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Table 6

Inactivity duty cycle.

Name (nickname) Limiting ratea Limiting Fa Limiting La ΔTΣ Pshort IDC RateΔTΣ Distance Ref.
(0.210 keV) (210 keV) (210 keV) (0.210 keV)
(10-3 c s-1) (10-12 erg cm-2 s-1) (1034 erg s-1) (ks) (%) (%) (10-3c s-1) (kpc)

Initial monitoring sample
IGR J164794514 (J16479) 16 2.5 1.1 29.7 3 19 3.1 ± 0.5 4.9 1
XTE J1739302 (J1739) 13 1.6 0.18 71.5 10 39 4.0 ± 0.3 2.7 1
IGR J175442619 (J17544) 12 1.4 0.21 69.3 10 55 2.2 ± 0.2 3.6 1
AX J1841.00536 (J1841) 13 1.8 1.6 26.6 3 28 2.4 ± 0.4 7.8 ± 0.74 2
New monitoring sample
IGR J084084503 (J08408) 17 1.9 0.26 46.6 7 67 7.2 ± 0.6 3.4 ± 0.34 2
IGR J163284726 (J16328) 14 2.7 2.5 47.5 12 61 4.0 ± 0.4 6.5 ± 3.5 3
IGR J164654507 (J16465) 16 2.0 4.4 3.0 0 5 14.6 ± 0.4 12.7 ± 1.3 2
Orbital monitoring sample
IGR J164184532 (J16418) 19 12.5 36 4.8 0 11 >9.2b 13 1
IGR J173543255 (J17354) 14 2.2 3.3 7.8 1 33 >4.6b 8.5 4
IGR J184830311 (J18483) 11 1.8 0.24 11.8 0 27 3.6 ± 0.8 2.83 ± 0.05 5

Notes. Count rates (Col. 2) are in units of 10-3 counts s-1 in the 0.210 keV energy band. Observed fluxes (Col. 3) are in units of 10-12 erg cm-2 s-1 and luminosities (Col. 4) in units of 1034 erg s-1, both in the 210 keV energy band. ΔTΣ (Col. 5) is the sum of the exposures accumulated in all observations, each in excess of 900 s, where only a 3σ upper limit was achieved; Pshort (Col. 6) is the percentage of time lost to short observations; IDC (Col. 7, detailed in Sect. 4.2) is the inactivity duty cycle, the time each source spends undetected down to a flux limit of reported in Col. 3. RateΔTΣ (Col. 8, detailed in Sect. 4.3) is the observed count rate in the data for which no detections were obtained as single observations. Values for the initial monitoring sample were recalculated based on the whole length of the campaigns (Romano et al. 2011).

(a)

Based on a single 900 s exposure.

(b)

3σ upper limit.

Reference. (1) Rahoui et al. (2008); (2) Coleiro et al. (2013); (3) Fiocchi et al. (2013, 3; (4) Tomsick et al. (2009); (5) Torrejón et al. (2010).

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