def makeEmptyCEATemplate(raSizeDeg, decSizeDeg,meanRa = 180., meanDec = 0.,\
pixScaleXarcmin = 0.5, pixScaleYarcmin=0.5):
assert (meanDec == 0., 'mean dec other than zero not implemented yet')
cdelt1 = -pixScaleXarcmin / 60.
cdelt2 = pixScaleYarcmin / 60.
naxis1 = numpy.int(raSizeDeg / pixScaleXarcmin * 60. + 0.5)
naxis2 = numpy.int(decSizeDeg / pixScaleYarcmin * 60. + 0.5)
refPix1 = naxis1 / 2.
refPix2 = naxis2 / 2.
pv2_1 = 1.0
cardList = pyfits.CardList()
cardList.append(pyfits.Card('NAXIS', 2))
cardList.append(pyfits.Card('NAXIS1', naxis1))
cardList.append(pyfits.Card('NAXIS2', naxis2))
cardList.append(pyfits.Card('CTYPE1', 'RA---CEA'))
cardList.append(pyfits.Card('CTYPE2', 'DEC--CEA'))
cardList.append(pyfits.Card('CRVAL1', meanRa))
cardList.append(pyfits.Card('CRVAL2', meanDec))
cardList.append(pyfits.Card('CRPIX1', refPix1 + 1))
cardList.append(pyfits.Card('CRPIX2', refPix2 + 1))
cardList.append(pyfits.Card('CDELT1', cdelt1))
cardList.append(pyfits.Card('CDELT2', cdelt2))
cardList.append(pyfits.Card('CUNIT1', 'DEG'))
cardList.append(pyfits.Card('CUNIT2', 'DEG'))
hh = pyfits.Header(cards=cardList)
wcs = astLib.astWCS.WCS(hh, mode='pyfits')
data = numpy.zeros([naxis2, naxis1])
ltMap = liteMap.liteMapFromDataAndWCS(data, wcs)
return ltMap
def _get_ids(self):
"""Find source name information and return as a list."""
name_key = ''
# deprecated, removed at 3.2
#cards = self.hdu.header.ascardlist()
cards = pf.CardList(self.hdu.header.cards)
#First check for UCD in header
for card in cards:
if card.keyword[:5]=='TBUCD' and card.value in ['ID_MAIN','meta.id;meta.main']:
name_key = cards['TTYPE'+card.key[5:8]].value
break
#Sometimes UCDs are declared in comments
#May be fragile - depends on specific format for comments as in gamma-egr catalog
value_comment = card.image.split('/') ##ascardimage().split('/')
if len(value_comment)>1:
comment = value_comment[1]
ucd_string = comment[comment.find('UCD'):].split()
if ucd_string:
try:
if ucd_string[0].split('=')[1].strip('.')=='ID_MAIN':
name_key = cards[''.join(['TTYPE',card.key[5:8]])].value
break
except IndexError:
pass
if card.keyword[:5]=='TTYPE' and card.value.upper() in ['NAME','ID','PSR_NAME','SOURCE_NAME']:
name_key = card.value
break
try:
return self.hdu.data.field(name_key)
except KeyError:
return
def demo_header():
cards = pyfits.CardList()
for l in open("sample_fits01.header"):
card = pyfits_card_fromstring(l.strip())
cards.append(card)
h = pyfits.Header(cards)
return h
def test_header():
cards = pyfits.CardList()
for l in open("test.header"):
card = pyfits_card_fromstring(l.strip())
cards.append(card)
h = pyfits.Header(cards)
return h
def makeEmptyCEATemplateAdvanced(ra0, dec0, \
ra1, dec1,\
pixScaleXarcmin = 0.5, \
pixScaleYarcmin= 0.5):
"""
ALL RA DEC IN DEGREES
"""
assert ra0<ra1
assert dec0<dec1
refDec = (dec0+dec1)/2.
cosRefDec = np.cos(refDec/180.*np.pi)
raSizeDeg = (ra1 - ra0)*cosRefDec
decSizeDeg = (dec1-dec0)
cdelt1 = -pixScaleXarcmin/(60.*cosRefDec)
cdelt2 = pixScaleYarcmin/(60.*cosRefDec)
naxis1 = np.int(raSizeDeg/pixScaleXarcmin*60.+0.5)
naxis2 = np.int(decSizeDeg/pixScaleYarcmin*60.+0.5)
refPix1 = np.int(-ra1/cdelt1+0.5)
refPix2 = np.int(np.sin(-dec0*np.pi/180.)\
*180./np.pi/cdelt2/cosRefDec**2+0.5)
pv2_1 = cosRefDec**2
cardList = pyfits.CardList()
cardList.append(pyfits.Card('NAXIS', 2))
cardList.append(pyfits.Card('NAXIS1', naxis1))
cardList.append(pyfits.Card('NAXIS2', naxis2))
cardList.append(pyfits.Card('EXTEND', True))
cardList.append(pyfits.Card('CTYPE1', 'RA---CEA'))
cardList.append(pyfits.Card('CTYPE2', 'DEC--CEA'))
cardList.append(pyfits.Card('CRVAL1', 0))
cardList.append(pyfits.Card('CRVAL2', 0))
cardList.append(pyfits.Card('CRPIX1', refPix1+1))
cardList.append(pyfits.Card('CRPIX2', refPix2+1))
cardList.append(pyfits.Card('CDELT1', cdelt1))
cardList.append(pyfits.Card('CDELT2', cdelt2))
cardList.append(pyfits.Card('CUNIT1', 'DEG'))
cardList.append(pyfits.Card('CUNIT2', 'DEG'))
cardList.append(pyfits.Card('PV2_1', pv2_1))
cardList.append(pyfits.Card('EQUINOX',2000))
cardList.append(pyfits.Card('PC1_1',1))
cardList.append(pyfits.Card('PC1_2',0))
cardList.append(pyfits.Card('PC2_1',0))
cardList.append(pyfits.Card('PC2_2',1))
hh = pyfits.Header(cards=cardList)
wcs = astLib.astWCS.WCS(hh, mode='pyfits')
data = np.zeros([naxis2,naxis1])
ltMap = liteMapFromDataAndWCS(data,wcs)
return ltMap
def _get_positions(self):
"""Find columns containing position info and return a list of SkyDirs"""
cards = pf.CardList(self.hdu.header.cards) #ascardlist()
#ucds = cards.filterList('TBUCD*')
#ttypes = cards.filterList('TTYPE*')
ucds = cards.filter_list('TBUCD*')
ttypes = cards.filter_list('TTYPE*')
lon_key = lat_key = ''
if not lon_key:
if 'POS_EQ_RA_MAIN' in ucds.values():
ucd = ucds.keys()[ucds.values().index('POS_EQ_RA_MAIN')]
lon_key = ttypes[''.join(['TTYPE',ucd[5:8]])].value
#Assumes that if POS_EQ_RA_MAIN exists, POS_EQ_DEC_MAIN does too.
ucd = ucds.keys()[ucds.values().index('POS_EQ_DEC_MAIN')]
lat_key = ttypes[''.join(['TTYPE',ucd[5:8]])].value
elif 'RAdeg' in ttypes.values():
lon_key = ttypes[ttypes.keys()[ttypes.values().index('RAdeg')]].value
lat_key = ttypes[ttypes.keys()[ttypes.values().index('DEdeg')]].value
elif '_RAJ2000' in ttypes.values():
lon_key = ttypes[ttypes.keys()[ttypes.values().index('_RAJ2000')]].value
lat_key = ttypes[ttypes.keys()[ttypes.values().index('_DEJ2000')]].value
elif 'RAJ2000' in ttypes.values():
lon_key = ttypes[ttypes.keys()[ttypes.values().index('RAJ2000')]].value
lat_key = ttypes[ttypes.keys()[ttypes.values().index('DEJ2000')]].value
elif 'RAJD' in ttypes.values(): # only for bigbfile?
lon_key = ttypes[ttypes.keys()[ttypes.values().index('RAJD')]].value
lat_key = ttypes[ttypes.keys()[ttypes.values().index('DECJD')]].value
elif 'RA' in ttypes.values():
lon_key = ttypes[ttypes.keys()[ttypes.values().index('RA')]].value
try:
lat_key = ttypes[ttypes.keys()[ttypes.values().index('DE')]].value
except ValueError:
lat_key = ttypes[ttypes.keys()[ttypes.values().index('DEC')]].value
if not lon_key:
self.coords = skymaps.SkyDir.GALACTIC
if 'POS_GAL_LON' in ucds.values():
lon_key = ucds.keys()[ucds.values().index('POS_GAL_LON')]
lat_key = ucds.keys()[ucds.values().index('POS_GAL_LAT')]
elif '_GLON' in ttypes.values():
lon_key = ttypes[ttypes.keys()[ttypes.values().index('_GLON')]].value
lat_key = ttypes[ttypes.keys()[ttypes.values().index('_GLAT')]].value
elif 'GLON' in ttypes.values():
lon_key = ttypes[ttypes.keys()[ttypes.values().index('GLON')]].value
lat_key = ttypes[ttypes.keys()[ttypes.values().index('GLAT')]].value
if lon_key:
return (self.hdu.data.field(lon_key).astype('float'),
self.hdu.data.field(lat_key).astype('float'))
else:
raise SrcidError('did not find position info in catalog' )
def _get_hdu(self,fits_cat):
"""Find and return HDU with catalog information."""
#First check for HDUS with CAT-NAME or EXTNAME in header.
for hdu in fits_cat:
cards = pf.CardList(hdu.header.cards) ## replaced this function: ascardlist()
try:
self.cat_name = cards['CAT-NAME'].value
return hdu
except KeyError:
try:
self.cat_name = cards['EXTNAME'].value
return hdu
except KeyError:
self.cat_name = self.class_module.catid
pass
#No CAT-NAME or EXTNAME found, just return second HDU
if len(fits_cat)>=2:
return fits_cat[1]
#Only one HDU, no name info, return None
return
def set_pha_data(filename, data, col_names, header=None,
ascii=False, clobber=False, packup=False):
if not packup and os.path.isfile(filename) and not clobber:
raise IOErr("filefound", filename)
hdrlist = pyfits.CardList()
for key in header.keys():
if header[key] is None:
continue
hdrlist.append(pyfits.Card( str(key.upper()), header[key] ))
collist = []
cols = []
coldefs = []
for name in col_names:
if data[name] is None:
continue
col = pyfits.Column(name=name.upper(),
format=data[name].dtype.name.upper(),
array=data[name])
cols.append(data[name])
coldefs.append(name.upper())
collist.append(col)
if ascii:
set_arrays(filename, cols, coldefs, ascii=ascii, clobber=clobber)
return
pha = pyfits.new_table(pyfits.ColDefs(collist),
header=pyfits.Header(hdrlist))
pha.name = 'SPECTRUM'
if packup:
return pha
pha.writeto(filename, clobber=True)
def init_SDFITS(DSS, tablesize, time_column=False):
"""
Initialize an SDFITS file and extension.
Call this first to initiate an SDFITS file. It creates the primary HDU
suitable for a binary table extension. It then creates a binary table with
columns that one always needs. The data array has at least four axes for
compatibility with ASAP.
Notes
=====
The default length of axis 4 (STOKES) is 1 for compatibility with a
"one spectrum per row" convention. If this is not to be followed then
subsequently called methods (probably Observatory.FITS_init_backends)
must change MAXIS4.
TDIMxx is calculated from MAXIS1 through MAXISn at the end.
@param DSS : instance of the Telescope class::
A front end with no telescope makes no sense.
@param tablesize : int::
Number of rows in the table
@param time_column : boolean::
If True, there will be a fourth data axis for time.
Otherwise, the data axes are frequency, RA and decl.
@return: tuple::
The primary HDU instance, the table CardList (header)
instance with initial header data, and the initial column set.
"""
# create the primary HDU and extension headers
prihdu = pyfits.PrimaryHDU()
hdr = pyfits.CardList()
cols = make_basic_columns(tablesize, time_column)
# add telescope location data to the table header
logger.debug("DSS: %s", DSS)
if type(DSS) == list:
# This may seem odd but in the most general case there could be two or
# more antennas, like in an interferometer. In that case, however,
# "single dish" FITS format doesn't apply. We'll just assume a list of
# length 1.
dss = DSS[0]
else:
dss = DSS
if dss != 0:
hdr.append(pyfits.Card('telescop', dss.name))
hdr.append(pyfits.Card('sitelong', dss['longitude']))
hdr.append(pyfits.Card('sitelat', dss['latitude']))
hdr.append(pyfits.Card('siteelev', dss['elevation']))
hdr.append(pyfits.Card('obsgeo-x', dss['geo-x']))
hdr.append(pyfits.Card('obsgeo-y', dss['geo-y']))
hdr.append(pyfits.Card('obsgeo-z', dss['geo-z']))
hdr.append(pyfits.Card('TIMESYS', 'UTC'))
# there will always be four axes in the data array
hdr.append(pyfits.Card('MAXIS', 4))
# we will always have the first data axis with frequency in the
# from of the observatory, or time-delay for correlation functions
# (cannot set MAXIS1 until we know the size of the spectrum)
# hdr.append(pyfits.Card('MAXIS1',?))
hdr.append(pyfits.Card('CTYPE1', 'FREQ-OBS'))
# the second and third axes will be right ascension and declination
hdr.append(pyfits.Card('MAXIS2', 1))
hdr.append(pyfits.Card('CTYPE2', 'RA---GLS'))
hdr.append(pyfits.Card('MAXIS3', 1))
hdr.append(pyfits.Card('CTYPE3', 'DEC--GLS'))
# the fourth axis is polarization. As a default
hdr.append(pyfits.Card('MAXIS4', 1))
hdr.append(pyfits.Card('CTYPE4', 'STOKES'))
if time_column:
# the optional fifth data axis will be time
# (cannot set MAXIS5 until we know the number of spectra)
# hdr.append(pyfits.Card('MAXIS4',?))
hdr.append(pyfits.Card('CTYPE5', 'TIME'))
return prihdu, hdr, cols
def set_image_data(filename, data, header, ascii=False, clobber=False,
packup=False):
if not packup and os.path.isfile(filename) and not clobber:
raise IOErr("filefound", filename)
if ascii:
set_arrays(filename, [data['pixels'].ravel()],
ascii=ascii, clobber=clobber)
return
hdrlist = pyfits.CardList()
# Write Image Header Keys
for key in header.keys():
if header[key] is None:
continue
_set_wcs_key(hdrlist, key, header[key])
# Write Image WCS Header Keys
if data['eqpos'] is not None:
cdeltw = data['eqpos'].cdelt
crpixw = data['eqpos'].crpix
crvalw = data['eqpos'].crval
equin = data['eqpos'].equinox
if data['sky'] is not None:
cdeltp = data['sky'].cdelt
crpixp = data['sky'].crpix
crvalp = data['sky'].crval
_set_wcs_key(hdrlist, 'MTYPE1', 'sky ')
_set_wcs_key(hdrlist, 'MFORM1', 'x,y ')
_set_wcs_key(hdrlist, 'CTYPE1P', 'x ')
_set_wcs_key(hdrlist, 'CTYPE2P', 'y ')
_set_wcs_key(hdrlist, 'WCSNAMEP','PHYSICAL')
_set_wcs_key(hdrlist, 'CDELT1P', cdeltp[0])
_set_wcs_key(hdrlist, 'CDELT2P', cdeltp[1])
_set_wcs_key(hdrlist, 'CRPIX1P', crpixp[0])
_set_wcs_key(hdrlist, 'CRPIX2P', crpixp[1])
_set_wcs_key(hdrlist, 'CRVAL1P', crvalp[0])
_set_wcs_key(hdrlist, 'CRVAL2P', crvalp[1])
if data['eqpos'] is not None:
# Simply the inverse of read transformations in get_image_data
cdeltw = cdeltw * cdeltp
crpixw = ((crpixw - crvalp) / cdeltp + crpixp )
if data['eqpos'] is not None:
_set_wcs_key(hdrlist, 'MTYPE2', 'EQPOS ')
_set_wcs_key(hdrlist, 'MFORM2', 'RA,DEC ')
_set_wcs_key(hdrlist, 'CTYPE1', 'RA---TAN')
_set_wcs_key(hdrlist, 'CTYPE2', 'DEC--TAN')
_set_wcs_key(hdrlist, 'CDELT1', cdeltw[0])
_set_wcs_key(hdrlist, 'CDELT2', cdeltw[1])
_set_wcs_key(hdrlist, 'CRPIX1', crpixw[0])
_set_wcs_key(hdrlist, 'CRPIX2', crpixw[1])
_set_wcs_key(hdrlist, 'CRVAL1', crvalw[0])
_set_wcs_key(hdrlist, 'CRVAL2', crvalw[1])
_set_wcs_key(hdrlist, 'CUNIT1', 'deg ')
_set_wcs_key(hdrlist, 'CUNIT2', 'deg ')
_set_wcs_key(hdrlist, 'EQUINOX', equin)
#
img = pyfits.PrimaryHDU(data['pixels'], header=pyfits.Header(hdrlist))
if packup:
return img
img.writeto(filename, clobber=True)