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A triggered 140 ks XMM-Newton observation of the narrow-line Seyfert 1 (NLS1) Mrk 335 in December 2015 caught the active galaxy at its lowest X-ray flux since 2007. The NLS1 is relatively quiescent for the first ~120 ks of the observation…

Variations in the X-ray emission from the narrow line Seyfert 1 galaxy, Markarian 335 (Mrk 335), are studied on both long and short timescales through observations made between 2006 and 2013 with XMM-Newton, Suzaku and NuSTAR. Changes in…

High Energy Astrophysical Phenomena · Physics 2015-06-23 D. R. Wilkins , L. C. Gallo

The narrow-line Seyfert 1 galaxy Mrk 335 was one of the X-ray brightest AGN, but it has systematically faded since 2007. Here, we report the discovery with Swift of a sequence of bright and rapid X-ray flare events that reveal the emergence…

High Energy Astrophysical Phenomena · Physics 2020-11-18 S. Komossa , D. Grupe , L. C. Gallo , P. Poulos , D. Blue , E. Kara , G. Kriss , A. L. Longinotti , M. L. Parker , D. Wilkins

We report on the deepest X-ray observation of the narrow-line Seyfert 1 galaxy Mrk 335 in the low-flux state obtained with Suzaku. The data are compared to a 2006 high-flux Suzaku observation when the source was ~10-times brighter.…

High Energy Astrophysical Phenomena · Physics 2015-06-23 L. C. Gallo , D. R. Wilkins , K. Bonson , C-Y. Chiang , D. Grupe , M. L. Parker , A. Zoghbi , A. C. Fabian , S. Komossa , A. L. Longinotti

Relativistically blurred reflection from the accretion disc provides a powerful probe of the extreme environments close to supermassive black holes; the inner regions of the accretion flow and the corona that produces the intense X-ray…

High Energy Astrophysical Phenomena · Physics 2015-11-05 D. R. Wilkins

We report on X-ray flares that were observed from the active galactic nucleus I Zwicky 1 (I Zw 1) in 2020 January by the NuSTAR and XMM-Newton observatories. The X-ray spectrum is well-described by a model comprised of the continuum…

High Energy Astrophysical Phenomena · Physics 2022-04-06 D. R. Wilkins , L. C. Gallo , E. Costantini , W. N. Brandt , R. D. Blandford

We examine a 200 ks XMM-Newton observation of the narrow-line Seyfert 1 galaxy Mrk 493. The active galaxy was half as bright as in a previous 2003 snapshot observation and the current lower flux enables a study of the putative reflection…

High Energy Astrophysical Phenomena · Physics 2018-04-18 K. Bonson , L. C. Gallo , D. R. Wilkins , A. C. Fabian

New high variability extragalactic sources may be identified by comparing the flux of sources seen in the XMM-Newton Slew Survey with detections and upper limits from the ROSAT All Sky Survey. In November 2012, X-ray emission was detected…

High Energy Astrophysical Phenomena · Physics 2014-11-19 R. D. Saxton , A. M. Read , S. Komossa , P. Rodriguez-Pascual , G. Miniutti , P. Dobbie , P. Esquej , M. Colless , K. W. Bannister

We report the discovery of the Narrow-Line Seyfert 1 galaxy Mkn 335 in an extremely low X-ray state. A comparison of Swift observations obtained in May and June/July 2007 with all previous X-ray observations between 1971 to 2006 show the…

Astrophysics · Physics 2009-11-13 Dirk Grupe , Stefanie Komossa , Luigi Gallo

The narrow-line Seyfert 1 galaxy (NLS1) Mrk 335 has been continuously monitored with Swift since May 2007 when it fell into a long-lasting, X-ray low-flux interval. Results from the nearly 11 years of monitoring are presented here.…

High Energy Astrophysical Phenomena · Physics 2018-05-16 L. C. Gallo , D. M. Blue , D. Grupe , S. Komossa , D. R. Wilkins

Starting in 2006, Swift has been targeting a region of ~21'X21' around Sagittarius A* (Sgr A*) with the onboard X-ray telescope. The short, quasi-daily observations offer an unique view of the long-term X-ray behavior of the supermassive…

High Energy Astrophysical Phenomena · Physics 2015-06-11 N. Degenaar , J. M. Miller , J. Kennea , N. Gehrels M. T. Reynolds , R. Wijnands

We report on observations of black hole Swift J1357.2-0933, a member of the modest population of very faint X-ray transients. This source has previously shown intense dips in the optical lightcurve, a phenomena that has been linked to the…

We performed a detailed broadband spectral and timing analysis of a small flaring event of ~120 ks in a narrow-line Seyfert 1 galaxy NGC 4051 using simultaneous XMM-Newton and NuSTAR observations. The ~300 ks long NuSTAR observation and the…

High Energy Astrophysical Phenomena · Physics 2023-03-29 Neeraj Kumari , Arghajit Jana , Sachindra Naik , Prantik Nandi

We present results for the first observed outburst from the transient X-ray binary source MAXI J0637-430. This study is based on eight observations from the Nuclear Spectroscopic Telescope Array (NuSTAR) and six observations from the Neil…

We present a spectral analysis of the NuSTAR and XMM-Newton observations of the Seyfert 1h galaxy/ULIRG IRAS 05189-2524 taken in 2013. We find evidence for relativistic disk reflection in the broadband X-ray spectrum: a highly asymmetric…

High Energy Astrophysical Phenomena · Physics 2017-03-08 Yanjun Xu , Mislav Balokovic , Dominic J. Walton , Fiona A. Harrison , Javier A. Garcia , Michael J. Koss

We report the discovery of strong soft X-ray emission lines and a hard continuum above 2 keV in the Narrow-Line Seyfert 1 galaxy Mrk 335 during an extremely low X-ray flux state. Mrk 335 was observed for 22 ks by XMM-Newton in July 2007 as…

As part of a long term monitoring campaign of Mrk 335, deep XMM-Newton observations catch the narrow-line Seyfert 1 galaxy (NLS1) in a complex, intermediate flux interval as the active galaxy is transiting from low- to high-flux. Other…

High Energy Astrophysical Phenomena · Physics 2015-06-11 L. C. Gallo , A. C. Fabian , D. Grupe , K. Bonson , S. Komossa , A. L. Longinotti , G. Miniutti , D. J. Walton , A. Zoghbi , S. Mathur

We report the discovery of an X-ray/UV stellar flare from the source LMC 335, captured by XMM-Newton in the field of the Large Magellanic Cloud. The flare event was recorded continuously in X-ray for its first 10 hours from the precursor to…

Solar and Stellar Astrophysics · Physics 2015-06-05 B. T. H. Tsang , C. S. J. Pun , R. Di Stefano , K. L. Li , A. K. H. Kong

We present XMM-Newton, NuSTAR, Swift and Hubble Space Telescope observations of the Narrow-line Seyfert 1 galaxy Mrk 335 in a protracted low state in 2018 and 2019. The X-ray flux is at the lowest level so far observed, and the extremely…

Detecting and modelling the reprocessed hard X-ray emission component in the accretion flow, so-called reflection spectrum is a main tool to estimate black hole spins in a wide range of astrophysical black holes regardless of their mass or…

High Energy Astrophysical Phenomena · Physics 2020-04-01 Wara Chamani , Karri Koljonen , Tuomas Savolainen
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