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相关论文: A NICER Look at Strong X-ray Obscuration in the Se…

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We present analysis of NuSTAR X-ray observations in the 3-79 keV energy band of the Seyfert 2 galaxy NGC 4388, taken in 2013. The broadband sensitivity of NuSTAR, covering the Fe K$\alpha$ line and Compton reflection hump, enables tight…

高能天体物理现象 · 物理学 2017-07-19 N. Kamraj , E. Rivers , F. A. Harrison , M. Brightman , M. Balokovic

We present first INTEGRAL and XMM-Newton observations of a Seyfert galaxy, the type 2 AGN NGC 4388. Several INTEGRAL observations performed in 2003 allow us to study the spectrum in the 20 - 300 keV range. In addition two XMM-Newton…

天体物理学 · 物理学 2009-11-10 V. Beckmann , N. Gehrels , P. Favre , R. Walter , T. J. -L. Courvoisier , P. -O. Petrucci , J. Malzac

We report on a study of the narrow Fe K$\alpha$ line and reflection spectrum in the well-known Seyfert-2 AGN, NGC 4388. X-ray spectra summed from two extensive NICER monitoring campaigns, separated by years, show strong evidence of…

高能天体物理现象 · 物理学 2024-03-05 B. Gediman , J. M. Miller , A. Zoghbi , P. Draghis , Z. Arzoumanian , W. N . Brandt , K. Gendreau

We report results from the simultaneous XRISM (183 ks) and NuSTAR (62 ks) observations of the Seyfert-2 galaxy NGC 4388. This AGN has the brightest Fe K$\alpha$ line among Compton-thin, obscured sources. To model the reflection continuum…

We present results on the Seyfert 2 galaxy NGC4388 in the Virgo cluster observed with ASCA during its PV phase. The 0.5-10 keV X-ray spectrum consists of multiple components; (1) a continuum component heavily absorbed by a column density NH…

天体物理学 · 物理学 2015-06-24 K. Iwasawa , A. C. Fabian , S. Ueno , H. Awaki , Y. Fukazawa , K. Matsushita , K. Makishima

We present a new analysis of the Suzaku X-ray spectrum of the Compton-thin Seyfert 2 galaxy NGC 4388. The spectrum above $\sim$2 keV can be described by a remarkably simple and rather mundane model, consisting of a uniform, neutral…

高能天体物理现象 · 物理学 2023-03-30 Tahir Yaqoob , P. Tzanavaris , S. LaMassa

We present Chandra imaging and spectral observations of Seyfert 2 galaxy NGC 4388. Three extended X-ray structures around the nucleus on kpc scale are well imaged, allowing an in-depth spatially resolved study. Both the extended hard…

星系天体物理 · 物理学 2021-03-03 Huili Yi , Junfeng Wang , Xinwen Shu , Giuseppina Fabbiano , Cirino Pappalardo , Chen Wang , Hanbo Yu

We present Gemini/GNIRS spectroscopy of the Seyfert 2 galaxy NGC 4388, with simultaneous coverage from 0.85 - 2.5 $\mu$m. Several spatially-extended emission lines are detected for the first time, both in the obscured and unobscured portion…

We present two Rossi Xray Timing Explorer (RXTE) PCA observations of the type~2 Seyfert galaxy NGC 4388 caught in an unusual low X-ray absorption state. The observations were triggered by a detection in the 1.5-3 keV band of the RXTE…

天体物理学 · 物理学 2009-11-10 Martin Elvis , G. Risaliti , F. Nicastro , J. M. Miller , F . Fiore , S. Puccetti

We present X-ray spectral analyses for three Seyfert 2 active galactic nuclei, NGC 424, NGC 1320, and IC 2560, observed by NuSTAR in the 3-79 keV band. The high quality hard X-ray spectra allow detailed modeling of the Compton reflection…

We present results from a joint Xmm-Newton/NuSTAR monitoring of the Seyfert 1 NGC 4593, consisting of 5x20 ks simultaneous observations spaced by two days, performed in January 2015. The source is variable, both in flux and spectral shape,…

高能天体物理现象 · 物理学 2016-08-17 F. Ursini , P. -O. Petrucci , G. Matt , S. Bianchi , M. Cappi , B. De Marco , A. De Rosa , J. Malzac , A. Marinucci , G. Ponti , A. Tortosa

The X-ray spectra of two intermediate type Seyfert galaxies are investigated using ASCA observations separated by more than a year. Both NGC 4388 and ESO 103-G35 exhibit strong, narrow Fe K alpha line emission and absorption by cold neutral…

天体物理学 · 物理学 2009-10-31 Karl Forster , Karen M. Leighly , Laura E. Kay

Suzaku observed a nearby Seyfert 2 galaxy NGC4945, which hosts one of the brightest active galactic nuclei above 20 keV. Combining data from the X-ray CCD camera (XIS) and the Hard X-ray Detector (HXD), the AGN intrinsic nuclear emission…

We present a flux-resolved X-ray analysis of the dwarf Seyfert 1.8 galaxy NGC 4395, based on three archival $XMM-Newton$ and one archival $NuSTAR$ observations. The source is known to harbor a low mass black hole ($\sim 10^4- {\rm a~…

We present a new X-ray analysis of the dwarf Seyfert galaxy NGC 4395, based on two archival XMM-Newton and Suzaku observations. This source is well known for a series of remarkable properties: one of the smallest estimated black hole masses…

宇宙学与河外天体物理 · 物理学 2015-05-28 Emanuele Nardini , Guido Risaliti

We present recent results from spectroscopic data and modeling of the biconical ionized gas in the Seyfert-2 galaxy NGC 4388. A field of ~2.6 x 2.4 kpc centered on the nucleus has been observed by means of the modern technique of integral…

天体物理学 · 物理学 2009-11-07 S. Ciroi , M. Contini , P. Rafanelli , G. M. Richter

We present a Suzaku observation of the dwarf Seyfert galaxy NGC4395 with an estimated black hole mass of ~10^5 Msun. Rapid and strong X-ray variability with an rms amplitude of ~60 per cent is observed in the 0.4-10 keV band with the XIS…

宇宙学与河外天体物理 · 物理学 2016-03-02 K. Iwasawa , Y. Tanaka , L. C. Gallo

The first X-ray observation of the Seyfert 2 galaxy NGC5252 is reported. ASCA collected $\sim 4000$ photons/detector enough to perform an accurate spectral analysis of this source. The luminosity of NGC5252 is L$_{\rm X}$(0.7-10 keV)…

天体物理学 · 物理学 2009-10-28 M. cappi , T. Mihara , M. Matsuoka , W. Brinkmann , M. A. Prieto , G. G. C. Palumbo

We present results from a half-day observation by XMM-Newton of the nucleus of the nearby Seyfert 2 galaxy NGC 6300. The X-ray spectrum of the nucleus consists of a heavily absorbed hard component dominating the 3--10 keV band and a soft…

天体物理学 · 物理学 2009-11-10 Chiho Matsumoto , Aida Nava , Larry A. Maddox , Karen M. Leighly , Dirk Grupe , Hisamitsu Awaki , Shiro Ueno

We report on X-ray emission from the Seyfert 2 galaxy NGC4388 observed with the Chandra X-ray Observatory. A hard X-ray peak is found at the position of the active nucleus suggested by optical and radio observations. Extended soft X-ray…

天体物理学 · 物理学 2009-09-17 K. Iwasawa , A. S. Wilson , A. C. Fabian , A. J. Young
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