Merge pull request #1521 from astropy/det-table

Update detection table output
astropy · Apr 6, 2023 · f88fc50 · f88fc50
2 parents 319e63d + 1372edc
commit f88fc50
Showing 1 changed file with 16 additions and 15 deletions.
diff --git a/docs/detection.rst b/docs/detection.rst
@@ -68,21 +68,22 @@ finder:
     >>> daofind = DAOStarFinder(fwhm=3.0, threshold=5.*std)  # doctest: +REMOTE_DATA
     >>> sources = daofind(data - median)  # doctest: +REMOTE_DATA
     >>> for col in sources.colnames:  # doctest: +REMOTE_DATA
-    ...     sources[col].info.format = '%.8g'  # for consistent table output
-    >>> print(sources)  # doctest: +REMOTE_DATA
-     id xcentroid ycentroid sharpness  ... sky peak    flux       mag
-    --- --------- --------- ---------- ... --- ---- --------- ------------
-      1 144.24757 6.3797904 0.58156257 ...   0 6903 5.6976747   -1.8892441
-      2 208.66907 6.8205805 0.48348966 ...   0 7896 6.7186388   -2.0682032
-      3 216.92614 6.5775933 0.69359525 ...   0 2195 1.6662764  -0.55436758
-      4 351.62519 8.5459013 0.48577834 ...   0 6977 5.8970385   -1.9265849
-      5 377.51991 12.065501 0.52038488 ...   0 1260 1.1178252  -0.12093477
-    ...       ...       ...        ... ... ...  ...       ...          ...
-    282 267.90091 398.61991 0.27117231 ...   0 9299 5.4379278   -1.8385836
-    283 271.46959 398.91242 0.36738752 ...   0 8028 5.0693475   -1.7623802
-    284 299.05003 398.78469 0.25895667 ...   0 9072 5.5584641    -1.862387
-    285 299.99359 398.76661 0.29412474 ...   0 9253 5.3233471    -1.815462
-    286 360.44533 399.52381 0.37315624 ...   0 8079 6.9203438   -2.1003192
+    ...     if col not in ('id', 'npix'):
+    ...         sources[col].info.format = '%.2f'  # for consistent table output
+    >>> sources.pprint(max_width=76)  # doctest: +REMOTE_DATA, +FLOAT_CMP
+     id xcentroid ycentroid sharpness roundness1 ... sky    peak  flux  mag
+    --- --------- --------- --------- ---------- ... ---- ------- ---- -----
+      1    144.25      6.38      0.58       0.20 ... 0.00 6903.00 5.70 -1.89
+      2    208.67      6.82      0.48      -0.13 ... 0.00 7896.00 6.72 -2.07
+      3    216.93      6.58      0.69      -0.71 ... 0.00 2195.00 1.67 -0.55
+      4    351.63      8.55      0.49      -0.34 ... 0.00 6977.00 5.90 -1.93
+      5    377.52     12.07      0.52       0.37 ... 0.00 1260.00 1.12 -0.12
+    ...       ...       ...       ...        ... ...  ...     ...  ...   ...
+    282    267.90    398.62      0.27      -0.43 ... 0.00 9299.00 5.44 -1.84
+    283    271.47    398.91      0.37       0.19 ... 0.00 8028.00 5.07 -1.76
+    284    299.05    398.78      0.26      -0.67 ... 0.00 9072.00 5.56 -1.86
+    285    299.99    398.77      0.29       0.36 ... 0.00 9253.00 5.32 -1.82
+    286    360.45    399.52      0.37      -0.19 ... 0.00 8079.00 6.92 -2.10
     Length = 286 rows
 
 Let's plot the image and mark the location of detected sources: