def test_process_and_accuracy(self):
# Checks that instantiating an observatory and phasing of
# topocentric times works. Verifies accuracy to the sub-mus
# level by comparison with stored Tempo2 "Fermi plugin" results.
modelin = pint.models.get_model(parfile)
get_satellite_observatory("Fermi", ft2file)
tl = load_Fermi_TOAs(eventfileraw, weightcolumn="PSRJ0030+0451")
# ts = toa.TOAs(toalist=tl)
ts = toa.get_TOAs_list(tl,
include_gps=False,
include_bipm=False,
planets=False,
ephem="DE405")
iphss, phss = modelin.phase(ts, abs_phase=True)
ph_pint = phss % 1
with fits.open(eventfileraw) as f:
ph_tempo2 = f[1].data.field("pulse_phase")
dphi = ph_pint - ph_tempo2
dphi[dphi < -0.1] += 1
dphi[dphi > 0.1] -= 1
resids_mus = dphi / modelin.F0.value * 1e6
# if the "2 mus" problem exists, the scatter in these values will
# be 4-5 mus, whereas if everything is OK it should be few 100 ns
# require range in TOAs to be less than 200ns
self.assertTrue((resids_mus.max() - resids_mus.min()) < 0.2)
# require absolute phase to be within 500 ns; NB this relies on
# GBT clock corrections since the TZR is referenced there
self.assertTrue(max(abs(resids_mus)) < 0.5)
def get_TZR_toa(self, toas):
"""Get the TOAs class for the TZRMJD.
We are treating the TZRMJD as a special TOA.
Note that any observatory clock corrections will be applied
to this TOA, as with any other TOA. This does not affect the
value of the TZRMJD parmeter, however.
"""
if self.tz_cache is not None:
# This should also verify that the clkc_info is the same so it is valid.
return self.tz_cache
else:
# NOTE: Using TZRMJD.quantity.jd[1,2] so that the time scale can be properly
# set to the TZRSITE default timescale (e.g. UTC for TopoObs and TDB for SSB)
TZR_toa = toa.TOA(
(self.TZRMJD.quantity.jd1 - 2400000.5,
self.TZRMJD.quantity.jd2),
obs=self.TZRSITE.value,
freq=self.TZRFRQ.quantity,
)
clkc_info = toas.clock_corr_info
tz = toa.get_TOAs_list(
[TZR_toa],
include_bipm=clkc_info["include_bipm"],
include_gps=clkc_info["include_gps"],
ephem=toas.ephem,
planets=toas.planets,
)
self.tz_cache = tz
return tz
def test_generate_polycos(tmpdir, par_file, obs, obsfreq, nspan, ncoeff):
output_polyco = tmpdir / "B1855_polyco_round_trip_from_par.dat"
mjd_start, mjd_end = 55000.0, 55001.0
model = get_model(str(par_file))
p = Polycos()
p.generate_polycos(model, mjd_start, mjd_end, obs, nspan, ncoeff, obsfreq)
p.write_polyco_file(output_polyco)
q = Polycos()
q.read_polyco_file(output_polyco)
mjds = np.linspace(mjd_start, mjd_end, 51)
t = toa.get_TOAs_list(
[toa.TOA(mjd, obs=obs, freq=obsfreq) for mjd in mjds],
ephem=model.EPHEM.value)
ph1 = p.eval_abs_phase(mjds)
ph2 = q.eval_abs_phase(mjds)
ph3 = model.phase(t, abs_phase=True)
assert np.allclose(ph1.int.value[0], ph3.int.value[0])
assert np.allclose(ph1.frac.value[0], ph3.frac.value[0])
assert np.allclose(ph2.int.value[0], ph3.int.value[0])
assert np.allclose(ph2.frac.value[0], ph3.frac.value[0])
def __call__(self, time):
"""Create list of TOAs for one or more times.
Parameters
----------
time : `~astropy.time.Time`
Input time stamps.
Returns
-------
toas : `~pint.toa.TOAs`
Combining all TOAs.
"""
# local import since we cannot count on PINT being present,
# and doing it globally messes up sphinx.
from pint import toa
if time.scale == 'utc':
time = time.replicate(format='pulsar_mjd')
freq, _ = np.broadcast_arrays(self.frequency, time.jd1, subok=True)
time = time._apply(np.broadcast_to, freq.shape)
toa_list = []
for t, f in zip(time.ravel(), freq.ravel()):
# This format converting should be done by PINT in the future.
toa_entry = toa.TOA(t, obs=self.observatory, freq=f)
toa_list.append(toa_entry)
toas = toa.get_TOAs_list(toa_list, **self.control_params)
toas.shape = time.shape
return toas
def main(argv=None):
parser = argparse.ArgumentParser(description="PINT tool for command-line barycentering calculations.")
parser.add_argument("time",help="MJD (UTC, by default)")
parser.add_argument("--timescale",default="utc",
help="Time scale for MJD argument ('utc', 'tt', 'tdb'), default=utc")
parser.add_argument("--format",
help="Format for time argument ('mjd' or any astropy.Time format (e.g. 'isot'), see <http://docs.astropy.org/en/stable/time/#time-format>)",
default="mjd")
parser.add_argument("--freq",type=float,default=np.inf,
help="Frequency to use, MHz")
parser.add_argument("--obs",default="Geocenter",
help="Observatory code (default = Geocenter)")
parser.add_argument("--parfile",help="par file to read model from",default=None)
parser.add_argument("--ra",
help="RA to use (e.g. '12h22m33.2s' if not read from par file)")
parser.add_argument("--dec",
help="Decl. to use (e.g. '19d21m44.2s' if not read from par file)")
parser.add_argument("--dm",
help="DM to use (if not read from par file)",type=float,default=0.0)
parser.add_argument("--ephem",default="DE421",help="Ephemeris to use")
parser.add_argument("--use_gps",default=False,action='store_true',help="Apply GPS to UTC clock corrections")
parser.add_argument("--use_bipm",default=False,action='store_true',help="Use TT(BIPM) instead of TT(TAI)")
args = parser.parse_args(argv)
if args.format in ("mjd","jd", "unix"):
# These formats require conversion from string to longdouble first
fmt = args.format
# Never allow format == 'mjd' because it fails when scale is 'utc'
# Change 'mjd' to 'pulsar_mjd' to deal with this.
if fmt == "mjd":
fmt = "pulsar_mjd"
t = Time(np.longdouble(args.time),scale=args.timescale,format=fmt,
precision=9)
print(t)
else:
t = Time(args.time,scale=args.timescale,format=args.format, precision=9)
log.debug(t.iso)
t = toa.TOA(t,freq=args.freq,obs=args.obs)
# Build TOAs and compute TDBs and positions from ephemeris
ts = toa.get_TOAs_list([t],ephem=args.ephem, include_bipm=args.use_bipm,
include_gps=args.use_gps, planets=False)
if args.parfile is not None:
m=pint.models.get_model(args.parfile)
else:
# Construct model by hand
m=pint.models.StandardTimingModel
# Should check if 12:13:14.2 syntax is used and support that as well!
m.RAJ.quantity = Angle(args.ra)
m.DECJ.quantity = Angle(args.dec)
m.DM.quantity = args.dm*u.parsec/u.cm**3
tdbtimes = m.get_barycentric_toas(ts)
print("{0:.16f}".format(tdbtimes[0].value))
return
def get_barycentric_correction(orbfile, parfile, dt=5, ephem='DE421'):
no = SatelliteObs(name="NuSTAR", FPorbname=orbfile, tt2tdb_mode="pint")
with fits.open(orbfile) as hdul:
mjdref = high_precision_keyword_read(hdul[1].header, 'MJDREF')
mjds = np.arange(no.X.x[1], no.X.x[-2], dt / 86400)
mets = (mjds - mjdref) * 86400
obs, scale = 'nustar', "tt"
toalist = [None] * len(mjds)
for i in range(len(mjds)):
# Create TOA list
toalist[i] = toa.TOA(mjds[i], obs=obs, scale=scale)
if parfile is not None and os.path.exists(parfile):
modelin = pint.models.get_model(parfile)
else:
modelin = get_dummy_parfile_for_position(orbfile)
ts = toa.get_TOAs_list(
toalist,
ephem=ephem,
include_bipm=False,
include_gps=False,
planets=False,
tdb_method='default',
)
bats = modelin.get_barycentric_toas(ts)
return interp1d(mets, (bats.value - mjds) * 86400,
assume_sorted=True,
bounds_error=False,
fill_value='extrapolate',
kind='quadratic')
def test_toas_read_list():
x = toa.get_TOAs("test1.tim")
toas, commands = toa.read_toa_file("test1.tim")
y = toa.get_TOAs_list(toas,
commands=commands,
filename=x.filename,
hashes=x.hashes)
assert x == y
def _gen_polyco(self, parfile, MJD_start, segLength = 60.0, ncoeff = 15, \
maxha=12.0, method="TEMPO", numNodes=20, usePINT = True):
"""
This will be a convenience function to generate polycos and subsequent parameters to replace the values in a
PSRFITS file header. The default way to do this will be to use PINT (usePINT = True), with other methods
currently unsupported. The input values are:
parfile [string] : path to par file used to generate the polycos. The observing frequency, and observatory will
come from the par file
MJD_start [float] : Start MJD of the polyco. Should start no later than the beginning of the observation
segLength [float] : Length in minutes of the range covered by the polycos generated. Default is 60 minutes
ncoeff [int] : number of polyco coeffeicients to generate. Default is 15, the same as in the PSRFITS file
maxha [float] : max hour angle needed by PINT. Default is 12.0
method [string] : Method PINT uses to generate the polyco. Currently only TEMPO is supported.
numNodes [int] : Number of nodes PINT will use to fit the polycos. Must be larger than ncoeff
usePINT [bool] : Method used to generate polycos. Currently only PINT is supported.
"""
if usePINT:
# Define dictionary to put parameters into
polyco_dict = {'NSPAN': segLength, 'NCOEF': ncoeff}
# load parfile to PINT model object
m = models.get_model(parfile)
# Determine MJD_end based on segLength
MJD_end = MJD_start + np.double(
make_quant(segLength, 'min').to('day').value) # MJD
# Determine obseratory and observing frequency
obsFreq = m.TZRFRQ.value # in MHz
polyco_dict['REF_FREQ'] = obsFreq
obs = m.TZRSITE.value # string
polyco_dict['NSITE'] = obs.encode(
'utf-8') # observatory code needs to be in binary
# Get pulsar frequency
polyco_dict['REF_F0'] = m.F0.value
# get the polycos
pcs = polycos.Polycos()
pcs.generate_polycos(m, MJD_start, MJD_end, obs, segLength, ncoeff, obsFreq, maxha=12.0, method="TEMPO", \
numNodes=20)
coeffs = pcs.polycoTable['entry'][-1].coeffs
polyco_dict['COEFF'] = coeffs
# Now we need to determine the reference MJD, and phase
REF_MJD = np.double(pcs.polycoTable['tmid'][-1])
polyco_dict['REF_MJD'] = REF_MJD
# Now find the phase difference
tmid_toa = toa.get_TOAs_list(
[toa.TOA(REF_MJD, obs=obs, freq=obsFreq)])
ref_phase = m.phase(tmid_toa)
# Need to force positive value
if ref_phase.frac.value[0] < 0.0:
ref_frac_phase = 1.0 - abs(ref_phase.frac.value[0])
else:
ref_frac_phase = ref_phase.frac.value[0]
polyco_dict['REF_PHS'] = ref_frac_phase
return polyco_dict
else:
print("Only PINT is currently supported for generating polycos")
raise NotImplementedError()
def test_roundtrip_bary_toa_Tempo2format(self):
# Create a barycentric TOA
t1time = Time(58534.0, 0.0928602471130208, format="mjd", scale="tdb")
t1 = toa.TOA(t1time, obs="Barycenter", freq=0.0)
ts = toa.get_TOAs_list([t1], ephem="DE421")
ts.write_TOA_file("testbary.tim", format="Tempo2")
ts2 = toa.get_TOAs("testbary.tim")
print(ts.table, ts2.table)
assert np.abs(ts.table["mjd"][0] - ts2.table["mjd"][0]) < 1.0e-15 * u.d
assert np.abs(ts.table["tdb"][0] - ts2.table["tdb"][0]) < 1.0e-15 * u.d
def test_roundtrip_topo_toa_TEMPOformat(self):
# Create a barycentric TOA
t1time = Time(58534.0, 0.0928602471130208, format="mjd", scale="utc")
t1 = toa.TOA(t1time, obs="gbt", freq=0.0)
ts = toa.get_TOAs_list([t1], ephem="DE421")
ts.write_TOA_file("testtopot1.tim", format="TEMPO")
ts2 = toa.get_TOAs("testtopot1.tim")
print(ts.table, ts2.table)
assert ts.table["mjd"][0] - ts2.table["mjd"][0] < 1.0e-15
assert ts.table["tdb"][0] - ts2.table["tdb"][0] < 1.0e-15
def __call__(self, time):
"""Create list of TOAs for one or more times.
Parameters
----------
time : `~astropy.time.Time`
Input time stamps.
"""
toa_list = make_toa_list(time, self.observatory, self.frequency)
return toa.get_TOAs_list(toa_list, **self.control_params)
def test_roundtrip_topo_toa_TEMPOformat(tmpdir):
# Create a barycentric TOA
t1time = Time(58534.0, 0.0928602471130208, format="mjd", scale="utc")
t1 = toa.TOA(t1time, obs="gbt", freq=0.0)
ts = toa.get_TOAs_list([t1], ephem="DE421")
outnm = os.path.join(tmpdir, "testtopot1.tim")
ts.write_TOA_file(outnm, format="TEMPO")
ts2 = toa.get_TOAs(outnm)
assert np.abs(ts.table["mjd"][0] - ts2.table["mjd"][0]) < 1.0e-15 * u.d
assert np.abs(ts.table["tdb"][0] - ts2.table["tdb"][0]) < 1.0e-15 * u.d
def get_TZR_toa(self, toas):
""" Get the TOAs class for the TZRMJD. We are treating the TZRMJD as a
special TOA.
"""
TZR_toa = toa.TOA(self.TZRMJD.quantity,
obs=self.TZRSITE.value,
freq=self.TZRFRQ.quantity)
clkc_info = toas.clock_corr_info
tz = toa.get_TOAs_list([
TZR_toa,
],
include_bipm=clkc_info['include_bipm'],
include_gps=clkc_info['include_gps'],
ephem=toas.ephem,
planets=toas.planets)
return tz
def get_TZR_toa(self, toas):
"""Get the TOAs class for the TZRMJD.
We are treating the TZRMJD as a special TOA.
Note that any observatory clock corrections will be applied
to this TOA, as with any other TOA. This does not affect the
value of the TZRMJD parmeter, however.
"""
clkc_info = toas.clock_corr_info
# If we have cached the TZR TOA and all the TZR* and clock info has not changed, then don't rebuild it
if self.tz_cache is not None:
if (self.tz_clkc_info["include_bipm"] == clkc_info["include_bipm"]
and self.tz_clkc_info["include_gps"]
== clkc_info["include_gps"]
and self.tz_planets == toas.planets
and self.tz_ephem == toas.ephem and self.tz_hash == hash(
(self.TZRMJD.value, self.TZRSITE.value,
self.TZRFRQ.value))):
return self.tz_cache
# Otherwise we have to build the TOA and apply clock corrections
# NOTE: Using TZRMJD.quantity.jd[1,2] so that the time scale can be properly
# set to the TZRSITE default timescale (e.g. UTC for TopoObs and TDB for SSB)
log.debug(
"Creating and dealing with the single TZR_toa for absolute phase")
TZR_toa = toa.TOA(
(self.TZRMJD.quantity.jd1 - 2400000.5, self.TZRMJD.quantity.jd2),
obs=self.TZRSITE.value,
freq=self.TZRFRQ.quantity,
)
tz = toa.get_TOAs_list(
[TZR_toa],
include_bipm=clkc_info["include_bipm"],
include_gps=clkc_info["include_gps"],
ephem=toas.ephem,
planets=toas.planets,
)
log.debug("Done with TZR_toa")
self.tz_cache = tz
self.tz_hash = hash(
(self.TZRMJD.value, self.TZRSITE.value, self.TZRFRQ.value))
self.tz_clkc_info = clkc_info
self.tz_planets = toas.planets
self.tz_ephem = toas.ephem
return tz
def get_TZR_toa(self, toas):
""" Get the TOAs class for the TZRMJD. We are treating the TZRMJD as a
special TOA.
"""
# NOTE: Using TZRMJD.quantity.jd[1,2] so that the time scale can be properly
# set to the TZRSITE default timescale (e.g. UTC for TopoObs and TDB for SSB)
TZR_toa = toa.TOA(
(self.TZRMJD.quantity.jd1 - 2400000.5, self.TZRMJD.quantity.jd2),
obs=self.TZRSITE.value,
freq=self.TZRFRQ.quantity)
clkc_info = toas.clock_corr_info
tz = toa.get_TOAs_list([
TZR_toa,
],
include_bipm=clkc_info['include_bipm'],
include_gps=clkc_info['include_gps'],
ephem=toas.ephem,
planets=toas.planets)
return tz
def change_pepoch(self, new_epoch, toas=None, delay=None):
"""Move PEPOCH to a new time and change the related paramters.
Parameters
----------
new_epoch: float or `astropy.Time` object
The new PEPOCH value.
toas: `toa` object, optional.
If current PEPOCH is not provided, the first pulsar frame toa will
be treated as PEPOCH.
delay: `numpy.array` object
If current PEPOCH is not provided, it is required for computing the
first pulsar frame toa.
"""
if isinstance(new_epoch, Time):
new_epoch = Time(new_epoch, scale='tdb', precision=9)
else:
new_epoch = Time(new_epoch, scale='tdb', format='mjd', precision=9)
# make new_epoch a toa for delay calculation.
new_epoch_toa = toa.get_TOAs_list([
toa.TOA(new_epoch),
],
ephem=toas.ephem)
if self.PEPOCH.value is None:
if toas is None or delay is None:
raise ValueError(
"`PEPOCH` is not in the model, thus, 'toa' and"
" 'delay' shoule be givne.")
tbl = toas.table
phsepoch_ld = time_to_longdouble(tbl['tdb'][0] - delay[0])
else:
phsepoch_ld = time_to_longdouble(self.PEPOCH.quantity)
dt = ((time_to_longdouble(new_epoch) - phsepoch_ld) * u.day)
fterms = [0.0 * u.Unit("")] + self.get_spin_terms()
# rescale the fterms
for n in range(len(fterms) - 1):
f_par = getattr(self, 'F{}'.format(n))
f_par.value = taylor_horner_deriv(dt.to(u.second),
fterms,
deriv_order=n + 1)
self.PEPOCH.value = new_epoch
def test_commenting_toas(tmpdir):
# Create a barycentric TOA
t1time = Time(58534.0, 0.0928602471130208, format="mjd", scale="utc")
t1 = toa.TOA(t1time, obs="gbt", freq=0.0)
t2 = toa.TOA(t1time, obs="gbt", freq=0.0)
ts = toa.get_TOAs_list([t1, t2], ephem="DE421")
assert ts.ntoas == 2
outnm = os.path.join(tmpdir, "testtopo.tim")
ts.write_TOA_file(outnm)
ts2 = toa.get_TOAs(outnm)
assert ts2.ntoas == 2 # none should be commented
ts.table[0]["flags"]["cut"] = "do_not_like" # cut flag
ts.table[1]["flags"]["ignore"] = str(1) # ignore flag
ts.write_TOA_file(outnm)
ts3 = toa.get_TOAs(outnm) # defaut is to not comment
assert ts3.ntoas == 2 # none should be commented by default
ts.write_TOA_file(outnm, commentflag="cut")
ts4 = toa.get_TOAs(outnm)
assert ts4.ntoas == 1 # one should be commented
ts.write_TOA_file(outnm, commentflag="ignore")
ts5 = toa.get_TOAs(outnm)
assert ts5.ntoas == 1 # one should be commented
def test_roundtrip_topo_toa_TEMPOformat(self):
# Create a barycentric TOA
t1time = Time(58534.0, 0.0928602471130208, format="mjd", scale="utc")
t1 = toa.TOA(t1time, obs="gbt", freq=0.0)
ts = toa.get_TOAs_list([t1], ephem="DE421")
ts.write_TOA_file("testtopot1.tim", format="TEMPO")
ts2 = toa.get_TOAs("testtopot1.tim")
print(ts.table, ts2.table)
assert np.abs(ts.table["mjd"][0] - ts2.table["mjd"][0]) < 1.0e-15 * u.d
assert np.abs(ts.table["tdb"][0] - ts2.table["tdb"][0]) < 1.0e-15 * u.d
# Comment out because TEMPO2 distro doesn't include gmrt2gps.clk so far
# def test_roundtrip_gmrt_toa_Tempo2format(self):
# if os.getenv("TEMPO2") is None:
# pytest.skip("TEMPO2 evnironment variable is not set, can't run this test")
# # Create a barycentric TOA
# t1time = Time(58534.0, 0.0928602471130208, format="mjd", scale="utc")
# t1 = toa.TOA(t1time, obs="gmrt", freq=0.0)
# ts = toa.get_TOAs_list([t1], ephem="DE421")
# ts.write_TOA_file("testgmrt.tim", format="Tempo2")
# ts2 = toa.get_TOAs("testgmrt.tim")
# print(ts.table, ts2.table)
assert np.abs(ts.table["mjd"][0] - ts2.table["mjd"][0]) < 1.0e-15 * u.d
assert np.abs(ts.table["tdb"][0] - ts2.table["tdb"][0]) < 1.0e-15 * u.d
def generate_polycos(self,
model,
mjdStart,
mjdEnd,
obs,
segLength,
ncoeff,
obsFreq,
maxha,
method="TEMPO",
numNodes=20):
"""
Generate the polyco file data file.
Parameters
---------
model : TimingModel
TimingModel for generate the Polycos with parameters
setup.
mjdStart : float / nump longdouble
Start time of polycos in mjd
mjdEnd : float / nump longdouble
Ending time of polycos in mjd
obs : str
Observatory code
segLength :
Length of polyco segement [unit: minutes]
ncoeff :
number of coefficents
obsFreq :
observing frequency
maxha :
Maximum hour angle
method : sting optional ['TEMPO','TEMPO2',...] Default TEMPO
Method to generate polycos. Now it is only support the TEMPO method.
numNodes : int optional. Default 20
Number of nodes for fitting. It can not be less then the number of
coefficents.
Return
---------
A polyco table.
"""
mjdStart = np.longdouble(mjdStart) * u.day
mjdEnd = np.longdouble(mjdEnd) * u.day
timeLength = mjdEnd - mjdStart
segLength = np.longdouble(segLength) * u.min
obsFreq = float(obsFreq)
month = [
'Jan', 'Feb', 'Mar', 'Apr', 'May', 'Jun', 'Jul', 'Aug', 'Sep',
'Oct', 'Nov', 'Dec'
]
# Alocate memery
coeffs = np.longdouble(np.zeros(ncoeff))
entryList = []
entryIntvl = np.arange(mjdStart.value, mjdEnd.value,
segLength.to('day').value)
if entryIntvl[-1] < mjdEnd.value:
entryIntvl = np.append(entryIntvl, mjdEnd.value)
# Make sure the number of nodes is bigger then number of coeffs.
if numNodes < ncoeff:
numNodes = ncoeff + 1
# generate the ploynomial coefficents
if method == "TEMPO":
# Using tempo1 method to create polycos
for i in range(len(entryIntvl) - 1):
tStart = entryIntvl[i]
tStop = entryIntvl[i + 1]
nodes = np.linspace(tStart, tStop, numNodes)
tmid = ((tStart + tStop) / 2.0) * u.day
toaMid = toa.get_TOAs_list([
toa.TOA((np.modf(tmid.value)[1], np.modf(tmid.value)[0]),
obs=obs,
freq=obsFreq),
])
refPhase = model.phase(toaMid.table)
mjdSpan = ((tStop - tStart) * u.day).to('min')
# Create node toas(Time sample using TOA class)
toaList = [
toa.TOA((np.modf(toaNode)[1], np.modf(toaNode)[0]),
obs=obs,
freq=obsFreq) for toaNode in nodes
]
toas = toa.get_TOAs_list(toaList)
ph = model.phase(toas.table)
dt = (nodes * u.day - tmid).to('min') # Use constant
rdcPhase = ph - refPhase
rdcPhase = rdcPhase.int - dt.value * model.F0.value * 60.0 + rdcPhase.frac
dtd = dt.value.astype(float) # Trancate to double
rdcPhased = rdcPhase.astype(float)
coeffs = np.polyfit(dtd, rdcPhased, ncoeff - 1)
coeffs = coeffs[::-1]
midTime = at.Time(int(tmid.value),
np.modf(tmid.value)[0],
format='mjd',
scale='utc')
date, hms = midTime.iso.split()
yy, mm, dd = date.split('-')
date = dd + '-' + month[int(mm) - 1] + '-' + yy[2:4]
hms = hms.replace(':', "")
entry = polycoEntry(tmid.value,
mjdSpan.to('day').value, refPhase.int,
refPhase.frac, model.F0.value, ncoeff,
coeffs, obs)
entryList.append(
(model.PSR.value, date, hms, tmid.value, model.DM.value,
0.0, 0.0, 0.0, obsFreq, entry))
pTable = table.Table(rows=entryList,
names=('psr', 'date', 'utc', 'tmid', 'dm',
'dopper', 'logrms', 'binary_phase',
'obsfreq', 'entry'),
meta={'name': 'Ployco Data Table'})
self.polycoTable = pTable
else:
# Reading from an old polycofile
pass
def main(argv=None):
import argparse
parser = argparse.ArgumentParser(
description=
"Use PINT to compute event phases and make plots of photon event files."
)
parser.add_argument(
"eventfile",
help=
"Photon event FITS file name (e.g. from NICER, RXTE, XMM, Chandra).")
parser.add_argument("parfile", help="par file to construct model from")
parser.add_argument("--orbfile", help="Name of orbit file", default=None)
parser.add_argument("--maxMJD",
help="Maximum MJD to include in analysis",
default=None)
parser.add_argument("--plotfile",
help="Output figure file name (default=None)",
default=None)
parser.add_argument("--addphase",
help="Write FITS file with added phase column",
default=False,
action='store_true')
parser.add_argument(
"--absphase",
help="Write FITS file with integral portion of pulse phase (ABS_PHASE)",
default=False,
action='store_true')
parser.add_argument(
"--barytime",
help=
"Write FITS file with a column containing the barycentric time as double precision MJD.",
default=False,
action='store_true')
parser.add_argument(
"--outfile",
help="Output FITS file name (default=same as eventfile)",
default=None)
parser.add_argument("--ephem",
help="Planetary ephemeris to use (default=DE421)",
default="DE421")
parser.add_argument(
'--tdbmethod',
help="Method for computing TT to TDB (default=astropy)",
default="default")
parser.add_argument("--plot",
help="Show phaseogram plot.",
action='store_true',
default=False)
parser.add_argument("--use_gps",
default=False,
action='store_true',
help="Apply GPS to UTC clock corrections")
parser.add_argument("--use_bipm",
default=False,
action='store_true',
help="Use TT(BIPM) instead of TT(TAI)")
# parser.add_argument("--fix",help="Apply 1.0 second offset for NICER", action='store_true', default=False)
args = parser.parse_args(argv)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# If plotfile is specified, that implies plot
if args.plotfile is not None:
args.plot = True
# Read event file header to figure out what instrument is is from
hdr = pyfits.getheader(args.eventfile, ext=1)
log.info('Event file TELESCOPE = {0}, INSTRUMENT = {1}'.format(
hdr['TELESCOP'], hdr['INSTRUME']))
if hdr['TELESCOP'] == 'NICER':
# Instantiate NICERObs once so it gets added to the observatory registry
if args.orbfile is not None:
log.info('Setting up NICER observatory')
NICERObs(name='NICER', FPorbname=args.orbfile, tt2tdb_mode='pint')
# Read event file and return list of TOA objects
try:
tl = load_NICER_TOAs(args.eventfile)
except KeyError:
log.error(
"Observatory not recognized. This probably means you need to provide an orbit file or barycenter the event file."
)
sys.exit(1)
elif hdr['TELESCOP'] == 'XTE':
# Instantiate RXTEObs once so it gets added to the observatory registry
if args.orbfile is not None:
# Determine what observatory type is.
log.info('Setting up RXTE observatory')
RXTEObs(name='RXTE', FPorbname=args.orbfile, tt2tdb_mode='pint')
# Read event file and return list of TOA objects
tl = load_RXTE_TOAs(args.eventfile)
elif hdr['TELESCOP'].startswith('XMM'):
# Not loading orbit file here, since that is not yet supported.
tl = load_XMM_TOAs(args.eventfile)
elif hdr['TELESCOP'].startswith('NuSTAR'):
# Not loading orbit file here, since that is not yet supported.
tl = load_NuSTAR_TOAs(args.eventfile)
else:
log.error(
"FITS file not recognized, TELESCOPE = {0}, INSTRUMENT = {1}".
format(hdr['TELESCOP'], hdr['INSTRUME']))
sys.exit(1)
# Now convert to TOAs object and compute TDBs and posvels
if len(tl) == 0:
log.error("No TOAs, exiting!")
sys.exit(0)
# Read in model
modelin = pint.models.get_model(args.parfile)
use_planets = False
if 'PLANET_SHAPIRO' in modelin.params:
if modelin.PLANET_SHAPIRO.value:
use_planets = True
# Discard events outside of MJD range
if args.maxMJD is not None:
tlnew = []
print("pre len : ", len(tl))
maxT = Time(float(args.maxMJD), format='mjd')
print("maxT : ", maxT)
for tt in tl:
if tt.mjd < maxT:
tlnew.append(tt)
tl = tlnew
print("post len : ", len(tlnew))
ts = toa.get_TOAs_list(tl,
ephem=args.ephem,
include_bipm=args.use_bipm,
include_gps=args.use_gps,
planets=use_planets,
tdb_method=args.tdbmethod)
ts.filename = args.eventfile
# if args.fix:
# ts.adjust_TOAs(TimeDelta(np.ones(len(ts.table))*-1.0*u.s,scale='tt'))
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(), mjds.max())
# Compute model phase for each TOA
iphss, phss = modelin.phase(ts, abs_phase=True)
# ensure all postive
negmask = phss < 0.0 * u.cycle
phases = np.where(negmask, phss + 1.0 * u.cycle, phss)
h = float(hm(phases))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h, h2sig(h)))
if args.plot:
phaseogram_binned(mjds, phases, bins=100, plotfile=args.plotfile)
if args.addphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile, mode='update')
else:
hdulist = pyfits.open(args.eventfile)
if len(hdulist[1].data) != len(phases):
raise RuntimeError(
'Mismatch between length of FITS table ({0}) and length of phase array ({1})!'
.format(len(hdulist[1].data), len(phases)))
data_to_add = {'PULSE_PHASE': [phases, 'D']}
if args.absphase:
data_to_add['ABS_PHASE'] = [iphss - negmask * u.cycle, 'K']
if args.barytime:
bats = modelin.get_barycentric_toas(ts)
data_to_add['BARY_TIME'] = [bats, 'D']
datacol = []
for key in data_to_add.keys():
if key in hdulist[1].columns.names:
log.info('Found existing %s column, overwriting...' % key)
# Overwrite values in existing Column
hdulist[1].data[key] = data_to_add[key][0]
else:
# Construct and append new column, preserving HDU header and name
log.info('Adding new %s column.' % key)
datacol.append(
pyfits.ColDefs([
pyfits.Column(name=key,
format=data_to_add[key][1],
array=data_to_add[key][0])
]))
if len(datacol) > 0:
cols = hdulist[1].columns
for c in datacol:
cols = cols + c
bt = pyfits.BinTableHDU.from_columns(cols,
header=hdulist[1].header,
name=hdulist[1].name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info('Overwriting existing FITS file ' + args.eventfile)
hdulist.flush(verbose=True, output_verify='warn')
else:
# Write to new output file
log.info('Writing output FITS file ' + args.outfile)
hdulist.writeto(args.outfile,
overwrite=True,
checksum=True,
output_verify='warn')
def d_phase_d_toa(self, toas, time_intval = 60 ,method = None,
num_sample = 20, order = 11):
"""Return the derivative of phase wrt TOA
time_intval: is in seconds
method: with finite difference and chebyshev interpolation
"""
d_phase_d_toa = np.zeros(len(toas))
if method is None or "FDM":
# Using finite difference to calculate the derivitve
dt = np.longdouble(time_intval)/np.longdouble(num_sample)
num_sample = int(num_sample)/2*2+1
for i,singal_toa in enumerate(toas):
toa_utc_ld = utils.time_to_longdouble(singal_toa['mjd'])
# Resample the toa points
domain = (toa_utc_ld-time_intval/2.0,toa_utc_ld+time_intval/2.0)
sample = np.linspace(domain[0],domain[1],num_sample)
toa_list = []
for sample_time in sample:
toa_list.append(toa.TOA((np.modf(sample_time)[1],
np.modf(sample_time)[0]),obs = singal_toa['obs'],
freq = singal_toa['freq']))
sample_toalist = toa.get_TOAs_list(toa_list)
ph = self.phase(sample_toalist.table)
p = ph.int-ph.int.min()+ph.frac
p = np.array(p,dtype='float64')
# Reduce the value of samples in order to use double precision
reduce_samepl = np.array((sample-sample.min())*86400.0,dtype = 'float64')
dx = np.gradient(reduce_samepl)
dp = np.gradient(p-p.mean(),dx)
d_phase_d_toa[i] = dp[num_sample/2]
if method is "chebyshev":
# Using chebyshev interpolation to calculate the
for i,singal_toa in enumerate(toas):
# Have more sample point around toa
toa_utc_ld = utils.time_to_longdouble(singal_toa['mjd'])
domain = (toa_utc_ld-time_intval/2.0,toa_utc_ld+time_intval/2.0)
sample = np.linspace(domain[0],domain[1],num_sample)
toa_list = []
for sample_time in sample:
toa_list.append(toa.TOA((np.modf(sample_time)[1],
np.modf(sample_time)[0]),obs = singal_toa['obs'],
freq = singal_toa['freq']))
sample_toalist = toa.get_TOAs_list(toa_list)
# Calculate phase
ph = self.phase(sample_toalist.table)
p = ph.int-ph.int.min()+ph.frac
p = np.array(p,dtype='float64')
# reduce the phase value to use double precision
reduce_samepl = np.array((sample-sample.min())*86400.0,dtype = 'float64')
coeff = np.polynomial.chebyshev.chebfit(reduce_samepl, p,order)
dcoeff = np.polynomial.chebyshev.chebder(coeff)
dy = np.polynomial.chebyshev.chebval(reduce_samepl,dcoeff)
d_phase_d_toa[i] = dy[num_sample/2]
return d_phase_d_toa
def main(argv=None):
import argparse
parser = argparse.ArgumentParser(
description=
"Use PINT to compute event phases and make plots of photon event files."
)
parser.add_argument(
"eventfile",
help=
"Photon event FITS file name (e.g. from NICER, RXTE, XMM, Chandra).",
)
parser.add_argument("parfile", help="par file to construct model from")
parser.add_argument("--orbfile", help="Name of orbit file", default=None)
parser.add_argument("--maxMJD",
help="Maximum MJD to include in analysis",
default=None)
parser.add_argument("--plotfile",
help="Output figure file name (default=None)",
default=None)
parser.add_argument(
"--addphase",
help="Write FITS file with added phase column",
default=False,
action="store_true",
)
parser.add_argument(
"--addorbphase",
help="Write FITS file with added orbital phase column",
default=False,
action="store_true",
)
parser.add_argument(
"--absphase",
help="Write FITS file with integral portion of pulse phase (ABS_PHASE)",
default=False,
action="store_true",
)
parser.add_argument(
"--barytime",
help=
"Write FITS file with a column containing the barycentric time as double precision MJD.",
default=False,
action="store_true",
)
parser.add_argument(
"--outfile",
help="Output FITS file name (default=same as eventfile)",
default=None,
)
parser.add_argument("--ephem",
help="Planetary ephemeris to use (default=DE421)",
default="DE421")
parser.add_argument(
"--tdbmethod",
help="Method for computing TT to TDB (default=astropy)",
default="default",
)
parser.add_argument("--plot",
help="Show phaseogram plot.",
action="store_true",
default=False)
parser.add_argument(
"--use_gps",
default=False,
action="store_true",
help="Apply GPS to UTC clock corrections",
)
parser.add_argument(
"--use_bipm",
default=False,
action="store_true",
help="Use TT(BIPM) instead of TT(TAI)",
)
# parser.add_argument("--fix",help="Apply 1.0 second offset for NICER", action='store_true', default=False)
args = parser.parse_args(argv)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# If plotfile is specified, that implies plot
if args.plotfile is not None:
args.plot = True
# Read event file header to figure out what instrument is is from
hdr = pyfits.getheader(args.eventfile, ext=1)
log.info("Event file TELESCOPE = {0}, INSTRUMENT = {1}".format(
hdr["TELESCOP"], hdr["INSTRUME"]))
if hdr["TELESCOP"] == "NICER":
# Instantiate NICERObs once so it gets added to the observatory registry
if args.orbfile is not None:
log.info("Setting up NICER observatory")
NICERObs(name="NICER", FPorbname=args.orbfile, tt2tdb_mode="pint")
# Read event file and return list of TOA objects
try:
tl = load_NICER_TOAs(args.eventfile)
except KeyError:
log.error(
"Observatory not recognized. This probably means you need to provide an orbit file or barycenter the event file."
)
sys.exit(1)
elif hdr["TELESCOP"] == "XTE":
# Instantiate RXTEObs once so it gets added to the observatory registry
if args.orbfile is not None:
# Determine what observatory type is.
log.info("Setting up RXTE observatory")
RXTEObs(name="RXTE", FPorbname=args.orbfile, tt2tdb_mode="pint")
# Read event file and return list of TOA objects
tl = load_RXTE_TOAs(args.eventfile)
elif hdr["TELESCOP"].startswith("XMM"):
# Not loading orbit file here, since that is not yet supported.
tl = load_XMM_TOAs(args.eventfile)
elif hdr["TELESCOP"].lower().startswith("nustar"):
if args.orbfile is not None:
log.info("Setting up NuSTAR observatory")
NuSTARObs(name="NuSTAR",
FPorbname=args.orbfile,
tt2tdb_mode="pint")
tl = load_NuSTAR_TOAs(args.eventfile)
else:
log.error(
"FITS file not recognized, TELESCOPE = {0}, INSTRUMENT = {1}".
format(hdr["TELESCOP"], hdr["INSTRUME"]))
sys.exit(1)
# Now convert to TOAs object and compute TDBs and posvels
if len(tl) == 0:
log.error("No TOAs, exiting!")
sys.exit(0)
# Read in model
modelin = pint.models.get_model(args.parfile)
use_planets = False
if "PLANET_SHAPIRO" in modelin.params:
if modelin.PLANET_SHAPIRO.value:
use_planets = True
if "AbsPhase" not in modelin.components:
log.error(
"TimingModel does not include AbsPhase component, which is required "
"for computing phases. Make sure you have TZR* parameters in your par file!"
)
raise ValueError("Model missing AbsPhase component.")
if args.addorbphase and (not hasattr(modelin, "binary_model_name")):
log.error(
"TimingModel does not include a binary model, which is required for "
"computing orbital phases. Make sure you have BINARY and associated "
"model parameters in your par file!")
raise ValueError("Model missing BINARY component.")
# Discard events outside of MJD range
if args.maxMJD is not None:
tlnew = []
print("pre len : ", len(tl))
maxT = Time(float(args.maxMJD), format="mjd")
print("maxT : ", maxT)
for tt in tl:
if tt.mjd < maxT:
tlnew.append(tt)
tl = tlnew
print("post len : ", len(tlnew))
ts = toa.get_TOAs_list(
tl,
ephem=args.ephem,
include_bipm=args.use_bipm,
include_gps=args.use_gps,
planets=use_planets,
tdb_method=args.tdbmethod,
)
ts.filename = args.eventfile
# if args.fix:
# ts.adjust_TOAs(TimeDelta(np.ones(len(ts.table))*-1.0*u.s,scale='tt'))
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(), mjds.max())
# Compute model phase for each TOA
iphss, phss = modelin.phase(ts, abs_phase=True)
# ensure all postive
negmask = phss < 0.0
phases = np.where(negmask, phss + 1.0, phss)
h = float(hm(phases))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h, h2sig(h)))
if args.plot:
phaseogram_binned(mjds, phases, bins=100, plotfile=args.plotfile)
# Compute orbital phases for each photon TOA
if args.addorbphase:
delay = modelin.delay(ts)
orbits = modelin.binary_instance.orbits()
# These lines are already in orbits.orbit_phase() in binary_orbits.py.
# What is the correct syntax is to call this function here?
norbits = np.array(np.floor(orbits), dtype=np.long)
orbphases = orbits - norbits # fractional phase
if args.addphase or args.addorbphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile, mode="update")
else:
hdulist = pyfits.open(args.eventfile)
datacol = []
data_to_add = {}
if args.addphase:
if len(hdulist[1].data) != len(phases):
raise RuntimeError(
"Mismatch between length of FITS table ({0}) and length of phase array ({1})!"
.format(len(hdulist[1].data), len(phases)))
data_to_add["PULSE_PHASE"] = [phases, "D"]
if args.absphase:
data_to_add["ABS_PHASE"] = [iphss - negmask, "K"]
if args.barytime:
bats = modelin.get_barycentric_toas(ts)
data_to_add["BARY_TIME"] = [bats, "D"]
if args.addorbphase:
if len(hdulist[1].data) != len(orbphases):
raise RuntimeError(
"Mismatch between length of FITS table ({0}) and length of orbital phase array ({1})!"
.format(len(hdulist[1].data), len(orbphases)))
data_to_add["ORBIT_PHASE"] = [orbphases, "D"]
# End if args.addorbphase
for key in data_to_add.keys():
if key in hdulist[1].columns.names:
log.info("Found existing %s column, overwriting..." % key)
# Overwrite values in existing Column
hdulist[1].data[key] = data_to_add[key][0]
else:
# Construct and append new column, preserving HDU header and name
log.info("Adding new %s column." % key)
datacol.append(
pyfits.ColDefs([
pyfits.Column(
name=key,
format=data_to_add[key][1],
array=data_to_add[key][0],
)
]))
if len(datacol) > 0:
cols = hdulist[1].columns
for c in datacol:
cols = cols + c
bt = pyfits.BinTableHDU.from_columns(cols,
header=hdulist[1].header,
name=hdulist[1].name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info("Overwriting existing FITS file " + args.eventfile)
hdulist.flush(verbose=True, output_verify="warn")
else:
# Write to new output file
log.info("Writing output FITS file " + args.outfile)
hdulist.writeto(args.outfile,
overwrite=True,
checksum=True,
output_verify="warn")
def main(argv=None):
import argparse
parser = argparse.ArgumentParser(description="Use PINT to compute event phases and make plots of photon event files.")
parser.add_argument("eventfile",help="Photon event FITS file name (e.g. from NICER, RXTE, XMM, Chandra).")
parser.add_argument("parfile",help="par file to construct model from")
parser.add_argument("--orbfile",help="Name of orbit file", default=None)
parser.add_argument("--maxMJD",help="Maximum MJD to include in analysis", default=None)
parser.add_argument("--plotfile",help="Output figure file name (default=None)", default=None)
parser.add_argument("--addphase",help="Write FITS file with added phase column",default=False,action='store_true')
parser.add_argument("--absphase",help="Write FITS file with integral portion of pulse phase (ABS_PHASE)",default=False,action='store_true')
parser.add_argument("--barytime",help="Write FITS file with a column containing the barycentric time as double precision MJD.",default=False,action='store_true')
parser.add_argument("--outfile",help="Output FITS file name (default=same as eventfile)", default=None)
parser.add_argument("--ephem",help="Planetary ephemeris to use (default=DE421)", default="DE421")
parser.add_argument('--tdbmethod',help="Method for computing TT to TDB (default=astropy)", default="default")
parser.add_argument("--plot",help="Show phaseogram plot.", action='store_true', default=False)
parser.add_argument("--use_gps",default=False,action='store_true',help="Apply GPS to UTC clock corrections")
parser.add_argument("--use_bipm",default=False,action='store_true',help="Use TT(BIPM) instead of TT(TAI)")
# parser.add_argument("--fix",help="Apply 1.0 second offset for NICER", action='store_true', default=False)
args = parser.parse_args(argv)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# If plotfile is specified, that implies plot
if args.plotfile is not None:
args.plot = True
# Read event file header to figure out what instrument is is from
hdr = pyfits.getheader(args.eventfile,ext=1)
log.info('Event file TELESCOPE = {0}, INSTRUMENT = {1}'.format(hdr['TELESCOP'],
hdr['INSTRUME']))
if hdr['TELESCOP'] == 'NICER':
# Instantiate NICERObs once so it gets added to the observatory registry
if args.orbfile is not None:
log.info('Setting up NICER observatory')
NICERObs(name='NICER',FPorbname=args.orbfile,tt2tdb_mode='pint')
# Read event file and return list of TOA objects
try:
tl = load_NICER_TOAs(args.eventfile)
except KeyError:
log.error("Observatory not recognized. This probably means you need to provide an orbit file or barycenter the event file.")
sys.exit(1)
elif hdr['TELESCOP'] == 'XTE':
# Instantiate RXTEObs once so it gets added to the observatory registry
if args.orbfile is not None:
# Determine what observatory type is.
log.info('Setting up RXTE observatory')
RXTEObs(name='RXTE',FPorbname=args.orbfile,tt2tdb_mode='pint')
# Read event file and return list of TOA objects
tl = load_RXTE_TOAs(args.eventfile)
elif hdr['TELESCOP'].startswith('XMM'):
# Not loading orbit file here, since that is not yet supported.
tl = load_XMM_TOAs(args.eventfile)
elif hdr['TELESCOP'].lower().startswith('nustar'):
if args.orbfile is not None:
log.info('Setting up NuSTAR observatory')
NuSTARObs(name='NuSTAR',FPorbname=args.orbfile, tt2tdb_mode='pint')
tl = load_NuSTAR_TOAs(args.eventfile)
else:
log.error("FITS file not recognized, TELESCOPE = {0}, INSTRUMENT = {1}".format(
hdr['TELESCOP'], hdr['INSTRUME']))
sys.exit(1)
# Now convert to TOAs object and compute TDBs and posvels
if len(tl) == 0:
log.error("No TOAs, exiting!")
sys.exit(0)
# Read in model
modelin = pint.models.get_model(args.parfile)
use_planets=False
if 'PLANET_SHAPIRO' in modelin.params:
if modelin.PLANET_SHAPIRO.value:
use_planets=True
# Discard events outside of MJD range
if args.maxMJD is not None:
tlnew = []
print("pre len : ",len(tl))
maxT = Time(float(args.maxMJD),format='mjd')
print("maxT : ",maxT)
for tt in tl:
if tt.mjd < maxT:
tlnew.append(tt)
tl=tlnew
print("post len : ",len(tlnew))
ts = toa.get_TOAs_list(tl, ephem=args.ephem, include_bipm=args.use_bipm,
include_gps=args.use_gps, planets=use_planets, tdb_method=args.tdbmethod)
ts.filename = args.eventfile
# if args.fix:
# ts.adjust_TOAs(TimeDelta(np.ones(len(ts.table))*-1.0*u.s,scale='tt'))
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(),mjds.max())
# Compute model phase for each TOA
iphss,phss = modelin.phase(ts,abs_phase=True)
# ensure all postive
negmask = phss < 0.0 * u.cycle
phases = np.where(negmask, phss + 1.0 * u.cycle, phss)
h = float(hm(phases))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h,h2sig(h)))
if args.plot:
phaseogram_binned(mjds,phases,bins=100,plotfile = args.plotfile)
if args.addphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile,mode='update')
else:
hdulist = pyfits.open(args.eventfile)
if len(hdulist[1].data) != len(phases):
raise RuntimeError('Mismatch between length of FITS table ({0}) and length of phase array ({1})!'.format(len(hdulist[1].data),len(phases)))
data_to_add = {'PULSE_PHASE':[phases,'D']}
if args.absphase:
data_to_add['ABS_PHASE'] = [iphss-negmask*u.cycle,'K']
if args.barytime:
bats = modelin.get_barycentric_toas(ts)
data_to_add['BARY_TIME'] = [bats,'D']
datacol = []
for key in data_to_add.keys():
if key in hdulist[1].columns.names:
log.info('Found existing %s column, overwriting...'%key)
# Overwrite values in existing Column
hdulist[1].data[key] = data_to_add[key][0]
else:
# Construct and append new column, preserving HDU header and name
log.info('Adding new %s column.'%key)
datacol.append(pyfits.ColDefs([pyfits.Column(name=key,
format=data_to_add[key][1], array=data_to_add[key][0])]))
if len(datacol)>0:
cols = hdulist[1].columns
for c in datacol:
cols = cols + c
bt = pyfits.BinTableHDU.from_columns(cols, header=hdulist[1].header,
name=hdulist[1].name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info('Overwriting existing FITS file '+args.eventfile)
hdulist.flush(verbose=True, output_verify='warn')
else:
# Write to new output file
log.info('Writing output FITS file '+args.outfile)
hdulist.writeto(args.outfile,overwrite=True, checksum=True, output_verify='warn')
def main(argv=None):
parser = argparse.ArgumentParser(
description=
"Use PINT to compute H-test and plot Phaseogram from a Fermi FT1 event file."
)
parser.add_argument("eventfile", help="Fermi event FITS file name.")
parser.add_argument("parfile", help="par file to construct model from")
parser.add_argument(
"weightcol",
help="Column name for event weights (or 'CALC' to compute them)")
parser.add_argument("--ft2", help="Path to FT2 file.", default=None)
parser.add_argument(
"--addphase",
help="Write FT1 file with added phase column",
default=False,
action="store_true",
)
parser.add_argument("--plot",
help="Show phaseogram plot.",
action="store_true",
default=False)
parser.add_argument("--plotfile",
help="Output figure file name (default=None)",
default=None)
parser.add_argument("--maxMJD",
help="Maximum MJD to include in analysis",
default=None)
parser.add_argument(
"--outfile",
help="Output figure file name (default is to overwrite input file)",
default=None,
)
parser.add_argument(
"--planets",
help="Use planetary Shapiro delay in calculations (default=False)",
default=False,
action="store_true",
)
parser.add_argument("--ephem",
help="Planetary ephemeris to use (default=DE421)",
default="DE421")
args = parser.parse_args(argv)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# Read in model
modelin = pint.models.get_model(args.parfile)
if "ELONG" in modelin.params:
tc = SkyCoord(
modelin.ELONG.quantity,
modelin.ELAT.quantity,
frame="barycentrictrueecliptic",
)
else:
tc = SkyCoord(modelin.RAJ.quantity,
modelin.DECJ.quantity,
frame="icrs")
if args.ft2 is not None:
# Instantiate FermiObs once so it gets added to the observatory registry
FermiObs(name="Fermi", ft2name=args.ft2)
# Read event file and return list of TOA objects
tl = load_Fermi_TOAs(args.eventfile,
weightcolumn=args.weightcol,
targetcoord=tc)
# Discard events outside of MJD range
if args.maxMJD is not None:
tlnew = []
print("pre len : ", len(tl))
maxT = Time(float(args.maxMJD), format="mjd")
print("maxT : ", maxT)
for tt in tl:
if tt.mjd < maxT:
tlnew.append(tt)
tl = tlnew
print("post len : ", len(tlnew))
# Now convert to TOAs object and compute TDBs and posvels
# For Fermi, we are not including GPS or TT(BIPM) corrections
ts = toa.get_TOAs_list(
tl,
include_gps=False,
include_bipm=False,
planets=args.planets,
ephem=args.ephem,
)
ts.filename = args.eventfile
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(), mjds.max())
# Compute model phase for each TOA
iphss, phss = modelin.phase(ts, abs_phase=True)
# ensure all postive
phases = np.where(phss < 0.0 * u.cycle, phss + 1.0 * u.cycle, phss)
mjds = ts.get_mjds()
weights = np.array([w["weight"] for w in ts.table["flags"]])
h = float(hmw(phases, weights))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h, h2sig(h)))
if args.plot:
log.info("Making phaseogram plot with {0} photons".format(len(mjds)))
phaseogram(mjds, phases, weights, bins=100, plotfile=args.plotfile)
if args.addphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile, mode="update")
else:
hdulist = pyfits.open(args.eventfile)
event_hdu = hdulist[1]
event_hdr = event_hdu.header
event_dat = event_hdu.data
if len(event_dat) != len(phases):
raise RuntimeError(
"Mismatch between length of FITS table ({0}) and length of phase array ({1})!"
.format(len(event_dat), len(phases)))
if "PULSE_PHASE" in event_hdu.columns.names:
log.info("Found existing PULSE_PHASE column, overwriting...")
# Overwrite values in existing Column
event_dat["PULSE_PHASE"] = phases
else:
# Construct and append new column, preserving HDU header and name
log.info("Adding new PULSE_PHASE column.")
phasecol = pyfits.ColDefs(
[pyfits.Column(name="PULSE_PHASE", format="D", array=phases)])
bt = pyfits.BinTableHDU.from_columns(event_hdu.columns + phasecol,
header=event_hdr,
name=event_hdu.name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info("Overwriting existing FITS file " + args.eventfile)
hdulist.flush(verbose=True, output_verify="warn")
else:
# Write to new output file
log.info("Writing output FITS file " + args.outfile)
hdulist.writeto(args.outfile,
overwrite=True,
checksum=True,
output_verify="warn")
return 0
def generate_polycos(
self,
model,
mjdStart,
mjdEnd,
obs,
segLength,
ncoeff,
obsFreq,
maxha=12.0,
method="TEMPO",
numNodes=20,
):
"""
Generate the polyco data.
Parameters
---------
model : TimingModel
TimingModel to generate the Polycos with parameters
setup.
mjdStart : float / nump longdouble
Start time of polycos in mjd
mjdEnd : float / nump longdouble
Ending time of polycos in mjd
obs : str
Observatory code
segLength : float
Length of polyco segement [unit: minutes]
ncoeff : int
number of coefficents
obsFreq : float
observing frequency [unit: MHz]
maxha : float optional. Default 12.0
Maximum hour angle
method : string optional ['TEMPO','TEMPO2',...] Default TEMPO
Method to generate polycos. Only the TEMPO method is supported for now.
numNodes : int optional. Default 20
Number of nodes for fitting. It cannot be less then the number of
coefficents.
Return
---------
A polyco table.
"""
mjdStart = data2longdouble(mjdStart) * u.day
mjdEnd = data2longdouble(mjdEnd) * u.day
timeLength = mjdEnd - mjdStart
segLength = data2longdouble(segLength) * u.min
obsFreq = float(obsFreq)
month = [
"Jan",
"Feb",
"Mar",
"Apr",
"May",
"Jun",
"Jul",
"Aug",
"Sep",
"Oct",
"Nov",
"Dec",
]
# Alocate memery
coeffs = data2longdouble(np.zeros(ncoeff))
entryList = []
entryIntvl = np.arange(mjdStart.value, mjdEnd.value,
segLength.to("day").value)
if entryIntvl[-1] < mjdEnd.value:
entryIntvl = np.append(entryIntvl, mjdEnd.value)
# Make sure the number of nodes is bigger then number of coeffs.
if numNodes < ncoeff:
numNodes = ncoeff + 1
# generate the ploynomial coefficents
if method == "TEMPO":
# Using tempo1 method to create polycos
for i in range(len(entryIntvl) - 1):
tStart = entryIntvl[i]
tStop = entryIntvl[i + 1]
nodes = np.linspace(tStart, tStop, numNodes)
tmid = ((tStart + tStop) / 2.0) * u.day
toaMid = toa.get_TOAs_list([
toa.TOA(
(np.modf(tmid.value)[1], np.modf(tmid.value)[0]),
obs=obs,
freq=obsFreq,
)
])
refPhase = model.phase(toaMid)
mjdSpan = ((tStop - tStart) * u.day).to("min")
# Create node toas(Time sample using TOA class)
toaList = [
toa.TOA(
(np.modf(toaNode)[1], np.modf(toaNode)[0]),
obs=obs,
freq=obsFreq,
) for toaNode in nodes
]
toas = toa.get_TOAs_list(toaList)
ph = model.phase(toas)
dt = (nodes * u.day - tmid).to("min") # Use constant
rdcPhase = ph - refPhase
rdcPhase = (rdcPhase.int -
(dt.value * model.F0.value * 60.0) * u.cycle +
rdcPhase.frac)
dtd = dt.value.astype(float) # Truncate to double
rdcPhased = rdcPhase.astype(float)
coeffs = np.polyfit(dtd, rdcPhased, ncoeff - 1)
coeffs = coeffs[::-1]
midTime = Time(int(tmid.value),
np.modf(tmid.value)[0],
format="mjd",
scale="utc")
date, hms = midTime.iso.split()
yy, mm, dd = date.split("-")
date = dd + "-" + month[int(mm) - 1] + "-" + yy[2:4]
hms = hms.replace(":", "")
entry = PolycoEntry(
tmid.value,
mjdSpan.to("day").value,
refPhase.int,
refPhase.frac,
model.F0.value,
ncoeff,
coeffs,
obs,
)
entryList.append((
model.PSR.value,
date,
hms,
tmid.value,
model.DM.value,
0.0,
0.0,
0.0,
mjdSpan.to("day").value,
tStart,
tStop,
obs,
obsFreq,
entry,
))
pTable = table.Table(
rows=entryList,
names=(
"psr",
"date",
"utc",
"tmid",
"dm",
"doppler",
"logrms",
"binary_phase",
"mjd_span",
"t_start",
"t_stop",
"obs",
"obsfreq",
"entry",
),
meta={"name": "Polyco Data Table"},
)
self.polycoTable = pTable
if len(self.polycoTable) == 0:
raise ValueError("Zero polycos found for table")
else:
# Reading from an old polycofile
pass
def main(argv=None):
parser = argparse.ArgumentParser(description="Use PINT to compute H-test and plot Phaseogram from a Fermi FT1 event file.")
parser.add_argument("eventfile",help="Fermi event FITS file name.")
parser.add_argument("parfile",help="par file to construct model from")
parser.add_argument("weightcol",help="Column name for event weights (or 'CALC' to compute them)")
parser.add_argument("--ft2",help="Path to FT2 file.",default=None)
parser.add_argument("--addphase",help="Write FT1 file with added phase column",
default=False,action='store_true')
parser.add_argument("--plot",help="Show phaseogram plot.", action='store_true', default=False)
parser.add_argument("--plotfile",help="Output figure file name (default=None)", default=None)
parser.add_argument("--maxMJD",help="Maximum MJD to include in analysis", default=None)
parser.add_argument("--outfile",help="Output figure file name (default is to overwrite input file)", default=None)
parser.add_argument("--planets",help="Use planetary Shapiro delay in calculations (default=False)", default=False, action="store_true")
parser.add_argument("--ephem",help="Planetary ephemeris to use (default=DE421)", default="DE421")
args = parser.parse_args(argv)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# Read in model
modelin = pint.models.get_model(args.parfile)
if 'ELONG' in modelin.params:
tc = SkyCoord(modelin.ELONG.quantity,modelin.ELAT.quantity,
frame='barycentrictrueecliptic')
else:
tc = SkyCoord(modelin.RAJ.quantity,modelin.DECJ.quantity,frame='icrs')
if args.ft2 is not None:
# Instantiate FermiObs once so it gets added to the observatory registry
FermiObs(name='Fermi',ft2name=args.ft2)
# Read event file and return list of TOA objects
tl = load_Fermi_TOAs(args.eventfile, weightcolumn=args.weightcol,
targetcoord=tc)
# Discard events outside of MJD range
if args.maxMJD is not None:
tlnew = []
print("pre len : ",len(tl))
maxT = Time(float(args.maxMJD),format='mjd')
print("maxT : ",maxT)
for tt in tl:
if tt.mjd < maxT:
tlnew.append(tt)
tl=tlnew
print("post len : ",len(tlnew))
# Now convert to TOAs object and compute TDBs and posvels
# For Fermi, we are not including GPS or TT(BIPM) corrections
ts = toa.get_TOAs_list(tl,include_gps=False,include_bipm=False,planets=args.planets,ephem=args.ephem)
ts.filename = args.eventfile
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(),mjds.max())
# Compute model phase for each TOA
iphss,phss = modelin.phase(ts,abs_phase=True)
# ensure all postive
phases = np.where(phss < 0.0 * u.cycle, phss + 1.0 * u.cycle, phss)
mjds = ts.get_mjds()
weights = np.array([w['weight'] for w in ts.table['flags']])
h = float(hmw(phases,weights))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h,h2sig(h)))
if args.plot:
log.info("Making phaseogram plot with {0} photons".format(len(mjds)))
phaseogram(mjds,phases,weights,bins=100,plotfile = args.plotfile)
if args.addphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile,mode='update')
else:
hdulist = pyfits.open(args.eventfile)
event_hdu = hdulist[1]
event_hdr=event_hdu.header
event_dat=event_hdu.data
if len(event_dat) != len(phases):
raise RuntimeError('Mismatch between length of FITS table ({0}) and length of phase array ({1})!'.format(len(event_dat),len(phases)))
if 'PULSE_PHASE' in event_hdu.columns.names:
log.info('Found existing PULSE_PHASE column, overwriting...')
# Overwrite values in existing Column
event_dat['PULSE_PHASE'] = phases
else:
# Construct and append new column, preserving HDU header and name
log.info('Adding new PULSE_PHASE column.')
phasecol = pyfits.ColDefs([pyfits.Column(name='PULSE_PHASE', format='D',
array=phases)])
bt = pyfits.BinTableHDU.from_columns( event_hdu.columns + phasecol,
header=event_hdr,name=event_hdu.name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info('Overwriting existing FITS file '+args.eventfile)
hdulist.flush(verbose=True, output_verify='warn')
else:
# Write to new output file
log.info('Writing output FITS file '+args.outfile)
hdulist.writeto(args.outfile,overwrite=True, checksum=True, output_verify='warn')
return 0
def main(argv=None):
import argparse
parser = argparse.ArgumentParser(
description=
"Use PINT to compute event phases and make plots of photon event files.",
formatter_class=argparse.ArgumentDefaultsHelpFormatter,
)
parser.add_argument(
"eventfile",
help=
"Photon event FITS file name (e.g. from NICER, RXTE, XMM, Chandra).",
)
parser.add_argument("parfile", help="par file to construct model from")
parser.add_argument("--orbfile", help="Name of orbit file", default=None)
parser.add_argument("--maxMJD",
help="Maximum MJD to include in analysis",
default=None)
parser.add_argument("--minMJD",
help="Minimum MJD to include in analysis",
default=None)
parser.add_argument("--plotfile",
help="Output figure file name",
default=None)
parser.add_argument(
"--addphase",
help="Write FITS file with added phase column",
default=False,
action="store_true",
)
parser.add_argument(
"--addorbphase",
help="Write FITS file with added orbital phase column",
default=False,
action="store_true",
)
parser.add_argument(
"--absphase",
help="Write FITS file with integral portion of pulse phase (ABS_PHASE)",
default=False,
action="store_true",
)
parser.add_argument(
"--barytime",
help=
"Write FITS file with a column containing the barycentric time as double precision MJD.",
default=False,
action="store_true",
)
parser.add_argument(
"--outfile",
help="Output FITS file name (default=same as eventfile)",
default=None,
)
parser.add_argument("--ephem",
help="Planetary ephemeris to use",
default="DE421")
parser.add_argument(
"--tdbmethod",
help="Method for computing TT to TDB (default=astropy)",
default="default",
)
parser.add_argument("--plot",
help="Show phaseogram plot.",
action="store_true",
default=False)
parser.add_argument(
"--use_gps",
default=False,
action="store_true",
help="Apply GPS to UTC clock corrections",
)
parser.add_argument(
"--use_bipm",
default=False,
action="store_true",
help="Use TT(BIPM) instead of TT(TAI)",
)
parser.add_argument(
"--log-level",
type=str,
choices=("TRACE", "DEBUG", "INFO", "WARNING", "ERROR"),
default="WARNING",
help="Logging level",
dest="loglevel",
)
# parser.add_argument("--fix",help="Apply 1.0 second offset for NICER", action='store_true', default=False)
parser.add_argument(
"--polycos",
default=False,
action="store_true",
help=
"Use polycos to calculate phases; use when working with very large event files",
)
args = parser.parse_args(argv)
log.remove()
log.add(
sys.stderr,
level=args.loglevel,
colorize=True,
format=pint.logging.format,
filter=pint.logging.LogFilter(),
)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# If plotfile is specified, that implies plot
if args.plotfile is not None:
args.plot = True
# set MJD ranges
maxmjd = np.inf if (args.maxMJD is None) else float(args.maxMJD)
minmjd = 0.0 if (args.minMJD is None) else float(args.minMJD)
# Read event file header to figure out what instrument is is from
hdr = pyfits.getheader(args.eventfile, ext=1)
log.info("Event file TELESCOPE = {0}, INSTRUMENT = {1}".format(
hdr["TELESCOP"], hdr["INSTRUME"]))
telescope = hdr["TELESCOP"].lower()
# Instantiate observatory once so it gets added to the observatory registry
if args.orbfile is not None:
log.info(f"Setting up {telescope.upper()} observatory")
try:
get_satellite_observatory(telescope, args.orbfile)
except Exception:
log.error(
"The orbit file is not recognized. It is likely that this mission is not supported. "
"Please barycenter the event file using the official mission tools before processing with PINT"
)
# Read event file and return list of TOA objects, if not using polycos
if args.polycos == False:
try:
tl = load_event_TOAs(args.eventfile,
telescope,
minmjd=minmjd,
maxmjd=maxmjd)
except KeyError:
log.error(
"Observatory not recognized. This probably means you need to provide an orbit file or barycenter the event file."
)
sys.exit(1)
# Now convert to TOAs object and compute TDBs and posvels
if len(tl) == 0:
log.error("No TOAs, exiting!")
sys.exit(0)
# Read in model
modelin = pint.models.get_model(args.parfile)
use_planets = False
if "PLANET_SHAPIRO" in modelin.params:
if modelin.PLANET_SHAPIRO.value:
use_planets = True
if "AbsPhase" not in modelin.components:
log.error(
"TimingModel does not include AbsPhase component, which is required "
"for computing phases. Make sure you have TZR* parameters in your par file!"
)
raise ValueError("Model missing AbsPhase component.")
if args.addorbphase and (not hasattr(modelin, "binary_model_name")):
log.error(
"TimingModel does not include a binary model, which is required for "
"computing orbital phases. Make sure you have BINARY and associated "
"model parameters in your par file!")
raise ValueError("Model missing BINARY component.")
# Use polycos to calculate pulse phases
if args.polycos:
log.info("Using polycos to get pulse phases.")
if args.addorbphase:
raise ValueError("Cannot use orbphase with polycos.")
# Polycos parameters
segLength = 120 # in minutes
ncoeff = 10
obsfreq = 0
# Open event file and get start and end mjds
hdulist = pyfits.open(args.eventfile)
data = hdulist[1].data
mjds = read_fits_event_mjds(hdulist[1])
minmjd = min(mjds)
maxmjd = max(mjds)
# Check if event file is barycentered
if hdulist[1].header["TIMESYS"] != "TDB":
raise ValueError(
"The event file has not been barycentered. Polycos can only be used with barycentered data."
)
# Create polycos table
log.debug("Generating polycos")
telescope_n = "@"
p = polycos.Polycos()
ptable = p.generate_polycos(modelin, minmjd, maxmjd, telescope_n,
segLength, ncoeff, obsfreq)
# Calculate phases
log.debug("Evaluating polycos")
phases = p.eval_phase(mjds)
phases[phases < 0] += 1.0
h = float(hm(phases))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h, h2sig(h)))
else: # Normal mode, not polycos
ts = toa.get_TOAs_list(
tl,
ephem=args.ephem,
include_bipm=args.use_bipm,
include_gps=args.use_gps,
planets=use_planets,
tdb_method=args.tdbmethod,
)
ts.filename = args.eventfile
# if args.fix:
# ts.adjust_TOAs(TimeDelta(np.ones(len(ts.table))*-1.0*u.s,scale='tt'))
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(), mjds.max())
# Compute model phase for each TOA
iphss, phss = modelin.phase(ts, abs_phase=True)
phases = phss.value % 1
h = float(hm(phases))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h, h2sig(h)))
if args.plot:
phaseogram_binned(mjds, phases, bins=100, plotfile=args.plotfile)
# Compute orbital phases for each photon TOA
if args.addorbphase:
delay = modelin.delay(ts)
orbits = modelin.binary_instance.orbits()
# These lines are already in orbits.orbit_phase() in binary_orbits.py.
# What is the correct syntax is to call this function here?
norbits = np.array(np.floor(orbits), dtype=int)
orbphases = orbits - norbits # fractional phase
if args.addphase or args.addorbphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile, mode="update")
else:
hdulist = pyfits.open(args.eventfile)
datacol = []
data_to_add = {}
# Handle case where minMJD/maxMJD do not exceed length of events
mjds_float = read_fits_event_mjds(hdulist[1])
time_mask = np.logical_and((mjds_float > minmjd),
(mjds_float < maxmjd))
if args.polycos:
time_mask = np.logical_and((mjds_float >= minmjd),
(mjds_float <= maxmjd))
if args.addphase:
if time_mask.sum() != len(phases):
raise RuntimeError(
"Mismatch between data selection {0} and length of phase array ({1})!"
.format(time_mask.sum(), len(phases)))
data_to_add["PULSE_PHASE"] = [phases, "D"]
if args.absphase:
data_to_add["ABS_PHASE"] = [iphss, "K"]
if args.barytime:
bats = modelin.get_barycentric_toas(ts)
data_to_add["BARY_TIME"] = [bats, "D"]
if args.addorbphase:
if time_mask.sum() != len(orbphases):
raise RuntimeError(
"Mismatch between data selection ({0}) and length of orbital phase array ({1})!"
.format(time_mask.sum(), len(orbphases)))
data_to_add["ORBIT_PHASE"] = [orbphases, "D"]
# End if args.addorbphase
for key in data_to_add.keys():
if key in hdulist[1].columns.names:
log.info("Found existing %s column, overwriting..." % key)
# Overwrite values in existing Column
hdulist[1].data[key][time_mask] = data_to_add[key][0]
else:
# Construct and append new column, preserving HDU header and name
log.info("Adding new %s column." % key)
new_dat = np.full(time_mask.shape,
-1,
dtype=data_to_add[key][0].dtype)
new_dat[time_mask] = data_to_add[key][0]
datacol.append(
pyfits.ColDefs([
pyfits.Column(name=key,
format=data_to_add[key][1],
array=new_dat)
]))
if len(datacol) > 0:
cols = hdulist[1].columns
for c in datacol:
cols = cols + c
bt = pyfits.BinTableHDU.from_columns(cols,
header=hdulist[1].header,
name=hdulist[1].name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info("Overwriting existing FITS file " + args.eventfile)
hdulist.flush(verbose=True, output_verify="warn")
else:
# Write to new output file
log.info("Writing output FITS file " + args.outfile)
hdulist.writeto(args.outfile,
overwrite=True,
checksum=True,
output_verify="warn")
def generate_polycos(
self,
model,
mjdStart,
mjdEnd,
obs,
segLength,
ncoeff,
obsFreq,
maxha=12.0,
method="TEMPO",
numNodes=20,
):
"""
Generate the polyco data.
Parameters
----------
model : TimingModel
TimingModel to generate the Polycos with parameters
setup.
mjdStart : float / numpy longdouble
Start time of polycos in mjd
mjdEnd : float / numpy longdouble
Ending time of polycos in mjd
obs : str
Observatory code
segLength : int
Length of polyco segement [minutes]
ncoeff : int
Number of coefficents
obsFreq : float
Observing frequency [MHz]
maxha : float optional. Default 12.0
Maximum hour angle. Only 12.0 is supported for now.
method : string optional ["TEMPO", "TEMPO2", ...] Default TEMPO
Method to generate polycos. Only the TEMPO method is supported for now.
numNodes : int optional. Default 20
Number of nodes for fitting. It cannot be less then the number of
coefficents.
Return
---------
A polyco table.
"""
mjdStart = data2longdouble(mjdStart)
mjdEnd = data2longdouble(mjdEnd)
segLength = int(segLength)
obsFreq = float(obsFreq)
# Use the planetary ephemeris specified in the model, if available.
if model.EPHEM.value is not None:
ephem = model.EPHEM.value
else:
log.info(
"No ephemeris specified in model, using DE421 to generate polycos"
)
ephem = "DE421"
if maxha != 12.0:
raise ValueError("Maximum hour angle != 12.0 is not supported.")
# Make sure the number of nodes is bigger than number of coeffs.
if numNodes < ncoeff:
numNodes = ncoeff + 1
mjdSpan = data2longdouble(segLength / MIN_PER_DAY)
# Generate "nice" MJDs for consistency with what tempo2 does
tmids = np.arange(
int(mjdStart * 24) * 60,
int(mjdEnd * 24) * 60 + segLength, segLength)
tmids = data2longdouble(tmids) / MIN_PER_DAY
# generate the ploynomial coefficents
if method == "TEMPO":
entryList = []
# Using tempo1 method to create polycos
# If you want to disable the progress bar, add disable=True to the tqdm() call.
for tmid in tqdm(tmids):
tStart = tmid - mjdSpan / 2
tStop = tmid + mjdSpan / 2
nodes = np.linspace(tStart, tStop, numNodes)
toaMid = toa.get_TOAs_list(
[
toa.TOA((np.modf(tmid)[1], np.modf(tmid)[0]),
obs=obs,
freq=obsFreq)
],
ephem=ephem,
)
refPhase = model.phase(toaMid, abs_phase=True)
# Create node toas(Time sample using TOA class)
toaList = [
toa.TOA(
(np.modf(toaNode)[1], np.modf(toaNode)[0]),
obs=obs,
freq=obsFreq,
) for toaNode in nodes
]
toas = toa.get_TOAs_list(toaList, ephem=ephem)
ph = model.phase(toas, abs_phase=True)
dt = (nodes - tmid) * MIN_PER_DAY
rdcPhase = ph - refPhase
rdcPhase = rdcPhase.int - (dt * model.F0.value *
60.0) + rdcPhase.frac
dtd = dt.astype(float) # Truncate to double
rdcPhased = rdcPhase.astype(float)
coeffs = np.polyfit(dtd, rdcPhased, ncoeff - 1)[::-1]
date, hms = Time(tmid, format="mjd", scale="utc").iso.split()
yy, mm, dd = date.split("-")
date = dd + "-" + MONTHS[int(mm) - 1] + "-" + yy[-2:]
hms = float(hms.replace(":", ""))
entry = PolycoEntry(
tmid,
segLength,
refPhase.int,
refPhase.frac,
model.F0.value,
ncoeff,
coeffs,
)
entry_dict = OrderedDict()
entry_dict["psr"] = model.PSR.value
entry_dict["date"] = date
entry_dict["utc"] = hms
entry_dict["tmid"] = tmid
entry_dict["dm"] = model.DM.value
entry_dict["doppler"] = 0.0
entry_dict["logrms"] = 0.0
entry_dict["mjd_span"] = segLength
entry_dict["t_start"] = entry.tstart
entry_dict["t_stop"] = entry.tstop
entry_dict["obs"] = obs
entry_dict["obsfreq"] = obsFreq
if model.is_binary:
binphase = model.orbital_phase(toaMid, radians=False)[0]
entry_dict["binary_phase"] = binphase
b = model.get_components_by_category()["pulsar_system"][0]
entry_dict["f_orbit"] = 1 / b.PB.value
entry_dict["entry"] = entry
entryList.append(entry_dict)
pTable = table.Table(entryList, meta={"name": "Polyco Data Table"})
self.polycoTable = pTable
if len(self.polycoTable) == 0:
raise ValueError("Zero polycos found for table")
else:
raise NotImplementedError(
"Only TEMPO method has been implemented.")
def d_phase_d_toa(self,
toas,
time_intval=60,
method=None,
num_sample=20,
order=11):
"""Return the derivative of phase wrt TOA
time_intval: is in seconds
method: with finite difference and chebyshev interpolation
"""
d_phase_d_toa = np.zeros(len(toas))
if method is None or "FDM":
# Using finite difference to calculate the derivitve
dt = np.longdouble(time_intval) / np.longdouble(num_sample)
num_sample = int(num_sample) / 2 * 2 + 1
for i, singal_toa in enumerate(toas):
toa_utc_ld = utils.time_to_longdouble(singal_toa['mjd'])
# Resample the toa points
domain = (toa_utc_ld - time_intval / 2.0,
toa_utc_ld + time_intval / 2.0)
sample = np.linspace(domain[0], domain[1], num_sample)
toa_list = []
for sample_time in sample:
toa_list.append(
toa.TOA(
(np.modf(sample_time)[1], np.modf(sample_time)[0]),
obs=singal_toa['obs'],
freq=singal_toa['freq']))
sample_toalist = toa.get_TOAs_list(toa_list)
ph = self.phase(sample_toalist.table)
p = ph.int - ph.int.min() + ph.frac
p = np.array(p, dtype='float64')
# Reduce the value of samples in order to use double precision
reduce_samepl = np.array((sample - sample.min()) * 86400.0,
dtype='float64')
dx = np.gradient(reduce_samepl)
dp = np.gradient(p - p.mean(), dx)
d_phase_d_toa[i] = dp[num_sample / 2]
if method is "chebyshev":
# Using chebyshev interpolation to calculate the
for i, singal_toa in enumerate(toas):
# Have more sample point around toa
toa_utc_ld = utils.time_to_longdouble(singal_toa['mjd'])
domain = (toa_utc_ld - time_intval / 2.0,
toa_utc_ld + time_intval / 2.0)
sample = np.linspace(domain[0], domain[1], num_sample)
toa_list = []
for sample_time in sample:
toa_list.append(
toa.TOA(
(np.modf(sample_time)[1], np.modf(sample_time)[0]),
obs=singal_toa['obs'],
freq=singal_toa['freq']))
sample_toalist = toa.get_TOAs_list(toa_list)
# Calculate phase
ph = self.phase(sample_toalist.table)
p = ph.int - ph.int.min() + ph.frac
p = np.array(p, dtype='float64')
# reduce the phase value to use double precision
reduce_samepl = np.array((sample - sample.min()) * 86400.0,
dtype='float64')
coeff = np.polynomial.chebyshev.chebfit(
reduce_samepl, p, order)
dcoeff = np.polynomial.chebyshev.chebder(coeff)
dy = np.polynomial.chebyshev.chebval(reduce_samepl, dcoeff)
d_phase_d_toa[i] = dy[num_sample / 2]
return d_phase_d_toa
def main(argv=None):
parser = argparse.ArgumentParser(
description=
"Use PINT to compute H-test and plot Phaseogram from a Fermi FT1 event file."
)
parser.add_argument("eventfile", help="Fermi event FITS file name.")
parser.add_argument("parfile", help="par file to construct model from")
parser.add_argument(
"weightcol",
help="Column name for event weights (or 'CALC' to compute them)")
parser.add_argument("--ft2", help="Path to FT2 file.", default=None)
parser.add_argument(
"--addphase",
help="Write FT1 file with added phase column",
default=False,
action="store_true",
)
parser.add_argument("--plot",
help="Show phaseogram plot.",
action="store_true",
default=False)
parser.add_argument("--plotfile",
help="Output figure file name (default=None)",
default=None)
parser.add_argument("--maxMJD",
help="Maximum MJD to include in analysis",
default=None)
parser.add_argument("--minMJD",
help="Minimum MJD to include in analysis",
default=None)
parser.add_argument(
"--outfile",
help="Output figure file name (default is to overwrite input file)",
default=None,
)
parser.add_argument(
"--planets",
help="Use planetary Shapiro delay in calculations (default=False)",
default=False,
action="store_true",
)
parser.add_argument("--ephem",
help="Planetary ephemeris to use (default=DE421)",
default="DE421")
args = parser.parse_args(argv)
# If outfile is specified, that implies addphase
if args.outfile is not None:
args.addphase = True
# Read in model
modelin = pint.models.get_model(args.parfile)
if "ELONG" in modelin.params:
tc = SkyCoord(
modelin.ELONG.quantity,
modelin.ELAT.quantity,
frame="barycentrictrueecliptic",
)
else:
tc = SkyCoord(modelin.RAJ.quantity,
modelin.DECJ.quantity,
frame="icrs")
if args.ft2 is not None:
# Instantiate Fermi observatory once so it gets added to the observatory registry
get_satellite_observatory("Fermi", args.ft2)
# Read event file and return list of TOA objects
maxmjd = np.inf if (args.maxMJD is None) else float(args.maxMJD)
minmjd = 0.0 if (args.minMJD is None) else float(args.minMJD)
tl = load_Fermi_TOAs(
args.eventfile,
maxmjd=maxmjd,
minmjd=minmjd,
weightcolumn=args.weightcol,
targetcoord=tc,
)
# Now convert to TOAs object and compute TDBs and posvels
# For Fermi, we are not including GPS or TT(BIPM) corrections
ts = toa.get_TOAs_list(
tl,
include_gps=False,
include_bipm=False,
planets=args.planets,
ephem=args.ephem,
)
ts.filename = args.eventfile
print(ts.get_summary())
mjds = ts.get_mjds()
print(mjds.min(), mjds.max())
# Compute model phase for each TOA
iphss, phss = modelin.phase(ts, abs_phase=True)
phss %= 1
phases = phss.value
mjds = ts.get_mjds()
weights = np.array([w["weight"] for w in ts.table["flags"]])
h = float(hmw(phases, weights))
print("Htest : {0:.2f} ({1:.2f} sigma)".format(h, h2sig(h)))
if args.plot:
log.info("Making phaseogram plot with {0} photons".format(len(mjds)))
phaseogram(mjds, phases, weights, bins=100, plotfile=args.plotfile)
if args.addphase:
# Read input FITS file (again).
# If overwriting, open in 'update' mode
if args.outfile is None:
hdulist = pyfits.open(args.eventfile, mode="update")
else:
hdulist = pyfits.open(args.eventfile)
event_hdu = hdulist[1]
event_hdr = event_hdu.header
event_dat = event_hdu.data
event_mjds = read_fits_event_mjds_tuples(event_hdu)
mjds_float = np.asarray([r[0] + r[1] for r in event_mjds])
time_mask = np.logical_and((mjds_float > minmjd),
(mjds_float < maxmjd))
new_phases = np.full(len(event_dat), -1, dtype=float)
new_phases[time_mask] = phases
if "PULSE_PHASE" in event_hdu.columns.names:
log.info("Found existing PULSE_PHASE column, overwriting...")
# Overwrite values in existing Column
event_dat["PULSE_PHASE"] = new_phases
else:
# Construct and append new column, preserving HDU header and name
log.info("Adding new PULSE_PHASE column.")
phasecol = pyfits.ColDefs([
pyfits.Column(name="PULSE_PHASE", format="D", array=new_phases)
])
bt = pyfits.BinTableHDU.from_columns(event_hdu.columns + phasecol,
header=event_hdr,
name=event_hdu.name)
hdulist[1] = bt
if args.outfile is None:
# Overwrite the existing file
log.info("Overwriting existing FITS file " + args.eventfile)
hdulist.flush(verbose=True, output_verify="warn")
else:
# Write to new output file
log.info("Writing output FITS file " + args.outfile)
hdulist.writeto(args.outfile,
overwrite=True,
checksum=True,
output_verify="warn")
return 0
def generate_polycos(self, model, mjdStart, mjdEnd, obs,
segLength, ncoeff, obsFreq, maxha,
method = "TEMPO",numNodes = 20):
"""
Generate the polyco file data file.
Parameters
---------
model : TimingModel
TimingModel for generate the Polycos with parameters
setup.
mjdStart : float / nump longdouble
Start time of polycos in mjd
mjdEnd : float / nump longdouble
Ending time of polycos in mjd
obs : str
Observatory code
segLength :
Length of polyco segement [unit: minutes]
ncoeff :
number of coefficents
obsFreq :
observing frequency
maxha :
Maximum hour angle
method : sting optional ['TEMPO','TEMPO2',...] Default TEMPO
Method to generate polycos. Now it is only support the TEMPO method.
numNodes : int optional. Default 20
Number of nodes for fitting. It can not be less then the number of
coefficents.
Return
---------
A polyco table.
"""
mjdStart = np.longdouble(mjdStart)*u.day
mjdEnd = np.longdouble(mjdEnd)*u.day
timeLength = mjdEnd-mjdStart
segLength = np.longdouble(segLength)*u.min
obsFreq = float(obsFreq)
month = ['Jan','Feb','Mar','Apr','May','Jun','Jul','Aug',
'Sep','Oct','Nov','Dec']
# Alocate memery
coeffs = np.longdouble(np.zeros(ncoeff))
entryList = []
entryIntvl = np.arange(mjdStart.value,mjdEnd.value,
segLength.to('day').value)
if entryIntvl[-1] < mjdEnd.value:
entryIntvl = np.append(entryIntvl, mjdEnd.value)
# Make sure the number of nodes is bigger then number of coeffs.
if numNodes < ncoeff:
numNodes = ncoeff+1
# generate the ploynomial coefficents
if method == "TEMPO":
# Using tempo1 method to create polycos
for i in range(len(entryIntvl)-1):
tStart = entryIntvl[i]
tStop = entryIntvl[i+1]
nodes = np.linspace(tStart,tStop,numNodes)
tmid = ((tStart+tStop)/2.0)*u.day
toaMid = toa.get_TOAs_list([toa.TOA((np.modf(tmid.value)[1],
np.modf(tmid.value)[0]),obs = obs,
freq = obsFreq),])
refPhase = model.phase(toaMid.table)
mjdSpan = ((tStop-tStart)*u.day).to('min')
# Create node toas(Time sample using TOA class)
toaList = [toa.TOA((np.modf(toaNode)[1],
np.modf(toaNode)[0]),obs = obs,
freq = obsFreq) for toaNode in nodes]
toas = toa.get_TOAs_list(toaList)
ph = model.phase(toas.table)
dt = (nodes*u.day - tmid).to('min') # Use constant
rdcPhase = ph-refPhase
rdcPhase = rdcPhase.int-dt.value*model.F0.value*60.0+rdcPhase.frac
dtd = dt.value.astype(float) # Trancate to double
rdcPhased = rdcPhase.astype(float)
coeffs = np.polyfit(dtd,rdcPhased,ncoeff-1)
coeffs = coeffs[::-1]
midTime = at.Time(int(tmid.value),np.modf(tmid.value)[0],
format = 'mjd',scale = 'utc')
date,hms = midTime.iso.split()
yy,mm,dd = date.split('-')
date = dd+'-'+month[int(mm)-1]+'-'+yy[2:4]
hms = hms.replace(':',"")
entry = polycoEntry(tmid.value,mjdSpan.to('day').value,
refPhase.int,refPhase.frac, model.F0.value, ncoeff,
coeffs,obs)
entryList.append((model.PSR.value, date, hms, tmid.value,
model.DM.value,0.0,0.0,0.0,obsFreq,entry))
pTable = table.Table(rows = entryList, names = ('psr','date','utc',
'tmid','dm','dopper','logrms','binary_phase',
'obsfreq','entry'),
meta={'name': 'Ployco Data Table'})
self.polycoTable = pTable
else:
# Reading from an old polycofile
pass
