A search for thermally emitting isolated neutron stars in the 2XMMp catalogue

Free Access

Table 4:

Results of follow-up investigations.
Candidate	r	R	U-B	B-R	LR	$P_{\rm {chance}}$	e	$\log(f_{\rm {X}}/f_{R})$ ^a
	(arcsec)					(%)
XMM J1210	1.55	20.13(3)	?	1.35(3)	8.4	2.8	0.037	0.18
XMM J0106	2.75	24.51(9)	?	$\ga$ 2.0	1.2	22.4	0.178	1.93
	1.68	24.58(9)	?	$\ga$ 1.9	1.2	22.4	0.162	1.96
XMM J0435	1.20	22.15(4)	-0.51(8)	0.93(7)	15.2	2.3	0.068	0.77
XMM J0314	0.67	21.37(3)	-0.13(7)	1.43(4)	32.1	1.7	0.022	0.41
XMM J2140	1.26	23.78(9)	-1.08(16)	1.06(15)	6.0	6.4	0.156	1.40
XMM J1259	1.34	21.64(4)	-1.08(4)	0.76(5)	25.5	1.0	0.098	0.61
XMM J1250	1.80	22.19(4)	-0.71(4)	0.74(4)	8.4	4.1	0.029	0.57

^a The X-ray flux is computed in the 0.15-3 keV energy band assuming an absorbed power-law model.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.