Not an easy one to detect ,
Flux is in the low range and the pulse is wide (W50 > 50msec), at the base is more than 100 msec long as can be easily seen from the profile.
Te power is therefore distributed on a large area lowering the peaks.
|
Date of Observation |
Monday, August 14, 2017 |
|
Length of Observation |
2 Hours |
|
Center Frequency |
1288 MHz |
|
Bandwidth |
10 MHz |
|
Pulsar Flux at 1400MHz |
10 mJy |
|
Distance |
1402 light years |
|
Pulsar Period |
1292 msec |
|
Age |
122000000 Years |
