Develop Reference

What is the equivalent of coo_matrix in Matlab?

I'm trying to translatethe following lines of code from Python to MATLAB. V, Id, and J are of size (6400,) which in MATLAB are 1 -by- 6400 row vectors. pts is of size 242.
My Python code
A = coo_matrix((V, (Id, J)), shape=(pts.size, pts.size)).tocsr()
A = A.tobsr(blocksize=(2, 2))
I translated the first line as follows to MATLAB
A = sparse(V,Id,J,242,242);
However, I got the error
Error using sparse
Index into matrix must be an integer.
How can I translate this code to MATLAB?

The MATLAB sparse function has several forms:
S = sparse(A)
S = sparse(m,n)
S = sparse(i,j,v)
S = sparse(i,j,v,m,n)
S = sparse(i,j,v,m,n,nz)
The form you are most likely looking for is the fourth one: S = sparse(i,j,v,m,n), and will want to call it (using your use case) as:
A = sparse(Id, J, V, 242, 242);
I think your error is that MATLAB wants the I and J indices first, followed by the value and you are making the value the first argument.

How can I get same results for fft2() in MATLAB and Python?

I am translating a MATLAB code to Python code but I get different results from numpy fft2() and MATLAB fft2(). Difference is not small. How can I get same result?
Where S is (10,10,3) array
In Python:
Normin1 = fft2(S)
print("Normin is\n",Normin1[:,:,0])
Output(Just first row):
Normin is
[[ 1.29098039e+01+0.00000000e+00j
-8.14368936e-01-4.02146547e-01j
4.57184468e-01+4.59545965e-01j
2.37898348e-01-1.58643666e-01j
-6.89491738e-02+1.65467814e-01j
3.29411765e-01-1.38777878e-17j
-6.89491738e-02-1.65467814e-01j
2.37898348e-01+1.58643666e-01j
4.57184468e-01-4.59545965e-01j
-8.14368936e-01+4.02146547e-01j]
But in MATLAB:
Normin1 = fft2(S);
Output of first row
44.27451 + 0.00000i
-1.04275 - 3.36765i
0.72446 - 1.92128i
0.02706 + 0.09694i
0.70692 + 0.28154i
-0.90980 + 0.00000i
0.70692 - 0.28154i
0.02706 - 0.09694i
0.72446 + 1.92128i
-1.04275 + 3.36765i

I solved my problem. Python does array operations row-wise. In contrast, Matlab/Octave does array operations column-wise. That why, it should be as follows to get same result,
MATLAB code:
Normin1 = fft2(S);
Python equivalent:
Normin1 = np.fft2(S.T).T

How do I vectorize the following loop in Numpy?

"""Some simulations to predict the future portfolio value based on past distribution. x is
a numpy array that contains past returns.The interpolated_returns are the returns
generated from the cdf of the past returns to simulate future returns. The portfolio
starts with a value of 100. portfolio_value is filled up progressively as
the program goes through every loop. The value is multiplied by the returns in that
period and a dollar is removed."""
portfolio_final = []
for i in range(10000):
portfolio_value = [100]
rand_values = np.random.rand(600)
interpolated_returns = np.interp(rand_values,cdf_values,x)
interpolated_returns = np.add(interpolated_returns,1)
for j in range(1,len(interpolated_returns)+1):
portfolio_value.append(interpolated_returns[j-1]*portfolio_value[j-1])
portfolio_value[j] = portfolio_value[j]-1
portfolio_final.append(portfolio_value[-1])
print (np.mean(portfolio_final))
I couldn't find a way to write this code using numpy. I was having a look at iterations using nditer but I was unable to move ahead with that.

I guess the easiest way to figure out how you can vectorize your stuff would be to look at the equations that govern your evolution and see how your portfolio actually iterates, finding patterns that could be vectorized instead of trying to vectorize the code you already have. You would have noticed that the cumprod actually appears quite often in your iterations.
Nevertheless you can find the semi-vectorized code below. I included your code as well such that you can compare the results. I also included a simple loop version of your code which is much easier to read and translatable into mathematical equations. So if you share this code with somebody else I would definitely use the simple loop option. If you want some fancy-pants vectorizing you can use the vector version. In case you need to keep track of your single steps you can also add an array to the simple loop option and append the pv at every step.
Hope that helps.
Edit: I have not tested anything for speed. That's something you can easily do yourself with timeit.
import numpy as np
from scipy.special import erf
# Prepare simple return model - Normal distributed with mu &sigma = 0.01
x = np.linspace(-10,10,100)
cdf_values = 0.5*(1+erf((x-0.01)/(0.01*np.sqrt(2))))
# Prepare setup such that every code snippet uses the same number of steps
# and the same random numbers
nSteps = 600
nIterations = 1
rnd = np.random.rand(nSteps)
# Your code - Gives the (supposedly) correct results
portfolio_final = []
for i in range(nIterations):
portfolio_value = [100]
rand_values = rnd
interpolated_returns = np.interp(rand_values,cdf_values,x)
interpolated_returns = np.add(interpolated_returns,1)
for j in range(1,len(interpolated_returns)+1):
portfolio_value.append(interpolated_returns[j-1]*portfolio_value[j-1])
portfolio_value[j] = portfolio_value[j]-1
portfolio_final.append(portfolio_value[-1])
print (np.mean(portfolio_final))
# Using vectors
portfolio_final = []
for i in range(nIterations):
portfolio_values = np.ones(nSteps)*100.0
rcp = np.cumprod(np.interp(rnd,cdf_values,x) + 1)
portfolio_values = rcp * (portfolio_values - np.cumsum(1.0/rcp))
portfolio_final.append(portfolio_values[-1])
print (np.mean(portfolio_final))
# Simple loop
portfolio_final = []
for i in range(nIterations):
pv = 100
rets = np.interp(rnd,cdf_values,x) + 1
for i in range(nSteps):
pv = pv * rets[i] - 1
portfolio_final.append(pv)
print (np.mean(portfolio_final))

Forget about np.nditer. It does not improve the speed of iterations. Only use if you intend to go one and use the C version (via cython).
I'm puzzled about that inner loop. What is it supposed to be doing special? Why the loop?
In tests with simulated values these 2 blocks of code produce the same thing:
interpolated_returns = np.add(interpolated_returns,1)
for j in range(1,len(interpolated_returns)+1):
portfolio_value.append(interpolated_returns[j-1]*portfolio[j-1])
portfolio_value[j] = portfolio_value[j]-1
interpolated_returns = (interpolated_returns+1)*portfolio - 1
portfolio_value = portfolio_value + interpolated_returns.tolist()
I assuming that interpolated_returns and portfolio are 1d arrays of the same length.

Using astropy.fits and numpy to apply coincidence corrections to SWIFT fits image

This question may be a little specialist, but hopefully someone might be able to help. I normally use IDL, but for developing a pipeline I'm looking to use python to improve running times.
My fits file handling setup is as follows:
import numpy as numpy
from astropy.io import fits
#Directory: /Users/UCL_Astronomy/Documents/UCL/PHASG199/M33_UVOT_sum/UVOTIMSUM/M33_sum_epoch1_um2_norm.img
with fits.open('...') as ima_norm_um2:
#Open UVOTIMSUM file once and close it after extracting the relevant values:
ima_norm_um2_hdr = ima_norm_um2[0].header
ima_norm_um2_data = ima_norm_um2[0].data
#Individual dimensions for number of x pixels and number of y pixels:
nxpix_um2_ext1 = ima_norm_um2_hdr['NAXIS1']
nypix_um2_ext1 = ima_norm_um2_hdr['NAXIS2']
#Compute the size of the images (you can also do this manually rather than calling these keywords from the header):
#Call the header and data from the UVOTIMSUM file with the relevant keyword extensions:
corrfact_um2_ext1 = numpy.zeros((ima_norm_um2_hdr['NAXIS2'], ima_norm_um2_hdr['NAXIS1']))
coincorr_um2_ext1 = numpy.zeros((ima_norm_um2_hdr['NAXIS2'], ima_norm_um2_hdr['NAXIS1']))
#Check that the dimensions are all the same:
print(corrfact_um2_ext1.shape)
print(coincorr_um2_ext1.shape)
print(ima_norm_um2_data.shape)
# Make a new image file to save the correction factors:
hdu_corrfact = fits.PrimaryHDU(corrfact_um2_ext1, header=ima_norm_um2_hdr)
fits.HDUList([hdu_corrfact]).writeto('.../M33_sum_epoch1_um2_corrfact.img')
# Make a new image file to save the corrected image to:
hdu_coincorr = fits.PrimaryHDU(coincorr_um2_ext1, header=ima_norm_um2_hdr)
fits.HDUList([hdu_coincorr]).writeto('.../M33_sum_epoch1_um2_coincorr.img')
I'm looking to then apply the following corrections:
# Define the variables from Poole et al. (2008) "Photometric calibration of the Swift ultraviolet/optical telescope":
alpha = 0.9842000
ft = 0.0110329
a1 = 0.0658568
a2 = -0.0907142
a3 = 0.0285951
a4 = 0.0308063
for i in range(nxpix_um2_ext1 - 1): #do begin
for j in range(nypix_um2_ext1 - 1): #do begin
if (numpy.less_equal(i, 4) | numpy.greater_equal(i, nxpix_um2_ext1-4) | numpy.less_equal(j, 4) | numpy.greater_equal(j, nxpix_um2_ext1-4)): #then begin
#UVM2
corrfact_um2_ext1[i,j] == 0
coincorr_um2_ext1[i,j] == 0
else:
xpixmin = i-4
xpixmax = i+4
ypixmin = j-4
ypixmax = j+4
#UVM2
ima_UVM2sum = total(ima_norm_um2[xpixmin:xpixmax,ypixmin:ypixmax])
xvec_UVM2 = ft*ima_UVM2sum
fxvec_UVM2 = 1 + (a1*xvec_UVM2) + (a2*xvec_UVM2*xvec_UVM2) + (a3*xvec_UVM2*xvec_UVM2*xvec_UVM2) + (a4*xvec_UVM2*xvec_UVM2*xvec_UVM2*xvec_UVM2)
Ctheory_UVM2 = - alog(1-(alpha*ima_UVM2sum*ft))/(alpha*ft)
corrfact_um2_ext1[i,j] = Ctheory_UVM2*(fxvec_UVM2/ima_UVM2sum)
coincorr_um2_ext1[i,j] = corrfact_um2_ext1[i,j]*ima_sk_um2[i,j]
The above snippet is where it is messing up, as I have a mixture of IDL syntax and python syntax. I'm just not sure how to convert certain aspects of IDL to python. For example, the ima_UVM2sum = total(ima_norm_um2[xpixmin:xpixmax,ypixmin:ypixmax]) I'm not quite sure how to handle.
I'm also missing the part where it will update the correction factor and coincidence correction image files, I would say. If anyone could have the patience to go over it with a fine tooth comb and suggest the neccessary changes I need that would be excellent.
The original normalised image can be downloaded here: Replace ... in above code with this file

One very important thing about numpy is that it does every mathematical or comparison function on an element-basis. So you probably don't need to loop through the arrays.
So maybe start where you convolve your image with a sum-filter. This can be done for 2D images by astropy.convolution.convolve or scipy.ndimage.filters.uniform_filter
I'm not sure what you want but I think you want a 9x9 sum-filter that would be realized by
from scipy.ndimage.filters import uniform_filter
ima_UVM2sum = uniform_filter(ima_norm_um2_data, size=9)
since you want to discard any pixel that are at the borders (4 pixel) you can simply slice them away:
ima_UVM2sum_valid = ima_UVM2sum[4:-4,4:-4]
This ignores the first and last 4 rows and the first and last 4 columns (last is realized by making the stop value negative)
now you want to calculate the corrections:
xvec_UVM2 = ft*ima_UVM2sum_valid
fxvec_UVM2 = 1 + (a1*xvec_UVM2) + (a2*xvec_UVM2**2) + (a3*xvec_UVM2**3) + (a4*xvec_UVM2**4)
Ctheory_UVM2 = - np.alog(1-(alpha*ima_UVM2sum_valid*ft))/(alpha*ft)
these are all arrays so you still do not need to loop.
But then you want to fill your two images. Be careful because the correction is smaller (we inored the first and last rows/columns) so you have to take the same region in the correction images:
corrfact_um2_ext1[4:-4,4:-4] = Ctheory_UVM2*(fxvec_UVM2/ima_UVM2sum_valid)
coincorr_um2_ext1[4:-4,4:-4] = corrfact_um2_ext1[4:-4,4:-4] *ima_sk_um2
still no loop just using numpys mathematical functions. This means it is much faster (MUCH FASTER!) and does the same.
Maybe I have forgotten some slicing and that would yield a Not broadcastable error if so please report back.
Just a note about your loop: Python's first axis is the second axis in FITS and the second axis is the first FITS axis. So if you need to loop over the axis bear that in mind so you don't end up with IndexErrors or unexpected results.

NumPy: matrix dot product incompatible with MATLAB

I'm trying to proceed some simple calculation in NumPy.
But it suddenly gives the results different with MATLAB calculations.
Here is the MATLAB example:
load temp; % here are the source matrices located
resp = ang_stv' * tmp;
respC = resp.'; % this is our variable to compare with Python
cd(fileparts(mfilename('fullpath')));
save('arythm_test.mat');
And here I try to calculate the same in Python:
dump_data = sp.io.loadmat("arythm_test.mat")
tmp = dump_data["tmp"]
ang_stv = dump_data["ang_stv"]
ref_resp = dump_data["respC"]
our_resp = np.dot(ang_stv.swapaxes(0, 1), tmp).swapaxes(0, 1)
np.testing.assert_allclose(our_resp, ref_resp)
Cannot you tell me, what am I doing wrong? And how to cope with it?
P.S. Here are temp.mat and arythm_test.mat

The answer was simple: the .' operator in MATLAB means simple transpose, and ' operator means transpose with complex conjugation. Oy vey...
tmp = dump_data["tmp"]
ang_stv = dump_data["ang_stv"]
print "tmp.shape", tmp.shape
print "ang_stv.shape", ang_stv.shape
ref_resp = dump_data["respC"]
our_resp = np.dot(np.conj(ang_stv.swapaxes(0, 1)), tmp).swapaxes(0, 1)