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Table 1.

PSD best-fit Results.

NGC 4051 NGC 4395
χ2/d.o.f. χ2/d.o.f. PSDamp νb ahigh χ2/d.o.f. χ2/d.o.f. PSDamp νb ahigh
(keV) (PL) (BPL) (×10−2) (×10−3 Hz) (PL) (BPL) (×10−2) (×10−3 Hz)
0.3–0.5 105.2/50 49.2/49 3 . 0 0.4 + 0.5 Mathematical equation: $ 3.0^{+0.5}_{-0.4} $ 0 . 20 0.04 + 0.06 Mathematical equation: $ 0.20^{+0.06}_{-0.04} $ 2.16 ± 0.06 22.4/20 15.9/19 10 . 3 2.3 + 2.9 Mathematical equation: $ 10.3^{+2.9}_{-2.3} $ 2 . 15 0.86 + 1.44 Mathematical equation: $ 2.15^{+1.44}_{-0.86} $ 2 . 22 0.42 + 0.52 Mathematical equation: $ 2.22^{+0.52}_{-0.42} $
0.5–0.8 103.5/50 56.4/49 3 . 5 0.5 + 0.6 Mathematical equation: $ 3.5^{+0.6}_{-0.5} $ 0 . 17 0.04 + 0.05 Mathematical equation: $ 0.17^{+0.05}_{-0.04} $ 2.09 ± 0.06 41.8/20 20.4/19 7 . 1 1.1 + 1.2 Mathematical equation: $ 7.1^{+1.2}_{-1.1} $ 2 . 53 0.57 + 0.74 Mathematical equation: $ 2.53^{+0.74}_{-0.57} $ 2 . 88 0.55 + 0.68 Mathematical equation: $ 2.88^{+0.68}_{-0.55} $
0.8–1.5 93.7/50 62.6/49 3 . 6 0.7 + 0.8 Mathematical equation: $ 3.6^{+0.8}_{-0.7} $ 0 . 13 0.04 + 0.06 Mathematical equation: $ 0.13^{+0.06}_{-0.04} $ 1.98 ± 0.06 42.1/20 27.3/19 4.7 ± 0.6 4 . 34 0.90 + 1.14 Mathematical equation: $ 4.34^{+1.14}_{-0.90} $ 2 . 82 0.60 + 0.77 Mathematical equation: $ 2.82^{+0.77}_{-0.60} $
1.5–5 76.3/50 57.7/49 4 . 2 1.0 + 1.2 Mathematical equation: $ 4.2^{+1.2}_{-1.0} $ 0 . 09 0.04 + 0.06 Mathematical equation: $ 0.09^{+0.06}_{-0.04} $ 1.88 ± 0.06 58.5/23 29.2/22 3.1 ± 0.4 1 . 56 0.34 + 0.43 Mathematical equation: $ 1.56^{+0.43}_{-0.34} $ 2 . 32 0.22 + 0.24 Mathematical equation: $ 2.32^{+0.24}_{-0.22} $
5–10 110.3/73 93.5/72 1.5 ± 0.3 0 . 19 0.08 + 0.12 Mathematical equation: $ 0.19^{+0.12}_{-0.08} $ 1 . 88 0.13 + 0.14 Mathematical equation: $ 1.88^{+0.14}_{-0.13} $ 54.4/44 48.0/43 1.9 ± 0.3 1 . 04 0.36 + 0.54 Mathematical equation: $ 1.04^{+0.54}_{-0.36} $ 2 . 01 0.27 + 0.31 Mathematical equation: $ 2.01^{+0.31}_{-0.27 } $
10–20 26.0/21 < 1 > 0.12 1.8a 17.7/20 < 7.2 > 0.03 2a

Notes. PSD best-fit results for NGC 4051 and NGC 4395 in the various energy bands. Columns (2,3), and (7,8) list the best-fit χ2 for the PL and BPL models to the NGC 4051 and NGC 4395 PSDs, respectively. Columns (4,5,6) and (9, 10, 11) list the best-fit BPL parameters. Errors correspond to 1σ confidence range. a The BPL high-frequency slope is frozen at −1.8 and −2.0 for NGC 4051 and NGC 4395, respectively.

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