Caption: Simulated 50 ks X-IFU observed frame energy spectrum of MG J0414+0534 (a QSO at z=2.64) based on a model consisting of warmabs model based on Xstar (Dadina et al. 2018). The outflow velocity is set to 0.28 c. The ionization state (Log(ξ) ≈ 4) implies that the absorption line is likely due to FeXXVI. A narrow Fe Kα line is also present in the system. Additional comments: The spectral simulation was carried out for the parameters of model #3 from Table 1 of Dadina et al. (2018). The response files used for the simulation are XIFU_CC_BASELINECONF_2018_10_10, and the background TOTALBKG5arcsec.pha (Jul. 25th 2018).

Reference: Data for the plots are courtesy of Mauro Dadina (01/19). Dadina, M.; Vignali, C.; Cappi, M.; Lanzuisi, G.; Ponti, G.; Torresi, E.; De Marco, B.; Chartas, G.; Giustini, M., 2018, Yet another UFO in the X-ray spectrum of a high-z lensed QSO, Astronomy & Astrophysics, Volume 610, id.L13.

Creation date: 07/01/2019. Version #: 3.

Credits: X-IFU Consortium. Copyrights: © DB/X-IFU.