Option Name |
Description |
DEFAULT |
-outlist |
specifies name of output list of
mag files |
- |
-min_good |
minimum number of pixels >0
after dark subtraction to process image ( skip if less ) |
100000 |
-save_map_fits |
OBSOLATE |
FALSE |
-subtr_backgr |
if subtract fitted background
map, number of squares to divide image can be specified as parameter
value ( -subtr_backgr=10) default number of squares is 10 |
FALSE |
-n_apert |
number of apertures written to
mag file |
3 |
-on_parts |
if program is working on small
parts of bigger images |
FALSE |
-aperture |
if ciircular aperture should be
used as main apeture , radius of aperture must specified as value of
this parameter In case <0 do not use circular aperture but 3x3+3 |
-1 |
-fit_line |
if fit calibration line -
converting aparature magnitudo to normalized magnitudo |
FALSE |
-force |
if force processing of already
processed fit/fitc files |
FALSE |
-gzip |
if gzip mag files |
FALSE |
-dir |
output directory , NOTE : directory
should be finished with / to work properly , example use : -dir=../mag1/ instead of -dir=../mag1 |
current directory |
-dark |
path to dark frame file ( no
dark subtraction if not set ) |
empty |
-flat |
path to flat frame file ( no
flat division without this option ) |
empty |
-tresh_cluster |
treshold for cluster
determination ( in sigmas ) |
3 |
-tresh |
treshold for star detection ( in
sigmas ) |
5 |
-border |
size of border to be ignored in
photometry |
30 |
-verb |
level of verbosity can be
specified ( -verb=3 ) or maximaly verbose in case -verb without value |
not set |
-list |
specify name of list file :
-list=fits_files_list_file |
not set |
-flip |
if execute flip when saving mag
, flip type according to paramter CCD_ASAS_REVERSE_FOR_TRANSFORM in ccd.cfg file |
|
-txt |
OBSOLATE - if save to txt file
also |
FALSE |
-cluster |
if cluster photometry algorithm
should be used |
FALSE |
-starx -stary |
show details on star in this
position |
|
-pixels |
number of pixels in aperture (
if other then 3x3+3=12 ) |
12 |
-window |
specify window to perform
photometry , example : -window=(500,500)-(550,550) |
full image - border |
-calib |
EXPERIMENTAL : calibrate image
with specfied calibration frame |
|
-corr |
correct image with correction
frame specified in this option |
|
-test_fill |
fill some testing apertures |
FALSE |
-test |
run test version of
fast-photometry |