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Related papers: XMM-Newton observations of the BL Lac MS 0737+7441

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The high-frequency-peaked BL Lac, MS0205.7+3509 was observed twice with XMM-Newton. Both X-ray spectra are synchrotron-dominated, with mean 0.2--10keV fluxes of 2.80+/-0.01 and 3.34+/-0.02 E-12 erg/cm^2/s. The X-ray spectra are well fit by…

Astrophysics · Physics 2009-11-10 D. Watson , B. McBreen , L. Hanlon , J. N. Reeves , N. Smith , E. Perlman , J. Stocke , T. A. Rector

We present an XMM-Newton catalogue of BL Lac X-ray, optical, and UV properties based on cross-correlation with the 1151 BL Lacs listed in the fifth edition of the Roma-BZCAT. We searched for the X-ray counterparts to these objects in the…

High Energy Astrophysical Phenomena · Physics 2022-01-13 I. de la Calle Pérez , N. Álvarez Crespo , E. Racero , A. Rouco

We present XMM-Newton observations of four BL Lac objects (1H1219+301, H1426+428, Markarian 501 and PKS 0548-322), which have been found with past X-ray missions to contain evidence of broad soft X-ray absorption features. Observations with…

Astrophysics · Physics 2009-11-10 A. J. Blustin , M. J. Page , G. Branduardi-Raymont

In this paper, we make a multi-epoch analysis of NGC 1052, one of the prototypical LLAGN, using XMM-Newton, Suzaku and NuSTAR observations, taken from 2001 to 2017. This is the first time that results from NuSTAR observations are reported…

(abridged) We analyzed the archived XMM-Newton observation of the poorly studied low-mass X-ray binary XTE J1710-281 performed in 2004 that covered one orbital period of the system (3.8 hr). The source shows dips as well as eclipses, hence…

High Energy Astrophysical Phenomena · Physics 2015-05-13 G. Younes , L. Boirin , B. Sabra

On 2003 September 17 INTEGRAL discovered a bright transient source 3 degrees from the Galactic Center, IGR J17544-2619. The field containing the transient was observed by XMM-Newton on 2003 March 17 and September 11 and 17. A bright source,…

Astrophysics · Physics 2009-11-10 R. Gonzalez-Riestra , T. Oosterbroek , E. Kuulkers , A. Orr , A. N. Parmar

We present the results of a detailed temporal analysis of the bright BL Lac object Mrk 421 using the three available long timing mode observations by the EPIC PN camera. This detector mode is characterized by its long life time and is…

Astrophysics · Physics 2009-11-11 W. Brinkmann , I. E. Papadakis , C. Raeth , P. Mimica , F. Haberl

This paper reports the first discovery of possible inverse Compoton (IC) X-ray emission below 10 keV in the typical high-energy peaked BL Lac object (HBL) PKS 2155--304. Two XMM-Newton observations performed in 2006 reveal that the 0.6--10…

Astrophysics · Physics 2009-11-13 Y. H. Zhang

We report on an X-ray observation of the Seyfert 1.5 galaxy Mrk 6 obtained with the EPIC instruments onboard XMM-Newton. Archival BeppoSAX PDS data from 18-120 keV were also used to constrain the underlying hard power-law continuum. The…

Astrophysics · Physics 2009-11-07 S. Immler , W. N. Brandt , C. Vignali , F. Bauer , D. M. Crenshaw , J. J. Feldmeier , S. B. Kraemer

We report on the results of an EPIC XMM-Newton observation of the faint source SAXJ1748.2-2808 and the surrounding field. This source was discovered during the BeppoSAX Galactic center survey performed in 1997-1998. A spatial analysis…

Astrophysics · Physics 2009-11-11 L. Sidoli , S. Mereghetti , F. Favata , T. Oosterbroek , A. N. Parmar

We constrain the X-ray properties of the nearby $(360\,{\rm pc})$, old ($5\,{\rm Myr}$) pulsar B1133+16 with $\sim 100\,{\rm ks}$ effective exposure time by {\it XMM-Newton}. The observed pulsar flux in the 0.2-3 keV energy range is $\sim…

High Energy Astrophysical Phenomena · Physics 2017-02-08 Andrzej Szary , Janusz Gil , Bing Zhang , Frank Haberl , George I. Melikidze , Ulrich Geppert , Dipanjan Mitra , Ren-Xin Xu

We report the results of XMM-Newton observations of the X-ray bright, radio-loud blazar GB B1428+4217 at a redshift of z=4.72. We confirm the presence of soft X-ray spectral flattening at energies <0.7 keV as reported in previous ROSAT and…

Astrophysics · Physics 2009-11-10 M. A. Worsley , A. C. Fabian , A. Celotti , K. Iwasawa

We report on the XMM-Newton observation of the bright Seyfert 1 galaxy, MCG+8-11-11. Data from the EPIC/p-n camera, the Reflection Gratings Spectrometers (RGS) and the Optical Monitor (OM) have been analyzed. The p-n spectrum is well fitted…

Astrophysics · Physics 2009-11-11 G. Matt , S. Bianchi , A. De Rosa , P. Grandi , G. C. Perola

The BL Lac object Mrk 421 was observed on May 25, 2000 during the XMM - Newton CAL/PV phase. The high throughput of the X-ray telescopes and the spectral capabilities of the instruments allow an uninterrupted temporal and spectral study of…

We present the high resolution X-ray spectrum of the BL Lac object PKS 2155-304 taken with the RGS units onboard XMM-Newton in November 2000. We detect a OVII Kalpha resonant absorption line from warm/hot local gas at 21.59A (~4.5 sigma…

Astrophysics · Physics 2009-11-10 I. Cagnoni , F. Nicastro , L. Maraschi , A. Treves , F. Tavecchio

In August 2002, XMM-Newton devoted two full orbits to the observation of 1E 1207.4-5209, making this isolated neutron star the most deeply scrutinized galactic target of the mission. Thanks to the high throughput of the EPIC instrument,…

Astrophysics · Physics 2009-11-10 A. De Luca , S. Mereghetti , P. A. Caraveo , M. Moroni , R. P. Mignani , G. F. Bignami

We present a spectroscopic analysis of XMM-Newton and NuSTAR observations of the 'complex' NLS1 PG 1535+547 at redshift $z=0.038$. These observations span three epochs: 2002 and 2006 with XMM-Newton alone, covering the $0.3-10$ keV energy…

The second XMM-Newton serendipitous source catalogue, 2XMM, provides the ideal data base for performing a statistical evaluation of the flux cross-calibration of the XMM-Newton European Photon Imaging Cameras (EPIC). We aim to evaluate the…

Instrumentation and Methods for Astrophysics · Physics 2009-11-13 S. Mateos , R. D. Saxton , A. M. Read , S. Sembay

Aim of this work is a broad-band study with INTEGRAL, Swift and XMM-Newton satellites of a sample of 9 blazars (7 FSRQ and 2 BL Lac) with redshift up to about 4. The spectral analysis has shown clear evidence of a flattening of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 S. Gianni' , A. De Rosa , L. Bassani , A. Bazzano , A. J. Dean , P. Ubertini

We present a comprehensive study of the X-ray spectral variability observed in 13 TeV photon emitting high energy peaked BL Lacs(HBLs). These data come from 54 XMM-Newton EPIC-PN pointed observations made during its operational period from…

High Energy Astrophysical Phenomena · Physics 2025-05-01 P. U. Devanand , Alok C. Gupta , V. Jithesh , Paul J. Wiita , Archana Gupta
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