[gnuastro-commits] master d81c651: Book: minor typo fixed in the radial profile script section

[Mohammad Akhlaghi]

branch: master
commit d81c65187086f036dc7708df46ba6d47e19cc5db
Author: Raul Infante-Sainz <infantesainz@gmail.com>
Commit: Mohammad Akhlaghi <mohammad@akhlaghi.org>

    Book: minor typo fixed in the radial profile script section
    
    With this commit, a very minor typo has been corrected.
---
 doc/gnuastro.texi | 2 +-
 1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/doc/gnuastro.texi b/doc/gnuastro.texi
index 4c8b14c..913b274 100644
--- a/doc/gnuastro.texi
+++ b/doc/gnuastro.texi
@@ -20501,7 +20501,7 @@ To obtain these values, you can use @ref{NoiseChisel} 
to detect signal in the im
 @noindent
 @strong{Masking other sources:} The image of an astronomical object will 
usually have many other sources with your main target.
 A crude solution is to use sigma-clipped measurements for the profile.
-However, sigma-clipped measurements can easily be baised when the number of 
sources at each radial distance increases at larger distances.
+However, sigma-clipped measurements can easily be biased when the number of 
sources at each radial distance increases at larger distances.
 Therefore a robust solution is to mask all other detections within the image.
 You can use @ref{NoiseChisel} and @ref{Segment} to detect and segment the 
sources, then set all pixels that don't belong to your target to blank using 
@ref{Arithmetic} (in particular, its @code{where} operator).
 @end cartouche