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      On the multiwavelength properties of several {\gamma}-ray detected narrow-line Seyfert 1 galaxies

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          Abstract

          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 classical blazars. However, the sample of those {\gamma}-ray detected NLS1s available is still not large enough for a comprehensive and statistical study. We provide a summary of our detections and follow-up studies of three {\gamma}-ray-emitting NLS1s: SDSS J211852.96-073227.5 with flaring {\gamma}-ray radiation (Yang et al. 2018, Paliya et al. 2018) and SDSS J122222.55+041315.7 with the highest redshift by far (z~1) (Yao et al. 2015a), along with the prototype 1H 0323+342 (Zhou et al. 2007, Yao et al. 2015b). And we will discuss their multiwavelength properties and variability properties, including implications from high-energy observations in {\gamma}-rays and X-rays, infrared and radio properties, and correlated variability between several wavebands.

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          SDSS J094857.3+002225: A Very Radio Loud, Narrow‐Line Quasar with Relativistic Jets?

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            Author and article information

            Journal
            26 July 2018
            Article
            1807.10074
            dcf9f566-cf17-4a73-835a-8ba8b5004c6e

            http://arxiv.org/licenses/nonexclusive-distrib/1.0/

            History
            Custom metadata
            PoS(NLS1-2018)016
            6 pages, 2 figures, accepted for publication in Proceedings of Science. Contributed article in the conference on "Revisiting narrow-line Seyfert 1 galaxies and their place in the Universe" held in Padova university, Italy, 9-13 April 2018
            astro-ph.HE astro-ph.GA

            Galaxy astrophysics,High energy astrophysical phenomena
            Galaxy astrophysics, High energy astrophysical phenomena

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