Update README.md

Author: ankit7540

README.md

@@ -33,7 +33,7 @@ In most cases, determining the individual performance of each optical element is
 
 In our work, we assume <i>M</i>(&nu;) &cong; C<sub>1</sub>(&nu;) C<sub>2</sub>(&nu;) / C<sub>0</sub>(&nu;) [The wavenumber dependence in not explicitly stated when C<sub>0</sub>, C<sub>1</sub> and C<sub>2</sub> are discussed in the following text. ]  The three contributions, C<sub>0</sub>(&nu;) to C<sub>2</sub>(&nu;)  are determined in two steps in this analysis.
 
-- In the first step, (C<sub>0</sub> / C<sub>1</sub>) correction are determined using the wavenumber axis and the spectrum of a broad band white light source. [(See example)](https://github.com/ankit7540/IntensityCalbr/blob/master/PythonModule/determine_C0_C1_correction/Examples/Example_for_C0_C1.ipynb)
+- In the first step, (C<sub>0</sub> / C<sub>1</sub>) correction are determined using the wavenumber axis and the spectrum of a broad band white light source. [(See example)](https://github.com/ankit7540/RamanSpecCalibration/blob/master/python_module/intensity_calibration/determine_C0_C1/Examples/Example_for_C0_C1.ipynb)
 - C<sub>2</sub> is determined from the observed Raman intensities, where the reference or true intensities are known or can be computed. This can be done using (i) pure-rotational Raman bands of molecular hydrogen and isotopologues, (ii) vibration-rotation Raman bands of the same gases and (iii) vibrational Raman bands of some liquids.
 
 The multiplicative correction to the Raman spectrum for intensity calibration is then : (C<sub>0</sub> / C<sub>1</sub>C<sub>2</sub>)
@@ -114,4 +114,4 @@ Ankit Raj, Chihiro Kato, Henryk A. Witek and Hiro‐o Hamaguchi<br>
 **Other repositories on this topic :**
 
 This repository is concerned with the anti-Stokes and Stokes region spanning from -1040 to 1700 cm<sup>-1</sup> using H<sub>2</sub>, HD, D<sub>2</sub> and O<sub>2</sub>. The 
-online repository [IntensityCalbr](https://github.com/ankit7540/IntensityCalbr) and the article ([(JRS.6221)](https://analyticalsciencejournals.onlinelibrary.wiley.com/doi/10.1002/jrs.6221)) are concerned with the higher wavenumber region (from 2300 to 4200 cm<sup>-1</sup>).
+online repository [IntensityCalbr](https://github.com/ankit7540/IntensityCalbr) and the article ([JRS.6221](https://analyticalsciencejournals.onlinelibrary.wiley.com/doi/10.1002/jrs.6221)) are concerned with the higher wavenumber region (from 2300 to 4200 cm<sup>-1</sup>).