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Table 3

X-ray properties of π Aqr derived from Swift observations.

ObsID HJD Exp. time Ct rate in T HR = HS NH Norm (d.o.f.)

–2 458 000. (s) (cts s−1) (1022 cm−2) (10−3 cm−5) (10−11 erg cm−2 s−1)
00010659001 223.678 1281 0.224 ± 0.017 0.91 ± 0.14 0.39 ± 0.12 8.04 ± 0.73 1.27 ± 0.11 1.48 ± 0.14 1.30 (28)
00010659002 232.494 1426 0.288 ± 0.030 0.76 ± 0.16 0.11 ± 0.10 6.13 ± 0.65 1.05 ± 0.08 1.13 ± 0.12 1.40 (30)
00010659003 236.481 980 0.240 ± 0.021 0.57 ± 0.10 0.18 ± 0.11 7.10 ± 0.78 1.19 ± 0.11 1.31 ± 0.15 0.60 (18)
00010659005 255.425 968 0.301 ± 0.021 0.68 ± 0.10 0.20 ± 0.09 9.72 ± 0.85 1.62 ± 0.12 1.79 ± 0.14 0.76 (27)
00010659006 261.000 1003 0.211 ± 0.019 0.89 ± 0.16 0.51 ± 0.13 8.18 ± 0.82 1.26 ± 0.10 1.50 ± 0.09 1.23 (17)
00010659007 267.237 1018 0.297 ± 0.019 0.94 ± 0.12 0.45 ± 0.11 10.87 ± 0.97 1.69 ± 0.11 2.00 ± 0.18 0.73 (26)
00010659008 272.692 1008 0.90 ± 0.27 6.97 ± 0.94 1.01 ± 0.11 1.28 ± 0.17 0.69 (15)
00010659009 278.858 888 0.208 ± 0.017 4.19 ± 1.01 3.15 ± 0.64 14.95 ± 2.00 1.76 ± 0.20 2.75 ± 0.37 1.06 (16)
00010659010 285.368 1013 0.308 ± 0.020 1.53 ± 0.21 1.76 ± 0.33 15.07 ± 1.58 1.97 ± 0.16 2.77 ± 0.27 1.22 (27)
00010659011 291.413 389 0.204 ± 0.027 0.95 ± 0.25 0.76 ± 0.38 7.24 ± 1.45 1.07 ± 0.18 1.33 ± 0.28 1.53 (5)
00010659013 309.148 824 0.339 ± 0.025 0.66 ± 0.09 0.15 ± 0.09 9.69 ± 0.98 1.64 ± 0.14 1.78 ± 0.18 1.15 (21)
00010659014 317.543 920 0.236 ± 0.018 1.22 ± 0.19 0.70 ± 0.19 10.02 ± 1.09 1.49 ± 0.14 1.84 ± 0.21 0.63 (20)
00010659016 324.685 1131 1.91 ± 0.49 7.92 ± 1.26 1.02 ± 0.15 1.46 ± 0.24 1.53 (10)
00010659017 326.626 923 0.275 ± 0.030 2.07 ± 0.44 1.69 ± 0.44 13.72 ± 2.10 1.81 ± 0.21 2.53 ± 0.40 1.22 (16)
00010659018 332.970 894 0.218 ± 0.031 0.90 ± 0.21 0.43 ± 0.20 10.65 ± 1.48 1.67 ± 0.20 1.96 ± 0.21 0.87 (13)
00010659019 338.971 820 0.230 ± 0.032 1.13 ± 0.32 0.83 ± 0.26 9.99 ± 1.48 1.45 ± 0.19 1.84 ± 0.28 0.52 (9)
00010659020 351.253 1008 0.285 ± 0.020 1.21 ± 0.18 0.63 ± 0.15 11.13 ± 1.04 1.68 ± 0.13 2.05 ± 0.19 0.74 (27)
00010659022 362.741 923 0.269 ± 0.020 0.95 ± 0.14 0.58 ± 0.14 9.61 ± 0.92 1.46 ± 0.12 1.77 ± 0.17 0.87 (21)
00010659024 386.429 879 0.333 ± 0.023 1.87 ± 0.29 1.01 ± 0.21 14.91 ± 1.51 2.12 ± 0.16 2.74 ± 0.28 0.97 (23)
00010659026 390.210 960 0.195 ± 0.019 1.43 ± 0.30 0.67 ± 0.17 9.60 ± 0.98 1.43 ± 0.12 1.77 ± 0.18 0.33 (19)
00010659027 392.907 1013 0.328 ± 0.022 1.35 ± 0.18 0.68 ± 0.14 13.58 ± 1.18 2.03 ± 0.14 2.50 ± 0.37 0.73 (30)
00010659028 399.079 922 0.325 ± 0.027 1.14 ± 0.19 0.41 ± 0.11 12.49 ± 1.10 1.96 ± 0.13 2.30 ± 0.20 0.86 (29)
00010659029 405.390 1038 0.191 ± 0.018 1.24 ± 0.25 0.80 ± 0.19 9.24 ± 0.97 1.35 ± 0.12 1.70 ± 0.18 0.68 (17)
00010659031 416.608 1013 0.280 ± 0.022 1.27 ± 0.21 0.39 ± 0.12 10.36 ± 0.97 1.64 ± 0.14 1.90 ± 0.18 1.22 (25)
00010659032 422.717 995 0.334 ± 0.023 0.90 ± 0.12 0.19 ± 0.07 10.85 ± 0.85 1.81 ± 0.13 1.99 ± 0.16 0.66 (29)
00010659033 429.427 978 0.229 ± 0.020 1.16 ± 0.20 0.46 ± 0.24 8.33 ± 1.19 1.30 ± 0.12 1.54 ± 0.21 1.19 (22)
00010659034 435.073 1098 0.152 ± 0.014 2.65 ± 0.60 1.72 ± 0.39 9.00 ± 1.21 1.18 ± 0.12 1.66 ± 0.22 0.58 (15)
00010659035 441.179 978 0.203 ± 0.019 1.05 ± 0.20 0.31 ± 0.12 7.23 ± 0.78 1.16 ± 0.11 1.33 ± 0.14 0.99 (17)
00010659036 446.889 812 0.246 ± 0.022 0.87 ± 0.15 0.52 ± 0.15 10.38 ± 1.11 1.60 ± 0.15 1.91 ± 0.15 0.69 (18)
00010659039 465.012 983 0.63 ± 0.35 4.76 ± 0.94 0.72 ± 0.13 0.88 ± 0.14 1.73 (7)

Notes. For count rates, total (T), soft (S), and hard (H) bands are defined as 0.5–10, 0.5–2, and 2–10 keV, respectively. For spectral fits, a model tbabs × phabs × apec was used, with the first absorption fixed to the interstellar value of 3.6 × 1020 cm−2 and the temperature fixed to 14.8 keV (see text for details). Errors (found using the “error” command for the spectral parameters and the absorption-corrected fluxes, or the “flux err” command for the observed fluxes) correspond to 1σ; when the errors were asymmetric, the highest value is provided here. Fluxes were determined in the 0.5–10.0 keV band; absorption-corrected fluxes, found using “cflux” in front of the thermal component, are corrected for the full (i.e., interstellar + local) absorbing column.

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