table of contents
other versions
- stretch 2016.2.0+dfsg-1
- testing 2018.0.0+dfsg-3+b1
- unstable 2018.0.0+dfsg-3+b1
- experimental 2019.0.0~rc1+dfsg-1
CELESTE_STANDALONE(1) | HUGIN | CELESTE_STANDALONE(1) |
NAME¶
celeste_standalone - Cloud identificationSYNOPSIS¶
celeste_standalone [options] image1 image2 [..]DESCRIPTION¶
Celeste has been trained using Support vector machine techniques to identify clouds in photos and remove control points from these areas. celeste_standalone is a command-line tool with all the same functionality as Celeste in hugin.Simple usage is to just 'clean' an existing project file:
celeste_standalone -i project.pto -o project.pto
OPTIONS¶
- -i <filename>
- Input Hugin PTO file. Control points over SVM threshold will be removed before being written to the output file. If -m is set to 1, images in the file will be also be masked.
- -o <filename>
- Output Hugin PTO file. Default: '<filename>_celeste.pto'
- -d <filename>
- SVM model file. Default: 'data/celeste.model'
- -s <int>
- Maximum dimension for re-sized image prior to processing. A higher value will increase the resolution of the mask but is significantly slower. Default: 800
- -t <float>
- SVM threshold. Raise this value to remove fewer control points, lower it to remove more. Range 0 to 1. Default: 0.5
- -m <1|0>
- Create masks when processing Hugin PTO file. Default: 0
- -f <string>
- Mask file format. Options are PNG, JPEG, BMP, GIF and TIFF. Default: PNG
- -r <1|0>
- Filter radius. 0 = large (more accurate), 1 = small (higher resolution mask, slower, less accurate). Default: 0
- -h
- Print usage.
AUTHORS¶
Written by Tim Nugent.2017-02-26 | "Version: 2016.2.0" |