Table C.2
Bright stars in Fig. C.1 that were used to derive a PSF.
Id | x | y | bg. | r max | colour | T |
|
||||||
1 | 195 | 409 | 1759 | 115.5 | solid black | ° |
2 | 262 | 252 | 1759 | 115.5 | dash-dotted black | ° |
3 | 801 | 870 | 1762 | 13 | blue | ° |
4 | 840 | 193 | 1760 | 25 | magenta | – |
5 | 256 | 565 | 1758 | 24 | red | • |
6 | 1164 | 1126 | 1760 | 20 | orange | x |
7 | 395 | 894 | 1758 | 18 | purple | • |
Notes.Column 1, identifier; Cols. 2 and 3, x and y positions in the reduced image (px.); Col. 4, background value used (ADU); Cols. 5 and 6, maximum radius (arcsec) and line colour in Fig. C.2; and Col. 7, four symbols specify if the region falls on top of the (T)idal streams around NGC 5907 that are seen in Fig. 2 in Martínez-Delgado et al. (2008): x outside of the field, – away, ° partly on top, • right on top.
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