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#from .. pywcs.sip import SIP
from pywcs import WCS, DistortionLookupTable
import pyfits
import instruments
#from .. distortion import models
from updatewcs.distortion import models
import numpy as np
from pytools import fileutil
from pytools.fileutil import DEGTORAD, RADTODEG
#from .. mappings import inst_mappings, ins_spec_kw, DEGTORAD, RADTODEG, basic_wcs
import mappings
from mappings import inst_mappings, ins_spec_kw
from mappings import basic_wcs, prim_hdr_kw
__docformat__ = 'restructuredtext'
__version__ = '0.3'
class HSTWCS(WCS):
"""
Purpose
=======
Create a WCS object based on the instrument.
It has all basic WCS kw as attribbutes (set by pywcs).
It also uses the primary and extension header to define
instrument specific attributes.
"""
def __init__(self, fobj=None, ext=None, instrument=None, detector=None, minerr=0.0):
"""
:Parameters:
`fobj`: string or PyFITS HDUList object or None
a file name, e.g j9irw4b1q_flt.fits
a fully qualified filename[EXTNAME,EXTNUM], e.g. j9irw4b1q_flt.fits[sci,1]
a pyfits file object, e.g pyfits.open('j9irw4b1q_flt.fits')
`ext`: int or None
extension number
if ext==None, it is assumed the data is in the primary hdu
`instrument`: string
one of 'ACS', 'NICMOS', 'WFPC2', 'STIS', 'WFC3'
Used only to define a default HSTWCS object, when fobj==None
`detector`: string
for example 'WFC'
If instrument and detector parameters are given, a default HSTWCS
instrument is created. Used only with fobj==None
`minerr`: float
minimum value a distortion correction must have in order to be applied.
If CPERRja, CQERRja are smaller than minerr, the corersponding
distortion is not applied.
"""
self.inst_kw = ins_spec_kw
self.minerr = minerr
if instrument == None:
filename, hdr0, ehdr, phdu = self.parseInput(f=fobj, ext=ext)
self.filename = filename
self.setHDR0kw(hdr0, ehdr)
WCS.__init__(self, ehdr, fobj=phdu, minerr=minerr)
# If input was a pyfits HDUList object, it's the user's
# responsibility to close it, otherwise, it's closed here.
if not isinstance(fobj, pyfits.HDUList):
phdu.close()
self.setInstrSpecKw(hdr0, ehdr)
self.setPscale()
self.setOrient()
self.readIDCCoeffs(ehdr)
extname = ehdr.get('EXTNAME', "")
extnum = ehdr.get('EXTVER', None)
self.extname = (extname, extnum)
else:
# create a default HSTWCS object based on
#instrument and detector parameters
self.instrument = instrument
self.detector = detector
self.setInstrSpecKw()
def parseInput(self, f=None, ext=None):
if isinstance(f, str):
# create an HSTWCS object from a filename
if ext != None:
filename = f
extnum = ext
elif ext == None:
filename, extname = fileutil.parseFilename(f)
if extname == None:
#data may be in the primary array
extnum = 0
else:
extnum = fileutil.parseExtn(extname)
phdu = pyfits.open(filename)
hdr0 = pyfits.getheader(filename)
try:
ehdr = pyfits.getheader(filename, ext=extnum)
except IndexError:
print 'Unable to get extension %d. /n' % ext
elif isinstance(f, pyfits.HDUList):
phdu = f
if ext == None:
extnum = 0
else:
extnum = ext
ehdr = f[extnum].header
hdr0 = f[0].header
filename = hdr0.get('FILENAME', "")
return filename, hdr0, ehdr, phdu
def setHDR0kw(self, primhdr, ehdr):
# Set attributes from kw defined in the primary header.
self.instrument = primhdr.get('INSTRUME', None)
self.offtab = primhdr.get('OFFTAB', None)
self.idctab = primhdr.get('IDCTAB', None)
self.date_obs = primhdr.get('DATE-OBS', None)
self.ra_targ = primhdr.get('RA_TARG', None)
self.dec_targ = primhdr.get('DEC_TARG', None)
self.det2imfile = primhdr.get('D2IMFILE', None)
self.det2imext = primhdr.get('D2IMEXT', None)
self.axiscorr = primhdr.get('AXISCORR', None)
self.d2imerr = primhdr.get('D2IMERR', 0.0)
try:
self.pav3 = primhdr['PA_V3']
except KeyError:
print 'Keyword PA_V3 not found in primary header.'
print 'This is typical for some old files. Please retrieve the files from the archive again.'
#print 'Quitting ...'
#raise
def readIDCCoeffs(self, header):
"""
Reads in first order IDCTAB coefficients if present in the header
"""
coeffs = ['ocx10', 'ocx11', 'ocy10', 'ocy11', 'idcscale']
for c in coeffs:
self.__setattr__(c, header.get(c, None))
def setInstrSpecKw(self, prim_hdr=None, ext_hdr=None):
# Based on the instrument kw creates an instalnce of an instrument WCS class
# and sets attributes from instrument specific kw
if self.instrument in inst_mappings.keys():
inst_kl = inst_mappings[self.instrument]
inst_kl = instruments.__dict__[inst_kl]
insobj = inst_kl(prim_hdr, ext_hdr)
for key in self.inst_kw:
try:
self.__setattr__(key, insobj.__getattribute__(key))
except AttributeError:
# Some of the instrument's attributes are recorded in the primary header and
# were already set, (e.g. 'DETECTOR'), the code below is a check for that case.
if not self.__getattribute__(key):
raise
else:
pass
else:
raise KeyError, "Unsupported instrument - %s" %self.instrument
def setPscale(self):
# Calculates the plate scale from the cd matrix
cd11 = self.wcs.cd[0][0]
cd21 = self.wcs.cd[1][0]
self.pscale = np.sqrt(np.power(cd11,2)+np.power(cd21,2)) * 3600.
def setOrient(self):
# Recompute ORIENTAT
cd12 = self.wcs.cd[0][1]
cd22 = self.wcs.cd[1][1]
self.orientat = RADTODEG(np.arctan2(cd12,cd22))
def updatePscale(self, pscale):
"""Given a plate scale, update the CD matrix"""
old_pscale = self.pscale
self.pscale = pscale
self.wcs.cd = self.wcs.cd * pscale/old_pscale
self.naxis1 = self.naxis1 * old_pscale/ pscale
self.naxis2 = self.naxis2 * old_pscale/ pscale
self.wcs.crpix = self.wcs.crpix *old_pscale/pscale
def updateOrient(self, orient):
"""Given n angle update the CD matrix"""
if self.orientat == orient:
return
old_orient = self.orientat
self.orientat = orient
angle = fileutil.DEGTORAD(orient)
cd11 = -np.cos(angle)
cd12 = np.sin(angle)
cd21 = cd12
cd22 = -cd11
cdmat = np.array([[cd11, cd12],[cd21,cd22]])
self.wcs.cd = cdmat * self.pscale/3600
def readModel(self, update=False, header=None):
"""
Purpose
=======
Read distortion model from idc table.
Save some of the information as kw needed for interpreting the distortion
If header is provided and update is True, some IDC model kw
will be recorded in the header.
"""
if self.idctab == None or self.date_obs == None:
print 'idctab or date_obs not available\n'
self.idcmodel = None
return
if self.filter1 ==None and self.filter2 == None:
'No filter information available\n'
self.idcmodel = None
return
self.idcmodel = models.IDCModel(self.idctab,
chip=self.chip, direction='forward', date=self.date_obs,
filter1=self.filter1, filter2=self.filter2,
offtab=self.offtab, binned=self.binned)
if update:
if header==None:
print 'Update header with IDC model kw requested but header was not provided\n.'
return
else:
self.updatehdr(header)
"""
The next four methods overwrite the corresponding PyWCS methods
If detector to image correction is specified in the primary science
header and a correction extension exists (D2IMEXT keyword) then
this correction is applied before the corrsponding PyWCS method is called.
"""
def all_pix2sky(self, *args, **kwargs):
origin = self.get_origin(*args)
if self.det2imext != None and self.d2imerr > self.minerr:
return WCS.all_pix2sky(self, self.det2im(*args),origin )
else:
return WCS.all_pix2sky(self, *args)
all_pix2sky.__doc__ = """
Applies detector to image correction before it does the
following pixel transformations:
%s
""" % (WCS.all_pix2sky.__doc__)
def pix2foc(self, *args, **kwargs):
origin = self.get_origin(*args)
if self.det2imext != None and self.d2imerr > self.minerr:
return WCS.pix2foc(self, self.det2im(*args), origin)
else:
return WCS.pix2foc(self, *args)
pix2foc.__doc__ = """
Applies detector to image correction before it does the
following pixel transformations:
%s
""" % (WCS.pix2foc.__doc__)
def p4_pix2foc(self, *args, **kwargs):
origin = self.get_origin(*args)
if self.det2imext != None and self.d2imerr > self.minerr:
return WCS.p4_pix2foc(self, self.det2im(*args), origin)
else:
return WCS.p4_pix2foc(self, *args)
p4_pix2foc.__doc__ = """
Applies detector to image correction before it does the
following pixel transformations:
%s
""" % (WCS.p4_pix2foc.__doc__)
def sip_pix2foc(self, *args, **kwargs):
origin = self.get_origin(*args)
if self.det2imext != None and self.d2imerr > self.minerr:
return WCS.sip_pix2foc(self, self.det2im(*args), origin)
else:
return WCS.sip_pix2foc(self, *args)
sip_pix2foc.__doc__ = """
Applies detector to image correction before it does the
following pixel transformations:
%s
""" % (WCS.sip_pix2foc.__doc__)
def get_origin(self, *args):
# Parse the arguments to get the origin of the
#transformation: 0 or 1
if len(args) == 2:
return args[1]
elif len(args) == 3:
return args[2]
raise TypeError("Expected 2 or 3 arguments, %d given" % len(args))
def det2im(self, *args):
"""
Convert detector to image coordinates
"""
cpdis = self.get_d2im_lookup()
d2im_wcs = WCS()
if self.axiscorr == 1:
d2im_wcs.cpdis1 = cpdis
else:
d2im_wcs.cpdis2 = cpdis
if len(args) == 2:
xy, origin = args
try:
xy = np.asarray(xy)
origin = int(origin)
except:
raise TypeError(
"When providing two arguments, they must be (xy, origin)")
return d2im_wcs.p4_pix2foc(xy,origin)
elif len(args) == 3:
x, y, origin = args
try:
x = np.asarray(x)
y = np.asarray(y)
origin = int(origin)
except:
raise TypeError(
"When providing three arguments, they must be (x, y, origin)")
if len(x) != len(y):
raise ValueError("x and y arrays are not the same size")
length = len(x)
xy = np.hstack((x.reshape((length, 1)),
y.reshape((length, 1))))
img = d2im_wcs.p4_pix2foc(xy,origin)
return [img[:, i] for i in range(img.shape[1])]
def get_d2im_lookup(self):
"""
Create a paper IV type lookup table from a reference file
"""
d2im_data = pyfits.getdata(self.filename, ext=('D2IMARR', 1))
d2im_data = np.array([d2im_data])
d2im_hdr = pyfits.getheader(self.filename, ext=('D2IMARR', 1))
crpix = (d2im_hdr['CRPIX1'],d2im_hdr['CRPIX2'])
crval = (d2im_hdr['CRVAL1'],d2im_hdr['CRVAL2'])
cdelt = (d2im_hdr['CDELT1'],d2im_hdr['CDELT2'])
return DistortionLookupTable(d2im_data, crpix, crval, cdelt)
def restore(self, header=None):
"""
Restore a WCS archive in memory and update the WCS object.
Restored are the basic WCS kw as well as pscale and orient.
"""
from pywcs import Wcsprm
backup = {}
if header == None:
print 'Need a valid header in order to restore archive\n'
return
for k in basic_wcs:
try:
nkw = ('O'+k)[:7]
backup[k] = header[nkw]
except KeyError:
pass
if backup == {}:
print 'No archive was found\n'
return
cdl=pyfits.CardList()
for item in backup.items():
card = pyfits.Card(key=item[0], value=item[1])
cdl.append(card)
h = pyfits.Header(cdl)
wprm = Wcsprm("".join([str(x) for x in h.ascardlist()]))
self.wcs = wprm
self.setPscale()
self.setOrient()
def updatehdr(self, ext_hdr, newkeywords=None):
#kw2add : OCX10, OCX11, OCY10, OCY11
# record the model in the header for use by pydrizzle
ext_hdr.update('OCX10', self.idcmodel.cx[1,0])
ext_hdr.update('OCX11', self.idcmodel.cx[1,1])
ext_hdr.update('OCY10', self.idcmodel.cy[1,0])
ext_hdr.update('OCY11', self.idcmodel.cy[1,1])
ext_hdr.update('IDCSCALE', self.idcmodel.refpix['PSCALE'])
ext_hdr.update('IDCTHETA', self.idcmodel.refpix['THETA'])
ext_hdr.update('IDCXREF', self.idcmodel.refpix['XREF'])
ext_hdr.update('IDCYREF', self.idcmodel.refpix['YREF'])
ext_hdr.update('IDCV2REF', self.idcmodel.refpix['V2REF'])
ext_hdr.update('IDCV3REF', self.idcmodel.refpix['V3REF'])
def help():
print 'How to create an HSTWCS object:\n\n'
print """ \
1. Using a pyfits HDUList object and an extension number \n
Example:\n
fobj = pyfits.open('some_file.fits')\n
w = wcsutil.HSTWCS(fobj, 3)\n\n
2. Create an HSTWCS object using a qualified file name. \n
Example:\n
w = wcsutil.HSTWCS('j9irw4b1q_flt.fits[sci,1]')\n\n
3. Create an HSTWCS object using a file name and an extension number. \n
Example:\n
w = wcsutil.HSTWCS('j9irw4b1q_flt.fits', ext=2)\n\n
4. Create a template HSTWCS object for an instrument/detector combination.]n
Example:\n
w = wcsutil.HSTWCS(instrument='ACS', detector='WFC'\n\n
"""
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