XMM-Newton spectroscopy of high redshift quasars
| dc.creator | Brocksopp, C. | |
| dc.creator | Puchnarewicz, E. M. | |
| dc.creator | Mason, K. O. | |
| dc.creator | Cordova, F. A. | |
| dc.creator | Priedhorsky, W. C. | |
| dc.date | 2003-12-16 | |
| dc.date.accessioned | 2026-07-07T10:47:45Z | |
| dc.date.available | 2026-07-07T10:47:45Z | |
| dc.description | We present XMM-Newton X-ray spectra and optical photometry of four high redshift (z=2.96-3.77) quasars, [HB89] 0438-436, [HB89] 2000-330, [SP89] 1107+487 and RX J122135.6+280613; of these four objects the former two are radio-loud, the latter two radio-quiet. Model fits require only a power law with Galactic absorption in each case; additional intrinsic absorption is also needed for [HB89] 0438-436 and RX J122135.6+280613. The spectra are hard (Gamma \~1.7 for [HB89] 0438-436, [HB89] 2000-330 and ~1.4 for RX J122135.6+280613) with the exception of [SP89]~1107+487 which is softer (Gamma ~2.0); the combined Galactic and intrinsic absorption of lower energy X-rays in the latter source is much less significant than in the other three. The two intrinsically unabsorbed sources have greater optical fluxes relative to the X-ray contributions at the observed energies. While there is no need to include reflection or iron line components in the models, our derived upper limits (99% confidence) on these parameters are not stringent; the absence of these features, if confirmed, may be explained in terms of the high power law contribution and/or a potentially lower albedo due to the low disc temperature. However, we note that the power-law spectrum can be produced via mechanisms other than the Comptonization of accretion disc emission by a corona; given that all four of these quasars are radio sources at some level we should also consider the possibility that the X-ray emission originates, at least partially, in a jet. | |
| dc.description | Accepted for publication in MNRAS | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0312418 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0312418 | |
| dc.identifier | Mon.Not.Roy.Astron.Soc.349:687,2004 | |
| dc.identifier | doi:10.1111/j.1365-2966.2004.07540.x | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183645 | |
| dc.subject | Astrophysics | |
| dc.title | XMM-Newton spectroscopy of high redshift quasars | |
| dc.type | text |