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Related papers: BL Lacertae: X-ray spectral evolution and a black-…

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BL Lacertae is a unique blazar for which the X-ray band can cover either the synchrotron or the inverse Compton, or both parts of the broadband spectral energy distribution. In the latter case, when the spectral upturn is located in the…

High Energy Astrophysical Phenomena · Physics 2024-12-30 Alicja Wierzcholska , Stefan Wagner

We report the results of Swift/XRT observations (2008-2015) of a hyper-luminous X-ray source, ESO 243-49 HLX-1. We found a strong observational evidence that ESO 243-49 HLX-1 underwent spectral transitions from the low/hard state to the…

High Energy Astrophysical Phenomena · Physics 2016-11-15 Lev Titarchuk , Elena Seifina

We present the results of an extensive analysis of the optical, ultraviolet, X-ray and $\gamma$-ray data collected from the observations of the BL Lac objects prototype BL Lacertae carried out over a period of nearly 13 years, between…

High Energy Astrophysical Phenomena · Physics 2022-04-20 N. Sahakyan , P. Giommi

We presented a study of outburst activity in the BL Lacertae source OJ~287, observed extensively with the X-ray telescope (XRT) onboard Neil Gehrels Swift Observatory. We demonstrated that the results of our analysis of X-ray flaring…

High Energy Astrophysical Phenomena · Physics 2023-03-29 Lev Titarchuk , Elena Seifina , Chris Shrader

This paper reports on the X-ray emission from BL Lacertae during its July 1997 outburst as observed with the Rossi X-ray Timing Explorer (RXTE), compares the RXTE data to previous measurements, and interprets the overall electromagnetic…

Astrophysics · Physics 2022-01-26 G. Madejski , M. Sikora , T. Jaffe , M. Blazejowski , K. Jahoda , R. Moderski

BL Lacertae is a blazar known for its high flux variability and occasional broadband flares of unknown origin. It was in an extended flaring state from July 2020 until the end of 2021, making it an ideal candidate to study spectral and…

High Energy Astrophysical Phenomena · Physics 2026-04-01 A. Priyana Noel , Alicja Wierzcholska , Raj Prince

X-ray properties of the BL Lacertae object OJ 287, observed with ASCA on 1997 April 26 and November 17, are reported. The 0.5 -- 10 keV flux was lower than those obtained in previous X-ray observations, and no evidence of intensity…

Astrophysics · Physics 2015-06-24 Naoki Isobe , Makoto Tashiro , Masahiko Sugiho , Kazuo Makishima

We have analysed optical spectra of BL Lacertae, the prototype of its class, to verify the presence and possible flux variations of its broad Ha line. We used the spectroscopic information also to investigate the question of its parent…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-14 Alessandro Capetti , Claudia Raiteri , Sara Buttiglione

Blazars are the established sources of an intense and variable non-thermal radiation extending from radio wavelengths up to HE and VHE gamma-rays. Understanding the spectral evolution of blazars in selected frequency ranges, as well as…

High Energy Astrophysical Phenomena · Physics 2014-12-24 Alicja Wierzcholska , Michał Ostrowski , Łukasz Stawarz , Stefan Wagner , Marcus Hauser

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

The multi-wavelength outburst activity in the BL Lacertae source OJ 287 has sparked a lot of controversy about whether the source contains one or two black holes (BHs) and what characteristics of this black hole binary would be. In this…

High Energy Astrophysical Phenomena · Physics 2024-03-27 Sergey Kuznetsov , Lev Titarchuk

BL Lacertae was the target of an extensive multiwavelength monitoring campaign in the second half of 2000. Simultaneous or quasi-simultaneous observations were taken at radio (UMRAO and Metsaehovi) and optical(WEBT collaboration)…

Astrophysics · Physics 2009-11-10 M. Boettcher

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 study the X-ray spectra of 85 BL Lacertae objects using the hardness ratios as given in the WGA catalogue of {\it ROSAT} sources. This sample includes all WGA BL Lacs with high-quality data and comprises about 50 per cent of presently…

Astrophysics · Physics 2015-06-24 Paolo Padovani , Paolo Giommi

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

During a period of strong $\gamma$-ray flaring activity from BL Lacertae, we organized Swift, Neutron star Interior Composition Explorer (NICER), and Nuclear Spectroscopic Telescope Array (NuSTAR) follow-up observations. The source has been…

High Energy Astrophysical Phenomena · Physics 2021-11-10 Filippo D'Ammando

We present an expanded sample of low-mass black holes (BHs) found in galactic nuclei. Using standard virial mass techniques to estimate BH masses, we select from the Fourth Data Release of the Sloan Digital Sky Survey all broad-line active…

Astrophysics · Physics 2009-11-13 Jenny E. Greene , Luis C. Ho

This talk focuses on the statistical properties of X-ray selected BL Lacertae objects (XBLs) whose catalogue has been compiled. It consists of 312 sources from different X-ray surveys, unambiguously identified to mid-2010. Results of the…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-03 B. Z. Kapanadze

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 X-ray properties of optically-selected intermediate-mass (~10^5--10^6 M_Sun) black holes (BHs) in active galaxies (AGNs), using data from the Chandra X-Ray Observatory. Our observations are a continuation of a pilot study by…

Astrophysics of Galaxies · Physics 2011-02-11 Louis-Benoit Desroches , Jenny E. Greene , Luis C. Ho
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