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Related papers: Intrinsic Absorption in NGC 7469

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We conducted a multi-wavelength six-month campaign to observe the Seyfert galaxy NGC~7469, using the space-based observatories \textit{HST}, \textit{Swift}, \textit{XMM-Newton} and \textit{NuSTAR}. Here we report the results of the spectral…

Between July 2012 and February 2013, NuSTAR and XMM-Newton performed four long-look joint obser- vations of the type 1.8 Seyfert, NGC 1365. We have analyzed the variable absorption seen in these observations in order to characterize the…

During an extensive multiwavelength campaign that we performed in 2013-14 the prototypical Seyfert 1 galaxy NGC 5548 has been found in an unusual condition of heavy and persistent obscuration. The newly discovered "obscurer" absorbs most of…

Active Galactic Nuclei often show evidence of photoionized outflows. A major uncertainty in models for these outflows is the distance ($R$) to the gas from the central black hole. In this paper we use the HST/COS data from a massive…

We have observed the much studied Seyfert 1 galaxy NGC5548 with the GHRS spectrometer on HST. Our 14ksec observation covers the CIV emission line at a resolution of >20,000. Our purpose was to study the absorption line found at lower…

Astrophysics · Physics 2009-10-31 Smita Mathur , Martin Elvis , Belinda Wilkes

We observed the Seyfert 1 galaxy NGC 4151 on eleven occasions at 1-2 day intervals using the Berkeley spectrometer during the ORFEUS-SPAS II mission in 1996 November. The mean spectrum covers 912-1220 A at ~0.3 A resolution with a total…

Astrophysics · Physics 2009-10-30 B. R. Espey , G. A. Kriss , J. H. Krolik , W. Zheng , Z. Tsvetanov , A. F. Davidsen

In 2013 we conducted a large multi-wavelength campaign on the archetypical Seyfert 1 galaxy NGC 5548. Unexpectedly, this usually unobscured source appeared strongly absorbed in the soft X-rays during the entire campaign, and signatures of…

We present three Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the Narrow-Line Seyfert 1 galaxy NGC4051. The most prominent features in the far-ultraviolet (FUV) spectrum are the OVI emission and absorption lines and the HI…

Astrophysics · Physics 2009-11-10 Shai Kaspi , W. N. Brandt , M. J. Collinge , Martin Elvis , Christopher S. Reynolds

We present Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the molecular, neutral atomic, weakly ionized, and highly ionized components of the interstellar and intergalactic material toward the quasar 3C 273. We identify…

Astrophysics · Physics 2009-11-07 K. R. Sembach , J. C. Howk , B. D. Savage , J. M. Shull , W. R. Oegerle

In this paper we analyze the X-ray, UV and optical data of the Seyfert 1.5 galaxy 1H0419-577, with the aim of detecting and studying an ionized-gas outflow. The source was observed simultaneously in the X-rays with XMM and in the UV with…

High Energy Astrophysical Phenomena · Physics 2015-06-16 L. Di Gesu , E. Costantini , N. Arav , B. Borguet , R. G. Detmers , J. Ebrero , D. Edmonds , J. S. Kaastra , E. Piconcelli , F. Verbunt

We present HST/STIS and FUSE spectra of the QSO PG 1211+143 (z_em = 0.081) and a galaxy survey of the surrounding field. This sightline shows two strong intergalactic absorption systems at cz ~ 15,300 and 19,300. This sightline addresses…

Astrophysics · Physics 2009-11-10 Jason Tumlinson , J. Michael Shull , Mark L. Giroux , John T. Stocke

We present the analysis of five O VI absorbers identified across a redshift path of z $\sim (0.6 - 1.3)$ towards the background quasar PG $1522+101$ with information on five consecutive ionization stages of oxygen from O II to O VI. The…

We present the far-ultraviolet spectrum of the Seyfert 1 galaxy 2MASX J21362313-6224008 obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). The spectrum features absorption from Galactic OVI at two velocities and redshifted HI…

Astrophysics · Physics 2009-11-10 Massimiliano Bonamente , W. Van Dyke Dixon

The emission and absorption attributes of the UV-blue nuclear spectra of the Narrow-Line Seyfert 1 (NLS1) galaxies are analyzed based on high quality archival HST observations. Measurements from composite spectra as well as from individual…

Astrophysics · Physics 2007-05-23 Anca Constantin , Joseph C. Shields

We present an investigation into the impact of feedback from outflowing UV and X-ray absorbers in nearby z < 0.04 AGN. From studies of the kinematics, physical conditions, and variability of the absorbers in the literature, we calculate the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 D. M. Crenshaw , S. B. Kraemer

Winds outflowing from Active Galactic Nuclei (AGNs) may carry significant amount of mass and energy out to their host galaxies. In this paper we report the detection of a sub-relativistic outflow observed in the Narrow Line Seyfert 1 Galaxy…

We report the serendipitous discovery of an absorption feature at 4.8 keV in the NuSTAR spectra of ESP 39607, a Seyfert 2 galaxy at $z = 0.201$, observed in May 2023 and August 2024. The feature is detected in both observations with…

High Energy Astrophysical Phenomena · Physics 2025-07-01 Alessandro Peca , Michael J. Koss , Roberto Serafinelli , Claudio Ricci , C. Megan Urry , Giulia Cerini , Peter G. Boorman

High-quality Far-Ultraviolet Spectroscopic Explorer (FUSE) observations at 20 km /s resolution of interstellar and intergalactic absorption from 910 to 1187 A are presented for the X-ray bright BL Lac object Mrk 421. In this study we…

Astrophysics · Physics 2009-11-10 B. D. Savage , B. P. Wakker , A. J. Fox , K. R. Sembach

The existence of ionized X-ray absorbing layers of gas along the line of sight to the nuclei of Seyfert galaxies is a well established observational fact. This material is systematically outflowing and shows a large range in parameters.…

High Energy Astrophysical Phenomena · Physics 2015-06-12 F. Tombesi , M. Cappi , J. N. Reeves , R. S. Nemmen , V. Braito , M. Gaspari , C. S. Reynolds

We present a multi-wavelength spectral study of NGC 4151 based on five epochs of simultaneous AstroSat observations in the near ultra-violet (NUV) to hard X-ray band ($\sim 0.005-80$ keV) during $2017 - 2018$. We derived the intrinsic…

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