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Related papers: Ultraluminous IRAS galaxy 10026+4347

200 papers

We present the first look at the spectral and timing analysis of Narrow-Line Seyfert 1 Galaxies (NLS1s) with the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) mission. The…

High Energy Astrophysical Phenomena · Physics 2023-01-04 G. Grünwald , Th. Boller , S. Rakshit , J. Buchner , T. Dauser , M. Freyberg , T. Liu , M. Salvato , A. Schichtel

The present paper discusses the results from an analysis of the images presented in Paper I (astro-ph/0207373) supplemented with new spectroscopic data obtained at Keck. All but one object in the 1-Jy sample show signs of a strong tidal…

Astrophysics · Physics 2008-11-26 S. Veilleux , D. -C. Kim , D. B. Sanders

We report the discovery of a Narrow Line QSO located at about 1.3' from the Broad Line Radio Galaxy 3C445. The source,1WGA J2223.7-0206, although already revealed by ROSAT has never been optically identified previously. An XMM-Newton…

Astrophysics · Physics 2009-11-10 Paola Grandi , Luigi Foschini , Nicola Masetti , Eliana Palazzi

Narrow-line Seyfert\,1 galaxies (NLS1s) with very small broad-line widths (say, FWHM(\hb) $\la $ 1200\,\kms) represent the extreme type of Seyfert\,1 galaxies that have small black hole masses (\mbh) and/or high Eddington ratios (\redd).…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Y. L. Ai , W. Yuan , H. Y. Zhou , T. G. Wang , S. H. Zhang

We present XMM-Newton spectra of the Seyfert 2 Galaxy IRAS 00521-7054. A strong feature at ~6 keV (observer's frame) can be formally fitted with a strong (EW=1.3+-0.3 keV in the rest frame) and broad Fe Ka line, extending down to 3 keV. The…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Ying Tan , Junxian Wang , Xinwen Shu , Youyuan Zhou

Methods. We analyse two observations taken with the Low Energy Transmission Grating Spectrometer of Chandra. We investigated the spectral response to a sudden flux decrease by a factor of 5, which occurred during the second observation.…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 K. C. Steenbrugge , M. Fenovcik , J. S. Kaastra , E. Costantini , F. Verbunt

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…

We present the identification and characterization of the optical counterpart to 2XMM J011942.7+032421, one of the most luminous and distant ultra-luminous X-ray sources (ULXs). The counterpart is located near a star forming region in a…

Astrophysics of Galaxies · Physics 2015-06-23 C. M. Gutierrez , D. -S. Moon

(Abridged) We present an analysis of a 10-day continuous ASCA observation of the narrow-line Seyfert 1 galaxy IRAS 13224-3809. The soft (0.7-1.3 keV) and hard (1.3-10 keV) X-ray band light curves binned to 5000s reveal trough-to-peak…

Astrophysics · Physics 2009-11-07 G. C. Dewangan , Th. Boller , K. P. Singh , K. M. Leighly

We present the results of a deep 300 ks Chandra HETG observation of the highly variable narrow-line Seyfert Type 1 galaxy NGC 4051. The HETG spectrum reveals 28 significant soft X-ray ionised lines in either emission or absorption;…

High Energy Astrophysical Phenomena · Physics 2015-05-27 A. P. Lobban , J. N. Reeves , L. Miller , T. J. Turner , V. Braito , S. B. Kraemer , D. M. Crenshaw

IRAS 00521$-$7054 is the first Seyfert 2 in which the presence of an extremely large Fe K$\alpha$ line has been claimed. We report here on the analysis of a 100 ks Suzaku observation of the source. We confirm the existence of a very strong…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Claudio Ricci , Fumie Tazaki , Yoshihiro Ueda , Stephane Paltani , Rozenn Boissay , Yuichi Terashima

We report results from a Suzaku observation of the narrow-line Seyfert 1 NGC 4051. During our observation, large amplitude rapid variability is seen and the averaged 2--10 keV flux is 8.1x10^-12 erg s^-1 cm^-2, which is several times lower…

We present NuSTAR hard X-ray observations of Sh 2-104, a compact HII region containing several young massive stellar clusters (YMSCs). We have detected distinct hard X-ray sources coincident with localized VERITAS TeV emission recently…

We report the first detection of a sharp spectral feature in a Narrow-Line Seyfert 1 galaxy. Using XMM-Newton we have observed 1H0707-495 and find a drop in flux by a factor of more than 2 at a rest-frame energy of ~7 keV without any…

We report results from a 2003 FUSE observation, and reanalysis of a 1996 HST observation of the unusual X-ray transient Narrow-line Seyfert 1 galaxy WPVS 007. The HST FOS spectrum revealed mini-BALs with V_max ~ 900 km s^-1 and FWHM ~ 550…

Cosmology and Nongalactic Astrophysics · Physics 2009-07-24 Karen M. Leighly , Fred Hamann , Darrin A. Casebeer , Dirk Grupe

We have conducted a new long-term multi-wavelength campaign on one of the most super- Eddington narrow-line Seyfert 1s (NLS1s) known, namely RX J0134.2-4258. In this first paper, we report deep simultaneous X-ray observations performed by…

High Energy Astrophysical Phenomena · Physics 2022-04-20 Chichuan Jin , Chris Done , Martin Ward , Francesca Panessa , Bo Liu , Heyang Liu

We present a detailed timing and spectral study of an extremely variable narrow-line Seyfert~1 galaxy NGC 4748 using observations in the year 2017 and 2014 performed with AstroSat and XMM-Newton, respectively. Both observations show…

High Energy Astrophysical Phenomena · Physics 2021-01-13 Main Pal , Neeraj Kumari , Pankaj Kushwaha , K. P. Singh , Alok C. Gupta , Sachindra Naik , G. C. Dewangan , P. Tripathi , Rathin Adhikari , O. Adegoke , H. Nandan

On 2019 October 25, the Fermi-Large Area Telescope observed the first gamma-ray flare from the radio-loud narrow-line Seyfert 1 (NLSy 1) galaxy PKS 2004$-$447 ($z=0.24$). We report on follow-up observations in the radio, optical-UV, and…

We present the results of a 17 ks Chandra ACIS-S observation of the nearby dwarf spiral galaxy NGC 4395. Chandra affords the first high-quality, broadband X-ray detection of the active nucleus of this object that is uncontaminated by nearby…