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Related papers: The multiwavelength variability of 3C 273

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We present a detailed multi-frequency analysis of an intense monitoring programme of Seyfert 1 galaxy NGC 4593 over a duration of nearly for a month with Swift observatory. We used 185 pointings to study the variability in six…

High Energy Astrophysical Phenomena · Physics 2019-08-17 Main Pal , Sachindra Naik

We present UBVRIJHK polarization and flux density observations of the quasar 3C 273 obtained during a time of outburst over two weeks in 1988 February. We have modelled these data with two power law components, each with…

Astrophysics · Physics 2007-05-23 Lara L. Cross , Beverley J. Wills , J. H. Hough , J. A. Bailey

Recent multi-wavelength observations of 3C454.3, in particular during its giant outburst in 2005, put severe constraints on the location of the 'blazar zone', its dissipative nature, and high energy radiation mechanisms. As the optical,…

Astrophysics · Physics 2010-11-11 M. Sikora , R. Moderski , G. M. Madejski

The X-ray spectrum of the Galactic microquasar SS 433 contains a rich set of emission lines of highly ionized atoms of heavy elements whose significant Doppler shift leaves no doubt that they are produced in collimated relativistic jets of…

High Energy Astrophysical Phenomena · Physics 2020-05-27 P. Medvedev , I. Khabibullin , S. Sazonov

We present Spitzer IRAC imaging of the large-scale jet in the quasar PKS 1136-135 at wavelengths of 3.6 and 5.8 um, combined with previous VLA, HST, and Chandra observations. We clearly detect infrared emission from the jet, resulting in…

We investigate the flux intensities spanning from radio waves to X-rays across 39 light curves of Quasar 3C 273, utilizing publicly available data collected by the Integral Science Data Centre (ISDC) database. Our results suggest that…

High Energy Astrophysical Phenomena · Physics 2025-02-07 C. V. da Silva , S. G. A. Barbosa , F. V. Alencar Filho , J. P. Bravo , D. B. de Freitas

Context. Investigation of the hard X-ray emission properties of blazars is key to the understanding of the central engine of the sources and associated jet process. In particular, simultaneous spectral and timing analyses of the intra-day…

High Energy Astrophysical Phenomena · Physics 2018-11-14 Gopal Bhatta , Maksym Mohorian , Illya Bilinsky

Blazars are variable targets in the sky, whose variation mechanism remains an open question. In this work, we make a comprehensive study on the variation phenomena of the spectral index and polarization degree (PD) to deeply understand the…

High Energy Astrophysical Phenomena · Physics 2021-08-11 Yifang Wang , Yunguo Jiang

All the observations available in the Chandra and XMM-Newton archives have been used to investigate the X-ray spectral properties of 3C 33. In this paper is presented a complete X-ray analysis of the nuclear emission of this narrow line…

High Energy Astrophysical Phenomena · Physics 2009-11-13 E. Torresi , P. Grandi , M. Guainazzi , G. G. C. Palumbo , G. Ponti , S. Bianchi

Preliminary results of a systematic study on the simultaneous optical-to-X-rays variability in blazars are presented. Data from Swift observations of four bright gamma-ray blazars (3C 279, ON+231, S5 0716+71, PKS 2155-304) have been…

Astrophysics · Physics 2009-11-13 L. Foschini

INTEGRAL has observed the bright quasar 3C 273 on 3 epochs in January 2003 as one of the first observations of the open programme. The observation on January 5 was simultaneous with RXTE and XMM-Newton observations. We present here a first…

The correlation often observed in blazars between optical-to-radio outbursts and gamma-ray flares suggests that the high-energy emission region shall be co-spatial with the radio knots, several parsecs away from the central engine. This…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Marc Türler , Claes-Ingvar Björnsson

We show results from a 7 year VLBI monitoring programme of 3C273 at millimeter wavelengths. We find evidence for component acceleration, motion or rotation of fluid dynamical patterns in the VLBI jet, and evidence for an outburst-ejection…

The gamma-ray blazar 3C 279 was monitored on a nearly daily basis with IUE, ROSAT and EGRET for three weeks between December 1992 and January 1993. During this period, the blazar was at a historical minimum at all wavelengths. Here we…

We present a series of X-ray variability results from a long XMM-Newton + NuSTAR campaign on the bright, variable AGN NGC 3227. We present an analysis of the lightcurves, showing that the source displays typically softer-when-brighter…

High Energy Astrophysical Phenomena · Physics 2020-04-30 A. P. Lobban , T. J. Turner , J. N. Reeves , V. Braito , L. Miller

Here we report our recent results of variability studies in optical and X-ray bands of three blazars namely 3C 273, PKS 2155 - 304 and BL Lacertae with XMM-Newton. We found large amplitude optical to X-rays variability in 3C 273, and PKS…

High Energy Astrophysical Phenomena · Physics 2017-12-20 A. C. Gupta

We report on the {\it Chandra} discovery of large scale non--thermal emission features in the double lobed SSRL quasar 3C 207 (z=0.684). These are: a diffuse emission well correlated with the western radio lobe, a bright one sided jet whose…

Astrophysics · Physics 2009-11-07 G. Brunetti , M. Bondi , A. Comastri , G. Setti

We investigate the relationship between the variable gamma-ray emission and jet properties in the blazar 3C 279, by combining the Fermi/LAT data spanning a period of eight years with concurrent radio measurements made at multiple epochs…

High Energy Astrophysical Phenomena · Physics 2019-09-25 Víctor M. Patiño-Álvarez , Sergio A. Dzib , Andrei Lobanov , Vahram Chavushyan

The VERITAS Collaboration recently reported the detection of very-high-energy (VHE) gamma-ray emission from the prototypical radio quasar 3C273. The temporal and the spectral properties of this component do not appear compatible with the…

High Energy Astrophysical Phenomena · Physics 2025-11-07 F. Tavecchio

Unexpectedly strong X-ray emission from extragalactic radio jets on kiloparsec scales has been one of the major discoveries of Chandra, the only X-ray observatory capable of sub-arcsecond-scale imaging. The origin of this X-ray emission,…

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