Quasi-simultaneous XMM–Newton and NuSTAR spectra of IGR J17329-2731. The EPIC-pn is in black, the EPIC-MOS2 in red, the FPMA in green, and the FPMB in blue. The best fit to the data is obtained with the model CONST*TBABS*TBPCF*GABS*GABS*GABS* (GAUSSIAN+GAUSSIAN+GAUSSIAN+HIGHECUT*POWERLAW). The residuals from the best fit are shown in the bottom panel. The second panel from the top shows the residuals obtained using a simple absorbed power law with a high energy cutoff (TBABS*HIGHECUT*POWERLAW). The third panel from the top shows the residuals obtained using a simple absorbed power law with a high energy cutoff and the three lines at 2.3 keV, 6.4 eV, and 7.1 keV (TBABS*(GAUSSIAN+GAUSSIAN+GAUSSIAN+HIGHECUT*POWERLAW)). The fourth panel fromthe top shows the residuals obtained by including a GABS component with a centroid energy of ~20 keV, while the fifth panel reports the residuals obtained when a second GABS component with a centroid energy of ~30 keV is accountedfor in the model as well.
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.