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Table 2.

XMM-Newton observations of six sources analyzed in this work.

Sources Stacking approach Obs. ID Labels
1H 1934-063 Individual (1) 0761870201 2015
Flux-resolved (2) 0891010101, 0891010201 F1, F2

RE J1034+396 Time-averaged (1) 0506440101, 0561580201, 0675440301 High
Flux-resolved (2) 0865010101, 0865011001, 0865011101, F1, F2
0865011201, 0865011301, 0865011401,
0865011501, 0865011601, 0865011701, 0865011801

PG 1244+026 Flux-resolved (4) 0675320101, 0744440101, 0744440201 F1, F2, F3, F4
0744440301, 0744440401, 0744440501

PG 1211+143 Time-resolved (11) 0112610101, 0208020101, 0502050101, 0502050201 T1, T2, T3, T4
0745110101, 0745110201, 0745110301, 0745110401 T5, T6, T7, T8
0745110501, 0745110601, 0745110701 T9, T10, T11

I ZW 1 Individual (1) 0300470101 2005
Flux-resolved (2) 0743050301, 0743050801 F1, F2
Time-averaged (1) 0851990101, 0851990201 2020

IRAS 17020+4544 Flux-resolved (3) 0206860101, 0206860201, 0721220101, 0721220301 F1, F2, F3

Notes. The second column lists the stacking approach according to the observations. The number in the brackets means the number of the generated spectra after stacking. The individual XMM-Newton observations are shown in the third column. For clarity, the corresponding labels of the stacked and individual spectra are listed in the fourth column, where the time-resolved spectra are referred to as T1...T11 chronologically and the flux-resolved spectra are referred to as F1...F4, from the faintest to brightest state. For each source, except for 1H 1934-063, the time-averaged spectrum from all observations is also generated and referred to as the ‘avg’ spectrum, while for 1H 1934-063, the two new observations (Obs. ID: 08910101(2)01) are stacked and named as ‘2021’.

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