[gnuastro-commits] master c47dfb35 1/2: README: added description of newly added zero point script

[Mohammad Akhlaghi]

branch: master
commit c47dfb35335e1b0df737a9935b923e6a699c1682
Author: Mohammad Akhlaghi <mohammad@akhlaghi.org>
Commit: Mohammad Akhlaghi <mohammad@akhlaghi.org>

    README: added description of newly added zero point script
    
    Until now, there was no description of the newly added zero point script in
    the README file or in the list of Gnuastro programs within the book.
    
    With this commit, a description of them has been added in these two parts.
---
 README            | 4 ++++
 doc/gnuastro.texi | 3 +++
 2 files changed, 7 insertions(+)

diff --git a/README b/README
index 22cd08ef..40d522ba 100644
--- a/README
+++ b/README
@@ -152,6 +152,10 @@ very similarly (with minor differences, as explained in 
the book).
     coordinates of a star in the image, do sub-pixel re-positioning of the
     PSF, scale it to the star and subtract it from the image.
 
+  - astscript-zeropoint: Estimate the zero point (to calibrate pixel
+    values) of an input image using a reference image or a reference
+    catalog.
+
 All the programs share the same basic command-line user interface and a set
 of common options for the comfort of both the users and
 developers. Gnuastro is written to comply fully with the GNU coding
diff --git a/doc/gnuastro.texi b/doc/gnuastro.texi
index 56720ee6..74439261 100644
--- a/doc/gnuastro.texi
+++ b/doc/gnuastro.texi
@@ -1123,6 +1123,9 @@ The object can be at any location in the image, using 
various measures (median,
 @item astscript-sort-by-night
 (See @ref{Sort FITS files by night}) Given a list of FITS files, and a HDU and 
keyword name (for a date), this script separates the files in the same night 
(possibly over two calendar days).
 
+@item astscript-zeropoint
+(see @ref{Zero point estimation}) Estimate the zero point (to calibrate pixel 
values) of an input image using a reference image or a reference catalog.
+
 @item astscript-psf-*
 The following scripts are used to estimate the extended PSF estimation and 
subtraction as described in the tutorial @ref{Building the extended PSF}: