def __init__(self, freqbands=[[0, 'inf']]):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files. Also find output .par file.
inputfiles_re = re.compile(r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
match = inputfiles_re.search(line)
if match:
intimfn = match.group(1).strip()
inparfn = match.group(2).strip()
else:
match = outputfile_re.search(line)
if match:
outparfn = "%s.par" % match.group(1).strip()
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
# Need to check if on 32-bit or 64-bit computer
#(the following is a hack to find out if we're on a borg or borgii node)
#PATRICKS QUICK FIX 10/14 - 3/39/11 read_residuals_64bit does not work on nimrod or my machine, but 32bit does...
#print os.uname()[4]
if True: #os.uname()[4]=='i686':
# 32-bit computer
r = residuals.read_residuals()
else:
# 64-bit computer
r = residuals.read_residuals_64bit()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
self.freqbands = freqbands
self.residuals = {}
for lo,hi in self.freqbands:
indices = (r.bary_freq>=lo) & (r.bary_freq<hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices], \
np.arange(r.numTOAs)[indices], r.orbit_phs[indices], \
r.postfit_phs[indices], r.postfit_sec[indices], \
r.prefit_phs[indices], r.prefit_sec[indices], \
r.uncertainty[indices], r.weight[indices], \
self.inpar, self.outpar)
def __init__(self, freqbands):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files. Also find output .par file.
inputfiles_re = re.compile(
r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
if line[:15] == "Input data from":
sline = line.split()
intimfn = sline[3][:-1] # strip the comma
intimbase = os.path.splitext(intimfn)[0]
inparfn = intimbase + ".par" if sline[6] == 'def' else sline[6]
if inparfn[-1] == ".": inparfn = inparfn[:-1]
elif line[:15] == "Assumed paramet":
outparfn = line.split()[-1] + ".par"
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
r = residuals.read_residuals()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
if freqbands is None:
self.freqbands = find_freq_clusters(r.bary_freq)
else:
self.freqbands = freqbands
self.residuals = {}
for lo, hi in self.freqbands:
indices = (r.bary_freq >= lo) & (r.bary_freq < hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices], \
np.arange(r.numTOAs)[indices], r.orbit_phs[indices], \
r.postfit_phs[indices], r.postfit_sec[indices], \
r.prefit_phs[indices], r.prefit_sec[indices], \
r.uncertainty[indices], r.weight[indices], \
self.inpar, self.outpar)
def __init__(self, freqbands):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files. Also find output .par file.
inputfiles_re = re.compile(
r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
match = inputfiles_re.search(line)
if match:
intimfn = match.group(1).strip()
inparfn = match.group(2).strip()
else:
match = outputfile_re.search(line)
if match:
outparfn = "%s.par" % match.group(1).strip()
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
r = residuals.read_residuals()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
if freqbands is None:
self.freqbands = find_freq_clusters(r.bary_freq)
else:
self.freqbands = freqbands
self.residuals = {}
for lo, hi in self.freqbands:
indices = (r.bary_freq >= lo) & (r.bary_freq < hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices], \
np.arange(r.numTOAs)[indices], r.orbit_phs[indices], \
r.postfit_phs[indices], r.postfit_sec[indices], \
r.prefit_phs[indices], r.prefit_sec[indices], \
r.uncertainty[indices], r.weight[indices], \
self.inpar, self.outpar)
def __init__(self, freqbands):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files. Also find output .par file.
inputfiles_re = re.compile(r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
if line[:15]=="Input data from":
sline = line.split()
intimfn = sline[3][:-1] # strip the comma
intimbase = os.path.splitext(intimfn)[0]
inparfn = intimbase+".par" if sline[6]=='def' else sline[6]
if inparfn[-1]==".": inparfn = inparfn[:-1]
elif line[:15]=="Assumed paramet":
outparfn = line.split()[-1]+".par"
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
r = residuals.read_residuals()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
if freqbands is None:
self.freqbands = find_freq_clusters(r.bary_freq)
else:
self.freqbands = freqbands
self.residuals = {}
for lo,hi in self.freqbands:
indices = (r.bary_freq>=lo) & (r.bary_freq<hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices], \
np.arange(r.numTOAs)[indices], r.orbit_phs[indices], \
r.postfit_phs[indices], r.postfit_sec[indices], \
r.prefit_phs[indices], r.prefit_sec[indices], \
r.uncertainty[indices], r.weight[indices], \
self.inpar, self.outpar)
def __init__(self, freqbands):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files. Also find output .par file.
inputfiles_re = re.compile(r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
match = inputfiles_re.search(line)
if match:
intimfn = match.group(1).strip()
inparfn = match.group(2).strip()
else:
match = outputfile_re.search(line)
if match:
outparfn = "%s.par" % match.group(1).strip()
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
r = residuals.read_residuals()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
if freqbands is None:
self.freqbands = find_freq_clusters(r.bary_freq)
else:
self.freqbands = freqbands
self.residuals = {}
for lo,hi in self.freqbands:
indices = (r.bary_freq>=lo) & (r.bary_freq<hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices], \
np.arange(r.numTOAs)[indices], r.orbit_phs[indices], \
r.postfit_phs[indices], r.postfit_sec[indices], \
r.prefit_phs[indices], r.prefit_sec[indices], \
r.uncertainty[indices], r.weight[indices], \
self.inpar, self.outpar)
def parse_eph(filenm):
global period, time
suffix = filenm.split(".")[-1]
if suffix=="bestprof":
x = bestprof.bestprof(filenm)
fs = pu.p_to_f(x.p0_bary, x.p1_bary, x.p2_bary)
epoch = x.epochi_bary + x.epochf_bary
T = x.T
elif suffix=="par":
x = parfile.psr_par(filenm)
# Try to see how many freq derivs we have
fs = [x.F0]
for ii in range(1, 20): # hopefully 20 is an upper limit!
attrib = "F%d"%ii
if hasattr(x, attrib):
fs.append(getattr(x, attrib))
else:
break
epoch = x.PEPOCH
T = (x.FINISH - x.START) * 86400.0
else:
print("I don't recognize the file type for", filenm)
sys.exit()
newts = epoch + num.arange(int(T/10.0+0.5), dtype=num.float)/8640.0
time = num.concatenate((time, newts))
newps = 1.0 / pu.calc_freq(newts, epoch, *fs)
period = num.concatenate((period, newps))
print("%13.7f (%0.1f sec): " % (epoch, T), fs)
def __init__(self, parfilenm):
self.par = parfile.psr_par(parfilenm)
if not hasattr(self.par, 'BINARY'):
print("'%s' doesn't contain parameters for a binary pulsar!")
return None
self.PBsec = self.par.PB * SECPERDAY
self.T0 = self.par.T0
def read_par(pfname,f1errmax=999.0):
pf = parfile.psr_par(pfname)
f0 = pf.F0
p0 = pf.P0
try:
f0err = pf.F0_ERR
except:
f0err = 2.0e-5
if not isfinite(f0err):
f0err = 3.0e-5
f1 = pf.F1
try:
p1 = pf.P1
except:
p1 = 0.0
try:
f1err = pf.F1_ERR
except:
f1err = 10.0e-8
mjd = pf.PEPOCH
if (verbose):
# print "%6s: %.4f F0 %10.9g +/- %8.03g F1 %10.5g +/- %8.03g" % (pfname,mjd,f0,f0err,f1,f1err)
print "%.4f %10.9g %8.3g %10.5g %8.3g" % (mjd,f0,f0err,f1,f1err),
if (f1err > f1errmax):
print " * Ignored *"
else:
print
# print " P0 = %g, P1 = %g" % (p0,p1)
print "----- ",pfname
print "PEPOCH ",mjd
print "F0 ", f0
print "F1 ", f1
return mjd,f0,f0err,f1,f1err
def parse_eph(filenm):
global period, time
suffix = filenm.split(".")[-1]
if suffix == "bestprof":
x = bestprof.bestprof(filenm)
fs = pu.p_to_f(x.p0_bary, x.p1_bary, x.p2_bary)
epoch = x.epochi_bary + x.epochf_bary
T = x.T
elif suffix == "par":
x = parfile.psr_par(filenm)
# Try to see how many freq derivs we have
fs = [x.F0]
for ii in range(1, 20): # hopefully 20 is an upper limit!
attrib = "F%d" % ii
if hasattr(x, attrib):
fs.append(getattr(x, attrib))
else:
break
epoch = x.PEPOCH
T = (x.FINISH - x.START) * 86400.0
else:
print "I don't recognize the file type for", filenm
sys.exit()
newts = epoch + num.arange(int(T / 10.0 + 0.5), dtype=num.float) / 8640.0
time = num.concatenate((time, newts))
newps = 1.0 / pu.calc_freq(newts, epoch, *fs)
period = num.concatenate((period, newps))
print "%13.7f (%0.1f sec): " % (epoch, T), fs
def create_polycos(parfn, telescope_id, center_freq, start_mjd, end_mjd, \
max_hour_angle=None, span=SPAN_DEFAULT, \
numcoeffs=NUMCOEFFS_DEFAULT, keep_file=False):
"""Create polycos object from a parfile.
Inputs:
parfn: parfile's filename, or a parfile object.
telescope_id: The TEMPO 1-character telescope identifier.
center_freq: The observation's center frequencies in MHz.
start_mjd: MJD on which the polycos should start.
end_mjd: MJD until the polycos should extend.
max_hour_angle: The maximum hour angle as expected by tempo.
(Default: Use default value chosen for given telescope).
span: Span of each set of polycos in min.
(Default: 60 min).
numcoeffs: Number of coefficients to use.
(Default: 12).
keep_file: If true do not delete polyco.dat file.
(Default: delete polyco.dat file).
Output:
new_polycos: a polycos object.
"""
if type(parfn)==types.StringType:
# assume parfn is a filename
par = parfile.psr_par(parfn)
else:
# assume par is already a parfile.psr_par object
par = parfn
if max_hour_angle is None:
telescope_name = id_to_telescope[telescope_id]
max_hour_angle = telescope_to_maxha[telescope_name]
tzfile = open("tz.in", "w")
# Default parameters for prediction mode
tzfile.write("%s %d %d %d %0.5f\n" % (telescope_id, max_hour_angle, \
SPAN_DEFAULT, NUMCOEFFS_DEFAULT, center_freq))
# TEMPO ignores lines 2 and 3 in tz.in file
tzfile.write("\n\n")
if hasattr(par, "PSR"):
psrname = par.PSR
else:
psrname = par.PSRJ
tzfile.write("%s %d %d %d %0.5f\n" % (psrname, SPAN_DEFAULT, \
NUMCOEFFS_DEFAULT, max_hour_angle, center_freq))
tzfile.close()
tempo = subprocess.Popen("tempo -z -f %s" % par.FILE, shell=True, \
stdin=subprocess.PIPE, stdout=subprocess.PIPE, \
stderr=subprocess.PIPE)
(out, err) = tempo.communicate("%d %d\n" % (start_mjd, end_mjd))
if err:
raise TempoError("The following error message was encountered " \
"when running TEMPO to generate polycos from " \
"the input parfile (%s):\n\n%s\n" % (parfn, err))
new_polycos = polycos(psrname, filenm='polyco.dat')
# Remove files created by us and by TEMPO
os.remove("tz.in")
if not keep_file:
os.remove("polyco.dat")
return new_polycos
def __init__(self, parfilenm):
self.par = parfile.psr_par(parfilenm)
if not hasattr(self.par, 'BINARY'):
print "'%s' doesn't contain parameters for a binary pulsar!"
return None
self.PBsec = self.par.PB*SECPERDAY
self.T0 = self.par.T0
def create_polycos(parfn, telescope_id, center_freq, start_mjd, end_mjd, \
max_hour_angle=None, span=SPAN_DEFAULT, \
numcoeffs=NUMCOEFFS_DEFAULT, keep_file=False):
"""Create polycos object from a parfile.
Inputs:
parfn: parfile's filename, or a parfile object.
telescope_id: The TEMPO 1-character telescope identifier.
center_freq: The observation's center frequencies in MHz.
start_mjd: MJD on which the polycos should start.
end_mjd: MJD until the polycos should extend.
max_hour_angle: The maximum hour angle as expected by tempo.
(Default: Use default value chosen for given telescope).
span: Span of each set of polycos in min.
(Default: 60 min).
numcoeffs: Number of coefficients to use.
(Default: 12).
keep_file: If true do not delete polyco.dat file.
(Default: delete polyco.dat file).
Output:
new_polycos: a polycos object.
"""
if type(parfn) == types.StringType:
# assume parfn is a filename
par = parfile.psr_par(parfn)
else:
# assume par is already a parfile.psr_par object
par = parfn
if max_hour_angle is None:
telescope_name = id_to_telescope[telescope_id]
max_hour_angle = telescope_to_maxha[telescope_name]
tzfile = open("tz.in", "w")
# Default parameters for prediction mode
tzfile.write("%s %d %d %d %0.5f\n" % (telescope_id, max_hour_angle, \
SPAN_DEFAULT, NUMCOEFFS_DEFAULT, center_freq))
# TEMPO ignores lines 2 and 3 in tz.in file
tzfile.write("\n\n")
if hasattr(par, "PSR"):
psrname = par.PSR
else:
psrname = par.PSRJ
tzfile.write("%s %d %d %d %0.5f\n" % (psrname, SPAN_DEFAULT, \
NUMCOEFFS_DEFAULT, max_hour_angle, center_freq))
tzfile.close()
tempo = subprocess.Popen("tempo -z -f %s" % par.FILE, shell=True, \
stdin=subprocess.PIPE, stdout=subprocess.PIPE, \
stderr=subprocess.PIPE)
(out, err) = tempo.communicate("%d %d\n" % (start_mjd, end_mjd))
if err:
raise TempoError("The following error message was encountered " \
"when running TEMPO to generate polycos from " \
"the input parfile (%s):\n\n%s\n" % (parfn, err))
new_polycos = polycos(psrname, filenm='polyco.dat')
# Remove files created by us and by TEMPO
os.remove("tz.in")
if not keep_file:
os.remove("polyco.dat")
return new_polycos
def __init__(self, parfilenm, leap=True):
self.par = parfile.psr_par(parfilenm)
if not hasattr(self.par, 'BINARY'):
print "'%s' doesn't contain parameters for a binary pulsar!"
return None
self.PBsec = self.par.PB * SECPERDAY
self.T0 = self.par.T0
self.leap = leap
self.leap_MJDs = np.r_[41499., 41683., 42048., 42413., 42778., 43144.,
43509., 43874., 44239., 44786., 45151., 45516.,
46247., 47161., 47892., 48257., 48804., 49169.,
49534., 50083., 50630., 51179., 53736., 54832.,
56109., 57204.]
def read_par(pfname, f1errmax=999.0):
pf = parfile.psr_par(pfname)
# Try to see how many freq derivs we have
fs = [pf.F0]
for ii in range(1, 20): # hopefully 20 is an upper limit!
attrib = "F%d" % ii
if hasattr(pf, attrib):
fs.append(getattr(pf, attrib))
else:
break
epoch = pf.PEPOCH
Tobs = (pf.FINISH - pf.START) * 86400.0
return epoch, Tobs, fs
def read_par(pfname, f1errmax=999.0):
pf = parfile.psr_par(pfname)
# Try to see how many freq derivs we have
fs = [pf.F0]
for ii in range(1, 20): # hopefully 20 is an upper limit!
attrib = "F%d" % ii
if hasattr(pf, attrib):
fs.append(getattr(pf, attrib))
else:
break
epoch = pf.PEPOCH
Tobs = (pf.FINISH - pf.START) * 86400.0
return epoch, Tobs, fs
def read_par(pfname, f1errmax=999.0):
pf = parfile.psr_par(pfname)
f0 = pf.F0
p0 = pf.P0
try:
f0err = pf.F0_ERR
except:
f0err = 2.0e-5
if not isfinite(f0err):
f0err = 3.0e-5
f1 = pf.F1
try:
p1 = pf.P1
except:
p1 = 0.0
try:
f1err = pf.F1_ERR
except:
f1err = 10.0e-8
mjd = pf.PEPOCH
if (verbose):
# print "%6s: %.4f F0 %10.9g +/- %8.03g F1 %10.5g +/- %8.03g" % (pfname,mjd,f0,f0err,f1,f1err)
print("%.4f %10.9g %8.3g %10.5g %8.3g" % (mjd, f0, f0err, f1, f1err),
end=' ')
if (f1err > f1errmax):
print(" * Ignored *")
else:
print()
# print " P0 = %g, P1 = %g" % (p0,p1)
print("----- ", pfname)
print("PEPOCH ", mjd)
print("F0 ", f0)
print("F1 ", f1)
return mjd, f0, f0err, f1, f1err
def __init__(self, freqbands):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files.
# Also find output .par file.
inputfiles_re = re.compile(
r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
match = inputfiles_re.search(line)
if match:
intimfn = match.group(1).strip()
inparfn = match.group(2).strip()
else:
match = outputfile_re.search(line)
if match:
outparfn = "%s.par" % match.group(1).strip()
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
self.phase_wraps = {}
#self.jump_ranges = []
tim = tempy_io.TOAfile.from_tim_file(intimfn)
#tim_ordered_index = np.argsort(tim.TOAs)
# if there are phase wraps in the tim file, we want to include those
# in the intial plot
for tim_wrap_pos in tim.phase_wraps:
#wrap_index = tim_ordered_index[tim_wrap_index]
wrap_index = tim.get_nTOAs(tim_wrap_pos[0]) + tim_wrap_pos[1]
self.phase_wraps[wrap_index] = \
tim.phase_wraps[tim_wrap_pos]
# if there are jumps in the tim file, we want to include those in the
# initial plot
self.jump_ranges = tim.get_jump_ranges()
#self.ordered_jump_ranges = tim.get_jump_ranges(chronological=True)
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
r = residuals.read_residuals()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
self.ordered_index = np.argsort(r.bary_TOA)
self.ordered_MJDs = r.bary_TOA[self.ordered_index]
timfile_index = np.arange(r.numTOAs)
if freqbands is None:
self.freqbands = find_freq_clusters(r.bary_freq)
else:
self.freqbands = freqbands
self.residuals = {}
for lo, hi in self.freqbands:
indices = (r.bary_freq >= lo) & (r.bary_freq < hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices],
np.arange(r.numTOAs)[indices],
#ordered_index[indices],
r.orbit_phs[indices],
r.postfit_phs[indices], r.postfit_sec[indices],
r.prefit_phs[indices], r.prefit_sec[indices],
r.uncertainty[indices], r.weight[indices],
self.inpar, self.outpar)
help="choose subintegration number",
default='5')
args = parser.parse_args()
# Open pfds.
pfdtype = '*.pfd'
pfds = glob.glob(pfdtype)
pfds.sort()
# Basic Labeling
pulsar = args.name
timingfolder = '/opt/pulsar/puma/config/timing/'
timingpar = timingfolder + '{}.par'.format(pulsar)
pulsarpar = parfile.psr_par(timingpar)
scoord = pulsarpar.RAJ + pulsarpar.DECJ
for pfd in pfds:
subprocess.call([
'psredit', '-c', 'coord=' + scoord, '-c', 'name=' + pulsar, '-m', pfd
])
subprocess.call([
'psredit', '-c', 'obs:projid=PuMA', '-c', 'be:name=Ettus-SDR', '-m',
pfd
])
# Choose a given template named 'pulsar.pfd.std'
usingtemplate = timingfolder + '{}.pfd.std'.format(pulsar)
from astropy import log
if __name__ == '__main__':
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. Should be GEOCENTERED.")
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("--maxMJD",help="Maximum MJD to include in analysis", default=None)
parser.add_argument("--outfile",help="Output figure file name (default=None)", 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()
pf = psr_par(args.parfile)
# Read event file and return list of TOA objects
tl = load_Fermi_TOAs(args.eventfile, weightcolumn=args.weightcol,
targetcoord=SkyCoord(pf.RAJ,pf.DECJ,unit=(u.hourangle,u.degree),frame='icrs'))
# 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
def generateObservingPlan(session,startAt,endAt,minTimePerSource=2200.0, tslew = 600.0):
lastRise = startAt
radecs = {}
riseSet = {}
riseSetList = []
parfiles = []
for source,parfile,band in session:
if radecs.has_key(parfile):
continue
parfiles.append(parfile)
par = psr_par(parfile)
try:
ra = par.RAJ
dec = par.DECJ
except:
try:
ra = par.RA
dec = par.DEC
except:
raise Exception( "Error reading RA/DEC from parfile.")
rh,rm,rs = map(float,ra.split(':'))
dd,dm,ds = map(float,dec.split(':'))
radeg = astro_utils.hms_to_rad(rh,rm,rs)*astro_utils.RADTODEG
decdeg = dd + dm/60.0 + ds/3600.0
radecs[parfile] = (radeg,decdeg)
ts = np.arange(lastRise-2*3600,lastRise+5*3600,60.0)
zas = np.array([astro_utils.radec_to_azza(radeg,decdeg,epochToMJD(x),scope="ARECIBO")[1] for x in ts])
#print zas[0],zas[-1]
upTimes = ts[(zas<zaLimit)]
keyHole = ts[(zas<2.0)]
if len(keyHole):
print "Warning:",parfile,"is in the key hole from",time.ctime(keyHole[0]),"to",time.ctime(keyHole[1])
riseT,setT = (upTimes[0],upTimes[-1])
riseSet[parfile] = riseT,setT
lastRise = upTimes[0]
riseSetList.append((riseT,setT))
print "%10s: Rise %s Set %s Up %.1f min." % (source[:10],time.ctime(riseT),time.ctime(setT), (setT-riseT)/60.)
first = riseSetList[0]
if first[0]< startAt:
first = (startAt,first[1])
begin = startAt
else:
begin = first[0]
riseSetList[0] = first
last = riseSetList[-1]
if last[1]>endAt:
last = (last[0],endAt)
riseSetList[-1] = last
ss,fv = optimizeSchedule(riseSetList, minTimePerSource = minTimePerSource)
startTimes = ss[::2]
stopTimes = ss[1::2]
sourceEndTimes = dict(zip(parfiles,stopTimes))
sourceStartTimes = dict(zip(parfiles,startTimes))
nscans = {}
for source,parfile,band in session:
if nscans.has_key(parfile):
nscans[parfile] += 1
else:
nscans[parfile] = 1
scanEndTimes = []
scanStart = begin
lastpar = None
for source,parfile,band in session:
sourceEnd = sourceEndTimes[parfile]
sourceStart = sourceStartTimes[parfile]
if sourceStart < begin:
sourceStart = begin
timePerScan = (sourceEnd-sourceStart-tslew)/nscans[parfile]
if lastpar == parfile:
#we're on the same source
scanEnd = scanStart + timePerScan
else:
#switching sources so add extra time for slewing
scanEnd = sourceStart + timePerScan + tslew
scanEndTimes.append(scanEnd)
scanStart = scanEnd
lastpar = parfile
return riseSetList,startTimes,stopTimes,scanEndTimes
#!/usr/bin/env python
"""
Given a parfile and an epoch compute the frequency and
its uncertainty at a requested epoch.
"""
import sys
import numpy as np
import parfile
import psr_utils
print sys.argv
par = parfile.psr_par(sys.argv[1])
for epoch in sys.argv[2:]:
epoch = float(epoch)
interval_seconds = (epoch - par.PEPOCH)*psr_utils.SECPERDAY
f = par.F0 + interval_seconds*par.F1
ferr = np.sqrt(par.F0_ERR**2+interval_seconds**2*par.F1_ERR**2)
print "MJD: %f\n\tf: %0.10f\n\t+- %0.12f" % (epoch, f, ferr)
def parse_cmd_line(args):
"""
Parse command line argumentss
Input
-----
args - a list of command line aruments and values
Output
------
user-supplied values for the given arguments
"""
# create a list of valid command line arguments
valid_args = ["-p", "-pb", "-x", "-T0", "-e", "-w", "-par", "-nofit", "-o"]
if len(args) == 0:
print_usage()
exit(0)
for arg in args:
# check to make sure all arguments are valid
if (arg.startswith("-")) and (arg not in valid_args) and \
not arg.strip("-").replace(".","").isdigit():
print "ERROR: Unknown arg %s" % arg
print_usage()
exit(0)
# go through the given arguments and store user-supplied values
try:
const_params = args.pop(args.index("-nofit") + 1)
args.remove("-nofit")
except ValueError:
const_params = ""
pass
if "-par" in args:
try:
par_file_name = args.pop(args.index("-par") + 1)
args.remove("-par")
par = parfile.psr_par(par_file_name)
p = par.P0
pb_days = par.PB
x = par.A1
T0 = par.T0
e = par.E
w = par.OM
except IOError:
print "ERROR: %s not found\n" % par_file_name
exit(0)
except AttributeError:
print "ERROR: %s does not appear to be a valid binary .par file\n" \
%par_file_name
exit(0)
else:
try:
p = float(args.pop(args.index("-p") + 1))
args.remove("-p")
except ValueError:
print "ERROR: You must specify a spin period\n"
exit(0)
try:
pb_days = float(args.pop(args.index("-pb") + 1))
args.remove("-pb")
except ValueError:
print "ERROR: You must specify an orbital period\n"
exit(0)
try:
x = float(args.pop(args.index("-x") + 1))
args.remove("-x")
except ValueError:
print "ERROR: You must specify a projected semi-major axis\n"
exit(0)
try:
T0 = float(args.pop(args.index("-T0") + 1))
args.remove("-T0")
except ValueError:
print "ERROR: You must specify a time of periastron passage\n"
exit(0)
try:
e = float(args.pop(args.index("-e") + 1))
args.remove("-e")
except ValueError:
print "WARNING: Orbital eccentricity not specified, assuming e = 0\n"
e = 0.0
const_params = const_params + ",e"
pass
try:
w = float(args.pop(args.index("-w") + 1))
args.remove("-w")
except ValueError:
print "WARNING: Longitude of periastron not specified, assuming w = 0\n"
w = 0.0
const_params = const_params + ",w"
pass
try:
out_file_root = args.pop(args.index("-o") + 1)
args.remove("-o")
except ValueError:
out_file_root = "fitorb"
pass
in_files = args
return p, pb_days, x, T0, e, w, const_params, out_file_root, in_files
def parse_cmd_line(args):
"""
Parse command line argumentss
Input
-----
args - a list of command line aruments and values
Output
------
user-supplied values for the given arguments
"""
# create a list of valid command line arguments
valid_args = ["-p", "-pb", "-x", "-T0", "-e", "-w", "-par", "-nofit", "-o"]
if len(args) == 0:
print_usage()
exit(0)
for arg in args:
# check to make sure all arguments are valid
if (arg.startswith("-")) and (arg not in valid_args) and not arg.strip("-").replace(".", "").isdigit():
print "ERROR: Unknown arg %s" % arg
print_usage()
exit(0)
# go through the given arguments and store user-supplied values
try:
const_params = args.pop(args.index("-nofit") + 1)
args.remove("-nofit")
except ValueError:
const_params = ""
pass
if "-par" in args:
try:
par_file_name = args.pop(args.index("-par") + 1)
args.remove("-par")
par = parfile.psr_par(par_file_name)
p = par.P0
pb_days = par.PB
x = par.A1
T0 = par.T0
e = par.E
w = par.OM
except IOError:
print "ERROR: %s not found\n" % par_file_name
exit(0)
except AttributeError:
print "ERROR: %s does not appear to be a valid binary .par file\n" % par_file_name
exit(0)
else:
try:
p = float(args.pop(args.index("-p") + 1))
args.remove("-p")
except ValueError:
print "ERROR: You must specify a spin period\n"
exit(0)
try:
pb_days = float(args.pop(args.index("-pb") + 1))
args.remove("-pb")
except ValueError:
print "ERROR: You must specify an orbital period\n"
exit(0)
try:
x = float(args.pop(args.index("-x") + 1))
args.remove("-x")
except ValueError:
print "ERROR: You must specify a projected semi-major axis\n"
exit(0)
try:
T0 = float(args.pop(args.index("-T0") + 1))
args.remove("-T0")
except ValueError:
print "ERROR: You must specify a time of periastron passage\n"
exit(0)
try:
e = float(args.pop(args.index("-e") + 1))
args.remove("-e")
except ValueError:
print "WARNING: Orbital eccentricity not specified, assuming e = 0\n"
e = 0.0
const_params = const_params + ",e"
pass
try:
w = float(args.pop(args.index("-w") + 1))
args.remove("-w")
except ValueError:
print "WARNING: Longitude of periastron not specified, assuming w = 0\n"
w = 0.0
const_params = const_params + ",w"
pass
try:
out_file_root = args.pop(args.index("-o") + 1)
args.remove("-o")
except ValueError:
out_file_root = "fitorb"
pass
in_files = args
return p, pb_days, x, T0, e, w, const_params, out_file_root, in_files
help="Maximum MJD to include in analysis",
default=None)
parser.add_argument("--outfile",
help="Output figure file name (default=None)",
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()
pf = psr_par(args.parfile)
# Read event file and return list of TOA objects
tl = load_Fermi_TOAs(args.eventfile,
weightcolumn=args.weightcol,
targetcoord=SkyCoord(pf.RAJ,
pf.DECJ,
unit=(u.hourangle, u.degree),
frame='icrs'))
# 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)
# Relevant filenames
parfile_name = 'fake.par'
outputfile_name = 'fake.fits'
# Create the Archive instance.
# This is kind of a weird hack, if we create a PSRFITS
# Archive directly, some header info does not get filled
# in. If we instead create an ASP archive, it will automatically
# be (correctly) converted to PSRFITS when it is unloaded...
arch = psrchive.Archive_new_Archive("ASP")
arch.resize(nsub, npol, nchan, nbin)
# Get/set some parameters from the par file. If you don't have
# Presto parfile package installed, can replace this with hard-coded
# (or whatever) values.
par = parfile.psr_par(parfile_name)
arch.set_source(par.PSR)
arch.set_dispersion_measure(par.DM)
# Dec needs to have a sign for the following sky_coord call
if (par.DECJ[0] != '+' and par.DECJ[0] != '-'):
par.DECJ = "+" + par.DECJ
arch.set_coordinates(psrchive.sky_coord(par.RAJ + par.DECJ))
# Set some other stuff
arch.set_centre_frequency(freq)
arch.set_bandwidth(bw)
arch.set_telescope('1')
if npol == 4:
arch.set_state('Coherence') # Could also do 'Stokes' here
# Fill in some integration attributes
# Relevant filenames
parfile_name = 'fake.par'
outputfile_name = 'fake.fits'
# Create the Archive instance.
# This is kind of a weird hack, if we create a PSRFITS
# Archive directly, some header info does not get filled
# in. If we instead create an ASP archive, it will automatically
# be (correctly) converted to PSRFITS when it is unloaded...
arch = psrchive.Archive_new_Archive("ASP")
arch.resize(nsub,npol,nchan,nbin)
# Get/set some parameters from the par file. If you don't have
# Presto parfile package installed, can replace this with hard-coded
# (or whatever) values.
par = parfile.psr_par(parfile_name)
arch.set_source(par.PSR)
arch.set_dispersion_measure(par.DM)
# Dec needs to have a sign for the following sky_coord call
if (par.DECJ[0] != '+' and par.DECJ[0] != '-'):
par.DECJ = "+" + par.DECJ
arch.set_coordinates(psrchive.sky_coord(par.RAJ + par.DECJ))
# Set some other stuff
arch.set_centre_frequency(freq)
arch.set_bandwidth(bw)
arch.set_telescope('1')
if npol==4:
arch.set_state('Coherence') # Could also do 'Stokes' here
# Fill in some integration attributes
#!/usr/bin/env python
"""
Given a parfile and an epoch compute the frequency and
its uncertainty at a requested epoch.
"""
import sys
import numpy as np
import parfile
import psr_utils
print sys.argv
par = parfile.psr_par(sys.argv[1])
for epoch in sys.argv[2:]:
epoch = float(epoch)
interval_seconds = (epoch - par.PEPOCH) * psr_utils.SECPERDAY
f = par.F0 + interval_seconds * par.F1
ferr = np.sqrt(par.F0_ERR**2 + interval_seconds**2 * par.F1_ERR**2)
print "MJD: %f\n\tf: %0.10f\n\t+- %0.12f" % (epoch, f, ferr)
import glob
import os
import shutil
import parfile
# Open pfds.
pfdtype = '*.pfd'
pfds = glob.glob(pfdtype)
pfds.sort()
# Basic Labeling
pardest = './../timing/'
greppar = glob.glob(pardest+'*.par')
pulsarpar= parfile.psr_par(greppar[0])
pulsar= pulsarpar.PSRJ
scoord = pulsarpar.RAJ+pulsarpar.DECJ
for pfd in pfds:
subprocess.check_call(['psredit','-c',
'coord='+scoord,'-c',
'name='+pulsar,
'-m',pfd])
subprocess.check_call(['psredit','-c',
'obs:projid=PuMA','-c',
'be:name=Ettus-SDR',
'-m',pfd])
# Choose a given template named 'pulsar.pfd.std'
def __init__(self, freqbands):
"""Read TEMPO results (resid2.tmp, tempo.lis, timfile and parfiles)
freqbands is a list of frequency pairs to display.
"""
# Open tempo.lis. Parse it and find input .tim and .par files.
# Also find output .par file.
inputfiles_re = re.compile(r"Input data from (.*\.tim.*), Parameters from (.*\.par.*)")
outputfile_re = re.compile(r"Assumed parameters -- PSR (.*)$")
tempolisfile = open("tempo.lis")
intimfn, inparfn, outparfn = None, None, None
for line in tempolisfile:
match = inputfiles_re.search(line)
if match:
intimfn = match.group(1).strip()
inparfn = match.group(2).strip()
else:
match = outputfile_re.search(line)
if match:
outparfn = "%s.par" % match.group(1).strip()
if (intimfn != None) and (inparfn != None) and (outparfn != None):
# Found what we're looking for no need to continue parsing the file
break
tempolisfile.close()
self.phase_wraps = {}
self.jump_ranges = []
tim = tempy_io.TOAset.from_tim_file(intimfn)
tim_ordered_index = np.argsort(tim.TOAs)
# if there are phase wraps in the tim file, we want to include those
# in the intial plot
for tim_wrap_index in tim.phase_wraps:
wrap_index = tim_ordered_index[tim_wrap_index]
self.phase_wraps[wrap_index] = \
tim.phase_wraps[tim_wrap_index]
# if there are jumps in the tim file, we want to include those in the
# initial plot
for tim_jstart,tim_jend in tim.jump_ranges:
jstart = tim_ordered_index[tim_jstart]
jend = tim_ordered_index[tim_jend]
self.jump_ranges.append((jstart, jend))
# Record filename
self.inparfn = inparfn
self.outparfn = outparfn
self.intimfn = intimfn
# Read parfiles
self.inpar = par.psr_par(inparfn)
self.outpar = par.psr_par(outparfn)
# Read residuals
r = residuals.read_residuals()
self.max_TOA = r.bary_TOA.max()
self.min_TOA = r.bary_TOA.min()
ordered_index = np.argsort(r.bary_TOA)
self.ordered_MJDs = r.bary_TOA[ordered_index]
if freqbands is None:
self.freqbands = find_freq_clusters(r.bary_freq)
else:
self.freqbands = freqbands
self.residuals = {}
for lo,hi in self.freqbands:
indices = (r.bary_freq>=lo) & (r.bary_freq<hi)
self.residuals[get_freq_label(lo, hi)] = \
Resids(r.bary_TOA[indices], r.bary_freq[indices],
#np.arange(r.numTOAs)[indices],
ordered_index[indices],
r.orbit_phs[indices],
r.postfit_phs[indices], r.postfit_sec[indices],
r.prefit_phs[indices], r.prefit_sec[indices],
r.uncertainty[indices], r.weight[indices],
self.inpar, self.outpar)