[gnuastro-commits] master 5542d786 2/2: Book: corrected three minor typos in general tutorial

[Mohammad Akhlaghi]

branch: master
commit 5542d786ea6bd967bf5751af45bfa8fc3306a8ba
Author: Haleh Mesgari <haleh.mesgari@gmail.com>
Commit: Mohammad Akhlaghi <mohammad@akhlaghi.org>

    Book: corrected three minor typos in general tutorial
    
    Until now, there were three minor typos in the book that I noticed while
    reading the general program usage tutorial.
    
    With this commit, I have corrected them.
---
 doc/gnuastro.texi | 6 +++---
 1 file changed, 3 insertions(+), 3 deletions(-)

diff --git a/doc/gnuastro.texi b/doc/gnuastro.texi
index 052ef541..3be4b1c2 100644
--- a/doc/gnuastro.texi
+++ b/doc/gnuastro.texi
@@ -2630,7 +2630,7 @@ $ astscript-fits-view z-vs-tandist.fits
 @end example
 
 After TOPCAT opens, you will see the name of the table 
@file{z-vs-tandist.fits} in the left panel.
-On the top menu bar, select the ``Graphics'' menu, then select ``Plain plot'' 
to visualize the two columns printed above as a plot and get a better 
impression of the turn over point of the image cosmological coverage.
+On the top menu bar, select the ``Graphics'' menu, then select ``Plane plot'' 
to visualize the two columns printed above as a plot and get a better 
impression of the turn over point of the image cosmological coverage.
 
 
 
@@ -2673,7 +2673,7 @@ main(void)
   /* Constants from Plank 2018 (arXiv:1807.06209, Table 2) */
   double H0=67.66, olambda=0.6889, omatter=0.3111, oradiation=0;
 
-  /* Do the same thing for all redshifts (z) between 0.1 and 5. */
+  /* Do the same thing for all redshifts (z) between 0.1 and 10. */
   for(z=0.1; z<10; z+=0.01)
     @{
       /* Calculate the angular diameter distance. */
@@ -2918,7 +2918,7 @@ $ astscript-fits-view flat-ir/xdf-f160w.fits 
xdf-f160w_rotated.fits
 @end example
 
 Warp can generally be used for many kinds of pixel grid manipulation 
(warping), not just rotations.
-For example, the outputs of the commands below will have larger pixels 
respectively (new resolution being one quarter the original resolution), get 
shifted by 2.8 (by sub-pixel), get a shear of 2, and be tilted (projected).
+For example, the outputs of the commands below will have larger pixels 
respectively (new resolution being one quarter the original resolution), get 
shifted by 2.8 (by sub-pixel), get a shear of 0.2, and be tilted (projected).
 Run each of them and open the output file to see the effect, they will become 
handy for you in the future.
 
 @example