Table 6.

Comparison of the goodness of fit of the best-fitting models BPL and BPLGRE to the soft-band PSDs. The number in parentheses corresponds to the values for the iron-line band.

BPLBPLGRE
AGN nameF-testAICc, 1AICc, 2Δ[AICc, 2]W[AICc, 2]ϵ2
ratio, prob. (per cent)
NGC 73140.498, 68.658.32464.8136.4890.0380.039
(0.255, 85.7)(76.591)(82.848)(6.256)(0.042)(0.044)
NGC 40510.822, 48.964.90469.2744.3690.1010.113
(1.185, 32.6)(56.060)(59.733)(3.673)(0.137)(0.159)
Mrk 7662.33, 8.755.45256.1860.7340.4090.693
Ark 5641.64, 19.6561.31763.2051.8880.2800.389
(0.378, 76.9)(82.090)(87.602)(5.512)(0.060)(0.064)
1H 0707−4950.910, 44.475.01178.4383.4270.1530.180
MCG–6-30-150.248, 86.360.68267.2446.5620.0360.038
(1.660, 18.9)(59.634)(61.676)(2.042)(0.265)(0.360)
IRAS 13224−38091.520, 22.349.10052.5883.4870.1490.175
SWIFT J2127.4+56540.510, 67.774.95880.0845.1250.0720.077
Mrk 3350.701, 55.654.70359.9595.2560.0670.072
NGC 35160.209, 88.984.71091.0096.2990.0410.043
PG 1211+1430.645, 59.068.21273.0944.8820.0800.086
PKS 0558−5041.162, 33.528.35834.1945.8350.0510.054
BPLBPLGRE
AGN nameF-testAICc, 1AICc, 2Δ[AICc, 2]W[AICc, 2]ϵ2
ratio, prob. (per cent)
NGC 73140.498, 68.658.32464.8136.4890.0380.039
(0.255, 85.7)(76.591)(82.848)(6.256)(0.042)(0.044)
NGC 40510.822, 48.964.90469.2744.3690.1010.113
(1.185, 32.6)(56.060)(59.733)(3.673)(0.137)(0.159)
Mrk 7662.33, 8.755.45256.1860.7340.4090.693
Ark 5641.64, 19.6561.31763.2051.8880.2800.389
(0.378, 76.9)(82.090)(87.602)(5.512)(0.060)(0.064)
1H 0707−4950.910, 44.475.01178.4383.4270.1530.180
MCG–6-30-150.248, 86.360.68267.2446.5620.0360.038
(1.660, 18.9)(59.634)(61.676)(2.042)(0.265)(0.360)
IRAS 13224−38091.520, 22.349.10052.5883.4870.1490.175
SWIFT J2127.4+56540.510, 67.774.95880.0845.1250.0720.077
Mrk 3350.701, 55.654.70359.9595.2560.0670.072
NGC 35160.209, 88.984.71091.0096.2990.0410.043
PG 1211+1430.645, 59.068.21273.0944.8820.0800.086
PKS 0558−5041.162, 33.528.35834.1945.8350.0510.054
Table 6.

Comparison of the goodness of fit of the best-fitting models BPL and BPLGRE to the soft-band PSDs. The number in parentheses corresponds to the values for the iron-line band.

BPLBPLGRE
AGN nameF-testAICc, 1AICc, 2Δ[AICc, 2]W[AICc, 2]ϵ2
ratio, prob. (per cent)
NGC 73140.498, 68.658.32464.8136.4890.0380.039
(0.255, 85.7)(76.591)(82.848)(6.256)(0.042)(0.044)
NGC 40510.822, 48.964.90469.2744.3690.1010.113
(1.185, 32.6)(56.060)(59.733)(3.673)(0.137)(0.159)
Mrk 7662.33, 8.755.45256.1860.7340.4090.693
Ark 5641.64, 19.6561.31763.2051.8880.2800.389
(0.378, 76.9)(82.090)(87.602)(5.512)(0.060)(0.064)
1H 0707−4950.910, 44.475.01178.4383.4270.1530.180
MCG–6-30-150.248, 86.360.68267.2446.5620.0360.038
(1.660, 18.9)(59.634)(61.676)(2.042)(0.265)(0.360)
IRAS 13224−38091.520, 22.349.10052.5883.4870.1490.175
SWIFT J2127.4+56540.510, 67.774.95880.0845.1250.0720.077
Mrk 3350.701, 55.654.70359.9595.2560.0670.072
NGC 35160.209, 88.984.71091.0096.2990.0410.043
PG 1211+1430.645, 59.068.21273.0944.8820.0800.086
PKS 0558−5041.162, 33.528.35834.1945.8350.0510.054
BPLBPLGRE
AGN nameF-testAICc, 1AICc, 2Δ[AICc, 2]W[AICc, 2]ϵ2
ratio, prob. (per cent)
NGC 73140.498, 68.658.32464.8136.4890.0380.039
(0.255, 85.7)(76.591)(82.848)(6.256)(0.042)(0.044)
NGC 40510.822, 48.964.90469.2744.3690.1010.113
(1.185, 32.6)(56.060)(59.733)(3.673)(0.137)(0.159)
Mrk 7662.33, 8.755.45256.1860.7340.4090.693
Ark 5641.64, 19.6561.31763.2051.8880.2800.389
(0.378, 76.9)(82.090)(87.602)(5.512)(0.060)(0.064)
1H 0707−4950.910, 44.475.01178.4383.4270.1530.180
MCG–6-30-150.248, 86.360.68267.2446.5620.0360.038
(1.660, 18.9)(59.634)(61.676)(2.042)(0.265)(0.360)
IRAS 13224−38091.520, 22.349.10052.5883.4870.1490.175
SWIFT J2127.4+56540.510, 67.774.95880.0845.1250.0720.077
Mrk 3350.701, 55.654.70359.9595.2560.0670.072
NGC 35160.209, 88.984.71091.0096.2990.0410.043
PG 1211+1430.645, 59.068.21273.0944.8820.0800.086
PKS 0558−5041.162, 33.528.35834.1945.8350.0510.054
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close