Table 6: continued.

a Foreground star     b Galaxy     c Supersoft source candidate     d Globular cluster     e SNR
$\star$ bulge source     $\sim$ Variable source (ref. Tables 2, 3 and footnote in Sect. 4.1.1)     $\dagger$ Source with uncertain count rate.
RXJ	SI	RA		(J2000)		Dec		$\sigma_{\rm Pos}$	Cl.	Maxlik	Rate (B)	Rate (S)	Rate (H)	Rate ($H_{\rm 1}$)	Rate ($H_{\rm 2}$)
No.	No.	(h)	(m)	(s)	( $\hbox{$^\circ$ }$)	(')	('')	('')		(LH)	$\rm (ct \cdot ks^{-1})$	$\rm (ct \cdot ks^{-1})$	$\rm (ct \cdot ks^{-1})$	$\rm (ct \cdot ks^{-1})$	$\rm (ct \cdot ks^{-1})$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)	(16)
RX J0047.0+4204	357-	0	47	3.4	42	4	55	8	1	43.7	$1.89 \pm 0.37$	$< 0.53 \hspace{8ex}$	$1.39 \pm 0.27$	$< 0.58 \hspace{8ex}$	$1.05 \pm 0.23$
RX J0047.0+4222	359	0	47	5.6	42	22	18	8	1	14.5	$0.47 \pm 0.24$	$< 0.04 \hspace{8ex}$	$0.46 \pm 0.11$	$< 0.33 \hspace{8ex}$	$< 0.14 \hspace{8ex}$
RX J0047.1+4218	360	0	47	8.6	42	18	11	5	1	18.1	$0.94 \pm 0.27$	$0.39 \pm 0.31$	$< 0.59 \hspace{8ex}$	$< 0.10 \hspace{8ex}$	$< 0.50 \hspace{8ex}$
RX J0047.2+4135	365-	0	47	16.2	41	35	46	12	1	16.9	$< 1.90 \hspace{8ex}$	$< 0.53 \hspace{8ex}$	$1.42 \pm 0.38$	$< 0.78 \hspace{8ex}$	$0.77 \pm 0.27$
RX J0047.2+4140	363-	0	47	15.4	41	40	41	9	1	40.0	$1.81 \pm 0.45$	$< 0.36 \hspace{8ex}$	$1.94 \pm 0.39$	$0.70 \pm 0.25$	$1.18 \pm 0.30$
RX J0047.2+4158	364	0	47	17.0	41	58	19	11	1	13.4	$0.93 \pm 0.40$	$0.86 \pm 0.39$	$< 0.16 \hspace{8ex}$	$< 0.07 \hspace{8ex}$	$0.09 \pm 0.03$
aRX J0047.2+4202	362-	0	47	13.8	42	2	13	8	1	68.9	$3.67 \pm 0.50$	$1.47 \pm 0.37$	$1.93 \pm 0.32$	$0.83 \pm 0.22$	$1.10 \pm 0.24$
RX J0047.2+4220	361+	0	47	14.2	42	20	39	5	1	62.4	$2.51 \pm 0.38$	$0.45 \pm 0.27$	$2.08 \pm 0.27$	$0.76 \pm 0.25$	$1.29 \pm 0.10$
RX J0047.2+4221	366	0	47	17.9	42	21	16	5	1	46.3	$1.75 \pm 0.34$	$0.59 \pm 0.28$	$1.30 \pm 0.23$	$0.53 \pm 0.21$	$0.71 \pm 0.07$
RX J0047.3+4148		0	47	20.1	41	48	37	10	1	18.0	$1.93 \pm 0.46$	$< 3.26 \hspace{8ex}$	$0.85 \pm 0.25$	$< 0.45 \hspace{8ex}$	$0.60 \pm 0.21$
RX J0047.4+4124		0	47	27.8	41	24	40	13	1	12.8	$< 5.97 \hspace{8ex}$	$< 1.65 \hspace{8ex}$	$3.64 \pm 1.34$	$< 1.07 \hspace{8ex}$	$3.01 \pm 1.23$
$\sim$RX J0047.4+4152		0	47	26.9	41	52	53	9	1	52.7	$3.35 \pm 0.54$	$< 0.88 \hspace{8ex}$	$2.49 \pm 0.40$	$1.00 \pm 0.26$	$1.48 \pm 0.30$
RX J0047.4+4208	368	0	47	24.2	42	8	44	5	1	22.6	$1.35 \pm 0.30$	$0.47 \pm 0.26$	$0.76 \pm 0.07$	$0.38 \pm 0.28$	$< 0.52 \hspace{8ex}$
RX J0047.4+4213	370	0	47	26.3	42	13	47	5	1	16.2	$0.55 \pm 0.22$	$< 0.12 \hspace{8ex}$	$0.42 \pm 0.19$	$< 0.05 \hspace{8ex}$	$0.38 \pm 0.17$
aRX J0047.4+4220	372	0	47	28.7	42	20	53	5	1	13.9	$0.61 \pm 0.24$	$< 0.29 \hspace{8ex}$	$< 0.34 \hspace{8ex}$	$< 0.03 \hspace{8ex}$	$< 0.28 \hspace{8ex}$
aRX J0047.4+4221	369+	0	47	26.2	42	21	52	5	1	192.2	$4.45 \pm 0.46$	$0.80 \pm 0.28$	$3.71 \pm 0.38$	$1.90 \pm 0.19$	$1.45 \pm 0.29$
RX J0047.4+4230	371	0	47	27.3	42	30	21	7	1	17.5	$2.08 \pm 0.42$	$0.85 \pm 0.35$	$1.03 \pm 0.16$	$0.55 \pm 0.38$	$< 0.68 \hspace{8ex}$
RX J0047.4+4248	367	0	47	24.1	42	48	32	35	2	19.4	$< 0.12 \hspace{8ex}$	$< 0.02 \hspace{8ex}$	$0.10 \pm 0.07$	$< 0.02 \hspace{8ex}$	$< 0.07 \hspace{8ex}$
RX J0047.5+4135		0	47	31.4	41	35	24	12	1	12.0	$< 1.73 \hspace{8ex}$	$< 0.45 \hspace{8ex}$	$1.17 \pm 0.40$	$< 1.00 \hspace{8ex}$	$< 0.68 \hspace{8ex}$
RX J0047.5+4140		0	47	30.9	41	40	42	11	1	10.3	$< 2.17 \hspace{8ex}$	$< 1.21 \hspace{8ex}$	$< 0.84 \hspace{8ex}$	$< 0.52 \hspace{8ex}$	$< 0.38 \hspace{8ex}$
RX J0047.5+4149	373-	0	47	30.6	41	49	24	8	1	81.3	$4.39 \pm 0.63$	$< 4.52 \hspace{8ex}$	$2.97 \pm 0.46$	$0.95 \pm 0.27$	$2.11 \pm 0.38$
$\dagger$RX J0047.6+4132	374	0	47	36.0	41	32	8	8	2	12.4	$< 0.32 \hspace{8ex}$	$0.04 \pm 0.01$	$< 0.25 \hspace{8ex}$	$< 0.27 \hspace{8ex}$	$< 0.02 \hspace{8ex}$
cRX J0047.6+4205	376	0	47	38.5	42	5	7	10	1	12.9	$1.05 \pm 0.36$	$0.99 \pm 0.35$	$< 0.04 \hspace{8ex}$	$< 0.02 \hspace{8ex}$	$< 0.02 \hspace{8ex}$
RX J0047.6+4208	375	0	47	36.5	42	8	42	5	1	15.0	$0.85 \pm 0.29$	$0.28 \pm 0.27$	$0.54 \pm 0.07$	$< 0.08 \hspace{8ex}$	$< 0.50 \hspace{8ex}$
RX J0047.7+4159	377	0	47	42.3	42	0	0	12	1	11.8	$1.23 \pm 0.44$	$1.15 \pm 0.41$	$< 0.12 \hspace{8ex}$	$< 0.07 \hspace{8ex}$	$< 0.05 \hspace{8ex}$
aRX J0047.7+4201	381-	0	47	43.2	42	1	19	9	1	24.6	$1.48 \pm 0.41$	$< 0.54 \hspace{8ex}$	$1.19 \pm 0.30$	$0.60 \pm 0.21$	$0.67 \pm 0.23$
RX J0047.7+4202	382+	0	47	44.5	42	2	46	9	1	19.3	$0.75 \pm 0.35$	$< 0.06 \hspace{8ex}$	$0.62 \pm 0.31$	$0.18 \pm 0.05$	$0.55 \pm 0.36$
RX J0047.7+4210	380	0	47	42.6	42	10	17	5	1	21.6	$1.21 \pm 0.30$	$< 0.23 \hspace{8ex}$	$0.98 \pm 0.13$	$< 0.53 \hspace{8ex}$	$< 0.51 \hspace{8ex}$
RX J0047.7+4211		0	47	45.0	42	11	3	11	1	10.9	$< 2.25 \hspace{8ex}$	$< 1.47 \hspace{8ex}$	$1.22 \pm 0.40$	$< 0.74 \hspace{8ex}$	$0.75 \pm 0.29$
RX J0047.7+4211	378	0	47	42.5	42	11	40	5	1	15.3	$1.41 \pm 0.34$	$0.58 \pm 0.32$	$< 0.71 \hspace{8ex}$	$< 0.44 \hspace{8ex}$	$< 0.38 \hspace{8ex}$
RX J0047.7+4222		0	47	44.5	42	22	37	5	1	15.8	$< 6.19 \hspace{8ex}$	$< 1.70 \hspace{8ex}$	$7.36 \pm 1.60$	$< 3.10 \hspace{8ex}$	$< 2.63 \hspace{8ex}$
RX J0047.7+4222	379+	0	47	42.5	42	22	22	5	1	63.7	$2.20 \pm 0.38$	$< 0.14 \hspace{8ex}$	$1.95 \pm 0.28$	$0.72 \pm 0.24$	$1.34 \pm 0.18$
RX J0047.7+4224	383+	0	47	45.4	42	24	28	5	1	70.4	$3.34 \pm 0.48$	$0.99 \pm 0.38$	$2.54 \pm 0.33$	$0.84 \pm 0.26$	$1.53 \pm 0.16$
RX J0047.8+4135		0	47	53.9	41	35	38	16	1	11.8	$< 3.40 \hspace{8ex}$	$3.07 \pm 0.94$	$< 0.45 \hspace{8ex}$	$< 0.27 \hspace{8ex}$	$< 0.36 \hspace{8ex}$
$\sim$RX J0047.8+4142		0	47	49.9	41	42	9	11	1	41.4	$7.02 \pm 1.15$	$< 1.63 \hspace{8ex}$	$13.74 \pm 1.37$	$4.06 \pm 0.78$	$7.97 \pm 1.05$
RX J0047.8+4153		0	47	49.4	41	53	26	10	1	16.9	$< 1.13 \hspace{8ex}$	$< 0.31 \hspace{8ex}$	$0.89 \pm 0.28$	$< 0.24 \hspace{8ex}$	$0.78 \pm 0.25$
RX J0047.8+4207		0	47	51.7	42	7	24	9	1	19.9	$2.46 \pm 0.59$	$< 3.90 \hspace{8ex}$	$1.23 \pm 0.36$	$0.80 \pm 0.28$	$< 0.69 \hspace{8ex}$
RX J0047.8+4219	384+	0	47	48.4	42	19	25	5	1	399.2	$7.87 \pm 0.62$	$0.78 \pm 0.31$	$7.85 \pm 0.60$	$1.63 \pm 0.27$	$5.02 \pm 0.43$
RX J0048.0+4140	385-	0	48	0.3	41	40	15	7	1	442.6	$27.75 \pm 2.07$	$< 3.14 \hspace{8ex}$	$25.92 \pm 1.97$	$10.22 \pm 1.22$	$16.23 \pm 1.58$
RX J0048.0+4156		0	48	4.2	41	56	48	10	1	13.1	$2.11 \pm 0.58$	$< 1.74 \hspace{8ex}$	$< 0.85 \hspace{8ex}$	$< 0.56 \hspace{8ex}$	$< 0.37 \hspace{8ex}$
RX J0048.0+4218	386	0	48	4.6	42	18	6	9	1	16.4	$1.24 \pm 0.37$	$0.48 \pm 0.28$	$0.65 \pm 0.19$	$0.26 \pm 0.18$	$0.50 \pm 0.12$
$\dagger$RX J0048.1+4149	387	0	48	6.8	41	49	56	6	2	18.8	$1.01 \pm 0.79$	$0.21 \pm 0.07$	$< 0.68 \hspace{8ex}$	$< 0.32 \hspace{8ex}$	$< 0.38 \hspace{8ex}$
$\dagger$RX J0048.3+4134	388	0	48	19.1	41	34	37	36	2	63.8	$4.94 \pm 1.15$	$< 0.61 \hspace{8ex}$	$4.09 \pm 0.84$	$0.76 \pm 0.39$	$3.68 \pm 0.83$
RX J0048.3+4210	389+	0	48	23.7	42	10	25	6	1	18.2	$0.84 \pm 0.37$	$0.15 \pm 0.14$	$0.69 \pm 0.35$	$< 0.10 \hspace{8ex}$	$0.63 \pm 0.34$
$\sim^a$RX J0048.4+4157	390-	0	48	24.6	41	57	18	6	1	614.1	$35.30 \pm 2.16$	$21.89 \pm 1.77$	$14.28 \pm 1.31$	$8.11 \pm 0.99$	$6.24 \pm 0.87$
$\dagger$RX J0048.4+4203	391	0	48	28.4	42	3	10	10	2	22.4	$0.58 \pm 0.49$	$0.02 \pm 0.01$	$0.59 \pm 0.52$	$< 0.18 \hspace{8ex}$	$< 0.43 \hspace{8ex}$
RX J0048.9+4223	392-	0	48	58.4	42	23	47	9	4	250.2	$9.21 \pm 0.99$	$< 0.52 \hspace{8ex}$	$15.95 \pm 1.07$	$6.21 \pm 0.69$	$9.84 \pm 0.81$
$\dagger$RX J0049.1+4200	393	0	49	6.7	42	0	7	16	2	32.4	$0.70 \pm 0.65$	$0.13 \pm 0.02$	$< 0.60 \hspace{8ex}$	$< 0.24 \hspace{8ex}$	$< 0.38 \hspace{8ex}$
$\dagger$RX J0049.2+4254	394	0	49	13.5	42	54	1	11	3	14.6	$< 0.09 \hspace{8ex}$	$0.02 \pm 0.01$	$< 0.07 \hspace{8ex}$	$< 0.00 \hspace{8ex}$	$< 0.06 \hspace{8ex}$
RX J0049.5+4158		0	49	30.6	41	58	23	13	1	22.1	$6.87 \pm 2.29$	$< 1.91 \hspace{8ex}$	$6.12 \pm 1.85$	$< 2.66 \hspace{8ex}$	$< 5.62 \hspace{8ex}$
RX J0049.5+4211	395	0	49	35.8	42	11	48	8	2	16.4	$1.90 \pm 0.85$	$< 0.21 \hspace{8ex}$	$1.41 \pm 0.44$	$0.55 \pm 0.41$	$1.12 \pm 0.31$
RX J0049.7+4220	396	0	49	45.1	42	20	9	27	2	11.6	$3.68 \pm 1.03$	$1.59 \pm 0.66$	$1.80 \pm 0.68$	$0.50 \pm 0.43$	$1.47 \pm 0.61$

 

 

Table 7: Table of the identifications of ROSAT PSPC sources with Einstein sources listed by TF. $F_{\rm R}$ gives the ROSAT source flux using the Einstein spectral model of TF and $F_{\rm E}$ gives the Einstein source flux of the correlated Einstein source (see Sect. 4.1.2). The distance between two correlating sources is given in arcseconds $(\hbox {$^{\prime \prime }$ }$) as well as in units of the combined positional error ($\sigma$) of both sources. The last column gives the flux ratio between the ROSAT and the Einstein measurements, showing possible long term variabilities between the epochs of the two observations. Sources with ROSAT numbers preceeded by a $\star$ belong to the bulge region.

ROSAT	$F_{\rm R} \, (\times 10^{13})$	Einstein	$F_{\rm E} \, (\times 10^{13})$	Distance		$F_{\rm R}/F_{\rm E}$
No.	(cgs)	No.	(cgs)	('')	$(\sigma)$
RX J0039.4+4035	$0.17 \pm 0.06$	1	$0.60 \pm 0.26$	59.1	1.31	$0.28 \pm 0.16$
RX J0040.0+4031	$1.04 \pm 0.10$	2	$1.64 \pm 0.42$	31.7	0.70	$0.63 \pm 0.17$
RX J0040.2+4050	$31.64 \pm 0.48$	3	$25.38 \pm 2.50$	3.6	0.59	$1.25 \pm 0.12$
RX J0040.3+4043	$13.82 \pm 0.29$	4	$16.35 \pm 2.09$	3.4	0.58	$0.85 \pm 0.11$
RX J0040.4+4029	$1.07 \pm 0.10$	5	$0.99 \pm 0.28$	13.4	0.30	$1.08 \pm 0.33$
RX J0040.4+4129	$2.30 \pm 0.41$	6	$1.06 \pm 0.35$	9.5	0.20	$2.17 \pm 0.81$
RX J0040.7+4051	$0.49 \pm 0.07$	7	$0.66 \pm 0.26$	6.0	0.13	$0.74 \pm 0.30$
RX J0041.4+4058	$1.94 \pm 0.12$	8	$1.77 \pm 0.50$	24.6	0.54	$1.09 \pm 0.32$
RX J0041.7+4134	$14.38 \pm 0.49$	9	$8.72 \pm 1.08$	1.8	0.29	$1.65 \pm 0.21$
RX J0041.8+4021	$24.25 \pm 0.76$	11	$15.54 \pm 0.88$	5.4	0.12	$1.56 \pm 0.10$
RX J0041.8+4113	$0.43 \pm 0.09$	10	$0.90 \pm 0.24$	32.9	0.73	$0.48 \pm 0.16$
RX J0042.2+4019	$40.38 \pm 1.23$	15	$48.83 \pm 1.61$	2.9	0.06	$0.83 \pm 0.04$
RX J0042.2+4039	$2.18 \pm 0.19$	13	$1.64 \pm 0.38$	18.4	0.41	$1.33 \pm 0.33$
RX J0042.2+4055	$2.71 \pm 0.18$	18	$1.67 \pm 0.48$	1.9	0.32	$1.62 \pm 0.48$
RX J0042.2+4101	$9.53 \pm 0.32$	16	$3.88 \pm 0.75$	0.7	0.12	$2.46 \pm 0.48$
RX J0042.2+4112	$9.04 \pm 0.25$	19	$4.26 \pm 0.54$	8.0	1.37	$2.12 \pm 0.28$
RX J0042.2+4117	$2.18 \pm 0.16$	17	$1.26 \pm 0.38$	5.0	0.86	$1.73 \pm 0.54$
RX J0042.2+4118	$9.71 \pm 0.32$	14	$3.23 \pm 0.51$	9.5	1.63	$3.01 \pm 0.49$
$\star$RX J0042.3+4113	$5.02 \pm 0.23$	20	$4.93 \pm 0.54$	9.1	1.55	$1.02 \pm 0.12$
$\star$RX J0042.3+4115	$16.06 \pm 0.41$	23	$6.88 \pm 0.61$	1.0	0.17	$2.33 \pm 0.21$
RX J0042.4+4104	$4.78 \pm 0.22$	28	$3.07 \pm 0.71$	6.4	0.99	$1.56 \pm 0.37$
RX J0042.4+4112	$5.92 \pm 0.25$	27	$3.38 \pm 0.52$	5.2	0.89	$1.75 \pm 0.28$
RX J0042.4+4125	$1.13 \pm 0.13$	30	$1.71 \pm 0.47$	38.7	0.85	$0.66 \pm 0.20$
RX J0042.5+4103	$1.34 \pm 0.13$	37	$2.61 \pm 0.85$	65.8	1.45	$0.51 \pm 0.17$
$\star$RX J0042.5+4113	$4.15 \pm 0.22$	34	$3.05 \pm 0.50$	7.1	1.22	$1.36 \pm 0.23$
$\star$RX J0042.5+4116	$6.01 \pm 0.21$	32	$3.62 \pm 0.51$	6.8	1.16	$1.66 \pm 0.24$
$\star$RX J0042.5+4119	$3.30 \pm 0.20$	33	$0.83 \pm 0.28$	9.2	1.58	$3.97 \pm 1.35$
RX J0042.5+4132	$1.69 \pm 0.16$	38	$1.56 \pm 0.29$	5.0	0.11	$1.08 \pm 0.23$
RX J0042.6+4052	$32.45 \pm 0.53$	51	$9.16 \pm 1.01$	11.6	1.98	$3.54 \pm 0.40$
$\star$RX J0042.6+4114	$3.75 \pm 0.17$	48	$0.97 \pm 0.27$	9.1	1.56	$3.87 \pm 1.09$
$\star$RX J0042.6+4115	$42.30 \pm 0.38$	41	$41.28 \pm 1.22$	6.9	1.19	$1.02 \pm 0.03$
$\star$RX J0042.7+4111	$4.13 \pm 0.21$	58	$1.59 \pm 0.44$	3.7	0.63	$2.60 \pm 0.73$
$\star$RX J0042.7+4115	$22.80 \pm 0.30$	52	$1.62 \pm 0.31$	4.5	0.77	$14.07 \pm 2.71$
$\star$RX J0042.7+4116	$29.89 \pm 0.28$	59	$1.81 \pm 0.34$	8.6	1.47	$16.51 \pm 3.14$
$\star$RX J0042.8+4115	$17.39 \pm 0.25$	63	$8.04 \pm 0.63$	5.6	0.96	$2.16 \pm 0.17$
$\star$RX J0042.8+4118	$9.68 \pm 0.33$	68	$5.64 \pm 0.58$	6.4	1.09	$1.72 \pm 0.19$
RX J0042.8+4125	$3.95 \pm 0.22$	62	$3.44 \pm 0.84$	6.2	1.06	$1.15 \pm 0.29$
RX J0042.8+4131	$18.62 \pm 0.45$	67	$11.95 \pm 1.10$	4.6	0.78	$1.56 \pm 0.15$
RX J0042.9+4111	$3.84 \pm 0.21$	73	$3.13 \pm 0.51$	5.4	0.92	$1.23 \pm 0.21$
$\star$RX J0042.9+4117	$8.46 \pm 0.13$	72	$0.77 \pm 0.27$	10.6	1.83	$10.99 \pm 3.82$
$\star$RX J0042.9+4119	$3.66 \pm 0.22$	76	$1.64 \pm 0.46$	4.6	0.78	$2.23 \pm 0.64$
RX J0042.9+4125	$3.05 \pm 0.19$	70	$3.77 \pm 0.34$	2.3	0.05	$0.81 \pm 0.09$
$\star$RX J0043.0+4115	$8.97 \pm 0.31$	79	$3.26 \pm 0.42$	1.7	0.30	$2.75 \pm 0.36$
$\star$RX J0043.0+4117	$6.19 \pm 0.27$	80	$1.92 \pm 0.35$	9.1	1.56	$3.22 \pm 0.61$
RX J0043.1+4048	$1.48 \pm 0.17$	81	$1.04 \pm 0.42$	52.4	1.15	$1.43 \pm 0.60$
RX J0043.1+4114	$8.60 \pm 0.30$	83	$7.51 \pm 0.61$	5.8	1.00	$1.15 \pm 0.10$
RX J0043.1+4118	$7.54 \pm 0.24$	82	$2.03 \pm 0.31$	2.4	0.41	$3.72 \pm 0.58$
RX J0043.2+4107	$3.08 \pm 0.19$	85	$4.27 \pm 0.94$	5.4	0.93	$0.72 \pm 0.16$
RX J0043.3+4117	$4.44 \pm 0.25$	88	$1.31 \pm 0.34$	32.7	0.72	$3.39 \pm 0.89$
RX J0043.3+4120	$1.80 \pm 0.17$	87	$2.15 \pm 0.52$	5.0	0.85	$0.84 \pm 0.22$
RX J0043.3+4159	$1.91 \pm 0.22$	86	$0.96 \pm 0.29$	12.1	0.27	$1.99 \pm 0.64$
RX J0043.4+4107	$1.67 \pm 0.15$	90	$1.64 \pm 0.28$	15.3	0.34	$1.02 \pm 0.20$
RX J0043.4+4118	$3.20 \pm 0.20$	89	$2.48 \pm 0.60$	15.5	1.99	$1.29 \pm 0.32$
RX J0043.5+4113	$6.31 \pm 0.27$	91	$6.24 \pm 1.02$	8.8	1.51	$1.01 \pm 0.17$
RX J0043.6+4114	$5.13 \pm 0.23$	92	$4.73 \pm 0.90$	9.3	1.41	$1.08 \pm 0.21$
RX J0043.7+4124	$1.00 \pm 0.13$	93	$2.86 \pm 0.74$	6.4	0.68	$0.35 \pm 0.10$
RX J0043.8+4116	$6.29 \pm 0.26$	94	$4.05 \pm 0.78$	5.3	0.82	$1.55 \pm 0.30$
RX J0043.9+4045	$0.85 \pm 0.19$	95	$1.64 \pm 0.50$	61.8	1.34	$0.52 \pm 0.19$
RX J0044.4+4121	$7.97 \pm 0.30$	97	$8.59 \pm 1.09$	2.6	0.45	$0.93 \pm 0.12$
RX J0044.9+4059	$0.84 \pm 0.17$	98	$2.07 \pm 0.73$	47.2	1.03	$0.40 \pm 0.16$
RX J0045.2+4136	$0.40 \pm 0.08$	99	$1.03 \pm 0.27$	52.7	1.15	$0.39 \pm 0.13$
RX J0045.4+4146	$0.32 \pm 0.32$	100	$0.71 \pm 0.23$	70.4	1.53	$0.46 \pm 0.48$
RX J0045.6+4208	$6.92 \pm 0.30$	101	$4.99 \pm 0.86$	0.6	0.09	$1.39 \pm 0.25$
RX J0045.7+4139	$36.00 \pm 0.52$	102	$43.18 \pm 3.15$	8.3	1.37	$0.83 \pm 0.06$
RX J0046.1+4208	$1.03 \pm 0.12$	103	$0.95 \pm 0.24$	28.2	0.62	$1.08 \pm 0.30$
RX J0046.4+4201	$10.08 \pm 0.31$	105	$5.52 \pm 0.89$	2.1	0.34	$1.83 \pm 0.30$
RX J0046.4+4204	$8.88 \pm 0.31$	104	$8.56 \pm 0.48$	15.1	0.33	$1.04 \pm 0.07$
RX J0046.9+4220	$5.19 \pm 0.24$	107	$3.54 \pm 0.53$	55.6	1.23	$1.47 \pm 0.23$
RX J0048.0+4140	$7.43 \pm 0.55$	108	$4.46 \pm 0.89$	44.1	0.97	$1.67 \pm 0.35$

 

 

Table 8: Table of all optical and radio identifications.

ROSAT	Obj.-Cl.	Identification	Distance
No.			('')	$(\sigma)$
RX J0036.3+4053	GC	BA87(5)	10.4	0.78
RX J0037.3+4043	Star (F5)	SIMBAD( SAO 36516)	13.0	1.49
RX J0038.0+4026	Star	HA94(38232)	6.1	1.21
RX J0038.4+4012	Star	HA94(9276)	6.9	1.38
RX J0038.4+4136	EO	87GB 003540.8+412038	34.9	1.51
RX J0038.6+4026	Star (K0)	SIMBAD( SAO 36541)	0.8	0.16
RX J0039.5+4008	EO	B3 0036+398	10.2	1.83
RX J0039.6+4011	Star	HA94(7297)	4.1	0.47
RX J0039.7+4039	Star	HA94(81094)	11.0	1.25
RX J0040.1+4006	Star	HA94(2646)	15.9	1.17
RX J0040.1+4044	Star	HA94(101871)	12.7	1.47
RX J0040.1+4047	Star	HA94(111215)	7.0	1.40
RX J0040.2+4015	Star	HA94(13652)	2.4	0.48
RX J0040.2+4050	EO	87GB 003730.5+403346	6.0	1.11
RX J0040.3+4043	GC	MA94a(6)	1.1	0.22
RX J0040.4+4050	Star	HA94(119503)	4.2	0.85
RX J0040.4+4129	GC	BA87(51)	20.4	1.76
RX J0040.5+4033	GC	MA94a(16)	3.8	0.24
RX J0040.5+4034	Star	HA94(61478)	4.0	0.56
RX J0040.7+4055	SNR	DO80(7)	11.3	0.64
RX J0040.8+4011	Star (K2V)	SIMBAD( GJ 28)	5.4	1.04
RX J0040.9+4056	Star	HA94(140092)	4.7	0.94
RX J0041.3+4012	EO	87GB 003844.0+395608	4.8	0.26
RX J0041.3+4051	Star	HA94(125532)	3.6	0.71
RX J0041.3+4109	Star	HA94(213303)	56.0	1.86
RX J0041.4+4025	Star	HA94(37411)	14.9	1.63
RX J0041.5+4106	SNR	MA95(3-041),DO80(11)	3.2	0.45
RX J0041.6+4103	Star	HA94(175678)	14.9	1.90
RX J0041.6+4112	Star	HA94(232216)	8.1	1.61
RX J0041.7+4105	Star	HA94(189885)	0.4	0.08
RX J0041.7+4134	GC	BA87(98)	1.6	0.28
RX J0041.8+4021	EO	MRK 0957	11.0	1.93
RX J0041.9+4046	SNR	MA95(2-021)	26.0	1.67
RX J0042.0+4031	Star	HA94(50780)	8.0	0.82
RX J0042.0+4033	Star	HA94(56227)	17.3	1.78
RX J0042.0+4041	Star (F5)	SIMBAD( HD 3914)	5.5	1.05
RX J0042.0+4102	GC	MA94a(130)	9.0	1.76
RX J0042.1+4016	Star	HA94(16045)	10.1	1.10
RX J0042.2+4101	GC	BA87(138),MA94a(159)	2.0	0.40
RX J0042.2+4105	Star	HA94(196074)	4.1	0.81
RX J0042.2+4118	Star	HA94(266451)	6.4	1.29
RX J0042.3+4113	GC	BA87(142),MA94a(164)	7.3	1.43
RX J0042.3+4126	Star	HA94(302803)	10.5	1.21
RX J0042.3+4129	EO	87GB 003934.6+411250	11.9	1.55
RX J0042.4+4055	Star	HA94(136397)	8.7	1.74
RX J0042.4+4057	GC	BA87(153),MA94a(173)	6.2	1.22
RX J0042.4+4108	Star	HA94(208922)	10.7	1.37
RX J0042.4+4129	Star	HA94(316946)	2.4	0.32
RX J0042.5+4103	GC	BA87(171),MA94a(196)	2.7	0.53
RX J0042.5+4119	GC	BA87(168),BA93(1),MA94a(192)	4.6	0.91
RX J0042.5+4132	GC	BA87(176),MA94a(205)	2.5	0.39
RX J0042.6+4052	EO	NGC 0221 = M 32	9.7	1.90
RX J0042.6+4115	GC	BA93(21)	7.0	1.38
RX J0042.8+4125	SNR	DO80(13)	20.4	1.15
RX J0042.8+4131	GC	BA87(196),MA94a(225)	1.6	0.31
RX J0042.9+4119	GC	BA87(203)	7.2	1.42
RX J0042.9+4125	SNR	DO80(13)	14.4	0.79
RX J0043.0+4110	Star	HA94(223193)	3.5	0.70
RX J0043.0+4115	GC	BA87(206)	3.0	0.60

 

Table 8: continued.

ROSAT	Obj.-Cl.	Identification	Distance
No.			('')	$(\sigma)$
RX J0043.0+4117	GC	BA87(208)	6.1	1.20
RX J0043.0+4121	GC	BA87(207),MA94a(240)	4.3	0.84
RX J0043.0+4130	GC	MA94a(236)	4.1	0.80
RX J0043.1+4114	GC	BA87(214),MA94a(251)	3.0	0.60
RX J0043.2+4107	GC	BA87(220),MA94a(257)	5.5	1.08
RX J0043.2+4112	GC	BA87(226),MA94a(269)	11.5	0.94
RX J0043.2+4127	GC	BA87(225),MA94a(266)	6.0	1.02
RX J0043.3+4114	Star	HA94(239273)	16.0	1.53
RX J0043.4+4118	SNR	MA95(2-032),DO80(15)	14.2	1.63
RX J0043.5+4116	Star	HA94(254312)	1.1	0.09
RX J0043.6+4054	EO	B3 0040+406	11.5	1.31
RX J0043.6+4114	GC	BA87(246),MA94a(299)	7.1	1.18
RX J0043.6+4126	SNR	MA95(3-059),DO80(16)	9.2	1.02
RX J0043.6+4138	Star	HA94(375268)	8.3	1.65
RX J0043.7+4128	GC	MA94a(311)	2.1	0.26
RX J0043.7+4136	GC	MA94a(314)	4.2	0.83
RX J0043.8+4106	Star	HA94(196928)	16.2	1.78
RX J0043.8+4111	SNR	BW93(230A)	10.7	0.85
RX J0043.8+4127	GC	MA94a(317)	39.9	0.83
RX J0043.9+4113	SNR	MA95(2-038),DO80(18),BW93(252)	24.7	1.78
RX J0043.9+4122	GC	BA87(267),MA94a(334)	3.0	0.58
RX J0043.9+4127	Star	HA94(307124)	7.6	1.53
RX J0043.9+4152	SNR	MA95(2-037),DO80(17)	11.7	1.06
RX J0043.9+4157	EO	87GB 004113.4+414049	7.4	0.87
RX J0044.0+4149	SNR	MA95(3-072)	19.5	1.51
RX J0044.2+4119	SNR	MA95(3-079),BW93(327)	9.1	1.28
RX J0044.2+4126	Star	HA94(302441)	7.5	0.75
RX J0044.4+4121	GC	MA94a(387)	1.9	0.36
RX J0044.4+4136	GC	MA94a(380)	5.8	1.14
RX J0044.6+4125	SNR	MA95(3-086),BW93(490A)	4.9	0.58
RX J0044.8+4129	SNR	MA95(B-012),BW93(566)	8.4	1.19
RX J0044.8+4229	Star (G5)	SIMBAD( HD4194)	6.6	0.56
RX J0045.1+4202	Star	HA94(441416)	6.4	1.28
RX J0045.2+4136	SNR	MA95(2-048),BW93(717),DO80(19)	11.9	1.23
RX J0045.2+4217	Star	HA94(466304)	14.8	1.48
RX J0045.4+4132	GC	MA94a(447)	15.5	1.85
RX J0045.4+4146	SNR	MA95(1-013)	17.3	1.54
RX J0045.5+4210	Star	HA94(456238)	7.8	1.48
RX J0045.7+4139	GC	BA87(318),MA94a(468)	5.8	1.08
RX J0045.9+4156	Star	HA94(431022)	6.1	1.21
RX J0045.9+4203	Star	HA94(442137)	8.5	1.10
RX J0045.9+4226	Star	HA94(479836)	8.1	1.61
RX J0046.0+4136	Star	HA94(364424)	20.4	1.78
RX J0046.2+4154	Star	HA94(425498)	6.3	1.26
RX J0046.4+4201	GC	BA87(329),MA94a(487)	3.0	0.53
RX J0046.6+4225	Star	HA94(478682)	3.8	0.76
RX J0046.7+4208	EO	87GB 004359.8+415217	6.1	1.20
RX J0046.7+4230	Star	HA94(483376)	18.9	1.86
RX J0047.0+4157	Star (F)	SIMBAD( HD4444)	1.9	0.22
RX J0047.0+4201	Star	HA94(440331)	9.8	0.66
RX J0047.2+4202	Star	HA94(441062)	14.5	1.92
RX J0047.4+4220	Star	HA94(472654)	7.7	1.54
RX J0047.4+4221	Star	HA94(474007)	5.6	1.12
RX J0047.7+4201	Star	HA94(439698)	12.8	1.46
RX J0048.4+4157	Star (F8)	SIMBAD( SAO 36677)	7.4	1.14

Acknowledgements

We thank the MPE ROSAT group for their support. Parts of our analysis used the SASS and EXSAS data analysis software. The authors would like to thank the referee for carefully reading this paper and making useful comments and suggestions. We thank NASA and the Centre de Données astronomiques for the online access to their data bases. WHGL is grateful for support from NASA.

RS remembers J. v. Paradijs as an always gentle and helpful excellent scientist who sadly passed away well ahead of his time - a great loss for the astronomical community.

The ROSAT project has been supported by the Bundesministerium für Bildung und Forschung (BMBF/DLR) and the Max-Planck-Gesellschaft (MPG).