Probabilistic classification of X-ray sources applied to Swift-XRT and XMM-Newton catalogs

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Volume 657 (January 2022)

A&A, 657 (2022) A138

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Table 7.

Classification of some 4XMM-DR10 sources from the test sample.

IAUNAME	Err_1σ	Flux	det	Q	b	pm	L_X	FxFw1	dIR	HR1	HR2	Fratio	P_AGN	P_Star	P_XRB	P_CV	cl	alt	O.M.
⁽¹⁾	⁽²⁾	⁽³⁾	⁽⁴⁾	⁽⁵⁾	⁽⁶⁾	⁽⁷⁾	⁽⁸⁾	⁽⁹⁾	⁽¹⁰⁾	⁽¹¹⁾	⁽¹²⁾	⁽¹³⁾	⁽¹⁴⁾	⁽¹⁵⁾	⁽¹⁶⁾	⁽¹⁷⁾	⁽¹⁸⁾	⁽¹⁹⁾	⁽²⁰⁾
J004238.9+401630	1.72	1.1e−14	1	2	−22.6	6.99	35.9	−0.46	3.58	−0.04	−0.09	0.0	0.56	0.09	0.24	0.12	AGN	Star XRB	10.86
J053031.7−265616	0.78	1.6e−13	1	3	−28.7	0.13		0.19	0.68	0.11	−0.04	0.0	1.0	0.0	0.0	0.0	AGN		6.48
J074147.6+702203	2.56	9.5e−14	1	2	29.6	0.44		0.82	1.49	−0.73	0.86	0.0	1.0	0.0	0.0	0.0	AGN		7.29
J080142.9+004342	1.71	1.9e−14	1	2	15.9	3.0		−0.14	2.24	0.36	0.47	0.0	0.93	0.0	0.01	0.05	AGN		7.58
J090143.2+355133	0.5	8.5e−14	1	3	41.0	107.89		−3.46	1.25	0.52	−0.57	0.0	0.0	1.0	0.0	0.0	Star		7.46
J104121.8+395616	0.94	1.1e−14	2	2	60.2			−0.17	0.97	0.91	0.54	0.07	0.98	0.0	0.02	0.01	AGN		6.34
J123536.6+123059	1.18	1.3e−14	8	4	74.9		38.59	−0.17	2.89	−0.07	0.51	0.57	0.05	0.0	0.95	0.0	XRB	AGN	8.45
J124649.0−593539	0.81	5.5e−15	1	3	3.3	5.5		−3.56	1.17	0.79	−0.15	0.0	0.0	1.0	0.0	0.0	Star		6.93
J165142.5−385515	2.23	1.4e−14	1	2	3.4	11.76		−2.61	0.74	0.91	−0.12	0.0	0.0	1.0	0.0	0.0	Star		7.18
J174739.0−282139	1.28	1e−14	1	2	−0.1	2.22		−1.35	3.66	−0.01	−0.41	0.0	0.58	0.32	0.04	0.06	AGN	Star	7.75
J182009.4−155744	2.15	2.2e−13	1	2	−0.5			−1.99	3.24	1.0	0.26	0.0	0.39	0.5	0.04	0.07	Star	AGN	7.67
J191357.0−211606	0.65	1.8e−13	1	3	−14.3	0.17		0.13	0.95	0.29	0.1	0.0	1.0	0.0	0.0	0.0	AGN		6.66
J204846.5−095358	1.16	5.1e−15	1	2	−30.5			−0.58	2.49	0.25	−0.08	0.0	0.97	0.01	0.01	0.01	AGN		6.27
J213521.0+312702	3.09	1.5e−13	1	3	−15.1	8.43		1.32	8.39	−0.18	0.59	0.0	0.84	0.01	0.01	0.14	AGN		8.33
J221635.7+000902	1.67	3.5e−14	3	3	−43.9			0.73	4.24	0.59	0.39	0.54	0.93	0.0	0.05	0.02	AGN		6.53

Notes. The full table is available at https://github.com/htranin/classificationXray/raw/main/data/XMM10out.fits and at the CDS. Description: ⁽¹⁾IAUNAME of the source (without prefix “4XMM”). ⁽²⁾1σ XMM position error (arcsec). ⁽³⁾Mean total band flux (0.2–12keV) of all XMM detections of this source. ⁽⁴⁾Number of X-ray detections, including Swift and Chandra. ⁽⁵⁾Number of quality rules followed. ⁽⁶⁾Galactic latitude, in degrees. ⁽⁷⁾Gaia proper motion of the optical counterpart. ⁽⁸⁾Logarithm of the mean X-ray luminosity, computed using the distance of associated GLADE galaxy. ^(9, 10)Hardness ratios between the bands 0.2–0.5 and 0.5–1 keV (resp. 0.5–1 and 1–2 keV) of XMM. ⁽¹¹⁾Logarithm of the X-ray to W1-band flux ratio. ⁽¹²⁾Angular distance (arcsec) to the infrared counterpart. ⁽¹³⁾Logarithm of the maximum to minimum X-ray flux ratio. ^{(14 − 17)}Probabilities of each class. ⁽¹⁸⁾Class giving the highest probability. ⁽¹⁹⁾Alternative classification, if any, when a property category is ignored. ⁽²⁰⁾Outlier measure (Sect. 3.2).

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