/usr/lib/python2.7/dist-packages/astLib/astImages.py is in python-astlib 0.8.0-3build1.
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(c) 2007-2014 Matt Hilton
U{http://astlib.sourceforge.net}
Some routines in this module will fail if, e.g., asked to clip a section from a .fits image at a
position not found within the image (as determined using the WCS). Where this occurs, the function
will return None. An error message will be printed to the console when this happens if
astImages.REPORT_ERRORS=True (the default). Testing if an astImages function returns None can be
used to handle errors in scripts.
"""
REPORT_ERRORS=True
import os
import sys
import math
from astLib import astWCS
# So far as I can tell in astropy 0.4 the API is the same as pyfits for what we need...
try:
import pyfits
except:
try:
from astropy.io import fits as pyfits
except:
raise Exception("couldn't import either pyfits or astropy.io.fits")
try:
from scipy import ndimage
from scipy import interpolate
except ImportError:
print("WARNING: astImages: failed to import scipy.ndimage - some functions will not work.")
import numpy
try:
import matplotlib
from matplotlib import pylab
matplotlib.interactive(False)
except ImportError:
print("WARNING: astImages: failed to import matplotlib - some functions will not work.")
#---------------------------------------------------------------------------------------------------
def clipImageSectionWCS(imageData, imageWCS, RADeg, decDeg, clipSizeDeg, returnWCS = True):
"""Clips a square or rectangular section from an image array at the given celestial coordinates.
An updated WCS for the clipped section is optionally returned, as well as the x, y pixel
coordinates in the original image corresponding to the clipped section.
Note that the clip size is specified in degrees on the sky. For projections that have varying
real pixel scale across the map (e.g. CEA), use L{clipUsingRADecCoords} instead.
@type imageData: numpy array
@param imageData: image data array
@type imageWCS: astWCS.WCS
@param imageWCS: astWCS.WCS object
@type RADeg: float
@param RADeg: coordinate in decimal degrees
@type decDeg: float
@param decDeg: coordinate in decimal degrees
@type clipSizeDeg: float or list in format [widthDeg, heightDeg]
@param clipSizeDeg: if float, size of square clipped section in decimal degrees; if list,
size of clipped section in degrees in x, y axes of image respectively
@type returnWCS: bool
@param returnWCS: if True, return an updated WCS for the clipped section
@rtype: dictionary
@return: clipped image section (numpy array), updated astWCS WCS object for
clipped image section, and coordinates of clipped section in imageData in format
{'data', 'wcs', 'clippedSection'}.
"""
imHeight=imageData.shape[0]
imWidth=imageData.shape[1]
xImScale=imageWCS.getXPixelSizeDeg()
yImScale=imageWCS.getYPixelSizeDeg()
if type(clipSizeDeg) == float:
xHalfClipSizeDeg=clipSizeDeg/2.0
yHalfClipSizeDeg=xHalfClipSizeDeg
elif type(clipSizeDeg) == list or type(clipSizeDeg) == tuple:
xHalfClipSizeDeg=clipSizeDeg[0]/2.0
yHalfClipSizeDeg=clipSizeDeg[1]/2.0
else:
raise Exception("did not understand clipSizeDeg: should be float, or [widthDeg, heightDeg]")
xHalfSizePix=xHalfClipSizeDeg/xImScale
yHalfSizePix=yHalfClipSizeDeg/yImScale
cPixCoords=imageWCS.wcs2pix(RADeg, decDeg)
cTopLeft=[cPixCoords[0]+xHalfSizePix, cPixCoords[1]+yHalfSizePix]
cBottomRight=[cPixCoords[0]-xHalfSizePix, cPixCoords[1]-yHalfSizePix]
X=[int(round(cTopLeft[0])),int(round(cBottomRight[0]))]
Y=[int(round(cTopLeft[1])),int(round(cBottomRight[1]))]
X.sort()
Y.sort()
if X[0] < 0:
X[0]=0
if X[1] > imWidth:
X[1]=imWidth
if Y[0] < 0:
Y[0]=0
if Y[1] > imHeight:
Y[1]=imHeight
clippedData=imageData[Y[0]:Y[1],X[0]:X[1]]
# Update WCS
if returnWCS == True:
try:
oldCRPIX1=imageWCS.header['CRPIX1']
oldCRPIX2=imageWCS.header['CRPIX2']
clippedWCS=imageWCS.copy()
clippedWCS.header['NAXIS1']=clippedData.shape[1]
clippedWCS.header['NAXIS2']=clippedData.shape[0]
clippedWCS.header['CRPIX1']=oldCRPIX1-X[0]
clippedWCS.header['CRPIX2']=oldCRPIX2-Y[0]
clippedWCS.updateFromHeader()
except KeyError:
if REPORT_ERRORS == True:
print("WARNING: astImages.clipImageSectionWCS() : no CRPIX1, CRPIX2 keywords found - not updating clipped image WCS.")
clippedData=imageData[Y[0]:Y[1],X[0]:X[1]]
clippedWCS=imageWCS.copy()
else:
clippedWCS=None
return {'data': clippedData, 'wcs': clippedWCS, 'clippedSection': [X[0], X[1], Y[0], Y[1]]}
#---------------------------------------------------------------------------------------------------
def clipImageSectionPix(imageData, XCoord, YCoord, clipSizePix):
"""Clips a square or rectangular section from an image array at the given pixel coordinates.
@type imageData: numpy array
@param imageData: image data array
@type XCoord: float
@param XCoord: coordinate in pixels
@type YCoord: float
@param YCoord: coordinate in pixels
@type clipSizePix: float or list in format [widthPix, heightPix]
@param clipSizePix: if float, size of square clipped section in pixels; if list,
size of clipped section in pixels in x, y axes of output image respectively
@rtype: numpy array
@return: clipped image section
"""
imHeight=imageData.shape[0]
imWidth=imageData.shape[1]
if type(clipSizePix) == float or type(clipSizePix) == int:
xHalfClipSizePix=int(round(clipSizePix/2.0))
yHalfClipSizePix=xHalfClipSizePix
elif type(clipSizePix) == list or type(clipSizePix) == tuple:
xHalfClipSizePix=int(round(clipSizePix[0]/2.0))
yHalfClipSizePix=int(round(clipSizePix[1]/2.0))
else:
raise Exception("did not understand clipSizePix: should be float, or [widthPix, heightPix]")
cTopLeft=[XCoord+xHalfClipSizePix, YCoord+yHalfClipSizePix]
cBottomRight=[XCoord-xHalfClipSizePix, YCoord-yHalfClipSizePix]
X=[int(round(cTopLeft[0])),int(round(cBottomRight[0]))]
Y=[int(round(cTopLeft[1])),int(round(cBottomRight[1]))]
X.sort()
Y.sort()
if X[0] < 0:
X[0]=0
if X[1] > imWidth:
X[1]=imWidth
if Y[0] < 0:
Y[0]=0
if Y[1] > imHeight:
Y[1]=imHeight
return imageData[Y[0]:Y[1],X[0]:X[1]]
#---------------------------------------------------------------------------------------------------
def clipRotatedImageSectionWCS(imageData, imageWCS, RADeg, decDeg, clipSizeDeg, returnWCS = True):
"""Clips a square or rectangular section from an image array at the given celestial coordinates.
The resulting clip is rotated and/or flipped such that North is at the top, and East appears at
the left. An updated WCS for the clipped section is also returned. Note that the alignment
of the rotated WCS is currently not perfect - however, it is probably good enough in most
cases for use with L{ImagePlot} for plotting purposes.
Note that the clip size is specified in degrees on the sky. For projections that have varying
real pixel scale across the map (e.g. CEA), use L{clipUsingRADecCoords} instead.
@type imageData: numpy array
@param imageData: image data array
@type imageWCS: astWCS.WCS
@param imageWCS: astWCS.WCS object
@type RADeg: float
@param RADeg: coordinate in decimal degrees
@type decDeg: float
@param decDeg: coordinate in decimal degrees
@type clipSizeDeg: float
@param clipSizeDeg: if float, size of square clipped section in decimal degrees; if list,
size of clipped section in degrees in RA, dec. axes of output rotated image respectively
@type returnWCS: bool
@param returnWCS: if True, return an updated WCS for the clipped section
@rtype: dictionary
@return: clipped image section (numpy array), updated astWCS WCS object for
clipped image section, in format {'data', 'wcs'}.
@note: Returns 'None' if the requested position is not found within the image. If the image
WCS does not have keywords of the form CD1_1 etc., the output WCS will not be rotated.
"""
halfImageSize=imageWCS.getHalfSizeDeg()
imageCentre=imageWCS.getCentreWCSCoords()
imScale=imageWCS.getPixelSizeDeg()
if type(clipSizeDeg) == float:
xHalfClipSizeDeg=clipSizeDeg/2.0
yHalfClipSizeDeg=xHalfClipSizeDeg
elif type(clipSizeDeg) == list or type(clipSizeDeg) == tuple:
xHalfClipSizeDeg=clipSizeDeg[0]/2.0
yHalfClipSizeDeg=clipSizeDeg[1]/2.0
else:
raise Exception("did not understand clipSizeDeg: should be float, or [widthDeg, heightDeg]")
diagonalHalfSizeDeg=math.sqrt((xHalfClipSizeDeg*xHalfClipSizeDeg) \
+(yHalfClipSizeDeg*yHalfClipSizeDeg))
diagonalHalfSizePix=diagonalHalfSizeDeg/imScale
if RADeg>imageCentre[0]-halfImageSize[0] and RADeg<imageCentre[0]+halfImageSize[0] \
and decDeg>imageCentre[1]-halfImageSize[1] and decDeg<imageCentre[1]+halfImageSize[1]:
imageDiagonalClip=clipImageSectionWCS(imageData, imageWCS, RADeg,
decDeg, diagonalHalfSizeDeg*2.0)
diagonalClip=imageDiagonalClip['data']
diagonalWCS=imageDiagonalClip['wcs']
rotDeg=diagonalWCS.getRotationDeg()
imageRotated=ndimage.rotate(diagonalClip, rotDeg)
if diagonalWCS.isFlipped() == 1:
imageRotated=pylab.fliplr(imageRotated)
# Handle WCS rotation
rotatedWCS=diagonalWCS.copy()
rotRadians=math.radians(rotDeg)
if returnWCS == True:
try:
CD11=rotatedWCS.header['CD1_1']
CD21=rotatedWCS.header['CD2_1']
CD12=rotatedWCS.header['CD1_2']
CD22=rotatedWCS.header['CD2_2']
if rotatedWCS.isFlipped() == 1:
CD11=CD11*-1
CD12=CD12*-1
CDMatrix=numpy.array([[CD11, CD12], [CD21, CD22]], dtype=numpy.float64)
rotRadians=rotRadians
rot11=math.cos(rotRadians)
rot12=math.sin(rotRadians)
rot21=-math.sin(rotRadians)
rot22=math.cos(rotRadians)
rotMatrix=numpy.array([[rot11, rot12], [rot21, rot22]], dtype=numpy.float64)
newCDMatrix=numpy.dot(rotMatrix, CDMatrix)
P1=diagonalWCS.header['CRPIX1']
P2=diagonalWCS.header['CRPIX2']
V1=diagonalWCS.header['CRVAL1']
V2=diagonalWCS.header['CRVAL2']
PMatrix=numpy.zeros((2,), dtype = numpy.float64)
PMatrix[0]=P1
PMatrix[1]=P2
# BELOW IS HOW TO WORK OUT THE NEW REF PIXEL
CMatrix=numpy.array([imageRotated.shape[1]/2.0, imageRotated.shape[0]/2.0])
centreCoords=diagonalWCS.getCentreWCSCoords()
alphaRad=math.radians(centreCoords[0])
deltaRad=math.radians(centreCoords[1])
thetaRad=math.asin(math.sin(deltaRad)*math.sin(math.radians(V2)) + \
math.cos(deltaRad)*math.cos(math.radians(V2))*math.cos(alphaRad-math.radians(V1)))
phiRad=math.atan2(-math.cos(deltaRad)*math.sin(alphaRad-math.radians(V1)), \
math.sin(deltaRad)*math.cos(math.radians(V2)) - \
math.cos(deltaRad)*math.sin(math.radians(V2))*math.cos(alphaRad-math.radians(V1))) + \
math.pi
RTheta=(180.0/math.pi)*(1.0/math.tan(thetaRad))
xy=numpy.zeros((2,), dtype=numpy.float64)
xy[0]=RTheta*math.sin(phiRad)
xy[1]=-RTheta*math.cos(phiRad)
newPMatrix=CMatrix - numpy.dot(numpy.linalg.inv(newCDMatrix), xy)
# But there's a small offset to CRPIX due to the rotatedImage being rounded to an integer
# number of pixels (not sure this helps much)
#d=numpy.dot(rotMatrix, [diagonalClip.shape[1], diagonalClip.shape[0]])
#offset=abs(d)-numpy.array(imageRotated.shape)
rotatedWCS.header['NAXIS1']=imageRotated.shape[1]
rotatedWCS.header['NAXIS2']=imageRotated.shape[0]
rotatedWCS.header['CRPIX1']=newPMatrix[0]
rotatedWCS.header['CRPIX2']=newPMatrix[1]
rotatedWCS.header['CRVAL1']=V1
rotatedWCS.header['CRVAL2']=V2
rotatedWCS.header['CD1_1']=newCDMatrix[0][0]
rotatedWCS.header['CD2_1']=newCDMatrix[1][0]
rotatedWCS.header['CD1_2']=newCDMatrix[0][1]
rotatedWCS.header['CD2_2']=newCDMatrix[1][1]
rotatedWCS.updateFromHeader()
except KeyError:
if REPORT_ERRORS == True:
print("WARNING: astImages.clipRotatedImageSectionWCS() : no CDi_j keywords found - not rotating WCS.")
imageRotated=diagonalClip
rotatedWCS=diagonalWCS
imageRotatedClip=clipImageSectionWCS(imageRotated, rotatedWCS, RADeg, decDeg, clipSizeDeg)
if returnWCS == True:
return {'data': imageRotatedClip['data'], 'wcs': imageRotatedClip['wcs']}
else:
return {'data': imageRotatedClip['data'], 'wcs': None}
else:
if REPORT_ERRORS==True:
print("""ERROR: astImages.clipRotatedImageSectionWCS() :
RADeg, decDeg are not within imageData.""")
return None
#---------------------------------------------------------------------------------------------------
def clipUsingRADecCoords(imageData, imageWCS, RAMin, RAMax, decMin, decMax, returnWCS = True):
"""Clips a section from an image array at the pixel coordinates corresponding to the given
celestial coordinates.
@type imageData: numpy array
@param imageData: image data array
@type imageWCS: astWCS.WCS
@param imageWCS: astWCS.WCS object
@type RAMin: float
@param RAMin: minimum RA coordinate in decimal degrees
@type RAMax: float
@param RAMax: maximum RA coordinate in decimal degrees
@type decMin: float
@param decMin: minimum dec coordinate in decimal degrees
@type decMax: float
@param decMax: maximum dec coordinate in decimal degrees
@type returnWCS: bool
@param returnWCS: if True, return an updated WCS for the clipped section
@rtype: dictionary
@return: clipped image section (numpy array), updated astWCS WCS object for
clipped image section, and corresponding pixel coordinates in imageData in format
{'data', 'wcs', 'clippedSection'}.
@note: Returns 'None' if the requested position is not found within the image.
"""
imHeight=imageData.shape[0]
imWidth=imageData.shape[1]
xMin, yMin=imageWCS.wcs2pix(RAMin, decMin)
xMax, yMax=imageWCS.wcs2pix(RAMax, decMax)
xMin=int(round(xMin))
xMax=int(round(xMax))
yMin=int(round(yMin))
yMax=int(round(yMax))
X=[xMin, xMax]
X.sort()
Y=[yMin, yMax]
Y.sort()
if X[0] < 0:
X[0]=0
if X[1] > imWidth:
X[1]=imWidth
if Y[0] < 0:
Y[0]=0
if Y[1] > imHeight:
Y[1]=imHeight
clippedData=imageData[Y[0]:Y[1],X[0]:X[1]]
# Update WCS
if returnWCS == True:
try:
oldCRPIX1=imageWCS.header['CRPIX1']
oldCRPIX2=imageWCS.header['CRPIX2']
clippedWCS=imageWCS.copy()
clippedWCS.header['NAXIS1']=clippedData.shape[1]
clippedWCS.header['NAXIS2']=clippedData.shape[0]
clippedWCS.header['CRPIX1']=oldCRPIX1-X[0]
clippedWCS.header['CRPIX2']=oldCRPIX2-Y[0]
clippedWCS.updateFromHeader()
except KeyError:
if REPORT_ERRORS == True:
print("WARNING: astImages.clipUsingRADecCoords() : no CRPIX1, CRPIX2 keywords found - not updating clipped image WCS.")
clippedData=imageData[Y[0]:Y[1],X[0]:X[1]]
clippedWCS=imageWCS.copy()
else:
clippedWCS=None
return {'data': clippedData, 'wcs': clippedWCS, 'clippedSection': [X[0], X[1], Y[0], Y[1]]}
#---------------------------------------------------------------------------------------------------
def scaleImage(imageData, imageWCS, scaleFactor):
"""Scales image array and WCS by the given scale factor.
@type imageData: numpy array
@param imageData: image data array
@type imageWCS: astWCS.WCS
@param imageWCS: astWCS.WCS object
@type scaleFactor: float or list or tuple
@param scaleFactor: factor to resize image by - if tuple or list, in format
[x scale factor, y scale factor]
@rtype: dictionary
@return: image data (numpy array), updated astWCS WCS object for image, in format {'data', 'wcs'}.
"""
if type(scaleFactor) == int or type(scaleFactor) == float:
scaleFactor=[float(scaleFactor), float(scaleFactor)]
scaledData=ndimage.zoom(imageData, scaleFactor)
# Take care of offset due to rounding in scaling image to integer pixel dimensions
properDimensions=numpy.array(imageData.shape)*scaleFactor
offset=properDimensions-numpy.array(scaledData.shape)
# Rescale WCS
try:
oldCRPIX1=imageWCS.header['CRPIX1']
oldCRPIX2=imageWCS.header['CRPIX2']
CD11=imageWCS.header['CD1_1']
CD21=imageWCS.header['CD2_1']
CD12=imageWCS.header['CD1_2']
CD22=imageWCS.header['CD2_2']
except KeyError:
# Try the older FITS header format
try:
oldCRPIX1=imageWCS.header['CRPIX1']
oldCRPIX2=imageWCS.header['CRPIX2']
CD11=imageWCS.header['CDELT1']
CD21=0
CD12=0
CD22=imageWCS.header['CDELT2']
except KeyError:
if REPORT_ERRORS == True:
print("WARNING: astImages.rescaleImage() : no CDij or CDELT keywords found - not updating WCS.")
scaledWCS=imageWCS.copy()
return {'data': scaledData, 'wcs': scaledWCS}
CDMatrix=numpy.array([[CD11, CD12], [CD21, CD22]], dtype=numpy.float64)
scaleFactorMatrix=numpy.array([[1.0/scaleFactor[0], 0], [0, 1.0/scaleFactor[1]]])
scaledCDMatrix=numpy.dot(scaleFactorMatrix, CDMatrix)
scaledWCS=imageWCS.copy()
scaledWCS.header['NAXIS1']=scaledData.shape[1]
scaledWCS.header['NAXIS2']=scaledData.shape[0]
scaledWCS.header['CRPIX1']=oldCRPIX1*scaleFactor[0]+offset[1]
scaledWCS.header['CRPIX2']=oldCRPIX2*scaleFactor[1]+offset[0]
scaledWCS.header['CD1_1']=scaledCDMatrix[0][0]
scaledWCS.header['CD2_1']=scaledCDMatrix[1][0]
scaledWCS.header['CD1_2']=scaledCDMatrix[0][1]
scaledWCS.header['CD2_2']=scaledCDMatrix[1][1]
scaledWCS.updateFromHeader()
return {'data': scaledData, 'wcs': scaledWCS}
#---------------------------------------------------------------------------------------------------
def intensityCutImage(imageData, cutLevels):
"""Creates a matplotlib.pylab plot of an image array with the specified cuts in intensity
applied. This routine is used by L{saveBitmap} and L{saveContourOverlayBitmap}, which both
produce output as .png, .jpg, etc. images.
@type imageData: numpy array
@param imageData: image data array
@type cutLevels: list
@param cutLevels: sets the image scaling - available options:
- pixel values: cutLevels=[low value, high value].
- histogram equalisation: cutLevels=["histEq", number of bins ( e.g. 1024)]
- relative: cutLevels=["relative", cut per cent level (e.g. 99.5)]
- smart: cutLevels=["smart", cut per cent level (e.g. 99.5)]
["smart", 99.5] seems to provide good scaling over a range of different images.
@rtype: dictionary
@return: image section (numpy.array), matplotlib image normalisation (matplotlib.colors.Normalize), in the format {'image', 'norm'}.
@note: If cutLevels[0] == "histEq", then only {'image'} is returned.
"""
oImWidth=imageData.shape[1]
oImHeight=imageData.shape[0]
# Optional histogram equalisation
if cutLevels[0]=="histEq":
imageData=histEq(imageData, cutLevels[1])
anorm=pylab.Normalize(imageData.min(), imageData.max())
elif cutLevels[0]=="relative":
# this turns image data into 1D array then sorts
sorted=numpy.sort(numpy.ravel(imageData))
maxValue=sorted.max()
minValue=sorted.min()
# want to discard the top and bottom specified
topCutIndex=len(sorted-1) \
-int(math.floor(float((100.0-cutLevels[1])/100.0)*len(sorted-1)))
bottomCutIndex=int(math.ceil(float((100.0-cutLevels[1])/100.0)*len(sorted-1)))
topCut=sorted[topCutIndex]
bottomCut=sorted[bottomCutIndex]
anorm=pylab.Normalize(bottomCut, topCut)
elif cutLevels[0]=="smart":
# this turns image data into 1Darray then sorts
sorted=numpy.sort(numpy.ravel(imageData))
maxValue=sorted.max()
minValue=sorted.min()
numBins=10000 # 0.01 per cent accuracy
binWidth=(maxValue-minValue)/float(numBins)
histogram=ndimage.histogram(sorted, minValue, maxValue, numBins)
# Find the bin with the most pixels in it, set that as our minimum
# Then search through the bins until we get to a bin with more/or the same number of
# pixels in it than the previous one.
# We take that to be the maximum.
# This means that we avoid the traps of big, bright, saturated stars that cause
# problems for relative scaling
backgroundValue=histogram.max()
foundBackgroundBin=False
foundTopBin=False
lastBin=-10000
for i in range(len(histogram)):
if histogram[i]>=lastBin and foundBackgroundBin==True:
# Added a fudge here to stop us picking for top bin a bin within
# 10 percent of the background pixel value
if (minValue+(binWidth*i))>bottomBinValue*1.1:
topBinValue=minValue+(binWidth*i)
foundTopBin=True
break
if histogram[i]==backgroundValue and foundBackgroundBin==False:
bottomBinValue=minValue+(binWidth*i)
foundBackgroundBin=True
lastBin=histogram[i]
if foundTopBin==False:
topBinValue=maxValue
#Now we apply relative scaling to this
smartClipped=numpy.clip(sorted, bottomBinValue, topBinValue)
topCutIndex=len(smartClipped-1) \
-int(math.floor(float((100.0-cutLevels[1])/100.0)*len(smartClipped-1)))
bottomCutIndex=int(math.ceil(float((100.0-cutLevels[1])/100.0)*len(smartClipped-1)))
topCut=smartClipped[topCutIndex]
bottomCut=smartClipped[bottomCutIndex]
anorm=pylab.Normalize(bottomCut, topCut)
else:
# Normalise using given cut levels
anorm=pylab.Normalize(cutLevels[0], cutLevels[1])
if cutLevels[0]=="histEq":
return {'image': imageData.copy()}
else:
return {'image': imageData.copy(), 'norm': anorm}
#---------------------------------------------------------------------------------------------------
def resampleToTanProjection(imageData, imageWCS, outputPixDimensions=[600, 600]):
"""Resamples an image and WCS to a tangent plane projection. Purely for plotting purposes
(e.g., ensuring RA, dec. coordinate axes perpendicular).
@type imageData: numpy array
@param imageData: image data array
@type imageWCS: astWCS.WCS
@param imageWCS: astWCS.WCS object
@type outputPixDimensions: list
@param outputPixDimensions: [width, height] of output image in pixels
@rtype: dictionary
@return: image data (numpy array), updated astWCS WCS object for image, in format {'data', 'wcs'}.
"""
RADeg, decDeg=imageWCS.getCentreWCSCoords()
xPixelScale=imageWCS.getXPixelSizeDeg()
yPixelScale=imageWCS.getYPixelSizeDeg()
xSizeDeg, ySizeDeg=imageWCS.getFullSizeSkyDeg()
xSizePix=int(round(outputPixDimensions[0]))
ySizePix=int(round(outputPixDimensions[1]))
xRefPix=xSizePix/2.0
yRefPix=ySizePix/2.0
xOutPixScale=xSizeDeg/xSizePix
yOutPixScale=ySizeDeg/ySizePix
cardList=pyfits.CardList()
cardList.append(pyfits.Card('NAXIS', 2))
cardList.append(pyfits.Card('NAXIS1', xSizePix))
cardList.append(pyfits.Card('NAXIS2', ySizePix))
cardList.append(pyfits.Card('CTYPE1', 'RA---TAN'))
cardList.append(pyfits.Card('CTYPE2', 'DEC--TAN'))
cardList.append(pyfits.Card('CRVAL1', RADeg))
cardList.append(pyfits.Card('CRVAL2', decDeg))
cardList.append(pyfits.Card('CRPIX1', xRefPix+1))
cardList.append(pyfits.Card('CRPIX2', yRefPix+1))
cardList.append(pyfits.Card('CDELT1', -xOutPixScale))
cardList.append(pyfits.Card('CDELT2', xOutPixScale)) # Makes more sense to use same pix scale
cardList.append(pyfits.Card('CUNIT1', 'DEG'))
cardList.append(pyfits.Card('CUNIT2', 'DEG'))
newHead=pyfits.Header(cards=cardList)
newWCS=astWCS.WCS(newHead, mode='pyfits')
newImage=numpy.zeros([ySizePix, xSizePix])
tanImage=resampleToWCS(newImage, newWCS, imageData, imageWCS, highAccuracy=True,
onlyOverlapping=False)
return tanImage
#---------------------------------------------------------------------------------------------------
def resampleToWCS(im1Data, im1WCS, im2Data, im2WCS, highAccuracy = False, onlyOverlapping = True):
"""Resamples data corresponding to second image (with data im2Data, WCS im2WCS) onto the WCS
of the first image (im1Data, im1WCS). The output, resampled image is of the pixel same
dimensions of the first image. This routine is for assisting in plotting - performing
photometry on the output is not recommended.
Set highAccuracy == True to sample every corresponding pixel in each image; otherwise only
every nth pixel (where n is the ratio of the image scales) will be sampled, with values
in between being set using a linear interpolation (much faster).
Set onlyOverlapping == True to speed up resampling by only resampling the overlapping
area defined by both image WCSs.
@type im1Data: numpy array
@param im1Data: image data array for first image
@type im1WCS: astWCS.WCS
@param im1WCS: astWCS.WCS object corresponding to im1Data
@type im2Data: numpy array
@param im2Data: image data array for second image (to be resampled to match first image)
@type im2WCS: astWCS.WCS
@param im2WCS: astWCS.WCS object corresponding to im2Data
@type highAccuracy: bool
@param highAccuracy: if True, sample every corresponding pixel in each image; otherwise, sample
every nth pixel, where n = the ratio of the image scales.
@type onlyOverlapping: bool
@param onlyOverlapping: if True, only consider the overlapping area defined by both image WCSs
(speeds things up)
@rtype: dictionary
@return: numpy image data array and associated WCS in format {'data', 'wcs'}
"""
resampledData=numpy.zeros(im1Data.shape)
# Find overlap - speed things up
# But have a border so as not to require the overlap to be perfect
# There's also no point in oversampling image 1 if it's much higher res than image 2
xPixRatio=(im2WCS.getXPixelSizeDeg()/im1WCS.getXPixelSizeDeg())/2.0
yPixRatio=(im2WCS.getYPixelSizeDeg()/im1WCS.getYPixelSizeDeg())/2.0
xBorder=xPixRatio*10.0
yBorder=yPixRatio*10.0
if highAccuracy == False:
if xPixRatio > 1:
xPixStep=int(math.ceil(xPixRatio))
else:
xPixStep=1
if yPixRatio > 1:
yPixStep=int(math.ceil(yPixRatio))
else:
yPixStep=1
else:
xPixStep=1
yPixStep=1
if onlyOverlapping == True:
overlap=astWCS.findWCSOverlap(im1WCS, im2WCS)
xOverlap=[overlap['wcs1Pix'][0], overlap['wcs1Pix'][1]]
yOverlap=[overlap['wcs1Pix'][2], overlap['wcs1Pix'][3]]
xOverlap.sort()
yOverlap.sort()
xMin=int(math.floor(xOverlap[0]-xBorder))
xMax=int(math.ceil(xOverlap[1]+xBorder))
yMin=int(math.floor(yOverlap[0]-yBorder))
yMax=int(math.ceil(yOverlap[1]+yBorder))
xRemainder=(xMax-xMin) % xPixStep
yRemainder=(yMax-yMin) % yPixStep
if xRemainder != 0:
xMax=xMax+xRemainder
if yRemainder != 0:
yMax=yMax+yRemainder
# Check that we're still within the image boundaries, to be on the safe side
if xMin < 0:
xMin=0
if xMax > im1Data.shape[1]:
xMax=im1Data.shape[1]
if yMin < 0:
yMin=0
if yMax > im1Data.shape[0]:
yMax=im1Data.shape[0]
else:
xMin=0
xMax=im1Data.shape[1]
yMin=0
yMax=im1Data.shape[0]
for x in range(xMin, xMax, xPixStep):
for y in range(yMin, yMax, yPixStep):
RA, dec=im1WCS.pix2wcs(x, y)
x2, y2=im2WCS.wcs2pix(RA, dec)
x2=int(round(x2))
y2=int(round(y2))
if x2 >= 0 and x2 < im2Data.shape[1] and y2 >= 0 and y2 < im2Data.shape[0]:
resampledData[y][x]=im2Data[y2][x2]
# linear interpolation
if highAccuracy == False:
for row in range(resampledData.shape[0]):
vals=resampledData[row, numpy.arange(xMin, xMax, xPixStep)]
index2data=interpolate.interp1d(numpy.arange(0, vals.shape[0], 1), vals)
interpedVals=index2data(numpy.arange(0, vals.shape[0]-1, 1.0/xPixStep))
resampledData[row, xMin:xMin+interpedVals.shape[0]]=interpedVals
for col in range(resampledData.shape[1]):
vals=resampledData[numpy.arange(yMin, yMax, yPixStep), col]
index2data=interpolate.interp1d(numpy.arange(0, vals.shape[0], 1), vals)
interpedVals=index2data(numpy.arange(0, vals.shape[0]-1, 1.0/yPixStep))
resampledData[yMin:yMin+interpedVals.shape[0], col]=interpedVals
# Note: should really just copy im1WCS keywords into im2WCS and return that
# Only a problem if we're using this for anything other than plotting
return {'data': resampledData, 'wcs': im1WCS.copy()}
#---------------------------------------------------------------------------------------------------
def generateContourOverlay(backgroundImageData, backgroundImageWCS, contourImageData, contourImageWCS, \
contourLevels, contourSmoothFactor = 0, highAccuracy = False):
"""Rescales an image array to be used as a contour overlay to have the same dimensions as the
background image, and generates a set of contour levels. The image array from which the contours
are to be generated will be resampled to the same dimensions as the background image data, and
can be optionally smoothed using a Gaussian filter. The sigma of the Gaussian filter
(contourSmoothFactor) is specified in arcsec.
@type backgroundImageData: numpy array
@param backgroundImageData: background image data array
@type backgroundImageWCS: astWCS.WCS
@param backgroundImageWCS: astWCS.WCS object of the background image data array
@type contourImageData: numpy array
@param contourImageData: image data array from which contours are to be generated
@type contourImageWCS: astWCS.WCS
@param contourImageWCS: astWCS.WCS object corresponding to contourImageData
@type contourLevels: list
@param contourLevels: sets the contour levels - available options:
- values: contourLevels=[list of values specifying each level]
- linear spacing: contourLevels=['linear', min level value, max level value, number
of levels] - can use "min", "max" to automatically set min, max levels from image data
- log spacing: contourLevels=['log', min level value, max level value, number of
levels] - can use "min", "max" to automatically set min, max levels from image data
@type contourSmoothFactor: float
@param contourSmoothFactor: standard deviation (in arcsec) of Gaussian filter for
pre-smoothing of contour image data (set to 0 for no smoothing)
@type highAccuracy: bool
@param highAccuracy: if True, sample every corresponding pixel in each image; otherwise, sample
every nth pixel, where n = the ratio of the image scales.
"""
# For compromise between speed and accuracy, scale a copy of the background
# image down to a scale that is one pixel = 1/5 of a pixel in the contour image
# But only do this if it has CDij keywords as we know how to scale those
if ("CD1_1" in backgroundImageWCS.header) == True:
xScaleFactor=backgroundImageWCS.getXPixelSizeDeg()/(contourImageWCS.getXPixelSizeDeg()/5.0)
yScaleFactor=backgroundImageWCS.getYPixelSizeDeg()/(contourImageWCS.getYPixelSizeDeg()/5.0)
scaledBackground=scaleImage(backgroundImageData, backgroundImageWCS, (xScaleFactor, yScaleFactor))
scaled=resampleToWCS(scaledBackground['data'], scaledBackground['wcs'],
contourImageData, contourImageWCS, highAccuracy = highAccuracy)
scaledContourData=scaled['data']
scaledContourWCS=scaled['wcs']
scaledBackground=True
else:
scaled=resampleToWCS(backgroundImageData, backgroundImageWCS,
contourImageData, contourImageWCS, highAccuracy = highAccuracy)
scaledContourData=scaled['data']
scaledContourWCS=scaled['wcs']
scaledBackground=False
if contourSmoothFactor > 0:
sigmaPix=(contourSmoothFactor/3600.0)/scaledContourWCS.getPixelSizeDeg()
scaledContourData=ndimage.gaussian_filter(scaledContourData, sigmaPix)
# Various ways of setting the contour levels
# If just a list is passed in, use those instead
if contourLevels[0] == "linear":
if contourLevels[1] == "min":
xMin=contourImageData.flatten().min()
else:
xMin=float(contourLevels[1])
if contourLevels[2] == "max":
xMax=contourImageData.flatten().max()
else:
xMax=float(contourLevels[2])
nLevels=contourLevels[3]
xStep=(xMax-xMin)/(nLevels-1)
cLevels=[]
for j in range(nLevels+1):
level=xMin+j*xStep
cLevels.append(level)
elif contourLevels[0] == "log":
if contourLevels[1] == "min":
xMin=contourImageData.flatten().min()
else:
xMin=float(contourLevels[1])
if contourLevels[2] == "max":
xMax=contourImageData.flatten().max()
else:
xMax=float(contourLevels[2])
if xMin <= 0.0:
raise Exception("minimum contour level set to <= 0 and log scaling chosen.")
xLogMin=math.log10(xMin)
xLogMax=math.log10(xMax)
nLevels=contourLevels[3]
xLogStep=(xLogMax-xLogMin)/(nLevels-1)
cLevels=[]
prevLevel=0
for j in range(nLevels+1):
level=math.pow(10, xLogMin+j*xLogStep)
cLevels.append(level)
else:
cLevels=contourLevels
# Now blow the contour image data back up to the size of the original image
if scaledBackground == True:
scaledBack=scaleImage(scaledContourData, scaledContourWCS, (1.0/xScaleFactor, 1.0/yScaleFactor))['data']
else:
scaledBack=scaledContourData
return {'scaledImage': scaledBack, 'contourLevels': cLevels}
#---------------------------------------------------------------------------------------------------
def saveBitmap(outputFileName, imageData, cutLevels, size, colorMapName):
"""Makes a bitmap image from an image array; the image format is specified by the
filename extension. (e.g. ".jpg" =JPEG, ".png"=PNG).
@type outputFileName: string
@param outputFileName: filename of output bitmap image
@type imageData: numpy array
@param imageData: image data array
@type cutLevels: list
@param cutLevels: sets the image scaling - available options:
- pixel values: cutLevels=[low value, high value].
- histogram equalisation: cutLevels=["histEq", number of bins ( e.g. 1024)]
- relative: cutLevels=["relative", cut per cent level (e.g. 99.5)]
- smart: cutLevels=["smart", cut per cent level (e.g. 99.5)]
["smart", 99.5] seems to provide good scaling over a range of different images.
@type size: int
@param size: size of output image in pixels
@type colorMapName: string
@param colorMapName: name of a standard matplotlib colormap, e.g. "hot", "cool", "gray"
etc. (do "help(pylab.colormaps)" in the Python interpreter to see available options)
"""
cut=intensityCutImage(imageData, cutLevels)
# Make plot
aspectR=float(cut['image'].shape[0])/float(cut['image'].shape[1])
pylab.figure(figsize=(10,10*aspectR))
pylab.axes([0,0,1,1])
try:
colorMap=pylab.cm.get_cmap(colorMapName)
except AssertionError:
raise Exception(colorMapName+" is not a defined matplotlib colormap.")
if cutLevels[0]=="histEq":
pylab.imshow(cut['image'], interpolation="bilinear", origin='lower', cmap=colorMap)
else:
pylab.imshow(cut['image'], interpolation="bilinear", norm=cut['norm'], origin='lower',
cmap=colorMap)
pylab.axis("off")
pylab.savefig("out_astImages.png")
pylab.close("all")
try:
from PIL import Image
except:
raise Exception("astImages.saveBitmap requires the Python Imaging Library to be installed.")
im=Image.open("out_astImages.png")
im.thumbnail((int(size),int(size)))
im.save(outputFileName)
os.remove("out_astImages.png")
#---------------------------------------------------------------------------------------------------
def saveContourOverlayBitmap(outputFileName, backgroundImageData, backgroundImageWCS, cutLevels, \
size, colorMapName, contourImageData, contourImageWCS, \
contourSmoothFactor, contourLevels, contourColor, contourWidth):
"""Makes a bitmap image from an image array, with a set of contours generated from a
second image array overlaid. The image format is specified by the file extension
(e.g. ".jpg"=JPEG, ".png"=PNG). The image array from which the contours are to be generated
can optionally be pre-smoothed using a Gaussian filter.
@type outputFileName: string
@param outputFileName: filename of output bitmap image
@type backgroundImageData: numpy array
@param backgroundImageData: background image data array
@type backgroundImageWCS: astWCS.WCS
@param backgroundImageWCS: astWCS.WCS object of the background image data array
@type cutLevels: list
@param cutLevels: sets the image scaling - available options:
- pixel values: cutLevels=[low value, high value].
- histogram equalisation: cutLevels=["histEq", number of bins ( e.g. 1024)]
- relative: cutLevels=["relative", cut per cent level (e.g. 99.5)]
- smart: cutLevels=["smart", cut per cent level (e.g. 99.5)]
["smart", 99.5] seems to provide good scaling over a range of different images.
@type size: int
@param size: size of output image in pixels
@type colorMapName: string
@param colorMapName: name of a standard matplotlib colormap, e.g. "hot", "cool", "gray"
etc. (do "help(pylab.colormaps)" in the Python interpreter to see available options)
@type contourImageData: numpy array
@param contourImageData: image data array from which contours are to be generated
@type contourImageWCS: astWCS.WCS
@param contourImageWCS: astWCS.WCS object corresponding to contourImageData
@type contourSmoothFactor: float
@param contourSmoothFactor: standard deviation (in pixels) of Gaussian filter for
pre-smoothing of contour image data (set to 0 for no smoothing)
@type contourLevels: list
@param contourLevels: sets the contour levels - available options:
- values: contourLevels=[list of values specifying each level]
- linear spacing: contourLevels=['linear', min level value, max level value, number
of levels] - can use "min", "max" to automatically set min, max levels from image data
- log spacing: contourLevels=['log', min level value, max level value, number of
levels] - can use "min", "max" to automatically set min, max levels from image data
@type contourColor: string
@param contourColor: color of the overlaid contours, specified by the name of a standard
matplotlib color, e.g., "black", "white", "cyan"
etc. (do "help(pylab.colors)" in the Python interpreter to see available options)
@type contourWidth: int
@param contourWidth: width of the overlaid contours
"""
cut=intensityCutImage(backgroundImageData, cutLevels)
# Make plot of just the background image
aspectR=float(cut['image'].shape[0])/float(cut['image'].shape[1])
pylab.figure(figsize=(10,10*aspectR))
pylab.axes([0,0,1,1])
try:
colorMap=pylab.cm.get_cmap(colorMapName)
except AssertionError:
raise Exception(colorMapName+" is not a defined matplotlib colormap.")
if cutLevels[0]=="histEq":
pylab.imshow(cut['image'], interpolation="bilinear", origin='lower', cmap=colorMap)
else:
pylab.imshow(cut['image'], interpolation="bilinear", norm=cut['norm'], origin='lower',
cmap=colorMap)
pylab.axis("off")
# Add the contours
contourData=generateContourOverlay(backgroundImageData, backgroundImageWCS, contourImageData, \
contourImageWCS, contourLevels, contourSmoothFactor)
pylab.contour(contourData['scaledImage'], contourData['contourLevels'], colors=contourColor,
linewidths=contourWidth)
pylab.savefig("out_astImages.png")
pylab.close("all")
try:
from PIL import Image
except:
raise Exception("astImages.saveContourOverlayBitmap requires the Python Imaging Library to be installed")
im=Image.open("out_astImages.png")
im.thumbnail((int(size),int(size)))
im.save(outputFileName)
os.remove("out_astImages.png")
#---------------------------------------------------------------------------------------------------
def saveFITS(outputFileName, imageData, imageWCS = None):
"""Writes an image array to a new .fits file.
@type outputFileName: string
@param outputFileName: filename of output FITS image
@type imageData: numpy array
@param imageData: image data array
@type imageWCS: astWCS.WCS object
@param imageWCS: image WCS object
@note: If imageWCS=None, the FITS image will be written with a rudimentary header containing
no meta data.
"""
if os.path.exists(outputFileName):
os.remove(outputFileName)
newImg=pyfits.HDUList()
if imageWCS!=None:
hdu=pyfits.PrimaryHDU(None, imageWCS.header)
else:
hdu=pyfits.PrimaryHDU(None, None)
hdu.data=imageData
newImg.append(hdu)
newImg.writeto(outputFileName)
newImg.close()
#---------------------------------------------------------------------------------------------------
def histEq(inputArray, numBins):
"""Performs histogram equalisation of the input numpy array.
@type inputArray: numpy array
@param inputArray: image data array
@type numBins: int
@param numBins: number of bins in which to perform the operation (e.g. 1024)
@rtype: numpy array
@return: image data array
"""
imageData=inputArray
# histogram equalisation: we want an equal number of pixels in each intensity range
sortedDataIntensities=numpy.sort(numpy.ravel(imageData))
median=numpy.median(sortedDataIntensities)
# Make cumulative histogram of data values, simple min-max used to set bin sizes and range
dataCumHist=numpy.zeros(numBins)
minIntensity=sortedDataIntensities.min()
maxIntensity=sortedDataIntensities.max()
histRange=maxIntensity-minIntensity
binWidth=histRange/float(numBins-1)
for i in range(len(sortedDataIntensities)):
binNumber=int(math.ceil((sortedDataIntensities[i]-minIntensity)/binWidth))
addArray=numpy.zeros(numBins)
onesArray=numpy.ones(numBins-binNumber)
onesRange=list(range(binNumber, numBins))
numpy.put(addArray, onesRange, onesArray)
dataCumHist=dataCumHist+addArray
# Make ideal cumulative histogram
idealValue=dataCumHist.max()/float(numBins)
idealCumHist=numpy.arange(idealValue, dataCumHist.max()+idealValue, idealValue)
# Map the data to the ideal
for y in range(imageData.shape[0]):
for x in range(imageData.shape[1]):
# Get index corresponding to dataIntensity
intensityBin=int(math.ceil((imageData[y][x]-minIntensity)/binWidth))
# Guard against rounding errors (happens rarely I think)
if intensityBin<0:
intensityBin=0
if intensityBin>len(dataCumHist)-1:
intensityBin=len(dataCumHist)-1
# Get the cumulative frequency corresponding intensity level in the data
dataCumFreq=dataCumHist[intensityBin]
# Get the index of the corresponding ideal cumulative frequency
idealBin=numpy.searchsorted(idealCumHist, dataCumFreq)
idealIntensity=(idealBin*binWidth)+minIntensity
imageData[y][x]=idealIntensity
return imageData
#---------------------------------------------------------------------------------------------------
def normalise(inputArray, clipMinMax):
"""Clips the inputArray in intensity and normalises the array such that minimum and maximum
values are 0, 1. Clip in intensity is specified by clipMinMax, a list in the format
[clipMin, clipMax]
Used for normalising image arrays so that they can be turned into RGB arrays that matplotlib
can plot (see L{astPlots.ImagePlot}).
@type inputArray: numpy array
@param inputArray: image data array
@type clipMinMax: list
@param clipMinMax: [minimum value of clipped array, maximum value of clipped array]
@rtype: numpy array
@return: normalised array with minimum value 0, maximum value 1
"""
clipped=inputArray.clip(clipMinMax[0], clipMinMax[1])
slope=1.0/(clipMinMax[1]-clipMinMax[0])
intercept=-clipMinMax[0]*slope
clipped=clipped*slope+intercept
return clipped
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