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Related papers: NGC 4051: Black hole mass and photon index-mass ac…

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We present the discovery of correlations between the X-ray spectral (photon) index and mass accretion rate observed in active galactic nuclei (AGNs) 3C~454.3 and M87. We analyzed spectral transition episodes observed in these AGNs using…

Astrophysics of Galaxies · Physics 2020-01-22 Lev Titarchuk , Elena Seifina , Alexandre Chekhtma , Indira Ocampo

We report the results of Swift and Chandra observations of an ultra-luminous X-ray source, ULX-1 in M101. We show strong observational evidence that M101 ULX-1 undergoes spectral transitions from the low/hard state to the high/soft state…

High Energy Astrophysical Phenomena · Physics 2015-12-23 Lev Titarchuk , Elena Seifina

We present the results of a reverberation-mapping program targeting NGC5273, a nearby early-type galaxy with a broad-lined active galactic nucleus. Over the course of the monitoring program, NGC5273 showed strong variability that allowed us…

In a recent work we demonstrated that a novel X-ray scaling method, originally introduced for Galactic black holes (GBHs), can be reliably extended to estimate the mass of supermassive black holes accreting at a moderate to high level. Here…

High Energy Astrophysical Phenomena · Physics 2015-06-19 I. Jang , M. Gliozzi , C. Hughes , L. Titarchuk

We present over 6.5 years of frequent X-ray observations of the NLS1 galaxy NGC4051 by RXTE together with a >100ks observation by XMM-Newton and so derive a 2-10 keV PSD covering an unprecedent frequency range of over 6.5 decades from…

Astrophysics · Physics 2008-11-26 I. M. McHardy , I. E. Papadakis , P. Uttley , M. J. Page , K. O. Mason

We present a comprehensive examination of the X-ray variability of the narrow line Seyfert 1 (NLS1) galaxy NGC4051. We combine over 6.5 years of frequent monitoring observations by RXTE with a >100ks continuous observation by XMM-Newton and…

Astrophysics · Physics 2009-11-10 I. M. McHardy , I. E. Papadakis , P. Uttley , K. O. Mason , M. J. Page

The determination of the central black hole mass is crucial to the understanding of AGN physics. In this paper we briefly review some methods that are currently used to estimate the black hole mass of AGNs. Particularly we demonstrate the…

Astrophysics · Physics 2007-05-23 Xue-Bing Wu , F. K. Liu , R. Wang , M. Z. Kong , J. L. Han

We present a study of correlations between X-ray spectral and timing properties observed from a number of Galactic Black Hole (BH) binaries during hard-soft state spectral evolution. We analyze 17 transition episodes from 8 BH sources…

High Energy Astrophysical Phenomena · Physics 2011-02-11 Nickolai Shaposhnikov , Lev Titarchuk

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 report on the results of a simultaneous monitoring campaign employing eight Chandra X-ray (0.5-10 keV) and six VLA/EVLA (8.4 GHz) radio observations of NGC 4051 over seven months. Evidence for compact jets is observed in the 8.4 GHz…

We derive masses of the central super-massive black hole (SMBH) and accretion rates for 154 type1 AGN belonging to a well-defined X-ray-selected sample, the XMM-Newton Serendipitous Sample (XBS). To this end, we use the most recent…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 A. Caccianiga , R. Fanali , P. Severgnini , R. Della Ceca , E. Marchese , S. Mateos

NGC 6240 is a pair of colliding disk galaxies, each with a black hole in its core. We have used laser guide star adaptive optics on the Keck II telescope to obtain high-resolution ($\sim 0.06$") near-infrared integral-field spectra of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Anne M. Medling , S. Mark Ammons , Claire E. Max , Richard I. Davies , Hauke Engel , Gabriela Canalizo

We present an analysis of the fundamental plane of black hole accretion, an empirical correlation of the mass of a black hole ($M$), its 5 GHz radio continuum luminosity ($\nu L_{\nu}$), and its 2-10 keV X-ray power-law continuum luminosity…

High Energy Astrophysical Phenomena · Physics 2019-01-30 Kayhan Gültekin , Ashley L. King , Edward M. Cackett , Kristina Nyland , Jon M. Miller , Tiziana Di Matteo , Sera Markoff , Michael P. Rupen

We present an XMM-Newton time-resolved spectral analysis of the NLS1 galaxy Mrk 766. We analyse eight available observations of the EPIC-pn camera taken between May 2000 and June 2005 to investigate the X-ray spectral variability as…

High Energy Astrophysical Phenomena · Physics 2015-06-17 S. Giacche` , R. Gilli , L. Titarchuk

We present a revised measurement of the mass of the central black hole (Mbh) in the Seyfert 1 galaxy NGC 4151. The new stellar dynamical mass measurement is derived by applying an axisymmetric orbit-superposition code to near-infrared…

We present a study of the correlations between spectral, timing properties and mass accretion rate observed in X-rays from the Galactic Black Hole (BH) binary GRS 1915+105 during the transition between hard and soft states. We analyze all…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Lev Titarchuk , Elena Seifina

Accurately determining the black hole mass ($M_\mathrm{BH}$) in active galactic nuclei (AGN) is crucial to constraining their properties and to studying their evolution. While direct methods yield reliable measurements of $M_\mathrm{BH}$ in…

Astrophysics of Galaxies · Physics 2023-03-29 James K. Williams , Mario Gliozzi , Kyle A. Bockwoldt , Onic I. Shuvo

We present our analysis of X-ray spectral properties observed from the Seyfrert 1 galactic nucleus NGC~7469 using the RXTE and ASCA observations. We demonstrate strong observational evidence that NGC~7469 undergoes spectral transitions from…

Astrophysics of Galaxies · Physics 2018-11-14 Elena Seifina , Lev Titarchuk , Lyubov Ugolkova

We model the spectral energy distribution of the type 1 Seyfert galaxy NGC 5548, fitting data from simultaneous optical, UV, and X-ray monitoring observations. We assume a geometry consisting of a hot central Comptonizing region surrounded…

Astrophysics · Physics 2009-11-07 James Chiang , Omer Blaes

Using bonafide black hole (BH) mass estimates from reverberation mapping and the line ratio [Si VI]1.963$\mu$m/Br$\gamma_{\rm broad}$ as tracer of the Active Galactic Nuclei (AGN) ionizing continuum, we find a novel BH-mass scaling relation…

Astrophysics of Galaxies · Physics 2021-11-30 Swayamtrupta Panda , Alberto Rodríguez Ardila
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