def getDate(self, line, columns):
if columns['sep'] == ',':
fields = line.split(columns['sep'])
dateStr = fields[columns['Date']['num']].strip()
else:
dateStr = line[columns['Date']['start']:columns['Date']['end']]
if columns['Date']['type'] == 'CAL':
dateFmt = columns['Date']['format']
if '.' in dateStr:
dateTimeStr, msecStr = dateStr.split('.')
msec = int(msecStr)
else:
dateTimeStr = dateStr
msec = 0
elif columns['Date']['type'] == 'JD':
# The subtraction is because sla_djcl wants an MJD
jd = float(dateStr)
yy, mm, dd, fracDay, j = slalib.sla_djcl(jd - 2400000.5)
sign, hmsf = slalib.sla_dd2tf(3, fracDay)
dateStr = '-'.join([str(yy), '%02d' % mm, '%02d' % dd])
timeStr = ':'.join(
['%02d' % hmsf[0],
'%02d' % hmsf[1],
'%02d' % hmsf[2]])
dateTimeStr = ' '.join([dateStr, timeStr])
dateFmt = '%Y-%m-%d %H:%M:%S'
msec = int(hmsf[3])
date = datetime.datetime.strptime(
dateTimeStr, dateFmt) + datetime.timedelta(milliseconds=msec)
return date
def mjd_to_greg(mjd):
"""
Convert MJD into gregorian date.
Parameters
----------
mjd : float
Date in the format MJD.
Returns
----------
greg : string
Gregorian date (format: YYYYMMDD_HHMMSS)
Examples
----------
>>> mjd = greg_to_mjd('19881103_000000')
>>> greg = mjd_to_greg(mjd)
>>> print('MJD={} ->'.format(round(mjd, 2)), 'GREG={}'.format(greg))
MJD=47468.0 -> GREG=19881103_000000
"""
year, month, day, fracday, baddate = slalib.sla_djcl(mjd)
if baddate:
raise ValueError(BadMJD)
sign, (hour, minute, second, frac) = slalib.sla_dd2tf(2, fracday)
s = '{:4d}{:2d}{:2d}_{:2d}{:2d}{:2d}'.format(year, month, day, hour,
minute, second)
s = s.replace(' ', '0')
return s
def mjd_utc2datetime(mjd):
"""Converts a passed Modified Julian date to a Python datetime object. 'None' is
returned if the conversion was not possible."""
year, month, day, frac, status = S.sla_djcl(mjd)
if status != 0:
return None
sign, hms = S.sla_dd2tf(0, frac)
dt = datetime(year, month, day, hms[0], hms[1], hms[2])
return dt
def utcFromMjd (mjd) :
from pyslalib import slalib
date = slalib.sla_djcl(mjd)
year = np.int(date[0])
month= np.int(date[1])
day = np.int(date[2])
hour = np.int(date[3]*24.)
minute = np.int( (date[3]*24.-hour)*60. )
#time = "UTC-{}-{}-{}-{:02d}:{:02d}:00"..format(year,month,day,hour,minute) old way
time = "UTC-{}-{:02d}-{:02d}-{:02d}:{:02d}:00".format(year,month,day,hour,minute)
return time
def jd_utc2datetime(jd):
"""Converts a passed Julian date to a Python datetime object. 'None' is
returned if the conversion was not possible."""
try:
mjd_utc = jd - 2400000.5
except TypeError:
try:
mjd_utc = float(jd) - 2400000.5
except:
return None
year, month, day, frac, status = S.sla_djcl(mjd_utc)
if status != 0:
return None
sign, hms = S.sla_dd2tf(0, frac)
dt = datetime(year, month, day, hms[0], hms[1], hms[2])
return dt
def parse_archive(filenm):
"""
Parse an input fits file header and create a remote path.
Parameters
----------
filenm : str
The name of the input archive.
Returns
-------
cornell_path : str
The path to send to the Cornell FTP server.
ubc_path : str
The path to send to the UBC data archive.
"""
# Open the file using pyfits and get the header
hdulist = PF.open(filenm)
hdr = hdulist[0].header
hdulist.close()
source = hdr["SRC_NAME"].strip("B").strip("J")
backend = hdr["BACKEND"]
if backend == "GUPPI2":
# This is for uniformity between incoherent/coherent GUPPI modes
backend = "GUPPI"
year = hdr["DATE-OBS"].split("-")[0]
elif backend == "PUPPI":
year = hdr["DATE-OBS"].split("-")[0]
elif backend == "xASP":
backend = "ASP"
MJD = hdr["STT_IMJD"] + hdr["STT_SMJD"]/SECPERDAY
year = str(sla_djcl(MJD)[0]) # Convert MJD to calendar date
else:
backend = None
year = None
return source,backend,year
def processDatetime(dateTime):
"""
Returns a Python datetime object.
Given a date/time, supplied as any any of the following:
- Python datetime object
- Julian date (JD)
- Modified Julian date (MJD)
- YYYYMMDD.DDDD
- YYYYMMDD HH:MM:SS (You can leave off the HH:MM:SS or some subset of that)
- YYYY-MM-DD HH:MM:SS (You can leave off the HH:MM:SS or some subset of that)
- YYYY/MM/DD HH:MM:SS (You can leave off the HH:MM:SS or some subset of that)
- YYYY-MMM-DD HH:MM
returns the equivalent date/time, expressed as a Python datetime
object.
Args:
jd: The date/time
Returns:
The date/time, expressed as a datetime object
"""
dateTimeFormats = ('%Y%m%d', '%Y-%m-%d', '%Y/%m/%d', '%Y%m%d %H',
'%Y%m%d %H%M', '%Y%m%d %H%M%S', '%Y%m%d %H',
'%Y%m%d %H:%M', '%Y%m%d %H:%M:%S', '%Y%m%d-%H',
'%Y%m%d-%H:%M', '%Y%m%d-%H:%M:%S', '%Y-%m-%dT%H',
'%Y-%m-%dT%H:%M', '%Y-%m-%dT%H:%M:%S', '%Y-%m-%d %H',
'%Y-%m-%d %H:%M', '%Y-%m-%d %H:%M:%S', '%Y/%m/%d %H',
'%Y/%m/%d %H:%M', '%Y/%m/%d %H:%M:%S', '%Y-%b-%d %H:%M')
# if the input value is already a datetime object, just return it.
if isinstance(dateTime, datetime.datetime):
return dateTime
else:
# The input value might be a JD, MJD, or a YYYYMMDD.DDDD. If
# it is any of those, we can convert it to a float. If we
# can't convert it to a float, it must be one of the string
# representations, e.g., YYYYMMDD HH:MM:SS.
try:
dateTime = float(dateTime)
except ValueError:
pass
if isinstance(dateTime, float):
# The input is a float. Now we have to determine if it is
# YYYYMMDD.DDDD or JD/MJD. If the string represention of
# the date portion of the input is the same length as
# 'YYYYMMDD', it must be a YYYYMMDD.DDDD. JD and MJD dates
# are typically either 7 or 5 characters long,
# respectively, not 8 characters, at least for the range
# of dates that we usually care about.
(fracDay, date) = math.modf(dateTime)
if len(str(int(date))) == len('YYYYMMDD'):
# Convert input YYYYMMDD.DDDD into datetime object
return datetime.datetime.strptime(str(
int(date)), '%Y%m%d') + datetime.timedelta(days=fracDay)
else:
# Input is either JD or MJD. Raise an exception if we
# slalib isn't available.
if not jdOk:
raise NoSlalibError(
'Julian dates require slalib, but slalib is not available'
)
# For the dates that we care about, if the value is
# greater than 2400000, we assume that it is a JD, so
# convert it to an MJD.
if dateTime > 2400000:
dateTime -= 2400000.5
yy, mm, dd, fracDay, j = slalib.sla_djcl(dateTime - 2400000.5)
sign, hmsf = slalib.sla_dd2tf(3, fracDay)
dateStr = '-'.join([str(yy), '%02d' % mm, '%02d' % dd])
timeStr = ':'.join(
['%02d' % hmsf[0],
'%02d' % hmsf[1],
'%02d' % hmsf[2]])
dateTimeStr = ' '.join([dateStr, timeStr])
dateFmt = '%Y-%m-%d %H:%M:%S'
msec = int(hmsf[3])
return datetime.datetime.strptime(
dateTimeStr,
dateFmt) + datetime.timedelta(milliseconds=msec)
elif isinstance(dateTime, str):
# The input date is a string. Using one of the acceptable
# formats, parse it and create a datetime object.
dateTimeObj = None
for format in dateTimeFormats:
try:
dateTimeObj = datetime.datetime.strptime(dateTime, format)
break
except ValueError:
pass
# If we were able to parse the input string, return the
# datetime object. Otherwise, raise an exception.
if dateTimeObj:
return dateTimeObj
else:
raise DateTimeFormatError('Unexpected date/time format: %s' %
dateTime)
else:
raise DateTimeFormatError('Unexpected date/time format: %s' %
dateTime)
def __init__(self,
ra,
dec,
values,
mjd,
alpha=0.,
degradeRes=True,
verbose=True):
self.verbose = verbose
data_dir = os.environ["DESGW_DATA_DIR"]
ctio_lat = -30.16527778
ctio_lon = -70.8125
ctio_height = 2215.
self.date = slalib.sla_djcl(mjd)
self.degToRad = 0.0174532925199
self.lat = ctio_lat * self.degToRad
self.lon = ctio_lon * self.degToRad
self.height = ctio_height
self.mjd = mjd
self.ra = ra * self.degToRad
self.dec = dec * self.degToRad
self.map = values
self.nside = hp.npix2nside(values.size)
# observational astronomy
self.lst = self.mjdToLST(self.mjd, self.lon)
self.ha, self.zd = self.equatorialToObservational(
self.ra, self.dec, self.lst, self.lat)
self.airmass = self.airmassModel(self.zd)
self.sunData = self.getSolarPosition(self.mjd, self.lon, self.lat,
self.lst)
self.sunZD = self.sunData[2]
self.moonData = self.getLunarPosition(self.mjd, self.lon, self.lat,
self.lst)
self.moonZD = self.moonData[2]
self.moonSep = self.getLunarSeparation(self.ra, self.dec,
self.moonData)
self.moonPhase = self.getLunarPhase()
# telescope limits
self.limits = 0.0
# galactic dust
dust_dir = data_dir
dust_file = "plank-ebv-HFI_CompMap_ThermaDustModel.fits"
ra, dec, ebv = dustModel.loadDust(dust_dir, dust_file)
if degradeRes:
ra, dec, ebv = hp2np.map2np(ebv,
resolution=self.nside,
fluxConservation=False)
self.dust_ra = ra
self.dust_dec = dec
self.ebv = ebv
# stellar density in the form of a probability of recognizing object map
print "\t loading inverse stellar density = probability of recognition map"
ra, dec, precog = hp2np.hp2np(data_dir + "precognize.fits")
if degradeRes:
ra, dec, precog = hp2np.map2np(precog,
resolution=self.nside,
fluxConservation=False)
self.pra = ra
self.pdec = dec
self.precog = precog
# limiting mag
self.maglim = ""
self.maglimall = ""
# where to put the central meridan in the mcbryde-thomas projection
# - the ra which one wants on the meridian
self.mcbryde_alpha = alpha