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相关论文: Gamma-loud quasars: a view with BeppoSAX

200 篇论文

We report the discovery of extended X-ray emission around the powerful high-redshift quasar GB 1508+5714 at z=4.3, revealed in a long Chandra ACIS observation. The emission feature is 3-4 arcsec away from the quasar core, which corresponds…

天体物理学 · 物理学 2009-11-10 W. Yuan , A. C. Fabian , A. Celotti , P. G. Jonker

We present the analysis of 31 observations of 20 bright Compton thin Seyfert 2s, in the 0.1-200 keV band, performed with the BeppoSAX satellite. The sample consists of all Seyfert 2s in the BeppoSAX public archive, with a 2-10 keV flux…

天体物理学 · 物理学 2009-11-07 G. Risaliti

We present BeppoSAX observations of the Seyfert 1.8 galaxy NGC1365 in the 0.1--100 keV range. The source was 6 times brighter than during an ASCA observation 3 years earlier. The 4--10 keV flux is highly variable during the BeppoSAX…

天体物理学 · 物理学 2007-05-23 G. Risaliti , R. Maiolino , L. Bassani

The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. From July 6 1999 to August 17 1999, the source was also simultaneously pointed by COMPTEL on-board of the satellite CGRO. Centaurus A has a…

We report on spectral and timing analysis of BeppoSAX data of the 13.6 s period transient X-ray pulsar EXO 0531-6609.2. Observations were carried out in March 1997 and October 1998, catching the source during a high and a low emission…

天体物理学 · 物理学 2009-11-10 Nanda Rea , Gian Luca Israel , Tiziana Di Salvo , Luciano Burderi , Gabriele Cocozza

We present the $\gamma$-ray observations of the flat-spectrum radio quasar PKS 1441+25 (z=0.939), using the {\it Fermi} large Area Telescope data accumulated during January - December 2015. A $\gamma$-ray flare was observed in January 24,…

高能天体物理现象 · 物理学 2017-07-26 N. Sahakyan , S. Gasparyan

We present X-ray spectra obtained with BeppoSAX (Satellite per Astronomia X) of 10 BL Lac objects, selected from the Einstein Medium Sensitivity and Slew Surveys. We find that in about half of the objects a fit in the 0.1-10 keV range with…

We present new BeppoSAX LECS, MECS and PDS observations of five lobe-dominated, broad-line active galactic nuclei selected from the 2-Jy sample of southern radio sources. These include three radio quasars and two broad-line radio galaxies.…

天体物理学 · 物理学 2008-11-26 Paolo Padovani , Raffaella Morganti , Joachim Siebert , Fausto Vagnetti , Andrea Cimatti

Using long-slit optical spectroscopy obtained at the 10.4 m Gran Telescopio Canarias, we have examined the gaseous environment of the radio-loud quasar TXS 1436+157 (z=2.54), previously known to be associated with a large Ly-alpha nebula…

宇宙学与河外天体物理 · 物理学 2015-06-11 Andrew Humphrey , Luc Binette , Montserrat Villar-Martin , Itziar Aretxaga , Polychronis Papaderos

We report on BeppoSAX observations of five transient black hole candidates during their quiescent phase. We confirm these sources are X-ray faint, improving on and complementing existing upper limits. We derive 1-10 keV upper limits for GRO…

天体物理学 · 物理学 2009-11-06 S. Campana , A. N. Parmar , L. Stella

We present a systematic analysis of all the BeppoSAX data of the soft gamma-ray repeater SGR 1900+14: these observations allowed us to study the long term properties of the source quiescent emission. In the observation carried out before…

天体物理学 · 物理学 2009-02-26 P. Esposito , S. Mereghetti , A. Tiengo , L. Sidoli , M. Feroci , P. Woods

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 analyze the BeppoSAX measurements of the prompt and afterglow emission of the gamma-ray burst GRB010222. Among 45 GRBs detected with the Wide Field Cameras on BeppoSAX, the 40-700 keV fluence of (9.3+/-0.3)E-5 erg cm-2 is only surpassed…

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

Outbursts from gamma-ray quasars provide insights on the relativistic jets of active galactic nuclei and constraints on the diffuse radiation fields that fill the Universe. The detection of significant emission above 100 GeV from a distant…

高能天体物理现象 · 物理学 2015-12-23 A. U. Abeysekara , S. Archambault , A. Archer , T. Aune , A. Barnacka , W. Benbow , R. Bird , J. Biteau , J. H. Buckley , V. Bugaev , J. V Cardenzana , M. Cerruti , X. Chen , J. L. Christiansen , L. Ciupik , M. P. Connolly , P. Coppi , W. Cui , H. J. Dickinson , J. Dumm , J. D. Eisch , M. Errando , A. Falcone , Q. Feng , J. P. Finley , H. Fleischhack , A. Flinders , P. Fortin , L. Fortson , A. Furniss , G. H. Gillanders , S. Griffin , J. Grube , G. Gyuk , M. Hütten , N. Håkansson , D. Hanna , J. Holder , T. B. Humensky , C. A. Johnson , P. Kaaret , P. Kar , N. Kelley-Hoskins , Y. Khassen , D. Kieda , M. Krause , F. Krennrich , S. Kumar , M. J. Lang , G. Maier , S. McArthur , A. McCann , K. Meagher , P. Moriarty , R. Mukherjee , D. Nieto , A. O'Faoláin de Bhróithe , R. A. Ong , A. N. Otte , N. Park , J. S. Perkins , A. Petrashyk , M. Pohl , A. Popkow , E. Pueschel , J. Quinn , K. Ragan , G. Ratliff , P. T. Reynolds , G. T. Richards , E. Roache , J. Rousselle , M. Santander , G. H. Sembroski , K. Shahinyan , A. W. Smith , D. Staszak , I. Telezhinsky , N. W. Todd , J. V. Tucci , J. Tyler , V. V. Vassiliev , S. Vincent , S. P. Wakely , O. M. Weiner , A. Weinstein , A. Wilhelm , D. A. Williams , B. Zitzer , P. S. Smith , T. W. -S. Holoien , J. L. Prieto , C. S. Kochanek , K. Z. Stanek , B. Shappee , T. Hovatta , W. Max-Moerbeck , T. J. Pearson , R. A. Reeves , J. L. Richards , A. C. S. Readhead , G. M. Madejski , S. G. Djorgovski , A. J. Drake , M. J. Graham , A. Mahabal

The Seyfert 2 galaxy NGC 2110 has been observed with BeppoSAX between 0.5 and 150 keV. The high energy instrument onboard, PDS, has succeeded in measuring for the first time the spectrum of this source in the 13-150 keV range. The PDS…

A BeppoSAX observation of the BLRG 3C390.3 is reported. For the first time, both the 6.4 keV iron line and a strong reflection hump, produced by the illumination of the primary X-ray emission on cold matter, are detected in this source. The…

天体物理学 · 物理学 2007-05-23 P. Grandi , M. Guainazzi , F. Haardt , L. Maraschi , E. Massaro , G. Matt , L. Piro , C. M. Urry

A systematic analysis of a large sample of radio-loud Active Galactic Nuclei available in the BeppoSAX public archive has been performed. The sample includes 3 Narrow Line Radio Galaxies (NLRG), 10 Broad Line Radio Galaxies (BLRG), 6 Steep…

天体物理学 · 物理学 2009-11-13 Paola Grandi , Giuseppe Malaguti , Mariateresa Fiocchi , --

PKS1510-089 is a flat spectrum radio quasar located at a redshift of 0.36. It is one of only a few such sources detected in very-high-energy (VHE, >100 GeV) gamma rays. Though PKS1510-089 is highly variable at GeV energies, until recently…

From the spectral analysis of a broadband (0.1-200 keV) BeppoSAX observation of the Seyfert 1 galaxy IC 4329A, the main results obtained are: a) the amount of reflection, together with the intensity of the iron K line, indicate a geometry…

天体物理学 · 物理学 2007-05-23 G. C. Perola