An updated catalog of sources is shown in
Table 1 and is
plotted in Figure 1. The criterion for inclusion
in this catalog is
that the detection should be significant and be published in the
refereed literature. Four sources have been added since the last catalog
(6).
Of more significance perhaps is that three
new classes of object are represented (starburst galaxies, radio
galaxies, OB Associations). It is noteworthy that many of the sources
listed are not in the EGRET Catalog
(7),
an indication that the TeV sky opens a new window on the universe. The
allotted
grade gives some measure of the credibility that should be assigned to
the reported detections; "A" sources have been independently
verified at the 5
level. On this scale the EGRET sources
would be classified as "B" (except for 3C273 which would be
classified as "A" since it was also detected by COS B
(8);
(9)).
In this new catalog the
status of several of the TeV sources (marked with an asterisk) has
been upgraded (and only one has been downgraded). This suggests that
the field has achieved a degree of maturity and that systematic
effects in most experiments (but perhaps not all) are understood and
accounted for. We propose therefore that an acceptable standard for
the publication of a claim for the detection of a new source by a
mature experiment should be the
4
level of significance.
TeV Catalog | Source | Type | Discovery | EGRET | Grade |
Name | Date/Group | 3rd. Cat. | |||
TeV 0047-2518 | NGC 253 | Starburst | 2003/CANG. | no | B* |
TeV 0219+4248 | 3C66A | Blazar | 1998/Crimea | yes | C- |
TeV 0535+2200 | Crab Nebula | SNR | 1989/Whipple | yes | A |
TeV 0834-4500 | Vela | SNR | 1997/CANG. | no | C* |
TeV 1121-6037 | Cen X-3 | Binary | 1999/Durham | yes | C |
TeV 1104+3813 | Mrk421 | Blazar | 1992/Whipple | yes | A |
TeV 1231+1224 | M87 | Radio Gal. | 2003/HEGRA | no | C |
TeV 1429+4240 | H1426+428 | Blazar | 2002/Whipple | no | A* |
TeV 1503-4157 | SN1006 | SNR | 1997/CANG. | no | B* |
TeV 1654+3946 | Mrk501 | Blazar | 1995/Whipple | no | A |
TeV 1710-4429 | PSR 1706-44 | SNR | 1995/CANG. | no | A |
TeV 1712-3932 | RXJ1713.7-39 | SNR | 1999/CANG. | no | B+* |
TeV 2000+6509 | 1ES1959+650 | Blazar | 1999/TA | no | A* |
TeV 2032+4131 | CygOB2 | OB assoc. | 2002/HEGRA | yes† | B |
TeV 2159-3014 | PKS2155-304 | Blazar | 1999/Durham | yes | A* |
TeV 2203+4217 | BL Lacertae | Blazar | 2001/Crimea | yes | C* |
TeV 2323+5849 | Cas A | SNR | 1999/HEGRA | no | B* |
TeV 2347+5142 | 1ES2344+514 | Blazar | 1997/Whipple | no | A* |
† CygOB2 lies within the 95% error ellipse of the EGRET source 3EG J0233+4118. |
![]() |
Figure 1. The 18 claimed sources of TeV gamma rays c. 2003; confirmed sources are drawn in red. |