Pulsar Basics
Pulsar Basics
Build intuition for archive data, DM, dedispersion, TOA extraction, RFI, and calibration.
This section is not a full astrophysics textbook. It exists to give PSRUI users the minimum conceptual model needed to interpret what the GUI is showing.
Start with:
Why this matters
The GUI makes workflows easier to inspect, but it does not remove the underlying terminology.
If you do not know:
- why DM affects alignment across frequency
- why folding accumulates a periodic signal
- why TOA extraction needs a template
- why calibration changes polarization-related views
then you may still click through the workflow without understanding the result.
Where to go next
- Stay with Handbook of Pulsar Astronomy if you want a fuller English path through observing, searching, timing, and instrumentation.
- Switch to Pulsar Physics if you also read Chinese and want a chapter-by-chapter physics guide built around discovery, timing properties, emission, and evolution.