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pintautils.py
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pintautils.py
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import shutil
import sys
import os
import numpy as np
import parse
import astropy.time as astrotime
import getopt
import time
import glob
import astropy.units as astrounit
def touch_file(fname):
with open(fname, 'w'):
os.utime(fname, None)
def process_timestamp(timestamp_file_name):
timestamp_file = open(timestamp_file_name,'r')
timestamp_file_lines = timestamp_file.readlines()
timestr = parse.parse("IST Time: {}\n",timestamp_file_lines[1])[0]
datestr = parse.parse("Date: {}\n",timestamp_file_lines[2])[0]
timestamp_file.close()
day,month,year = parse.parse("{}:{}:{}",datestr)
hh, mm, ss = parse.parse("{}:{}:{}", timestr)
#datetime_IST = "%s-%s-%sT%s"%(year,month,day,timestr)
date_IST = "%s-%s-%s"%(year,month,day)
datemjd_int = astrotime.Time(date_IST, format='isot', scale='utc').mjd
datemjd_frc = (float(hh) + float(mm)/60 + float(ss)/3600 - 5.5)/24
if datemjd_frc<0:
datemjd_frc += 1
datemjd_int -= 1
# This is an ugly hack. Will change this if there is a better option.
datemjd_frc_str = "{:.15f}".format(datemjd_frc).split('.')[1]
datetimemjd_str = "{}.{}".format(int(datemjd_int), datemjd_frc_str)
return datetimemjd_str
def fetch_f0(parfile_name):
f0 = -10.0
with open(parfile_name, 'r') as par_file:
for cnt, line in enumerate(par_file):
if f0<0.0:
try:
thestr = parse.parse("F0 {}\n",line)[0]
#print ("found in line %s \n "%line)
f0 = float(thestr.split()[0])
#print ("fetched F0 : %f \n "%f0)
except:
pass #print ("F0 is not in this line. ")
print ("[INPUT] Pulsar spin-frequency found : %f "%f0)
return f0
def prepare_par_line(line):
return line.strip().replace('\t',' ').replace('\n','')
def rad_to_hms(α):
# α will be in [-pi,pi]
if α<0:
α += 2*np.pi
hrs = α * 12 / np.pi
hh = int(hrs)
mm = int((hrs - hh)*60)
ss = int((hrs - hh - mm/60)*3600)
sf = (hrs - hh - mm/60)*3600 - ss
sfs = str(sf).split('.')[1]
return f'{hh:02}:{mm:02}:{ss:02}.{sfs}'
def rad_to_dms(δ):
# δ will be in [-pi/2, pi/2]
sgn = np.sign(δ)
pm = '-' if sgn<0 else '+'
degs = np.abs(δ) * 180 / np.pi
dd = int(degs)
mm = int((degs - dd)*60)
ss = int((degs - dd - mm/60)*3600)
sf = (degs - dd - mm/60)*3600 - ss
sfs = str(sf).split('.')[1]
return f'{pm}{dd:02}:{mm:02}:{ss:02}.{sfs}'
def ecliptic_to_equatorial(elat, elong):
"""
https://en.wikipedia.org/wiki/Astronomical_coordinate_systems#Equatorial_%E2%86%94_ecliptic
"""
# Obliquity value taken from PINT
# https://github.com/nanograv/PINT/blob/master/src/pint/data/runtime/ecliptic.dat
ε = astrounit.Quantity(84381.406000, astrounit.arcsec).to(astrounit.rad).value
β = astrounit.Quantity(elat, astrounit.deg).to(astrounit.rad).value
λ = astrounit.Quantity(elong, astrounit.deg).to(astrounit.rad).value
α = np.arctan2(np.cos(β)*np.sin(λ)*np.cos(ε) - np.sin(β)*np.sin(ε),
np.cos(β)*np.cos(λ))
δ = np.arcsin(np.sin(β)*np.cos(ε) + np.cos(β)*np.sin(λ)*np.sin(ε))
return rad_to_hms(α), rad_to_dms(δ)
def fetch_RAJ_DECJ(parfile_name):
with open(parfile_name, 'r') as par_file:
par_lines = par_file.readlines()
par_tokens = dict([list(filter(lambda x: len(x)>0,
prepare_par_line(line).split(' '))
)[:2]
for line in par_lines
if len(prepare_par_line(line))>0
]
)
if "RAJ" in par_tokens and "DECJ" in par_tokens:
raj = par_tokens["RAJ"]
decj = par_tokens["DECJ"]
return raj, decj
elif "ELAT" in par_tokens and "ELONG" in par_tokens:
elat = par_tokens["ELAT"]
elong = par_tokens["ELONG"]
return ecliptic_to_equatorial(elat, elong)
elif "LAMBDA" in par_tokens and "BETA" in par_tokens:
elat = par_tokens["BETA"]
elong = par_tokens["LAMBDA"]
return ecliptic_to_equatorial(elat, elong)
else:
print("[ERROR] Unable to read coordinates from par file. Setting 00:00:00+00:00:00.")
return "00:00:00","+00:00:00"
def make_rficlean_hdrfile(file_name, psrj,frequency,nchannels,bandwidth,samplingtime,whichband):
print('[INFO] Removing any previous rfiClean-gmhdr file %s ... '%(file_name), end=' ')
try:
os.remove("%s"%(file_name))
print("Done.")
except:
print("Could not delete the rfiClean-gmhdr file!")
with open(file_name, 'w') as hdrfile:
print("[INFO] Trying to make the rficlean-gmhdr file ...")
try:
hdrfile.write(str(float(samplingtime)*1000.0) + '\n')
hdrfile.write(str(frequency) + '\n')
if whichband == 'USB':
hdrfile.write(str(-1.0*float(nchannels)*float(bandwidth)) + '\n')
elif whichband == 'LSB':
hdrfile.write(str(float(nchannels)*float(bandwidth)) + '\n')
else:
print("[ERROR] Unrecognizable sideband. Quitting...")
sys.exit(0)
hdrfile.write(str(nchannels) + '\n')
hdrfile.write(psrj)
print("[INFO] The rfiClean-gmhdr file written out! {}".format(file_name))
except:
print("[ERROR] Could not make the rficlean-gmhdr file! Quitting...")
sys.exit(0)
return False
return True
def choose_int_freq(freq):
int_freqs = np.array((499,749,1459))
i = np.argmin(np.abs(int_freqs-freq))
return int_freqs[i]
def process_sideband(sideband_):
if sideband_ == 'USB':
sideband = 'gmgwbf'
elif sideband_ == 'LSB':
sideband = 'gmgwbr'
else:
raise ValueError("The given sideband {} is invalid.".format(sideband_))
return sideband
def process_freq(freq_lo, nchan, bandwidth, sideband, cohded):
if not cohded:
if sideband == 'LSB':
f1 = freq_lo
else:
f1 = freq_lo + bandwidth
else:
if sideband == 'LSB':
f1 = freq_lo - bandwidth/nchan
else:
f1 = freq_lo + bandwidth*(1 - 1./nchan)
return f1
def copy_gptool_in(gptdir, working_dir, intfreq):
src = "{}/gptool.in.{}".format(gptdir, intfreq)
#dst = "{}/gptool.in".format(current_dir)
dst = "{}/gptool.in".format(working_dir)
shutil.copyfile(src, dst)
print("[INFO] Copied gptool.in file for freq {}".format(intfreq))
print("[CMD] cp {} {}".format(src, dst))
def check_mkdir(dirname):
if not os.access(dirname, os.F_OK):
print("[INFO] Creating directory", dirname)
os.mkdir(dirname)
aux_files_wcards = [ "bandshape.gpt",
"benchmark_fillTime.gpt",
"benchmark.gpt",
"benchmark_readtime.gpt",
"benchmark_threadtime.gpt",
"benchmark_threadtime_indv.gpt",
"log.gpt",
"stats.gpt",
"gptool.in",
"gptool.in.oldver",
"pdmp.per",
"pdmp.posn",
"*-ttemp-gm.info" ]
def move_aux_files(session, item):
glb = lambda f : glob.glob("{}/{}".format(session.working_dir, f))
aux_files = set(sum(map(glb, aux_files_wcards), []))
for src in aux_files:
print("[INFO] Moving file {} to aux.".format(src))
dst = "{}/{}".format(item.auxdir, os.path.basename(src))
shutil.move(src, dst)
def remove_aux_files(session, item):
glb = lambda f : glob.glob("{}/{}".format(session.working_dir, f))
aux_files = set(sum(map(glb, aux_files_wcards), []))
for src in aux_files:
print("[INFO] Removing file {}".format(src))
os.unlink(src)
def print_log(session, message):
print(message)
if session.log_to_file:
session.logfile.write(message+"\n")
def find_nyquist_nbin(session, item):
F0 = item.f0psr
Tsmpl = item.tsmpl
nbin_nyq = 2**( int(np.log2( 1/(Tsmpl*F0) )) )
print ("[INFO] Default NBin = %d"%nbin_nyq)
return nbin_nyq
def find_band_number(session, item):
freq_lo = item.freq_lo
if freq_lo>119 and freq_lo<=250:
return 2
elif freq_lo>250 and freq_lo<501:
return 3
elif freq_lo>549 and freq_lo<851:
return 4
elif freq_lo>1059 and freq_lo<1461:
return 5
else:
raise ValueError("The value of freq_lo is outside valid ranges for uGMRT bands.")
def find_rcvr_name(session, item):
band_num = find_band_number(session, item)
return "uGMRT_B{}".format(band_num)
def find_gwb_mode(session, item):
return "CD" if item.cohded else "PA"
def generate_config_str(session, item):
flo = int(item.freq_lo)
bw = int(item.bandwidth)
nchn= item.nchan
sb = item.sideband
tsmp= item.tsmpl*1e6
cd = int(item.cohded)
config_str = "{}|{}|{}|{}|{}|{}".format(flo, bw, nchn, sb, tsmp, cd)
return config_str