Table 1.
Log of the XMM-Newton observation of NGC 3783 used in this work.
Obs ID | Start date | Flux | Exposure | |
---|---|---|---|---|
DD/MM/YYYY | ks | |||
U1 | 0112210101 | 28/12/2000 | 3.91 | 26 |
U2 | 0112210201 | 17/12/2001 | 3.13 | 87 |
U3 | 0112210501 | 19/12/2001 | 4.06 | 87 |
O1 | 0780860901 | 11/12/2016 | 2.11 | 76 |
O2 | 0780861001 | 21/12/2016 | 2.54 | 38 |
Notes. The columns report: (1) the nomenclature used throughout the paper to refer to each observation; 3) the observation ID; 3) the observation date; 4) the 4.5–10 keV flux (in units of 10−11 erg s−1 cm−2) taken from 4XMM-DR10 catalogue (Webb et al. 2020); 5) the effective exposure (after removal of flares). We note that observation U2 is split in two parts (U2a and U2b, of 40 ks and 47 ks respectively), separated by ∼4 ks.
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