Table 5:
Results of the analysis of unpulsed
-ray emission for each pulsar
data set using the standard cuts and assuming a point source at the
pulsar position. Dead-time corrected observation time,
,
mean offset of the pulsar direction with respect to the array pointing
direction,
,
approximate mean energy
threshold,
,
number of excess counts,
,
and corresponding significance, S, are given. In
addition to the mean threshold for the standard cuts, the
corresponding threshold for the low energy cuts is given in
parentheses if applicable. If the pulsar is in the vicinity (angular distance <1
)
of,
or associated with, a known VHE
-ray source, the source name is
given along with the corresponding reference. Note that the given
numbers can significantly differ from the published results for the
known sources which are located at different positions and might be
extended. References: A: Aharonian et al. (2006c), B: Aharonian et al. (2006b), C:
Aharonian et al. (2005), D: Aharonian et al. (2006a), E: Aharonian et al. (2005b), F: Aharonian et al. (2005d),
G: Aharonian et al. (2006d), H: Aharonian et al. (2005a).
Pulsar |
 |
 |
 |
 |
S |
HESS |
Reference |
PSR |
[h] |
[ ] |
[GeV] |
|
![$[\sigma]$](/articles/aa/full/2007/17/aa6737-06/img78.gif) |
catalogue
source |
|
B0531+21 |
25.4 |
0.6 |
510 (310) |
 |
164.8 |
Crab Nebula |
(A) |
B0833-45 |
16.3 |
0.6 |
250 (170) |
 |
2.81 |
HESS J0835-456 |
(B) |
B1259-63 |
55.8 |
0.6 |
380 (280) |
 |
16.7 |
HESS J1303-638 |
(C) |
J1420-6048 |
13.0 |
0.8 |
350 (240) |
 |
12.07 |
HESS J1420-607 |
(D) |
B1509-58 |
35.8 |
0.6 |
310 (210) |
 |
32.22 |
HESS J1514-591 |
(E) |
J1524-5625 |
15.5 |
1.0 |
330 (220) |
 |
-0.30 |
- |
|
B1706-44 |
16.6 |
0.5 |
255 |
 |
0.3 |
- |
(F) |
J1747-2958 |
103.3 |
1.1 |
200 (140) |
291 82 |
3.62 |
HESS J1745-303 |
(G) |
J1801-2451 |
9.8 |
1.2 |
180 (130) |
 |
-0.71 |
- |
|
J1811-1925 |
14.2 |
1.1 |
210 (150) |
 |
3.8  |
- |
|
J1826-1334 |
62.8 |
1.1 |
210 (140) |
 |
11.2 |
HESS J1825-137 |
(H) |
Comprises 14.4 h of 2-telescope data and 2.2 h of data from the full 4-telescope array.

See text.
|
Source LaTeX |
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