Table 1.
AGILE observations of the IGR J17354−3255 region.
| AGILE OB | l | b | Distance | Observation time |
|---|---|---|---|---|
| [deg] | [deg] | [deg] | [MJD] | |
| 1800 | 313.1 | −3.5 | 42.4 | 54335.5–54339.5 |
| 1900 | 334.4 | 10.1 | 23.3 | 54339.5–54344.5 |
| 4400 | 19.3 | −15.4 | 28.0 | 54386.5–54395.5 |
| 5400 | 332.1 | 0.0 | 23.4 | 54526.5–54541.5 |
| 5450 | 360.0 | 0.6 | 4.6 | 54541.5–54555.5 |
| 6200 | 355.5 | 7.4 | 7.7 | 54719.5–54749.5 |
| 6800 | 349.9 | 13.4 | 14.8 | 54890.5–54921.5 |
| 7010 | 18.1 | −13.8 | 26.2 | 54928.5–54936.5 |
| 7800 | 307.3 | 0.5 | 48.1 | 55055.5–55074.5 |
| 7900 | 343.1 | 11.1 | 16.8 | 55074.5–55084.5 |
| 8200 | 3.1 | 5.3 | 9.5 | 55090.5–55104.5 |
| 8300 | 10.1 | −6.5 | 15.9 | 55104.5–55119.5 |
| Spinning | – | – | – | 55197.0–60309.0 |
Notes. The columns show: (1) AGILE observation block (OB) number for pointing-mode observations; (2)–(3) Galactic coordinates (l, b) of the pointing centroids (in degrees); (4) distance of the pointing from IGR J17354−3255; (5) observation time interval in MJD. We selected a total of 1993 days of data, 174 of which in pointing mode and 1819 in spinning mode that maximise the exposure on the source.
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