From ac8def611cb6327b873ae395e6be74b27a2a2654 Mon Sep 17 00:00:00 2001
From: ankit7540 <ankit7540.ipm02g@nctu.edu.tw>
Date: Fri, 3 Apr 2020 15:42:33 +0800
Subject: [PATCH] Readme updates, spellings fixed, some ambiguous sentences
 removed.

---
 python_module/README.md                                       | 4 ++--
 .../model_rotationalRaman_spectra/README.md                   | 4 ++--
 2 files changed, 4 insertions(+), 4 deletions(-)

diff --git a/python_module/README.md b/python_module/README.md
index bca4b0e..51edc0c 100644
--- a/python_module/README.md
+++ b/python_module/README.md
@@ -4,7 +4,7 @@ This module is broadly divided  into two sections , intensity and wavenumber cal
 
 **Intensity  calibration :**  Includes following files,
 
-`compute_spectra.py` : This is an independent module which imports energy state data (for H<sub>2</sub>, HD and D<sub>2</sub>) along with ratio of polarizability anisotropy matrix (at 532.2 nm) elements to compute the theoretical rotational Raman spectra of these gases. Temperature is included for Boltzmann population using which observable Raman spectra can be modeled. For obtaining the ratio of theoretical Raman intensities originating from a common rotational state (required for the `wavelength_sensivity.py` module ), taking a ratio of the computed intensities from common  rotational  states is required. This ratio is independent of the  Boltzmann  population.
+`compute_spectra.py` : This is an independent module which imports energy state data (for H<sub>2</sub>, HD and D<sub>2</sub>) along with ratio of polarizability anisotropy matrix  elements (at 532.2 nm, for our experiment) to compute the theoretical rotational Raman spectra of these gases. Temperature is included for Boltzmann population using which observable Raman spectra can be modeled. For obtaining the ratio of theoretical Raman intensities originating from a common rotational state (required for the `wavelength_sensivity.py` module ), taking a ratio of the computed intensities from common  rotational  states is required. This ratio is independent of the  Boltzmann  populations.
 
 For matrix elements of polarizability anisotropy for H<sub>2</sub>, HD and D<sub>2</sub>, at other wavelengths refer to this GitHub repository (<https://github.com/ankit7540/H2-PolarizabilityMatrixElements>) and research paper (<https://aip.scitation.org/doi/abs/10.1063/1.5011433>).
 
@@ -12,7 +12,7 @@ For matrix elements of polarizability anisotropy for H<sub>2</sub>, HD and D<sub
 
 **Wavenumber calibration :**  Includes following file,
 
-`wavenumber_cal.py` : It requires data on the band positions in pixels with the uncertainties, as vectors in a 1D txt file. (NumPy array can be directly used as well). Core program is just fitting the pixel with the reference wavelength data. The reference data in already included in the file with the error.
+`wavenumber_cal.py` : It requires data on the band positions in pixels with the uncertainties, as vectors in a 1D txt file. (NumPy array can be directly used as well). Corresponding reference data is also required as 1D arrays containing values and the errors. Core program is just fitting the pixel with the reference wavelength data. Example data sets are included.
 
 
 Requirements
diff --git a/python_module/intensity_calibration/model_rotationalRaman_spectra/README.md b/python_module/intensity_calibration/model_rotationalRaman_spectra/README.md
index 5c133ad..8380290 100644
--- a/python_module/intensity_calibration/model_rotationalRaman_spectra/README.md
+++ b/python_module/intensity_calibration/model_rotationalRaman_spectra/README.md
@@ -1,6 +1,6 @@
 # Theoretical intensities  for rotational Raman  bands of H<sub>2</sub>, HD and D<sub>2</sub>
 
-This section includes one file `compute_spectra.py` for the computation of the rotational Raman intensities of the three gases. Temperature is required  for computing the Boltzmann population. Wavelength dependent polarizability anisotropy matrix elements are required for the transition probability of the rotational Raman transitions. As an example, the data for the 532.199323 nm, specific to our experiment, was obtained  from  this repository (<https://github.com/ankit7540/H2-PolarizabilityMatrixElements>),  will be used here.
+This section includes one file `compute_spectra.py` for the computation of the rotational Raman intensities of the three gases. Temperature is required to be input  for computing the Boltzmann population. Wavelength dependent polarizability anisotropy matrix elements are required for the transition probability of the rotational Raman transitions. As an example, the data for the 532.199323 nm, specific to our experiment, was obtained  from  this repository (<https://github.com/ankit7540/H2-PolarizabilityMatrixElements>), and will be used here.
 
 
 Requirements
@@ -9,7 +9,7 @@ Python 2.7 or Python 3.x with NumPy  and  matplotlib
 
 Usage
 ----------------
-Following commands are run under the Python interpreter environment. (Alternatively use any Python IDE like Spyder, IDLE or PyCharm). *Spyder3 is has been used while writing and debugging.*
+Following commands are run under the Python interpreter environment. (Alternatively use any Python IDE like Spyder, IDLE or PyCharm). *Spyder running on Python 3.6 is has been used while writing and debugging.*
 
 ***When using Python interpreter in terminal***