Presto OutputEven if many interferences the pulsar signal is allmost continueus in time and frequency domains
|
Date of Observation |
Thursday, May 21, 2017 |
|
Length of Observation |
2 Hours |
|
Center Frequency |
1290 MHz |
|
Bandwidth |
10 MHz |
|
Pulsar Flux at 1400MHz |
84 mJy |
|
Distance |
848 light years |
|
Pulsar Period |
253 msec |
|
Age |
175.000.000 Years |
Presto Output
Same pulsar received using the B200 System
In a much more difficult RFI environment a much better pulsar definition thanks to the wider bandwidth and higher number of channels(see B200_System paragraph)
The presto output shows how about 60 (out of 200) channels were removed and still a lot of remaining RFI.
|
Date of Observation |
Moday, March 21, 2018 |
|
Useful Length of Observation |
1 Hour |
|
Center Frequency |
1296 MHz |
|
Bandwidth |
50 MHz |
|
Pulsar Flux at 1400MHz |
84 mJy |
|
Distance |
848 light years |
|
Pulsar Period |
253 msec |
|
Age |
175.000.000 Years |
