[gnuastro-commits] master c9387c35 1/2: psf-scale-factor: missing 'quiet' option to Crop and Warp calls added

[Mohammad Akhlaghi]

branch: master
commit c9387c35cd404aef5cff60b74315bf8c711aa830
Author: Raul Infante-Sainz <infantesainz@gmail.com>
Commit: Mohammad Akhlaghi <mohammad@akhlaghi.org>

    psf-scale-factor: missing 'quiet' option to Crop and Warp calls added
    
    Until this commit, there were some calls to 'astcrop' and 'astwarp' without
    the option '$quiet'. As a consequence, even when the user asked for
    '--quiet' mode from  the command-line, the script printed out more lines
    than just the result.
    
    With this commit, the quiet option ('$quiet') has been added to these
    invokations of 'astcrop' and 'astwarp'. In addition to that, several minor
    changes have been done with the aim of having proper identations and the
    full '--quiet' option instead of '-q'.
---
 bin/script/psf-scale-factor.in | 16 ++++++++--------
 1 file changed, 8 insertions(+), 8 deletions(-)

diff --git a/bin/script/psf-scale-factor.in b/bin/script/psf-scale-factor.in
index a917910e..f85722c6 100644
--- a/bin/script/psf-scale-factor.in
+++ b/bin/script/psf-scale-factor.in
@@ -650,8 +650,8 @@ if [ $nocentering = 0 ]; then
 
     # Read the overlap range from the 'ICF1PIX' keyword (which is printed
     # in all outputs of Crop).
-    overlaprange=$(astfits $cropped -h1 --keyvalue=ICF1PIX -q \
-                       | sed -e's|:| |g' -e's|,| |')
+    overlaprange=$(astfits $cropped -h1 --keyvalue=ICF1PIX --quiet \
+                           | sed -e's|:| |g' -e's|,| |')
 
     # Calculate the position of the bottom-left pixel of the cropped image
     # in relation to the input image.
@@ -684,14 +684,14 @@ if [ $nocentering = 0 ]; then
     # output above).
     warpped=$tmpdir/cropped-masked-warpforcenter-$objectid.fits
     DXY=$(echo "$warpcoord" | awk '{print $1}')
-    astwarp $cropped_masked --translate=$DXY --output=$warpped
+    astwarp $cropped_masked --translate=$DXY --output=$warpped $quiet
 
     # Crop image based on the calculated shift (second component of the
     # output above).
     centermsk=$tmpdir/cropped-masked-centered-$objectid.fits
     CXY=$(echo "$warpcoord" | awk '{print $2}')
     astcrop $warpped -h1 \
-            --mode=img --output=$centermsk \
+            --mode=img --output=$centermsk $quiet \
             --center=$CXY --width=$xwidthinpix,$ywidthinpix
 else
     # If the user did not want to correct the center of image, we'll use
@@ -705,10 +705,10 @@ fi
 
 # Crop the PSF image with the same size.
 psfcropped=$tmpdir/cropped-psf-$objectid.fits
-psfxcenter=$(astfits $psf -h$psfhdu --keyvalue=NAXIS1 -q \
-                 | awk '{print $1/2+0.5}')
-psfycenter=$(astfits $psf -h$psfhdu --keyvalue=NAXIS2 -q \
-                 | awk '{print $1/2+0.5}')
+psfxcenter=$(astfits $psf -h$psfhdu --keyvalue=NAXIS1 --quiet \
+                     | awk '{print $1/2+0.5}')
+psfycenter=$(astfits $psf -h$psfhdu --keyvalue=NAXIS2 --quiet \
+                     | awk '{print $1/2+0.5}')
 astcrop $psf --hdu=$psfhdu --mode=img \
         --center=$psfxcenter,$psfycenter \
         --width=$xwidthinpix,$ywidthinpix \