Table 2.
Flares detected by AGILE/GRID from AGL J1736−3250 in the 100 MeV−10 GeV energy range in the one-day light curve, and simultaneous INTEGRAL observations available.
| AGILE | INTEGRAL | ||||||
|---|---|---|---|---|---|---|---|
| Flare | Observation date |  |
Photon Flux | Luminosity | Orbital | Observation date | Luminosity |
| ID | [MJD] | [10−6 ph s−1 cm−2] | [1037 erg s−1] | phase | [MJD] | [1035 erg s−1] | |
| E01 | 54343.0–54344.0 | 3.5 | 1.75 ± 0.63 | 0.66 ± 0.24 | 0.77 | 54343.1–54344 (12 ks) | < 1.2 |
| E02 | 54732.0–54733.0 | 3.4 | 1.51 ± 0.57 | 0.57 ± 0.21 | 0.82 | – | – |
| E03 | 54746.0–54747.0 | 3.4 | 1.46 ± 0.55 | 0.55 ± 0.21 | 0.48 | – | – |
| E04 | 54915.0–54916.0 | 4.2 | 2.19 ± 0.66 | 0.82 ± 0.25 | 0.48 | – | – |
| E05 | 54935.0–54936.0 | 5.7 | 3.33 ± 0.75 | 1.25 ± 0.28 | 0.85 | – | – |
| E06 | 55100.0–55101.0 | 3.3 | 1.21 ± 0.49 | 0.45 ± 0.18 | 0.38 | – | – |
| E07 | 55109.0–55110.0 | 3.6 | 1.92 ± 0.71 | 0.72 ± 0.27 | 0.45 | – | – |
| E08 | 55112.0–55113.0 | 3.6 | 1.84 ± 0.65 | 0.69 ± 0.24 | 0.80 | – | – |
| E09 | 55599.0–55600.0 | 3.7 | 3.07 ± 1.30 | 1.15 ± 0.49 | 0.45 | 55599.5–55600 (3 ks) | < 2.6 |
| E10 | 56182.0–56183.0 | 3.3 | 2.36 ± 1.07 | 0.88 ± 0.40 | 0.47 | – | – |
| E11 | 56199.0–56200.0 | 3.5 | 3.42 ± 1.36 | 1.28 ± 0.51 | 0.48 | 56199–56200 (9 ks) | < 1.5 |
| E12 | 56351.0–56352.0 | 3.3 | 3.10 ± 1.90 | 1.16 ± 0.71 | 0.48 | 56351.6–56351.8 (3 ks) | < 2.6 |
| E13 | 57786.0–57787.0 | 4.3 | 5.55 ± 1.89 | 2.08 ± 0.71 | 0.35 | – | – |
| E14 | 57823.0–57824.0 | 3.9 | 4.46 ± 1.52 | 1.67 ± 0.57 | 0.73 | 57823–57824 (5 ks) | < 2.2 |
| E15 | 58199.0–58200.0 | 3.6 | 3.32 ± 1.36 | 1.24 ± 0.51 | 0.24 | – | – |
| E16 | 58368.0–58369.0 | 3.3 | 3.02 ± 1.34 | 1.13 ± 0.50 | 0.24 | – | – |
| E17 | 58744.0–58745.0 | 4.0 | 3.74 ± 1.38 | 1.40 ± 0.52 | 0.76 | – | – |
| E18 | 59656.0–59657.0 | 3.3 | 2.95 ± 1.31 | 1.10 ± 0.49 | 0.72 | – | – |
| E19 | 59806.0–59807.0 | 3.4 | 4.21 ± 1.83 | 1.57 ± 0.69 | 0.48 | – | – |
Notes. When IGR J17354−3255 was within the INTEGRAL field of view (∼8 deg), we report the observations in the 18 − 60 keV energy range simultaneous to AGILE. The columns show: (1) AGILE flare ID; (2) AGILE integration time in MJD; (3) the statistical significance expressed in 
of the source detection according to the maximum likelihood ratio test; (4) the average photon flux and its 1σ statistical error, evaluated in the 100 MeV − 10 GeV range assuming a power-law spectrum with index 2.1; (5) the corresponding luminosity assuming a distance of 4.1 kpc; (6) the orbital phase centred in the integration time, considering the zero phase ephemeris at MJD 52698.205 and that the orbital period of the binary system is 8.4474 ± 0.0017 days; (7) INTEGRAL/IBIS observations time coverage (MJD) of the γ-ray flare duration and on-source effective exposure; and (8) INTEGRAL 3σ upper limit (18 − 60 keV) in 1035 erg s−1. The horizontal line separates the ‘pointing mode’ and the ‘spinning mode’ periods.
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