We report the first high-energy detection of PG 1700+518, a well-known low-ionization broad absorption line quasar (quasi-stellar object, QSO). Due to previous X-ray non-detection, it was classified as soft X-ray weak QSO. We observed PG 1700+518 with XMM-Newton for about 60 ks divided in three exposures. The spectrum below 2 keV is very steep, Γ˜ 2.4-3.8, while at higher energies the extremely flat emission (photon index Γ˜ 0.15, when modelled with a power law) suggests the presence of strong absorption (NH, pl˜ 2 × 10^23 cm-2, Γ fixed to 1.8) or a reflection-dominated continuum. The broad-band flux is consistent with previous non-detection. Simultaneous European Photon Imaging Camera (EPIC) and Optical Monitor (OM) data confirm its X-ray weakness (observedαox˜-2.2). The level of obscuration derived from the X-ray spectra of PG 1700+518 cannot explain its soft X-ray nuclear weakness unless a column density of NH≳ 2 × 10^24 cm-2 is present.
Ballo L., Piconcelli E., Vignali C., Schartel N. (2011). XMM-Newton first X-ray detection of the low-ionization broad absorption line quasar PG 1700+518. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 415, 2600-2606 [10.1111/j.1365-2966.2011.18883.x].
XMM-Newton first X-ray detection of the low-ionization broad absorption line quasar PG 1700+518
VIGNALI, CRISTIAN;
2011
Abstract
We report the first high-energy detection of PG 1700+518, a well-known low-ionization broad absorption line quasar (quasi-stellar object, QSO). Due to previous X-ray non-detection, it was classified as soft X-ray weak QSO. We observed PG 1700+518 with XMM-Newton for about 60 ks divided in three exposures. The spectrum below 2 keV is very steep, Γ˜ 2.4-3.8, while at higher energies the extremely flat emission (photon index Γ˜ 0.15, when modelled with a power law) suggests the presence of strong absorption (NH, pl˜ 2 × 10^23 cm-2, Γ fixed to 1.8) or a reflection-dominated continuum. The broad-band flux is consistent with previous non-detection. Simultaneous European Photon Imaging Camera (EPIC) and Optical Monitor (OM) data confirm its X-ray weakness (observedαox˜-2.2). The level of obscuration derived from the X-ray spectra of PG 1700+518 cannot explain its soft X-ray nuclear weakness unless a column density of NH≳ 2 × 10^24 cm-2 is present.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
