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Related papers: The Variable Optical Polarization of J0948+0022

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We report on VERITAS observations at energies above 200 GeV of known or potential galactic gamma-ray sources. The observed objects comprise pulsars, pulsar wind nebulae, high-mass X-ray binaries and gamma-ray sources with unknown…

Astrophysics · Physics 2019-08-13 G. Maier

We report the discovery with Fermi/LAT of gamma-ray emission from three radio-loud narrow-line Seyfert 1 galaxies: PKS 1502+036 (z=0.409), 1H 0323+342 (z=0.061) and PKS 2004-447 (z=0.24). In addition to PMN J0948+0022 (z=0.585), the first…

High Energy Astrophysical Phenomena · Physics 2011-02-11 LAT Collaboration , G. Ghisellini , L. Maraschi , F. Tavecchio

We analyse eight XMM-Newton observations of the bright Narrow-Line Seyfert 1 galaxy Arakelian 564 (Ark 564). These observations, separated by ~6 days, allow us to look for correlations between the simultaneous UV emission (from the Optical…

High Energy Astrophysical Phenomena · Physics 2016-07-13 Savithri H. Ezhikode , Gulab C. Dewangan , Ranjeev Misra , Shruti Tripathi , Ninan Sajeeth Philip , Ajit K. Kembhavi

By means of the data sets from the Pan-STARRAS1 survey, we have systematically examined the relationship between the variability characteristics and the physical parameters of the largest NLS1 galaxy sample up to now. The results are…

Astrophysics of Galaxies · Physics 2022-01-21 Hongtao Wang , Yanping Su , Xue Ge , Yongyun Chen , Xiaoling Yu

Gamma-ray binaries are stellar systems containing a neutron star or black hole with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our…

High Energy Astrophysical Phenomena · Physics 2012-02-16 The Fermi LAT Collaboration , M. J. Coe , F. Di Mille , P. G. Edwards , M. D. Filipović , J. L. Payne , J. Stevens , M. A. P. Torres

We report on the identification of a new $\gamma$-ray-emitting narrow-line Seyfert 1 (NLS1) galaxy, SDSS J122222.55+041315.7, which increases the number of known objects of this remarkable but rare type of active galactic nuclei (AGN) to…

High Energy Astrophysical Phenomena · Physics 2015-09-23 Su Yao , Weimin Yuan , Hongyan Zhou , S. Komossa , Jin Zhang , Erlin Qiao , Bifang Liu

We present an overview of new HST imaging polarimetry of six nearby radio galaxies with optical jets. These observations triple the number of extragalactic jets with subarcsecond-resolution optical polarimetry. We discuss the polarization…

Some progress in understanding AGN variability is reviewed. Reprocessing of X-ray radiation to produce significant amounts of longer-wavelength continua seems to be ruled out. In some objects where there has been correlated X-ray and…

Cosmology and Nongalactic Astrophysics · Physics 2009-07-27 C. Martin Gaskell , Elizabeth S. Klimek

We present results from several XMM-Newton observations of the radio loud Narrow-line Seyfert 1 galaxy (NLS1) PKS 0558-504. We find evidence for strong and persistent X-ray variability, both on short and long time-scales. On short time…

Astrophysics · Physics 2009-11-10 W. Brinkmann , P. Arevalo , M. Gliozzi , E. Ferrero

In a recent paper, Rol and colleagues present evidence for a variable polarization in the optical afterglow following the gamma-ray burst GRB 990712. The variation is highly significant, but the position angle appears time independent.…

Astrophysics · Physics 2009-10-31 G. Bjornsson , E. J. Lindfors

The {\gamma}-ray detection from several radio-loud (RL) narrow-line Seyfert 1 (NLS1) galaxies has enabled us to study powerful relativistic jets in active galactic nuclei (AGNs) with smaller black hole masses and higher accretion rates than…

High Energy Astrophysical Phenomena · Physics 2018-07-27 Hui Yang , Weimin Yuan , Su Yao , Hai-Wu Pan , S. Komossa

Study of the polarization behaviour in blazars is a powerful tool to discern the role of magnetic field in the variable emission process in their relativistic jets. We present here results of our systematic investigation on the correlation…

High Energy Astrophysical Phenomena · Physics 2022-01-12 Ashwani Pandey , Bhoomika Rajput , C. S. Stalin

The origin of the low luminosity radio emission in radio-quiet AGN, is unknown. The detection of a positive correlation between the radio and X-ray emission would imply a jet-like origin, similar to that seen in `hard state' X-ray binary…

High Energy Astrophysical Phenomena · Physics 2016-12-21 Sadie Jones , Ian McHardy , Thomas J. Maccarone

We present the results of our broadband study of the $\gamma$-ray emitting narrow line Seyfert 1 (NLSy1) galaxy SBS 0846+513 ($z=0.585$). This includes multi-band flux variations, $\gamma$-ray spectral analysis, broad band spectral energy…

High Energy Astrophysical Phenomena · Physics 2016-03-23 Vaidehi S. Paliya , Bhoomika Rajput , C. S. Stalin , S. B. Pandey

Significant gravitational wave emission is expected from gamma-ray bursts arising from compact stellar mergers, and possibly also from bursts associated with fast-rotating massive stellar core collapses. These models have in common a high…

Astrophysics · Physics 2009-11-07 Shiho Kobayashi , Peter Meszaros

Narrow-line Seyfert 1 galaxies (NLS1s) are active galactic nuclei (AGN) recently identified as a new class of $\gamma$-ray sources. The high energy emission is explained by the presence of a relativistic jet observed at small angles, just…

We performed a comprehensive analysis of flux and color variability in a redshift-matched sample of Seyfert galaxies, comprising 23 gamma-ray-detected narrow-line Seyfert 1 galaxies (gNLS1s), 190 non-gamma-ray-detected narrow-line Seyfert 1…

High Energy Astrophysical Phenomena · Physics 2025-09-17 Vineet Ojha , Xue-Bing Wu , Luis C. Ho

We present the preliminary results of a survey performed with Swift to observe a sample of radio-loud Narrow-Line Seyfert 1 Galaxies (RLNLS1s). Optical-to-X-ray data from Swift are complemented with gamma-ray observations from Fermi/LAT and…

We present the temporal analysis of X-ray observations of the radio-loud Narrow-Line Seyfert 1 galaxy (NLS1) PKS 0558-504 obtained during the XMM-Newton Calibration and Performance Verification (Cal/PV) phase. The long term light curve is…

Astrophysics · Physics 2009-10-31 M. Gliozzi , W. Brinkmann , P. T. O'Brien , J. N. Reeves , K. A. Pounds , M. Trifoglio , F. Gianotti

We compare the variability properties of very high energy gamma-ray emitting BL Lac objects in the optical and radio bands. We use the variability information to distinguish multiple emission components in the jet, to be used as a guidance…

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