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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.