def get_state(system):
# The table of TPM states is here
# http://phn.github.com/pytpm/conversions.html#function-convert-convertv6
# We set the epoch and equinox to get consistent results with
# astrolib.coords.Position, see Position._set_tpmstate there.
d = dict()
d['fk5'] = dict(state=tpm.TPM_S06, epoch=tpm.J2000, equinox=tpm.J2000)
d['fk4'] = dict(state=tpm.TPM_S05, epoch=tpm.B1950, equinox=tpm.B1950)
d['galactic'] = dict(state=tpm.TPM_S04, epoch=tpm.J2000, equinox=tpm.byear2jd(1958))
d['ecliptic'] = dict(state=tpm.TPM_S03, epoch=tpm.J2000, equinox=tpm.jyear2jd(1984))
# d['icrs'] = TPM_S06
return d[system]
def get_state(system):
# The table of TPM states is here
# http://phn.github.com/pytpm/conversions.html#function-convert-convertv6
# We set the epoch and equinox to get consistent results with
# astrolib.coords.Position, see Position._set_tpmstate there.
d = dict()
d['fk5'] = dict(state=tpm.TPM_S06, epoch=tpm.J2000, equinox=tpm.J2000)
d['fk4'] = dict(state=tpm.TPM_S05, epoch=tpm.B1950, equinox=tpm.B1950)
d['galactic'] = dict(state=tpm.TPM_S04,
epoch=tpm.J2000,
equinox=tpm.byear2jd(1958))
d['ecliptic'] = dict(state=tpm.TPM_S03,
epoch=tpm.J2000,
equinox=tpm.jyear2jd(1984))
# d['icrs'] = TPM_S06
return d[system]
def testByear2jd(self):
"""tpm.byear2jd() => convert Besselian year into Julian date."""
self.assertAlmostEqual(tpm.byear2jd(1950.0), tpm.B1950)
def testByear2jd(self):
"""tpm.byear2jd() => convert Besselian year into Julian date."""
self.assertAlmostEqual(tpm.byear2jd(1950.0), tpm.B1950)
