*Python is a very versatile piece of software. It offers many choices for Web applications and can be used in thousands of third party modules. Python is also an effective tool for regression analysis.*

I think that machine learning, data mining, chemometrics and statistics are not the same thing but there are aspects that are common to all four topics. For example, a chapter about regression analysis (the techniques for estimating the numeric relationship among data elements) can be found in books on each of them. Some examples include Reference 1 chapter 6, Reference 2 chapter 13, Reference 3 chapter 2, and Reference 4 chapter 7. In the real world, sometimes there are problems with the fundamentals of linear algebra. There is also the idea that a higher explained variance or a higher correlation means a better model. Or that the only way is the use of a commercial spreadsheet. For these reasons, I think that itās necessary to clarify some things with an introductory article.

From a more technical point of view, for example, if I need to measure the concentration of a certain substance in an underground water sample, I must be capable of measuring a concentration less than 10 times the minimum concentration admitted. For example, if the contamination limit is 1.1 micrograms per litre, I must, at least, be capable of measuring a concentration equal to 0.11 micrograms per litre (these values depend on national laws). With a limit settled by the law, the choice of a regression model becomes even more important. That choice is important also in ion chromatography, because it’s better to speak of calibration rather than linearity. The calibration can’t always be represented by a regression of the first order, but can be represented sometimes, by a second degree curve. So the concept of linearity should be carefully considered, particularly with regard to the measurement for suppressed conductivity (see Reference 5). This problem is not considered in some methods in which the calibration is valid only if it’s linear, discarding a *priori* any other type of model.

**The toolbox**

This article is based on Mint 18 Xfce, Emacs 24.5, Geany and Anaconda. The last software can be freely downloaded from *https://www.continuum.io/downloads.* Then, from the terminal window, type* bash Anaconda3-4.1.1-Linux-x86.sh* and just follow the instructions on the screen. Because the packages PrettyTable and Seaborn are not available in the Anaconda distribution, I have easily installed them by typing the following code in a terminal window:

cd /home/<your-username>/anaconda_4.1.1/bin easy_install prettytable easy_install seaborn

My Emacs configuration for Python on Linux is almost the same as on Windows (see the September 2016 issue of OSFY). There is only one difference, because I have replaced the line given below:

(add-to-list āexec-path āC:\\WinPython-32bit-3.4.4.2\\python-3.4.4ā)

ā¦ with the following ones:

(setq python-shell-interpreter ā/home/<your-username>/anaconda_4.1.1/bin/pythonā org-babel-python-command ā/home/<your-username>/anaconda_4.1.1/bin/pythonā)

With respect to Geany, I have settled only the āExecuteā command* /home/<your username>/anaconda_4.1.1/bin/python ā%fā*

**Regression models**

The first way to build a polynomial model is by using matrix algebra. Let’s consider the following code, which is used instead of equations:

w=xlrd.open_workbook(āfilename.xlsā).sheet_by_name(āSheet1ā) x,y=w.col_values(0),w.col_values(1) degree=1 weight=1/array(x)**2 f=zeros((w.nrows,degree+1)) for i in range(0,w.nrows): for j in range(0,degree+1): f[i,j]=x[i]**j q=diag(weight) fT=dot(transpose(f),q) fTf=dot(fT,f) # fTf=fTf+diag([0.001]*(degree+1)) fTy=dot(fT,y) coef=dot(inv(fTf),fTy) xx=linspace(min(x),max(x),1000) yp=polyval(coef[::-1],xx)

In the example, the degree is equal to 1 (a linear model) and the weight is equal to 1/x2 (this is a weighted model). For a simple linear model, degree=1 and weight=1 (or *weight=1/array(x)**0*). For a simple quadratic model, degree=2 and weight=1. With some simple matrix calculations, itās possible to know the coefficients *coef* of the model and then plot the curve *xx vs yp*. For fitting through zero, set *weight=1/array(x)**0* and* for j* *in range(1,degree+1);* add a small constant, for example 0.001, to the diagonal of *fTf*. For a linear model, the predicted values (x values back calculated) are calculated with *predicted*=*(y-intercept)*/*slope* and, for a quadratic model, with* predicted=(-b+sqrt(b**2-(4*a*delta)))/(2*a)* in which* delta=c-y.* The *a, b* and *c* values are about the coefficient of the second degree term, the coefficient of the first degree term and the constant value, respectively. The accuracy is then calculated as *accuracy=predicted*100/x*. The following tables present a linear simple and a linear weighted model for the same experimental data. Iām not a big fan of the squared correlation coefficient, but, considering only that, I should choose the linear model simple, because itās the one with the highest value of R2. I think it would be better to consider the āAccuracyā column in both tables and choose the weighted model. In this particular example, we must also consider what is already mentioned in the āIntroductionā section about the values established by law. Carry out these calculations using a spreadsheet (and without using macros), As I think that’s unnecessarily complicated.

Linear simple Intercept -9343.97333 Slope 16984.40793 R2 0.99860 +------+---------+-----------+-------------+ | X | Y | Predicted | Accuracy | +------+---------+-----------+-------------+ | 0.1 | 1633 | 0.65 | 646.30 | | 0.5 | 7610 | 1.00 | 199.64 | | 1.0 | 14930 | 1.43 | 142.92 | | 2.5 | 35347 | 2.63 | 105.25 | | 5.0 | 69403 | 4.64 | 92.73 | | 10.0 | 141643 | 8.89 | 88.90 | | 25.0 | 402754 | 24.26 | 97.05 | | 50.0 | 850161 | 50.61 | 101.21 | +-----+----------+-----------+-------------+ Linear weighted 1/x2 Intercept 123.19563 Slope 15010.23851 R2 0.99422 +--------+---------+--------------+-----------+ | X | Y | Predicted | Accuracy | +--------+---------+--------------+-----------+ | 0.1 | 1633 | 0.10 | 100.58 | | 0.5 | 7610 | 0.50 | 99.76 | | 1.0 | 14930 | 0.99 | 98.64 | | 2.5 | 35347 | 2.35 | 93.87 | | 5.0 | 69403 | 4.62 | 92.31 | | 10.0 | 141643 | 9.43 | 94.28 | | 25.0 | 402754 | 26.82 | 107.29 | | 50.0 | 850161 | 56.63 | 113.26 | +--------+---------+--------------+-----------+

Figure 1 shows the plot for another data set, a simulation more or less typical for a pharmacokinetics study.

Another way is to build a certain matrix via *vstack* and then apply *lstsq* on it. Each A matrix created with *vstack* has the structure shown in the following examples. There are two important things: if the model is built to fit through zero, there is a column of zeros and, if the model is quadratic, there is a column of squared *x*. The coefficients of each model are *a, b* and* c* (if quadratic).

Linear fit simple A=vstack([x,[1]*w.nrows]).T a,b=linalg.lstsq(A,y)[0] +------+-----+ A = | 0.1 | 1.0 | | 0.5 | 1.0 | | 1.0 | 1.0 | | 2.5 | 1.0 | | 5.0 | 1.0 | | 10.0 | 1.0 | | 25.0 | 1.0 | | 50.0 | 1.0 | +------+-----+ Linear fit through zero A=vstack([x,[0]*w.nrows]).T a,b=linalg.lstsq(A,y)[0] +------+-----+ A = | 0.1 | 0.0 | | 0.5 | 0.0 | | 1.0 | 0.0 | | 2.5 | 0.0 | | 5.0 | 0.0 | | 10.0 | 0.0 | | 25.0 | 0.0 | | 50.0 | 0.0 | +------+-----+ Quadratic fit simple A=vstack([x,[1]*w.nrows,array(x)**2]).T a,b,c=linalg.lstsq(A,y)[0] +------+-----+--------+ A = | 0.1 | 1.0 | 0.01 | | 0.5 | 1.0 | 0.25 | | 1.0 | 1.0 | 1.0 | | 2.5 | 1.0 | 6.25 | | 5.0 | 1.0 | 25.0 | | 10.0 | 1.0 | 100.0 | | 25.0 | 1.0 | 625.0 | | 50.0 | 1.0 | 2500.0 | +------+-----+--------+ Quadratic fit through zero A=vstack([x,array(x)**2,[0]*w.nrows]).T a,b,c=linalg.lstsq(A,y)[0] +------+--------+-----+ A = | 0.1 | 0.01 | 0.0 | | 0.5 | 0.25 | 0.0 | | 1.0 | 1.0 | 0.0 | | 2.5 | 6.25 | 0.0 | | 5.0 | 25.0 | 0.0 | | 10.0 | 100.0 | 0.0 | | 25.0 | 625.0 | 0.0 | | 50.0 | 2500.0 | 0.0 | +------+--------+-----+

Probably, the simplest way is the use of *polyfit* with the syntax *coef=polyfit(x,y,degree)*. For a better graphical presentation, I would like to say something about the use of LaTeX and about the couple Pandas + Seaborn, specifying also that the Pandas and Seaborn packages have more complex applications than the one presented here. LaTeX must be previously installed on your system; then just add rc(*ātextā,usetex=True*) in your script. The result is shown in Figure 2. About Pandas, in the following example, a *DataFrame* with three columns is created. Then, *x vs y* data are plotted using Seaborn with *regplot* (*lw=0 and marker=āoā*) and, last, the linear model is plotted always with *regplot* but with some different options* (lw=1 and marker=āā)*. The result is shown in Figure 3, which is practically the same as with *ggplot* for R. Note that the *ggplot* plotting system exists also for Python and it is available at *http://ggplot.yhathq.com*. Another way to obtain a *ggplot* like plot is with the use of a style sheet. For example, put *style.use(āggplotā)* before the plot command. To know all the styles available just use *print(style.available).*

import pandas as p import seaborn as s coef=polyfit(x,y,1) yp=polyval(coef,x) df=p.DataFrame({āConcā:x,āAbsā:y,āAbs predā:yp}) s.regplot(x=āConcā, y=āAbsā, data=df, ci=False, scatter_kws={ācolorā:āgā,āalphaā:0.5,āsā:90}, line_kws={ācolorā:āwā,āalphaā:0,ālwā:0}, marker=āoā) s.regplot(x=āConcā, y=āAbs predā, data=df, ci=False, scatter_kws={ācolorā:āwā,āalphaā:0,āsā:0}, line_kws={ācolorā:ākā,āalphaā:1,ālwā:1}, marker=āā)

The data frame here is printed via *prettytable*:

+------+-------+-----------+ | Conc | Abs | Abs pred | +------+-------+-----------+ | 0.05 | 0.046 | 0.053 | | 0.10 | 0.093 | 0.092 | | 0.20 | 0.171 | 0.172 | | 0.25 | 0.217 | 0.212 | | 0.50 | 0.418 | 0.412 | | 1.00 | 0.807 | 0.811 | +------+-------+-----------+

I have never used the confidence band in practice, but there are several ways to calculate and plot it. Here, a calculation is proposed based on the t-distribution from *scipy.stats*, where *ip* is the part below (inferior) the model and *sp* the part above (superior) it. The data set is taken from Reference 7. A nice explanation about the confidence intervals is reported, for example, in Reference 2 pages 86-91.

from scipy import stats n=w.nrows coef=polyfit(x,y,1) yp=polyval(coef,x) xx=linspace(min(x),max(x),1000) dx=sum((x-mean(x))**2) dy=sqrt(sum((y-yp)**2)/(n-2)) dd=((xx-mean(x))**2/dx) t=stats.t.ppf(0.95,n-2) ip=coef[1]+coef[0]*xx-(t*dy*sqrt(1/n+dd)) sp=coef[1]+coef[0]*xx+(t*dy*sqrt(1/n+dd)) plot(x,y,āoā,markerfacecolor=ālightgreenā,zorder=3) plot(x,yp,āk-ā,zorder=3) fill_between(xx,ip,sp,where=sp>=ip,edgecolor=ābā,facecolor=ābā,alpha=0.2,interpolate=True)

**The StatsModels package**

Another way to build a regression model is by using the StatsModels package in combination with the Pandas package. An example is shown in the following code. The values for x and y are read from an xls file, then the weight is defined as 1/x2. Using the Pandas package, a *DataFrame* is defined for the couple *x, y* and a *Series* for the weights. Two types of regression are then calculated: OLS (Ordinary Least Squares, the one previously called the linear fit simple) and WLS (Weighted Least Squares). Last, both models are plotted with a simple *plot*. More information can be printed for slope *ols_fit.params[1]*, intercept *ols_fit.params[0]*, r-squared* ols_fit.rsquared*, a little report *ols_fit.summary()* or the equivalent for the weighted model using āwlsā instead of āolsā. Two examples are shown in Figures 7 and 8. Further information, such as residuals and Cook’s distance, can be printed or plotted using *resid, resid_pearson* and *get_influence()* respectively. A nice and large collection of examples is presented in Reference 8.

import pandas as p import xlrd from statsmodels.formula.api import ols,wls w=xlrd.open_workbook(āpk.xlsā).sheet_by_name(āSheet1ā) x,y=w.col_values(0),w.col_values(1) weight=1/array(x)**2 df=p.DataFrame({āConcā:x,āRespā:y}) w=p.Series(weight) ols_fit=ols(āResp~Concā,data=df).fit() wls_fit=wls(āResp~Concā,data=df,weights=w).fit() figure(0) plot(x,y,āoā,markerfacecolor=ālightgreenā,zorder=3) plot(df[āConcā],ols_fit.predict(),color=ākā,zorder=3) figure(1) plot(x,y,āoā,markerfacecolor=ālightgreenā,zorder=3) plot(df[āConcā],wls_fit.predict(),color=ākā,zorder=3)

Even for the regression models, the Python language offers different ways to calculate the same things. Some of them have been presented here. I would like to say something about the piecewise, or segmented, regression models. In Python there are, for example, some techniques based on *numpy.piecewise* and* scipy.optimize*, but Iām not completely satisfied by them. For a segmented regression, as previously discussed in the article, āGet analytical with Rā published in September 2015 issue of OSFY, I prefer to use R with the package *segmented*. An interesting Python port called *pysegmented* is available from *https://github.com/e-koch/pysegmented* but, at present, itās only a partial port. More complex applications can be done with the Scikit-learn package (Reference 9), but this is another story, perhaps for another article in the future.