.01	$28\pm15$	0.58 $\pm0.12$	1.91 $\pm1.33$	1.10
11	$36\pm4$	$4.34\pm0.33$	$3.3\pm0.5$	1.56	$15\pm3$	$0.27\pm0.02$	(0.67)	1.67	$18\pm4$	0.49 $\pm$ 0.06	$1.49\pm0.27$	1.52
12	$20\pm3$	$4.51\pm0.57$	$3.2\pm0.8$	1.10	$8.2\pm2.2$	$0.25\pm0.03$	(0.67)	1.44	10 $\pm$ 4	0.42 $\pm$ 0.08	$1.50\pm0.43$	1.29
13	<0.9	(3.5)	(4.0)	-	<0.5	(0.50)	(0.67)	-	<0.4	(1.0)	(1.5)	-

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