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![[DIR]](/icons/folder.gif){kind=icon}
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| Name | Last modified | Size | Description |
|---|---|---|---|---|
| Parent Directory | - | ||
| bri.gnp | 2006-09-09 19:25 | 1.1K | |
| images/ | 2006-09-09 21:19 | - | |
| luminance_scale.png | 2006-05-18 10:30 | 1.9K | |
| new.zip | 2006-09-09 21:19 | 3.4M | |
| scripts/ | 2006-09-09 21:21 | - | |
| txt/ | 2006-09-09 21:16 | - | |
| xvpics/ | 2006-09-09 19:52 | - | |
| moon_bri.txt | 2006-09-11 12:51 | 383 | brightness from imag. |
| bri.png | 2006-09-09 22:46 | 9.6K | graph of brightness |
| sqm.txt | 2006-09-09 15:14 | 305 | pairs of SQM readings |
| values.txt | 2006-09-08 17:56 | 1.7K | selected f. infod.txt |
| infod.txt | 2006-09-08 17:01 | 40K | summary info on imag. |
| overview.htm | 2006-09-11 12:45 | 9.3K | thumbnails with text |
Some overview of the employed method is available as an August lecture in Commision 50 of the IAU in Prague, see 06IAU50t_small.pdf (8 MB) within http://amper.ped.muni.cz/light/lectures/. Another info is in ../../ directory.