Disentangling multiple high-energy emission components in the Vela X pulsar wind nebula with the Fermi Large Area Telescope

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Table A.1

Coordinates of candidate sources outside Vela X found during the morphological analysis in Sect. 2.2.

Name	RA	Dec	TS
PS J0821.5−4658	125.40 ± 0.07	− 46.98 ± 0.09	17.2
PS J0823.3−4247	125.83 ± 0.08	− 42.79 ± 0.07	34.0
PS J0839.5−4343	129.88 ± 0.16	− 43.73 ± 0.13	13.4
PS J0842.7−4443^a	130.69 ± 0.09	− 44.73 ± 0.09	11.6
PS J0847.7−4559	131.95 ± 0.08	− 45.99 ± 0.08	15.2

PS J0823.6−4328	125.92 ± 0.09	− 43.48 ± 0.07	11.5

Notes. Theupper section refers to the analysis in the LE range, the lower section to the HE range. ^(a) Source included also in the full-energy range analysis.

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