Table B.1
Coordinates of the Spitzer IRS observations used to extract the background spectra.
| RA (J2000) | Dec (J2000) | |||||||||||||
|
|
||||||||||||||
17 h 22 m 37  94 |
−23 ° 48 ′ 51  6 |
|||||||||||||
| 17 h 22 m 45 15 |
−23 ° 48 ′ 39 6 |
|||||||||||||
| 17 h 22 m 40 31 |
−23 ° 48 ′ 55 7 |
|||||||||||||
| 17 h 22 m 41 62 |
−23 ° 50 ′ 26 4 |
|||||||||||||
| 17 h 22 m 39 04 |
−23 ° 50 ′ 36 4 |
|||||||||||||
| 17 h 22 m 37 93 |
−23 ° 49 ′ 24 7 |
|||||||||||||
| 17 h 22 m 38 80 |
−23 ° 49 ′ 14 5 |
|||||||||||||
| 17 h 22 m 39 05 |
−23 ° 50 ′ 00 8 |
|||||||||||||
| 17 h 22 m 39 05 |
−23 ° 50 ′ 36 6 |
|||||||||||||
| 17 h 22 m 37 94 |
−23 ° 49 ′ 24 9 |
|||||||||||||
| 17 h 22 m 45 03 |
−23 ° 48 ′ 53 3 |
|||||||||||||
| 17 h 22 m 44 87 |
−23 ° 49 ′ 04 7 |
|||||||||||||
| 17 h 22 m 44 14 |
−23 ° 49 ′ 16 8 |
|||||||||||||
Notes. Apertures of 5 detector pixels in size corresponding to 9′′
were placed 20′′ left and right (in the detector frame) from the nominal target
position to avoid contamination from the stellar object a given observation was
aimed at. The slit width was 
. The coordinates are given in the
order of Fig. B.1.
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