Pulsar monitor undergoing overnight checkout
The pulsar antenna is now plugged into the pulsar receiver system, which consists of a pair of AirSpy SDR receivers, fed with a high-quality 10MHz OCXO timebase.
We’re running a pulsar-specific flow-graph, written by Marcus Leech, and using Gnu Radio underneath.
There are many unknowns–we don’t know if the ambient noise level is low enough without aggressive filtering, we don’t know if our antenna effective aperture is quite up to the task. This will be a useful test, but a negative result cannot be interpreted to mean “won’t work”.
Can we simulate a pulsar somehow, so we know the cables are plugged in?
In the flow-graph, Does the folding technique applied directly?
Congratulations on the new start!