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Related papers: Ultraluminous IRAS galaxy 10026+4347

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We report long, pointed ROSAT HRI observations of the hyperluminous galaxies IRAS F00235+1024, F12514+1027, F14481+4454 and F14537+1950. Two of them are optically classified as Seyfert-like. No X-ray sources are detected at the positions of…

Astrophysics · Physics 2009-10-30 R. J. Wilman , A. C. Fabian , R. M. Cutri , C. S. Crawford , W. N. Brandt

The observation of the Narrow-Line Seyfert 1 galaxy IRAS13349+2438 performed by XMM-Newton European Photon Imaging Camera between 0.3-10 keV, is presented here. The broadband spectrum of the source is dominated at low energies (E < 2 keV)…

Astrophysics · Physics 2009-11-10 A. L. Longinotti , M. Cappi , K. Nandra , M. Dadina , S. Pellegrini , ;

We present new, quasi-simultaneous hard X-ray and near-IR spectra of the ultraluminous infrared galaxy IRAS 05189-2524, and discuss them together with archival and literature data. The 1.9 Seyfert nucleus is Compton-thin. The near-IR broad…

Astrophysics · Physics 2009-10-31 P. Severgnini , G. Risaliti , A. Marconi , R. Maiolino , M. Salvati

We present a detailed analysis of the intrinsic X-ray absorption in the Seyfert 1 galaxy NGC 4151 using Chandra/HETGS data obtained 2002 May, as part of a program which included simultaneous UV spectra using HST/STIS and FUSE. NGC 4151 was…

We observed the X-ray-bright ultra-luminous infrared galaxy, IRAS 05189$-$2524, with XRISM during its performance verification phase. The unprecedented energy resolution of the onboard X-ray microcalorimeter revealed complex spectral…

We report identification of a narrow-line Seyfert 1 galaxy RXJ1236.9+2656. X-ray emission from the NLS1 galaxy undergoes long-term variability with 0.1--2.0 keV flux changing by a factor of 2 within about 3 yr. The ROSAT PSPC spectrum of…

Astrophysics · Physics 2007-05-23 G. C. Dewangan , K. P. Singh , Paula Szkody , D. W. Hoard

We present the results from the multi-wavelength monitoring observations of the Narrow-Line Seyfert 1 galaxy Mrk 335 with AstroSat. We analysed both the X-ray (SXT & LAXPC) and UV (UVIT) data of the source at two epochs, separated by ~18…

High Energy Astrophysical Phenomena · Physics 2021-06-30 Savithri H. Ezhikode , Gulab C. Dewangan , Ranjeev Misra

We present ROSAT HRI and ASCA observations of the well known ULIRG IRAS19254-7245 (the Superantennae). The object is not detected by ROSAT yielding a 3\sigma upper limit of L_x ~8x10^{41} erg/s in the 0.1-2 keV band. However, we obtain a…

Astrophysics · Physics 2009-10-31 A. Pappa , I. Georgantopoulos , G. C. Stewart

We present an optical and X-ray study of the quasar QSO 0117-2837. It exhibits an interesting combination of optical and X-ray properties: Despite its extremely steep observed X-ray spectrum (Gamma_x ~ -4 when fit by a simple powerlaw), its…

Astrophysics · Physics 2009-10-31 Stefanie Komossa , D. Grupe , V. Burwitz , M. Janek

The z=2.286 IRAS galaxy F10214+4724 remains one of the most luminous galaxies in the Universe, despite its gravitational lens magnification. We present optical and near-infrared spectra of F10214+4724, with clear evidence for three distinct…

We have discovered a Narrow-Line Seyfert 1 (NLS1) galaxy and identified it with an ultrasoft X-ray source RX 215319-1514 detected with ROSAT. We present its X-ray and optical spectral characteristics. Its redshift is found to be…

Astrophysics · Physics 2007-05-23 K. P. Singh , L. R. Jones

We present an X-ray study of the ultra-luminous infrared galaxy IRAS F00183-7111 (z=0.327), using data obtained from NuSTAR, Chandra X-ray Observatory, Suzaku and XMM-Newton. The Chandra imaging shows that a point-like X-ray source is…

Astrophysics of Galaxies · Physics 2017-10-25 K. Iwasawa , H. W. W. Spoon , A. Comastri , R. Gilli , G. Lanzuisi , E. Piconcelli , C. Vignali , M. Brusa , S. Puccetti

We present a detailed analysis of XMM-Newton X-ray spectra of the Narrow-Line Seyfert 1 galaxy Mrk 1044. We find robust evidence for a multi-phase, ultra-fast outflow, traced by four separate components in the grating spectrum. One…

We present results of temporal and spectral analyses on four XMM-Newton EPIC pn observations of IRAS 17020+4544, a narrow-line Seyfert 1 galaxy with evidence of a radio jet. Analysis of the light curves reveals that this radio-loud source…

High Energy Astrophysical Phenomena · Physics 2020-06-17 A. G. Gonzalez , L. C. Gallo , P. Kosec , A. C. Fabian , W. N. Alston , M. Berton , D. R. Wilkins

We report the discovery of a narrow-line QSO (NLQSO) RX J1334.2+3759 with a steep soft X-ray spectrum. Soft X-ray emission from the NLQSO is highly variable. Changes in the intensity by a factor of about 2 have been detected in the ROSAT…

Astrophysics · Physics 2009-11-06 G. C. Dewangan , K. P. Singh , L. R. Jones , I. M. McHardy , K. O. Mason , A. M. Newsam

The narrow line Seyfert 1 (NLS1) IRAS 13224-3809 is the most X-ray variable active galactic nucleus (AGN), exhibiting 0.3-10 keV flux changes of over an order of magnitude within an hour. We report on the results of the 1.5 Ms 2016…

High Energy Astrophysical Phenomena · Physics 2018-08-16 M. L. Parker , W. N. Alston , D. J. K Buisson , A. C. Fabian , J. Jiang , E. Kara , A. Lohfink , C. Pinto

We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524 which is classified as an ultra-luminous infrared galaxy (ULIRG) and optical Seyfert 2 at $z$ = 0.0426. We test a variety of spectral models which…

Astrophysics of Galaxies · Physics 2020-01-08 Robyn N. Smith , Francesco Tombesi , Sylvain Veilleux , Anne M. Lohfink , Alfredo Luminari

We report on the results of a three-year program of coordinated X-ray and optical monitoring of the narrow-line Seyfert 1 galaxy NGC 4051. The rapid continuum variations observed in the X-ray spectra are not detected in the optical,…

As part of the TANAMI multiwavelength progam, we discuss new X-ray observations of the $\gamma$-ray and radio-loud Narrow Line Seyfert galaxy ($\gamma$-NLS1) PKS 2004-447. The active galaxy is a member of a small sample of radio-loud NLS1s…

We report the identification of the optical counterpart to the transient ultraluminuos X-ray source in the blue dwarf galaxy UGC6456 (VII Zw 403). The source is highly variable in both the X-ray (more 100 times, 0.3-10 keV) and optical…

High Energy Astrophysical Phenomena · Physics 2020-10-13 Alexander Vinokurov , Kirill Atapin , Yulia Solovyeva
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