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Parkes High-Latitude Single Pulse Survey
Tape 
Pulsar 
File

DM(cm^-3 pc)

RAJ (hms)
DECJ (dms)
RAJ* (hms)
DECJ* (dms)
DM*(cm^-3 pc)
Period (s)
1
  
Done
              
2
J0846-3533
0954*
97
08:45:59
-35:38:07
08:46:06
-35:33:40
94
1.12
 
J0818-3232
0502*
138
08:18:19
-32:34:38
08:18:25
-32:32:30
131
2.16
 
J0828-3417
0532*
62.3
08:28:31
-34:13.03
08:28:16.6
-34:17:07
52.9
1.85
3
J0729-1836
0321*
61
07:29:19
-18:38:50
07:29:32
-18:36:42
61
0.510
5
  
DONE
             
6
J0828-3417
0048*
51
08:27:20
-34:13:09
08:28:16
-34:17:07
52
1.85
 
J0837-4135
013A*
145
08:36:16
-41:23:59
08:37:21
-41:35:15
147
0.751
 
J0729-1836
0171*
60
07:29:49
-18:26:52
07:29:32
-18:36:47
60
0.510
8
  
DONE
              
9
J0922+0638
020D*
35
09:22:04
+06:31:54
09:22:14
+06:38:23
27
0.431
10
  
001D
20.90
03:13:59
-28:25:23
        
 
J1022+1001
053A*
10.1
10:23:10
+09:59:48
10:22:58
+10:01:52
10
0.0165
11
  
DONE
              
12
 
0942
22.10
03:29:47
-33:13:42
        
 
J0437-4715
2.6
04:36:35
-47:22:41
04:37:15
-47:15:08
2.64
0.00576
   
076A
24.90
04:15:45
-49:44:22
        
13
  
0334
22.50
03:09:00
-44:28:01
        
 
J0437-4715
2.6
04:36:42
-47:08:44
04:37:15
-47:15:08
2.64
0.00576
   
0256
32.60
03:59:06
-40:42:20
        
   
012A
18.10
03:52:31
-38:50:17
        
14
J0828-3417
0372*
63
08:28:03
-34:25:46
08:28:16
-34:17:07
52
1.85
   
0919
8.7
09:02:49
-13:32:31
        
15
J0726-2612
0384*
68
07:25:53
-26:06:52
07:26:.08
-26:12:38
69
3.44
16
J0656-2228
0317*
37.40
06:56:59
-22:28:07
06:56:30
-22:28:25
32
1.22
17
  
DONE
              
18
J0437-4715
0244*
2.6
04:36:35
-47:22:41
04:37:15
-47:15:08
2.64
0.00576
19
  
DONE
              
20
  
DONE
              
21
  
DONE
              
22
J0738-4042
0272*
161.4
07:39:54
-40:36:18
07:38:32
-40:42:40
160.8
0.375
23
  
DONE
              
24
J0630-2834
033C*
35.80
06:30:18
-28:26:00
06:30:49
-28:34:43.1
34
1.24
 
J0630-2834
0325*
35.00
06:31:26
-28:28:32
06:30:49
-28:34:43.1
34
1.24
25
  
073D
22.1
08:40:07
-28:23:49
        
27
J0820-1350
0187*
41.4
08:19:53
-13:45:58
08:20:26
-13:50:55
40.94
1.24
29
J0820-1350
0171*
40.6
08:20:27
-13:58:41
08:20:26
-13:50:55
40.94
1.24
30
  
DONE
              
31
  
DONE
              
32
  
DONE
              
33
J0823+0159
063D*
35
08:23:08
+02:00:49
08:23:09
+01:59:12
23.73
0.865
34
  
DONE
              
35
  
DONE
              
36
NEW!
038C
35
04:18:19
-41:55:03
        
37
 J0953+0755
0171*
2.9
09:52:50
+07:57:59
09:53:09
+07:55:35
2.96
0253
  J0953+0755
2.9
09:52:53
+07:33:00
09:53:09
+07:55:35
2.96
0253
  J0953+0755
2.9
09:53:23
+07:45:26
09:53:09
+07:55:35
2.96
0253
  J0953+0755
0191*
3.2
09:53:48
+07:59:02
09:53:09
+07:55:35
2.96
0253
38
  
DONE
              
39
J0633-2015
0204*
93.7
06:33:23
-20:14:36
06:33:08
-20:15;07
92
3.25
40
J0742-2822
0386*
72.8
07:43:02
-28:23:30
07:42:49
-28:22;43
73.78
0.167
 
J0742-2822
0391*
72.8
07:41:53
-28:23:23
07:42:49
-28:22;43
73.78
0.167
 
J0437-4715
0734*
2.6
04:37:51
-47:14:38
04:37:15
-47:15:08
2.64
0.00576
   
0104
35
05:05:01
-35:35:35
        
41
J0738-4042
0098
137.2
07:39:12
-40:49:14
07:38:32
-40:42:40
160.8
0.375
42
J0908-1739
0379*
16.9
09:09:03
-17:35:42
09:08:38
-17:39:37
15.89
0.402
43
J0726-2612
0107*
71.2
07:26:22
-26:19:13
07:26:08
-26:12:38
69.4
3.44
44
  
DONE
              
46
J0630-28341
060C
35
06:31:03
-28:28:47
06:30:49
-28:34:43
34.47
1.24
47
  
DONE
              
48
J0738-4042
020A
137.2
07:44:35
-39:11:04
07:38:32
-40:42:40
160.8
0.375
51
BEST!
0585
114.5
07:55:29
-44:28:15
        
 
137.2
07:45:10
-39:23:15
        
52
  
0455
33.4
06:34:07
-35:55:24
        
 
BEST!
0313
42.5
05:57:09
-15:20:08
        
53
  
086C
48.7
4:10:53
-49:15:22
        
54
  
33
07:34:48
-08:05:54
        
56
  
DONE
              
57
  
DONE
              
59
  
DONE
              
62
  
DONE
              
63
  
DONE
              
64
  
DONE
              
65
  
DONE
              
66
J0855-3331
0633*
85.70
08:55:38
-33:33:51
08:55:38
-33:31:39
86
1.27
 
J0758-1528
0621*
63.10
07:58:06
-15:36:42
07:58:29
-15:28:08
63.33
0.682
67
J0922+0638
096C*
26.90
09:22:30
+06:45:28
09:22:14
+06:38:23
27
0.431
   
042D
28
06:55:13
-18:47:35
68
J1046+0304
070C*
23.3
10:47:04
+03:02:36
10:46:43
+03:04:06
25.3
0.326
69
  
1369
34.6
06:25:53
-23:26:52
        
   
0482
27.3
03:44:28
-34:17:12
        
70
J0835-3707
1088*
113.1
08:35:05
-37:07:13
08:35:03
-37:07:51
112.3
0.541
71
  
DONE
              
72
  
58.3
06:51:33
-47:25:35
        
73
  
DONE
              
75
J0630-2834
35.0
06:31:26
-28:28:32
06:30:49
-28:34:43
34.47
1.244
76
  
DONE
              
77
J0738-4042
005C*
137.20
07:39:06
-40:37:17
07:38:32
-40:42:40
160
0.375
78
  
DONE
              
79
  
DONE
              
80
  
DONE
              
82
  
DONE
              
83
  
DONE
              
84
  
DONE
              
85
  
DONE
              
86
  
DONE
              
87
  
DONE
              
                   

Last update: Sept 27, 2007

Pulsars with strong pulses detected, possible RRAT candidates.

Candidates that contain strong or more than one pulse.

New Pulsar - 0.75s period

*Already known pulsar being detected during the survey, values taken from the online pulsar catalog at http://www.atnf.csiro.au/research/pulsar/psrcat/

Please email George Habib with questions about this page

The Parkes High-Latitude (PH) Pulsar Survey covers the region enclosed by Galactic longitude 220° < l < 260° and Galactic latitude |b| < 60°, for a total of 6456 pointings of 265 s duration each. The observations, started in November 2000 and completed in December 2003, were made using the multibeam receiver on the Parkes 64-m radio telescope operating at a central frequency of 1347 MHz and consisting of 13 separate beams. The total 288 MHz bandwidth was subdivided into 96 X 3 MHz channels in order to minimize the pulse broadening due to dispersion in the interstellar medium. The signal was one-bit sampled every 125 μs and recorded on Digital Linear Tapes for off-line analysis.

This page contains the results from the Parkes High Latitude survey concerning the single pulse search. The best pulsar plots with the most RRAT-like emission are posted in red. The table below shows the information for the pulsars that are redetected as well the candidates. The information for the redetected pulsars is taken from the ATNF pulsar database and is noted by a star. The columns start with the tape number on which the data were stored followed by the pulsar name, if it is a redetected pulsar, then the file name from the tape. The DM, RAJ and DECJ values from the survey are posted followed by the real values and the period of the pulsar. The single pulse search helps in finding more RRAT type pulsars. Gathering more data about these amazing and mysterious object will help us to better understand how they work and the reasons that make them produce such sporadic emission.

A list of all known pulsars that were detected in the PH survey was created and compared to the detected pulsar in the single-pulse survey, click here to see the list.

crab

The Crab Nebula (catalogue designations M 1, NGC 1952, Taurus A) is a supernova remnant in the constellation of Taurus. The nebula was first observed in 1731 by John Bevis. It is the remnant of a supernova that was recorded, as a star visible in daylight, by Chinese and Arab astronomers in 1054.

VelaThe Vela Pulsar is a radio, optical, X-ray and gamma-emitting pulsar associated with Vela Supernova Remnant, in the constellation of Vela. The association of the Vela pulsar with the Vela Supernova Remnant, made by astronomers at the University of Sydney in 1968,was direct observational proof that supernovae form neutron stars