pint.pulsar_ecliptic

Functions

icrs_to_pulsarecliptic(from_coo, to_frame)
load_obliquity_file(filename)
pulsarecliptic_to_icrs(from_coo, to_frame)
pulsarecliptic_to_pulsarecliptic(from_coo, ...)

Classes

PulsarEcliptic(*args, **kwargs)

A Pulsar Ecliptic coordinate system is defined by rotating ICRS coordinate about x-axis by obliquity angle.