Table 1
Sample of Cassini ISS observations
| Image ID | Mid-time (UTC) | α c | δ c | TWIST | Line | Sample | α | δ | Body |
| (deg) | (deg) | (deg) | (px) | (px) | (deg) | (deg) | |||
|
|
|||||||||
| N1737793037 | 2013 Jan. 25 07:23:05.520 | 285.412852 | 36.716183 | 263.046719 | 609.39 | 510.68 | 285.454502 | 36.712389 | RHEA |
| N1741579125 | 2013 Mar. 10 03:04:09.504 | 270.623557 | −60.595875 | 289.597775 | 513.66 | 485.34 | 270.618847 | −60.587167 | RHEA |
| N1743357653 | 2013 Mar. 30 17:06:06.203 | 324.143836 | 66.000844 | 173.896805 | 515.52 | 511.77 | 324.143250 | 65.999481 | DIONE |
| N1745867263 | 2013 Apr. 28 18:12:40.241 | 279.208055 | 38.799972 | 263.343304 | 287.70 | 625.46 | 279.104368 | 38.769971 | DIONE |
| N1745867296 | 2013 Apr. 28 18:13:13.249 | 279.207869 | 38.800026 | 263.343304 | 332.70 | 603.70 | 279.124964 | 38.775671 | DIONE |
Notes. Columns αc, δc, and TWIST refer to the right ascension, declination, and twist angle of the camera’s pointing vector in the International Celestial Reference Frame (ICRF), while α and δ are the right ascension and declination in the ICRF for the body listed in the far right column. The full table is available from the CDS. The origin of the line, sample coordinate system is at the top left of the image with line y increasing downwards and sample x to the right. Image size is 1024 by 1024 pixels.
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