English
Related papers

Related papers: Gamma-loud quasars: a view with BeppoSAX

200 papers

We report on our XMM observations of the high redshift quasars BR 2237--0607 (z=4.558) and BR 0351--1034 (z=4.351), together with 14 other z>4 objects found in the XMM public archive. Contrary to former reports, we do not find high redshift…

Astrophysics · Physics 2010-11-11 D. Grupe , S. Mathur , B. Wilkes , P. Osmer

We present a comprehensive analysis of Chandra X-ray observations of 15 young radio quasars at redshifts $4.5 < z < 5.0$. All sources are detected in the $0.5-7.0$ keV energy band. Emission spectra are extracted, and the average photon…

We present new BeppoSAX LECS and MECS observations, covering the energy range 0.1 - 10 keV (observer's frame), of four BL Lacertae objects selected from the 1 Jy sample. All sources display a flat (alpha_x ~ 0.7) X-ray spectrum, which we…

Astrophysics · Physics 2009-11-10 P. Padovani , L. Costamante , P. Giommi , G. Ghisellini , A. Celotti , A. Wolter

BeppoSAX observations of the high redshift (z=4.72) blazar GB 1428+4217 confirm the presence of a complex soft X-ray spectrum first seen with the ROSAT PSPC. Flattening below a rest frame energy of 5 keV can be accounted for by absorption…

Astrophysics · Physics 2009-09-17 A. C. Fabian , A. Celotti , K. Iwasawa , G. Ghisellini

In the present work we report the BeppoSAX observation of the Seyfert 1.9 galaxy NGC 526A in the band 0.1-150 keV. The high energy instrument onboard, PDS, has succeeded in measuring for the first time the spectrum of this source in the…

We report the discovery by the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope of high-energy gamma-ray (GeV) emission from the flat-spectrum radio quasar PKS 1454-354 (z=1.424). On 4 September 2008 the source rose to…

High Energy Astrophysical Phenomena · Physics 2012-08-27 LAT Collaboration , A. A. Abdo , P. G. Edwards , M. M. Chester , D. N. Burrows , M. Hauser , S. Wagner

We report on the results of the spectral and timing analysis of a BeppoSAX observation of the microquasar system LS 5039/RX J1826.2-1450. The source was found in a low-flux state with Fx(1-10 keV)= 4.7 x 10^{-12} erg cm^{-2} s^{-1}, which…

Astrophysics · Physics 2009-11-07 P. Reig , M. Ribo , J. M. Paredes , J. Marti

We present new BeppoSAX LECS, MECS, and PDS observations of four flat-spectrum radio quasars (FSRQ) having effective spectral indices alpha_ro and alpha_ox typical of high-energy peaked BL Lacs. Our sources have X-ray-to-radio flux ratios…

Astrophysics · Physics 2009-11-07 P. Padovani , L. Costamante , G. Ghisellini , P. Giommi , E. Perlman

We report the results of XMM-Newton and BeppoSAX observations of the radio and X-ray emitting star LS I +61 303, likely associated with the gamma-ray source 2CG 135+01 and recently detected also at TeV energies. The data include a long…

The flat spectrum radio quasar (FSRQ) PKS 1510-089 (z=0.361) is known for its complex multiwavelength behavior. It has been monitored regularly at very high energy (VHE, $E>100\,$GeV) gamma-rays with H.E.S.S. since its discovery in 2009 in…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Michael Zacharias , Felix Jankowsky , Mahmoud Mohamed , Heike Prokoph , David Sanchez , Stefan Wagner , Alicja Wierzcholska

We present the results of two observations of the bright Seyfert 1 galaxy NGC 3516, obtained with BeppoSAX in 1996 November and 1997 March. Useful signal is detected between 0.2 and 60 keV, allowing for the first time the simultaneous…

Astrophysics · Physics 2015-06-24 G. M. Stirpe , B. J. Wilkes , A. Comastri , S. Mathur , P. T. O'Brien

Aims. The observation of gamma -ray flares from blazar 0836+710 in 2011, following a period of quiescence, offered an opportunity to study correlated activity at different wavelengths for a high-redshift (z=2.218) active galactic nucleus.…

High Energy Astrophysical Phenomena · Physics 2015-06-16 A. Akyuz , D. J. Thompson , D. Donato , J. S. Perkins , L. Fuhrmann , E. Angelakis , J. A. Zensus , S. Larsson , K. Sokolovsky , O. Kurtanidze

In this letter we present analysis of BeppoSAX data from a long look at the Seyfert 1 galaxy NGC 7469. The presence of a soft excess below 0.8 keV is confirmed by our analysis and no warm absorber component is required to fit the spectrum.…

Astrophysics · Physics 2009-11-07 A. De Rosa , A. C. Fabian , L. Piro

We report the discovery of an unambiguous, substantial low-energy cutoff in the broad band X-ray spectrum of the radio quasar RXJ1028.6-0844 at a redshift of 4.276 obtained with the ASCA satellite, which we preferably explained as…

Astrophysics · Physics 2009-10-31 W. Yuan , M. Matsuoka , T. Wang , S. Ueno , H. Kubo , T. Mihara

A brief Chandra observation of the ultraluminous quasar, SDSS J010013.02+280225.8 at redshift 6.326, showed it to be a relatively bright, soft X-ray source with a count rate of about 1 ct/ks. In this paper we present results for the quasar…

Astrophysics of Galaxies · Physics 2017-07-19 Yanli Ai , A. C. Fabian , Xiaohui Fan , S. A. Walker , G. Ghisellini , T. Sbarrato , Liming Dou , Feige Wang , Xue-Bing Wu , Longlong Feng

We study a broad-band X-ray observation by BeppoSAX of the broad-line radio galaxy 3C 120. The primary X-ray continuum is well described by a power law with the photon index of Gamma=1.85+-0.05 and a high-energy break or a cutoff. The…

Astrophysics · Physics 2009-10-31 A. A. Zdziarski , P. Grandi

We present {\it Chandra} X-ray Observatory observations of Giga-Hertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources. The {\it Chandra} sample contains 13 quasars and 3 galaxies with measured 2-10 keV X-ray luminosity…

We present spectra taken with the Low Resolution Imaging Spectrograph on the Keck 10m telescope of spatially-resolved structures ("fuzz") around the high-redshift radio-loud quasars PKS 0445+097 (z=2.108) and PKS 2338+042 (z=2.589). For PKS…

Astrophysics · Physics 2007-05-23 Matthew D. Lehnert , Robert H. Becker

We present the broadband analysis of the powerful quasar 4C04.42 (z=0.965) observed by XMM and INTEGRAL. The 0.2--200 keV spectrum is well reproduced with a hard power-law component ($\Gamma\sim$1.2), augmented by a soft component below 2…

Astrophysics · Physics 2008-05-15 A. De Rosa , L. Bassani , P. Ubertini , A. Malizia , A. J. Dean

We report on a puzzling event occurred during a long BeppoSAX observation of the slow-rotating binary pulsar GX 1+4. During this event, lasting about 1 day, the source X-ray flux was over a factor 10 lower than normal. The low-energy…

‹ Prev 1 3 4 5 6 7 10 Next ›