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相关论文: ASCA observations of two steep soft X-ray quasars

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We present the final results of a ROSAT PSPC program to study the soft X-ray emission properties of a complete sample of low $z$ quasars. The main results are: 1. There is no evidence for significant soft excess emission or excess…

天体物理学 · 物理学 2009-10-28 Ari Laor , Fabrizio Fiore , Martin Elvis , Belinda J. Wilkes , Jonathan C. McDowell

The XMM-Newton observation of the narrow-line quasar NAB 0205+024 reveals three striking differences since it was last observed in the X-rays with ASCA. Firstly, the 2-10 keV power-law is notably steeper. Secondly, a hard X-ray flare is…

天体物理学 · 物理学 2009-11-10 L. C. Gallo , Th. Boller , W. N. Brandt , A. C. Fabian , S. Vaughan

(abridged) We present and discuss our observations of the NL quasar PG1404+226 with ASCA and HST, and a re-analysis of our earlier observations with ROSAT. The soft X-ray spectrum is very steep and displays an absorption feature (edge or…

天体物理学 · 物理学 2016-08-30 Marie-Helene Ulrich , Andrea Comastri , Stefanie Komossa , Phil Crane

We present an X-ray spectral analysis of 21 low redshift quasars observed with XMM-Newton EPIC. All the sources are Palomar Green quasars with redshifts between 0.05 and 0.4 and have low Galactic absorption along the line-of-sight. A large…

天体物理学 · 物理学 2016-08-30 D. Porquet , J. N. Reeves , P. O'Brien , W. Brinkmann

BeppoSAX and ASCA observations of the nearby (z=0.184), high-luminosity, radio-quiet quasar PDS456 are presented. The X-ray spectrum is characterized by a prominent ionized edge at 8-9 keV (originally discovered by RXTE, Reeves et al. 2000)…

天体物理学 · 物理学 2007-05-23 C. Vignali , A. Comastri , F. Nicastro , G. Matt , F. Fiore , G. G. C. Palumbo

We present results from BeppoSAX observations of 10 low redshift quasars. The quasars are part of the Laor et al. (1997) sample of 23 optically selected PG quasars with redshift <0.4 and low Galactic absorption along the line of sight.…

天体物理学 · 物理学 2007-05-23 T. Mineo , F. Fiore , A. Laor , E. Costantini , W. N. Brandt , A. Comastri , R. Della Ceca , M. Elvis , T. Maccacaro , S. Molendi

This paper reports the X-ray spectral analysis of 5 high-redshift (z \ge 2) radio-quiet quasars observed by ASCA. A simple power law continuum plus cold Galactic absorption model well fits all the spectra (tipically between $\sim$ 2-30 keV…

天体物理学 · 物理学 2009-10-31 C. Vignali , A. Comastri , M. Cappi , G. G. C. Palumbo , M. Matsuoka , H. Kubo

Past X-ray observations by ASCA suggest that warm absorbers (O VII and O VIII edges) are apparently rare in high luminosity AGNs (quasars) while they are more common in low luminosity AGNs (Seyferts). However, this could be a selection…

天体物理学 · 物理学 2009-11-10 Shai Kaspi

We present the results of an analysis of data from XMM-Newton and CHANDRA observations of the high luminosity narrow-line quasar PG 1404+226. We confirm a strong soft X-ray excess in the X-ray spectrum and we find rapid variability (a…

天体物理学 · 物理学 2009-11-10 Surajit Dasgupta , A. R. Rao , G. C. Dewangan , V. K. Agrawal

The narrow-line quasar PHL 1092 was observed by XMM-Newton at two epochs separated by nearly thirty months. Timing analyses confirm the extreme variability observed during previous X-ray missions. A measurement of the radiative efficiency…

天体物理学 · 物理学 2009-09-17 L. C. Gallo , Th. Boller , W. N. Brandt , A. C. Fabian , D. Grupe

This paper presents a comprehensive study of the X-ray properties of low-ionization nuclear emission-line regions (LINERs) and low-luminosity Seyfert galaxies based on observations obtained with ASCA. We analyzed data of 53 observations of…

天体物理学 · 物理学 2009-11-07 Yuichi Terashima , Naoko Iyomoto , Luis C. Ho , Andrew F. Ptak

We present ASCA data on RE J2248-511, extending existing optical and soft X-ray coverage to 10 keV, and monitoring the soft component. These data show that, despite a very strong ultrasoft X-ray excess below 0.3 keV and a soft 0.3--2 keV…

天体物理学 · 物理学 2009-11-06 A. A. Breeveld , E. M. Puchnarewicz , C. Otani

We present a detailed analysis of broad band X-ray data of the Seyfert 2 galaxy NGC5506. 2-10 keV band are detected during a 1-day ASCA observation, while no significant change in the 2-10 keV continuum shape is found. The ASCA spectrum…

天体物理学 · 物理学 2009-10-31 T. G. Wang , T. Mihara , C. Otani , M. Matsuoka , H. Awaki

We present BeppoSAX observations of three gamma-ray emitting quasars, namely 0836+710, 1510-089 and 2230+114. The three objects have been detected up to 100 keV showing extremely flat power-law spectra above 2 keV (energy index…

We report the results from an ASCA observation of the high-luminosity, radio-loud quasar PKS 0637-752 (redshift 0.654), covering the 0.8-15 keV band in the quasar-frame. We find the source to have a luminosity ~10^46 erg/s in the 2-10 keV…

天体物理学 · 物理学 2009-10-30 T. Yaqoob , I. M. George , T. J. Turner , K. Nandra , A. Ptak , P. J. Serlemitsos

We present an XMM-Newton observation of the radio-quiet quasar Q0056-363 (z=0.162). This is the first time that this quasar is observed in the hard X-ray range (above 2 keV). We find that Q0056-363 is a powerful X-ray quasar, with a 0.3-12…

天体物理学 · 物理学 2009-11-10 Delphine Porquet , James N Reeves

We present the result of 27 ASCA observations of 26 radio-quiet quasars (RQQs) from the PG survey. All the RQQs were detected except 2 BALQSOs. We find the variability characteristics of the sources to be consistent with Seyf-1s. A powerlaw…

天体物理学 · 物理学 2009-10-31 I. M. George , T. J. Turner , T. Yaqoob , H. Netzer , A. Laor , R. F. Mushotzky , K. Nandra , T. Takahashi

We present results from a new XMM-Newton observation of the high-redshift quasar RXJ1028.6-0844 at a redshift of 4.276. The soft X-ray spectral flattening, as reported by a study with ASCA previously (Yuan et al. 2000, ApJ 545, 625), is…

天体物理学 · 物理学 2009-09-17 W. Yuan , A. C. Fabian , A. Celotti , R. G. McMahon , M. Matsuoka

We study X-ray and soft gamma-ray spectral properties of BLRGs using data from Ginga, ASCA, OSSE and EXOSAT. The X-ray spectra are well fitted by an intrinsic power-law continuum with an energy index of alpha ~ 0.7, moderately absorbed by a…

The newly discovered z=5.8 quasar SDSSp J104433.04-012502.2 was recently detected in X-rays and found to be extremely X-ray weak. Here we present the hardness ratio analysis of the XMM-Newton observation. We consider various models to…

天体物理学 · 物理学 2009-11-06 Smita Mathur
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