• Home
  • History
  • Annotate
Name Date Size #Lines LOC

..14-Jul-2006-

READMEH A D24-Oct-20051.3 KiB3027

block_3x3.convH A D24-Oct-200592 65

default.convH A D24-Oct-200588 65

default.nnwH A D24-Oct-20052.1 KiB2922

default.paramH A D24-Oct-20051.2 KiB125102

default.sexH A D14-Jul-20063.5 KiB7652

gauss_1.5_3x3.convH A D24-Oct-2005157 65

gauss_2.0_3x3.convH A D24-Oct-2005159 75

gauss_2.0_5x5.convH A D24-Oct-2005305 87

gauss_2.5_5x5.convH A D24-Oct-2005300 87

gauss_3.0_5x5.convH A D24-Oct-2005300 87

gauss_3.0_7x7.convH A D24-Oct-2005516 109

gauss_4.0_7x7.convH A D24-Oct-2005516 109

gauss_5.0_9x9.convH A D24-Oct-2005804 1211

mexhat_1.5_5x5.convH A D24-Oct-2005337 87

mexhat_2.0_7x7.convH A D24-Oct-2005575 109

mexhat_2.5_7x7.convH A D24-Oct-2005575 109

mexhat_3.0_9x9.convH A D24-Oct-2005893 1211

mexhat_4.0_9x9.convH A D24-Oct-2005889 1211

mexhat_5.0_11x11.convH A D24-Oct-20051.3 KiB1413

tophat_1.5_3x3.convH A D24-Oct-2005159 65

tophat_2.0_3x3.convH A D24-Oct-2005159 65

tophat_2.5_3x3.convH A D24-Oct-2005159 65

tophat_3.0_3x3.convH A D24-Oct-2005159 65

tophat_4.0_5x5.convH A D24-Oct-2005303 87

tophat_5.0_5x5.convH A D24-Oct-2005303 87

README

1This directory contains several ASCII files related to SExtractor
2configuration:
3
4default.sex:	an example of SExtractor .sex configuration file.
5default.param:	a .param file, containing all parameters known by SExtractor.
6		To prevent some parameters to figure in the output catalog,
7		just erase or comment their names (by adding a # at the
8		beginning of the line).
9default.nnw:	a "Neural-Network-Weights" file for star/galaxy separation on
10		images with Moffat-like PSFs.
11*.conv:		several "classical" convolution masks for optimal detection:
12		- default.conv		a small pyramidal function (fast),
13		- gauss*.conv		a set of gaussian functions, for
14					seeing FWHMs between 1.5 and 5 pixels
15					(best for faint object detection),
16		- tophat*.conv		a set of "top-hat" functions. Use them
17					to detect extended, low-surface
18					brightness objects, with a very low
19					THRESHOLD.
20		- mexhat*.conv		"wavelets", producing a passband-
21					filtering of the image, tuned to
22					seeing FWHMs between 1.5 and 5 pixels.
23					Useful in very crowded star fields,
24					or in the vicinity of a nebula.
25					WARNING: may need a high THRESHOLD!!
26		- block_3x3.conv	a small "block" function (for rebinned
27					images like those of the DeNIS survey).
28
29		All these convolution files are normalized by default.
30