Table 1:

0FGL sources and LAT pulsars with spatially coincident VHE counterpart.

LAT source	Associationa	Classb	l	b	Errorc	VHE -ray source	Associationd	l	b	Extensione	References
			( )	( )	( )			( )	( )	( )
0FGL J0534.6+2201	Crab	PSR	184.56	-5.76	0.05	HESS J0534+220	Crab nebula	184.56	-5.78	PS	1
0FGL J0835.4-4510	Vela	PSR	263.56	-2.77	0.04	HESS J0835-455	Vela X	263.86	-3.09	0.43	2
0FGL J1418.8-6058		PSR	313.34	0.11	0.07	HESS J1418-609	G313.3+0.1 (Rabbit)	313.25	0.15	0.06	3
PSR J1420-6048		PSR	313.5	0.2	PS	HESS J1420-607	PSR J1420-6048	313.56	0.27	0.07	3
0FGL J1709.7-4428	PSR B1706-44	PSR	343.11	-2.68	0.05	HESS J1708-443f	PSR B1706-44?	343.04	-2.38	0.29	4
PSR J1718-3825		PSR	349.0	-0.4	PS	HESS J1718-385		348.83	-0.49	0.015	5
0FGL J1907.5+0602		PSR	40.14	-0.82	0.08	HESS J1908+063		40.39	-0.79	0.34	6
0FGL J2032.2+4122		PSR	80.16	0.98	0.09	TeV J2032+4130		80.23	1.10	0.10	7
0FGL J0617.4+2234		SNR/PWN	189.08	3.07	0.06	VER J0616.9+2230	IC 443	189.08	2.92	0.16	8
0FGL J1615.6-5049		SNR/PWN	332.35	-0.01	0.23	HESS J1616-508	PSR J1617-5055?	332.39	-0.14	0.14	9
0FGL J1648.1-4606		SNR/PWN	339.47	-0.71	0.18	Westerlund 1 regionf,g		339.55	-0.40	0.9h	10
0FGL J1714.7-3827		SNR/PWN	348.53	0.1	0.13	HESS J1714-385	CTB 37A	348.39	0.11	0.07	11
0FGL J1801.6-2327		SNR/PWN	6.54	-0.31	0.11	HESS J1801-233	W 28	6.66	-0.27	0.17	12
0FGL J1834.4-0841		SNR/PWN	23.27	-0.22	0.1	HESS J1834-087	W 41	23.24	-0.32	0.09	9
0FGL J1923.0+1411	W 51Ci	SNR	49.13	-0.4	0.08	HESS J1923+141f	W 51	49.14	-0.6	0.15j	13
0FGL J1024.0-5754		Unid	284.35	-0.45	0.11	HESS J1023-575	Westerlund 2?	284.19	-0.39	0.18	14
0FGL J1805.3-2138		Unid	8.54	-0.17	0.19	HESS J1804-216	W 30/PSR J1803-2137?	8.40	-0.03	0.20	9
0FGL J1839.0-0549		Unid	26.34	0.08	0.12	HESS J1841-055		26.8	-0.2	0.42	15
0FGL J1844.1-0335		Unid	28.91	-0.02	0.15	HESS J1843-033f		29.08	0.16	0.2j	16
0FGL J1848.6-0138		Unid	31.15	-0.12	0.16	HESS J1848-018f		30.98	-0.16	0.32	17
0FGL J0240.3+6113	LS I +61 303	HMXB	135.66	1.08	0.07	VER J0240+612	LS I +61 303	135.70	1.08	PS	18
0FGL J1826.3-1451	LS 5039	HMXB	16.89	-1.32	0.11	HESS J1826-148	LS 5039	16.90	-1.28	PS	19

Notes.  ^(a) Based on timing information. ^(b) Source class according to Abdo et al. (2009a). PSR: pulsar; SNR/PWN: supernova remnant/PWN; HMXB: high-mass X-ray binary; Unid: unidentified sources. The classification of those sources as SNR/PWN is based on spatial coincidence only. ^(c) 95% positional error. ^(d) Based on spatial coincidence only. ^(e) An entry of ``PS'' indicates that the source is point-like with respect to the point spread function of the respective instrument. ^(f) These recent source discoveries are preliminary and they have been published in the referenced conference proceedings only. ^(g) The VHE emission has been detected by HESS towards the direction of the massive stellar cluster. The coordinates refer to the nominal position of Westerlund 1. ^(h) The extent of the source is not clear. The given value is estimated from the radial profile shown in Fig. 4 of the corresponding reference. ⁽ⁱ⁾ The association is based on a morphological study (Abdo et al. 2009e). ^(j) The extent of the source is not clear. The given value is estimated from the sky excess map in the corresponding reference.

References.  (1) Aharonian et al. (2006d); (2) Aharonian et al. (2006b); (3) Aharonian et al. (2006g); (4) Hoppe et al. (2009); (5) Aharonian et al. (2007b); (6) Aharonian et al. (2009); (7) Aharonian et al. (2005b); (8) Acciari et al. (2009b); (9) Aharonian et al. (2006f); (10) Ohm et al. (2009); (11) Aharonian et al. (2008b); (12) Aharonian et al. (2008c); (13) Fiasson et al. (2009); (14) Aharonian et al. (2007a); (15) Aharonian et al. (2008d); (16) Hoppe et al. (2008); (17) Chaves et al. (2009b); (18) Acciari et al. (2009a); (19) Aharonian et al. (2006e).