skypt
Converts between sample/line and ra/ dec positions
This program requires the user supply a "level 1" cube. That is, a
cube in raw camera geometry.
The user must also enter one of the following coordinates:
sample/line
ra/dec
The program will then compute the other coordinates and the ephemeris
time and pixel dn value.
Hint: If you would like to use this program for multiple points, look into the -batchlist option.
Categories
History
| Elizabeth Miller | 2006-03-21 | Original version |
| Elizabeth Miller | 2006-03-31 | Modified to output pvl and flat format files and added append option |
| Elizabeth Miller | 2006-04-14 | Added check for valid samp/line and ra/dec positions |
| Tracie Sucharski | 2006-04-21 | Do not check error on SetImage, because there might not be an intersection on the planet when dealing with sky images. |
| Sean Crosby | 2007-04-12 | Changed flatfile output so it duplicates PVL data. User now required to enter a flatfile name. |
| Debbie A. Cook | 2012-07-06 | Updated Spice members to be more compliant with Isis coding standards. References #972. |
| Kelvin Rodriguez | 2016-06-27 | Added functionality to compute celestial north clock angle, References #2365. |
| Sarah Sutton | 2024-03-26 | Converted to a callable app. References #5443. |