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Table 3:

0FGL sources with a possibly coincident VHE $\gamma $-ray source. See Table 1 for the nomenclature.

LAT source
Class l b Error VHE $\gamma $-ray source Association l b Extension References
    ( $\hbox {$^\circ $ }$) ( $\hbox {$^\circ $ }$) ( $\hbox {$^\circ $ }$)     ( $\hbox {$^\circ $ }$) ( $\hbox {$^\circ $ }$) ( $\hbox {$^\circ $ }$)  
0FGL J1814.3-1739 SNR/PWN 13.05 -0.09 0.19 HESS J1813-178 G12.8-0.2/AX J1813-178 12.81 -0.03 0.04 1
0FGL J1634.9-4737 Unid 336.84 -0.03 0.08 HESS J1634-472   337.11 0.22 0.11 1
0FGL J1741.4-3046 Unid 357.96 -0.19 0.2 HESS J1741-302a   358.4 0.01 ? 2
0FGL J1746.0-2900 Unid 359.99 -0.11 0.07 HESS J1745-290 Sgr A*/G359.95-0.04 359.94 -0.04 PS 3
0FGL J1836.1-0727 Unid 24.56 -0.03 0.22 HESS J1837-069   25.18 -0.12 7 $\hbox{$.\mkern-4mu^\prime$ }$2$\times$3 $\hbox{$^\prime$ }$ 1
0FGL J2021.5+4026 PSR 78.23 2.07 0.05 VER J2019+407a $\gamma$ Cygni SNR? 78.33 2.54 0.16$\times$0.11 4
0FGL J2229.0+6114 PSR 106.64 2.96 0.08 VER J2227+608   106.35 2.71 0.27$\times$0.18 5

Notes. (a) These recent source discoveries are preliminary and they have been published in the referenced conference proceedings only.

References. (1) Aharonian et al. (2006f); (2) Tibolla et al. (2009b); (3) Acero et al. (2010); (4) Weinstein et al. (2009); (5) Acciari et al. (2009c).


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