I'm plotting this dataset and making a logarithmic fit, but, for some reason, the fit seems to be strongly wrong, at some point I got a good enough fit, but then I re ploted and there were that bad fit. At the very beginning there were a 0.0 0.0076 but I changed that to 0.001 0.0076 to avoid the asymptote.
I'm using (not exactly this one for the image above but now I'm testing with this one and there is that bad fit as well) this for the fit
f(x) = a*log(k*x + b)
fit = fit f(x) 'R_B/R_B.txt' via a, k, b
And the output is this
Also, sometimes it says 7 iterations were as is the case shown in the screenshot above, others only 1, and when it did the "correct" fit, it did like 35 iterations or something and got a = 32 if I remember correctly
Edit: here is again the good one, the plot I got is this one. And again, I re ploted and get that weird fit. It's curious that if there is the 0.0 0.0076 when the good fit it's about to be shown, gnuplot says "Undefined value during function evaluation", but that message is not shown when I'm getting the bad one.
Do you know why do I keep getting this inconsistence? Thanks for your help
As I already mentioned in comments the method of fitting antiderivatives is much better than fitting derivatives because the numerical calculus of derivatives is strongly scattered when the data is slightly scatered.
The principle of the method of fitting an integral equation (obtained from the original equation to be fitted) is explained in https://fr.scribd.com/doc/14674814/Regressions-et-equations-integrales . The application to the case of y=a.ln(c.x+b) is shown below.
Numerical calculus :
In order to get even better result (according to some specified criteria of fitting) one can use the above values of the parameters as initial values for iterarive method of nonlinear regression implemented in some convenient software.
NOTE : The integral equation used in the present case is :
NOTE : On the above figure one can compare the result with the method of fitting an integral equation to the result with the method of fitting with derivatives.
Acknowledgements : Alex Sveshnikov did a very good work in applying the method of regression with derivatives. This allows an interesting and enlightening comparison. If the goal is only to compute approximative values of parameters to be used in nonlinear regression software both methods are quite equivalent. Nevertheless the method with integral equation appears preferable in case of scattered data.
UPDATE (After Alex Sveshnikov updated his answer)
The figure below was drawn in using the Alex Sveshnikov's result with further iterative method of fitting.
The two curves are almost indistinguishable. This shows that (in the present case) the method of fitting the integral equation is almost sufficient without further treatment.
Of course this not always so satisfying. This is due to the low scatter of the data.
In ADDITION , answer to a question raised in comments by CosmeticMichu :
The problem here is that the fit algorithm starts with "wrong" approximations for parameters a, k, and b, so during the minimalization it finds a local minimum, not the global one. You can improve the result if you provide the algorithm with starting values, which are close to the optimal ones. For example, let's start with the following parameters:
gnuplot> a=47.5087
gnuplot> k=0.226
gnuplot> b=1.0016
gnuplot> f(x)=a*log(k*x+b)
gnuplot> fit f(x) 'R_B.txt' via a,k,b
....
....
....
After 40 iterations the fit converged.
final sum of squares of residuals : 16.2185
rel. change during last iteration : -7.6943e-06
degrees of freedom (FIT_NDF) : 18
rms of residuals (FIT_STDFIT) = sqrt(WSSR/ndf) : 0.949225
variance of residuals (reduced chisquare) = WSSR/ndf : 0.901027
Final set of parameters Asymptotic Standard Error
======================= ==========================
a = 35.0415 +/- 2.302 (6.57%)
k = 0.372381 +/- 0.0461 (12.38%)
b = 1.07012 +/- 0.02016 (1.884%)
correlation matrix of the fit parameters:
a k b
a 1.000
k -0.994 1.000
b 0.467 -0.531 1.000
The resulting plot is
Now the question is how you can find "good" initial approximations for your parameters? Well, you start with
If you differentiate this equation you get
or
The left-hand side of this equation is some constant 'C', so the expression in the right-hand side should be equal to this constant as well:
In other words, the reciprocal of the derivative of your data should be approximated by a linear function. So, from your data x[i], y[i] you can construct the reciprocal derivatives x[i], (x[i+1]-x[i])/(y[i+1]-y[i]) and the linear fit of these data:
The fit gives the following values:
C*k = 0.0236179
C*b = 0.106268
Now, we need to find the values for a, and C. Let's say, that we want the resulting graph to pass close to the starting and the ending point of our dataset. That means, that we want
a*log(k*x1 + b) = y1
a*log(k*xn + b) = yn
Thus,
a*log((C*k*x1 + C*b)/C) = a*log(C*k*x1 + C*b) - a*log(C) = y1
a*log((C*k*xn + C*b)/C) = a*log(C*k*xn + C*b) - a*log(C) = yn
By subtracting the equations we get the value for a:
a = (yn-y1)/log((C*k*xn + C*b)/(C*k*x1 + C*b)) = 47.51
Then,
log(k*x1+b) = y1/a
k*x1+b = exp(y1/a)
C*k*x1+C*b = C*exp(y1/a)
From this we can calculate C:
C = (C*k*x1+C*b)/exp(y1/a)
and finally find the k and b:
k=0.226
b=1.0016
These are the values used above for finding the better fit.
UPDATE
You can automate the process described above with the following script:
# Name of the file with the data
data='R_B.txt'
# The coordinates of the last data point
xn=NaN
yn=NaN
# The temporary coordinates of a data point used to calculate a derivative
x0=NaN
y0=NaN
linearFit(x)=Ck*x+Cb
fit linearFit(x) data using (xn=$1,dx=$1-x0,x0=$1,$1):(yn=$2,dy=$2-y0,y0=$2,dx/dy) via Ck, Cb
# The coordinates of the first data point
x1=NaN
y1=NaN
plot data using (x1=$1):(y1=$2) every ::0::0
a=(yn-y1)/log((Ck*xn+Cb)/(Ck*x1+Cb))
C=(Ck*x1+Cb)/exp(y1/a)
k=Ck/C
b=Cb/C
f(x)=a*log(k*x+b)
fit f(x) data via a,k,b
plot data, f(x)
pause -1
Related
This is my problem:
The first input is the observed data of MUSE, which is an astronomical instrument provides cubes, i.e. an image for each wavelength with a certain range. This means that, taken all the wavelengths corresponding to the pixel i,j, I can extract the spectrum for this pixel. Since these images are observed, for each pixel I have an error.
The second input is a spectrum template, i.e. a model of a spectrum. This template is assumed to be without error. I map this spectra at various redshift (this means multiply the wavelenghts for a factor 1+z, where z belong to a certain range).
The core of my code is the cross-correlation between the cube, i.e. the spectra extracted from each pixel, and the template mapped at different redshift. The result is a cross-correlation function for each pixel for each z, let's call this computed function as f(z). Taking, for each pixel, the argmax of f(z), I get the best redshift.
This is a common and widely-used process, indeed, it actually works well.
My question:
Since my input, i.e. the MUSE cube, has an error, I have propagated this error through the cross-correlation, obtaining an error on f(z), i.e. each f_i has a error sigma_i. So, how can I compute the error on z_max, which is the value of z corresponding to the maximum of f?
Maybe a solution could be the implementation of bootstrap method: I can extract, within the error of f, a certain number of function, for each of them I computed the argamx, so i can have an idea about the scatter of z_max.
By the way, I'm using python (3.x) and tensorflow has been used to compute the cross-correlation function.
Thanks!
EDIT
Following #TF_Support suggestion I'm trying to add some code and some figures to better understand the problem. But, before this, maybe it's better a little of math.
With this expression I had computed the cross-correlation:
where S is the spectra, T is the template and N is the normalization coefficient. Since S has an error, I had propagated these errors through the previous relation founding:
where SST_k is the the sum of the template squared and sigma_ij is the error on on S_ij (actually, I should have written sigma_S_ij).
The follow function (implemented with tensorflow 2.1) makes the cross-correlation between one template and the spectra of batch pixels, and computes the error on the cross-correlation function:
#tf.function
def make_xcorr_err1(T, S, sigma_S):
sum_spectra_sq = tf.reduce_sum(tf.square(S), 1) #shape (batch,)
sum_template_sq = tf.reduce_sum(tf.square(T), 0) #shape (Nz, )
norm = tf.sqrt(tf.reshape(sum_spectra_sq, (-1,1))*tf.reshape(sum_template_sq, (1,-1))) #shape (batch, Nz)
xcorr = tf.matmul(S, T, transpose_a = False, transpose_b= False)/norm
foo1 = tf.matmul(sigma_S**2, T**2, transpose_a = False, transpose_b= False)/norm**2
foo2 = xcorr**2 * tf.reshape(sum_template_sq**2, (1,-1)) * tf.reshape(tf.reduce_sum((S*sigma_S)**2, 1), (-1,1))/norm**4
foo3 = - 2 * xcorr * tf.reshape(sum_template_sq, (1,-1)) * tf.matmul(S*(sigma_S)**2, T, transpose_a = False, transpose_b= False)/norm**3
sigma_xcorr = tf.sqrt(tf.maximum(foo1+foo2+foo3, 0.))
Maybe, in order to understand my problem, more important than code is an image representing an output. This is the cross-correlation function for a single pixel, in red the maximum value, let's call z_best, i.e. the best cross-correlated value. The figure also shows the 3 sigma errors (the grey limits are +3sigma -3sigma).
If i zoom-in near the peak, I get this:
As you can see the maximum (as any other value) oscillates within a certain range. I would like to find a way to map this fluctuations of maximum (or the fluctuations around the maximum, or the fluctuations of the whole function) to an error on the value corresponding the maximum, i.e. an error on z_best.
My data has two columns: date (in Month/Year format) and corresponding value. I plotted this data on x-log(y) scale using gnuplot. It looks very close to a straight line. I am interested to draw a straight line using curve fitting. I tried with few fit functions but did not get success.
I tried the following fit functions:
f(x) = a * x + b (f(x) is not linear as scale is x-log(y))
f(x) = a*10**x + b (overflow error)
Any help in this regard would be appreciated.
The overflow error should be due to at least one large value of x. If you can rescale the x data so that there is no overflow when calculating 10**x, the fit might work. As a test, try something like:
x_scaled = x / 1000.0
f(x_scaled) = a*10**x_scaled + b
Inspecting the maximum value of x will give you an idea of the scaling value, shown as 1000.0 in my example.
I am trying to implement Expectation Maximization algorithm(Gaussian Mixture Model) on a data set data=[[x,y],...]. I am using mv_norm.pdf(data, mean,cov) function to calculate cluster responsibilities. But after calculating new values of covariance (cov matrix) after 6-7 iterations, cov matrix is becoming singular i.e determinant of cov is 0 (very small value) and hence it is giving errors
ValueError: the input matrix must be positive semidefinite
and
raise np.linalg.LinAlgError('singular matrix')
Can someone suggest any solution for this?
#E-step: Compute cluster responsibilities, given cluster parameters
def calculate_cluster_responsibility(data,centroids,cov_m):
pdfmain=[[] for i in range(0,len(data))]
for i in range(0,len(data)):
sum1=0
pdfeach=[[] for m in range(0,len(centroids))]
pdfeach[0]=1/3.*mv_norm.pdf(data[i], mean=centroids[0],cov=[[cov_m[0][0][0],cov_m[0][0][1]],[cov_m[0][1][0],cov_m[0][1][1]]])
pdfeach[1]=1/3.*mv_norm.pdf(data[i], mean=centroids[1],cov=[[cov_m[1][0][0],cov_m[1][0][1]],[cov_m[1][1][0],cov_m[0][1][1]]])
pdfeach[2]=1/3.*mv_norm.pdf(data[i], mean=centroids[2],cov=[[cov_m[2][0][0],cov_m[2][0][1]],[cov_m[2][1][0],cov_m[2][1][1]]])
sum1+=pdfeach[0]+pdfeach[1]+pdfeach[2]
pdfeach[:] = [x / sum1 for x in pdfeach]
pdfmain[i]=pdfeach
global old_pdfmain
if old_pdfmain==pdfmain:
return
old_pdfmain=copy.deepcopy(pdfmain)
softcounts=[sum(i) for i in zip(*pdfmain)]
calculate_cluster_weights(data,centroids,pdfmain,soft counts)
Initially, I've passed [[3,0],[0,3]] for each cluster covariance since expected number of clusters is 3.
Can someone suggest any solution for this?
The problem is your data lies in some manifold of dimension strictly smaller than the input data. In other words for example your data lies on a circle, while you have 3 dimensional data. As a consequence when your method tries to estimate 3 dimensional ellipsoid (covariance matrix) that fits your data - it fails since the optimal one is a 2 dimensional ellipse (third dimension is 0).
How to fix it? You will need some regularization of your covariance estimator. There are many possible solutions, all in M step, not E step, the problem is with computing covariance:
Simple solution, instead of doing something like cov = np.cov(X) add some regularizing term, like cov = np.cov(X) + eps * np.identity(X.shape[1]) with small eps
Use nicer estimator like LedoitWolf estimator from scikit-learn.
Initially, I've passed [[3,0],[0,3]] for each cluster covariance since expected number of clusters is 3.
This makes no sense, covariance matrix values has nothing to do with amount of clusters. You can initialize it with anything more or less resonable.
I understand how to render (two dimensional) "Escape Time Group" fractals (Julia and Mandelbrot), but I can't seem to get a Mobius Transformation or a Newton Basin rendered.
I'm trying to render them using the same method (by recursively using the polynomial equation on each pixel 'n' times), but I have a feeling these fractals are rendered using totally different methods. Mobius 'Transformation' implies that an image must already exist, and then be transformed to produce the geometry, and the Newton Basin seems to plot each point, not just points that fall into a set.
How are these fractals graphed? Are they graphed using the same iterative methods as the Julia and Mandelbrot?
Equations I'm Using:
Julia: Zn+1 = Zn^2 + C
Where Z is a complex number representing a pixel, and C is a complex constant (Correct).
Mandelbrot: Cn+1 = Cn^2 + Z
Where Z is a complex number representing a pixel, and C is the complex number (0, 0), and is compounded each step (The reverse of the Julia, correct).
Newton Basin: Zn+1 = Zn - (Zn^x - a) / (Zn^y - a)
Where Z is a complex number representing a pixel, x and y are exponents of various degrees, and a is a complex constant (Incorrect - creating a centered, eight legged 'line star').
Mobius Transformation: Zn+1 = (aZn + b) / (cZn + d)
Where Z is a complex number representing a pixel, and a, b, c, and d are complex constants (Incorrect, everything falls into the set).
So how are the Newton Basin and Mobius Transformation plotted on the complex plane?
Update: Mobius Transformations are just that; transformations.
"Every Möbius transformation is
a composition of translations,
rotations, zooms (dilations) and
inversions."
To perform a Mobius Transformation, a shape, picture, smear, etc. must be present already in order to transform it.
Now how about those Newton Basins?
Update 2: My math was wrong for the Newton Basin. The denominator at the end of the equation is (supposed to be) the derivative of the original function. The function can be understood by studying 'NewtonRoot.m' from the MIT MatLab source-code. A search engine can find it quite easily. I'm still at a loss as to how to graph it on the complex plane, though...
Newton Basin:
f(x) = x - f(x) / f'(x)
In Mandelbrot and Julia sets you terminate the inner loop if it exceeds a certain threshold as a measurement how fast the orbit "reaches" infinity
if(|z| > 4) { stop }
For newton fractals it is the other way round: Since the newton method is usually converging towards a certain value we are interested how fast it reaches its limit, which can be done by checking when the difference of two consecutive values drops below a certain value (usually 10^-9 is a good value)
if(|z[n] - z[n-1]| < epsilon) { stop }
I'm using the following gnuplot script to plot a linear fit:
#!/usr/bin/gnuplot
set term cairolatex
set output "linear_fit.tex"
c = 299792458.
x(x) = c / x
y(x) = x
h(x) = a * x + b
fit h(x) "linear_fit.dat" u (x($1)):(y($2)) via a,b
plot "linear_fit.dat" u (x($1)):(y($2)) w points title "", \
(h(x)) with lines linecolor rgb "black" title "Linear Fit"
However, after the iterations converge, b is always 1.0: https://dpaste.de/ozReq/
How can I get gnuplot to adjust b as well as a?
Update: Repeating the fit command a few hundred times with alternating via a/via b does give pretty good results, but that just can't be how it's supposed to be done.
Update 2: Here's the data in linear_fit.dat:
# lambda, V
360e-9 1.119
360e-9 1.148
360e-9 1.145
400e-9 0.949
400e-9 0.993
400e-9 0.971
440e-9 0.883
440e-9 0.875
440e-9 0.863
490e-9 0.737
490e-9 0.728
490e-9 0.755
540e-9 0.575
540e-9 0.571
540e-9 0.592
590e-9 0.457
590e-9 0.455
590e-9 0.482
I think your troubles stem from the fact that your x-values are very large (on the order of 10e14).
If you do not provide gnuplot with an initial guess for a and b, it will assume a=1 and b=1 as starting points for the fit. However, this is a poor initial guess:
Please note the log scale on both the x- and y-axis.
From the gnuplot documentation:
fit may, and often will get "lost" if started far from a solution, where SSR is large and changing slowly as the parameters are varied, or it may reach a numerically unstable region (e.g., too large a number causing a floating point overflow) which results in an "undefined value" message or gnuplot halting.
To improve the chances of finding the global optimum, you should set the starting values at least roughly in the vicinity of the solution, e.g., within an order of magnitude, if possible. The closer your starting values are to the solution, the less chance of stopping at another minimum. One way to find starting values is to plot data and the fitting function on the same graph and change parameter values and replot until reasonable similarity is reached. The same plot is also useful to check whether the fit stopped at a minimum with a poor fit.
In your case, such starting values could be:
a = 1e-15
b = -0.5
I obtained these values by eye-balling your range of values.
With those starting values, the linear fit results in:
Final set of parameters Asymptotic Standard Error
======================= ==========================
a = 1.97355e-015 +/- 6.237e-017 (3.161%)
b = -0.5 +/- 0.04153 (8.306%)
Which looks like this:
You can play with the control setting of fit (such as setting FIT_LIMIT = 1.e-35) or the starting values to achieve a better fit than this.
EDIT
While I still have not been able to coax gnuplot into modifying both parameters a, b at the same time, I found an alternate approach using R. I am aware that there are many other (scripting) languages that can perform a linear fit and this question was about gnuplot. However, the required effort with R appeared to be minimal.
Here's an example, which, when saved as linear_fit.R and called with
R CMD BATCH linear_fit.R
will provide the two coefficients of the linear fit, that gnuplot failed to provide.
y <- c(1.119, 1.148, 1.145, 0.949, 0.993, 0.971, 0.883, 0.875, 0.863,
0.737, 0.728, 0.755, 0.575, 0.571, 0.592, 0.457, 0.455, 0.482)
x <- c(3.60E-007, 3.60E-007, 3.60E-007, 4.00E-007, 4.00E-007,
4.00E-007, 4.40E-007, 4.40E-007, 4.40E-007, 4.90E-007,
4.90E-007, 4.90E-007, 5.40E-007, 5.40E-007, 5.40E-007,
5.90E-007, 5.90E-007, 5.90E-007)
c = 299792458.
x <- c/x
lm.out <- lm(y ~ x)
svg("linear_fit.svg")
plot(x,y)
abline(lm.out,col="red")
summary(lm.out)
You will end up with an svg-file that contains the plot and a linear_fit.Rout text file. In there you'll find the following coefficients:
Coefficients:
Estimate Std. Error t value Pr(>|t|)
(Intercept) -5.429e-01 4.012e-02 -13.53 3.55e-10 ***
x 2.037e-15 6.026e-17 33.80 2.61e-16 ***
So, in the terminology of the original question, we obtain:
a = 2.037e-15
b = -5.429e-01
These values are very close to the values you quoted from alternating the fit.
In case the comments get purged, these questions were identified as related:
What is gnuplot's internal representation of floating point numbers?
Gnuplot behaves oddly in polynomial fit. Why is that?