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相关论文: ROSAT PSPC observations of six PG quasars and PHL …

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We utilize recent NuSTAR observations (co-added depth $\approx55$-120 ks) of PG $1001+054$, PG $1254+047$, and PHL 1811 to constrain their hard X-ray ($\gtrsim5$ keV) weakness and spectral shapes, and thus to investigate the nature of their…

高能天体物理现象 · 物理学 2022-09-14 Chaojun Wang , B. Luo , W. N. Brandt , D. M. Alexander , F. E. Bauer , S. C. Gallagher , Jian Huang , Hezhen Liu , D. Stern

We present the final results of a ROSAT PSPC program to study the soft X-ray emission properties of a complete sample of low $z$ quasars. The main results are: 1. There is no evidence for significant soft excess emission or excess…

天体物理学 · 物理学 2009-10-28 Ari Laor , Fabrizio Fiore , Martin Elvis , Belinda J. Wilkes , Jonathan C. McDowell

The nearby barred spiral galaxy NGC 1672 is thought to have a weak Seyfert nucleus in addition to its strong starburst activity. Observations with the PSPC and HRI instruments on board the ROSAT X-ray satellite show that three X-ray sources…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , J. P. Halpern , K. Iwasawa

We have studied the variability of 6 low redshift, radio quiet `PG' quasars on three timescales (days, weeks, and months) using the ROSAT HRI. The quasars were chosen to lie at the two extreme ends of the ROSAT PSPC spectral index…

天体物理学 · 物理学 2009-10-30 Fabrizio Fiore , Ari Laor , Martin Elvis , Fabrizio Nicastro , Emanuele Giallongo

We report the results from Chandra and XMM-Newton observations of a sample of 10 type 1 quasars selected to have unusual UV emission-line properties (weak and blueshifted high-ionization lines; strong UV Fe emission) similar to those of PHL…

We have used the WGA catalog of ROSAT PSPC X-ray sources to study the X-ray spectrum of about 500 quasars in the redshift interval 0.1--4.1, detected with a signal to noise better than 7. We have parameterized the PSPC spectrum in terms of…

天体物理学 · 物理学 2009-10-30 Fabrizio Fiore , Martin Elvis , Paolo Giommi , Paolo Padovani

(abridged) We present and discuss our observations of the NL quasar PG1404+226 with ASCA and HST, and a re-analysis of our earlier observations with ROSAT. The soft X-ray spectrum is very steep and displays an absorption feature (edge or…

天体物理学 · 物理学 2016-08-30 Marie-Helene Ulrich , Andrea Comastri , Stefanie Komossa , Phil Crane

This is the second of two papers reporting observations and analysis of the unusually bright (m_b=14.4), luminous (M_B=-25.5), nearby (z=0.192) narrow-line quasar PHL 1811. The first paper reported that PHL 1811 is intrinsically X-ray weak,…

天体物理学 · 物理学 2019-08-19 Karen M. Leighly , Jules P. Halpern , Edward B. Jenkins , Darrin Casebeer

The object PG 0043+039 has been identified as a broad absorption line (BAL) quasar based on its UV spectra. However, this optical luminous quasar has not been detected before in deep X-ray observations, making it the most extreme X-ray weak…

星系天体物理 · 物理学 2016-08-07 W. Kollatschny , N. Schartel , M. Zetzl , M. Santos-Lleó , P. M. Rodríguez-Pascual , L. Ballo , A. Talavera

We started a follow-up investigation of the Deep X-ray Radio Blazar Survey objects with declination >-10 deg. We undertook a survey with the EVN at 5GHz to make the first images of a complete sample of weak blazars, aiming at a comparison…

星系天体物理 · 物理学 2015-04-29 F. Mantovani , M. Bondi , K. -H. Mack , W. Alef , E. Ros , J. A. Zensus

We present an in-flight calibration of the ROSAT PSPC using the incident spectra of the hot white dwarf HZ43 and the polar AM Her. We derive an absolute flux calibration of the PSPC using the accurately known soft X-ray spectrum of HZ43.…

天体物理学 · 物理学 2008-02-20 K. Beuermann

Abridged) In the SDSS, several unusual QSOs have been discovered that have very blue rest-frame UV spectra but no discernible emission lines. Their UV spectra strongly resemble that of the newly discovered quasar PHL 1811 ($z=0.192$; $\rm…

天体物理学 · 物理学 2007-05-23 Karen M. Leighly , Jules P. Halpern , Edward B. Jenkins

We present and interpret several new X-ray features of the X-ray pulsar PSR J1838-0655. The X-ray data are obtained from the archival data of CHANDRA, RXTE}, and SUZAKU. We combine all these X-ray data and fit the spectra with different…

高能天体物理现象 · 物理学 2015-05-13 Lupin Chun-Che Lin , Jumpei Takata , Chorng-Yuan Hwang , Jau-Shian Liang

This is the first of two papers reporting observations and analysis of the unusually bright (m_b=14.4), luminous (M_B=-25.5), nearby (z=0.192) narrow-line quasar PHL 1811, focusing on the X-ray properties and the spectral energy…

We analyse the ROSAT PSPC spectrum of 19 X-ray selected Narrow Emission Line Galaxies (NELGs) discovered during the optical identification of sources in the ROSAT UK Deep Survey. Their properties are compared to those of broad line Active…

We have observed with ROSAT six blazars from the sample of 31 polarized objects constructed by Impey and Tapia (1988). Results of the spectral analysis in the ROSAT band of three objects, PKS 0301-243, PKS 1055+018 and PG 1424+240 are…

天体物理学 · 物理学 2009-10-22 L. Maraschi , G. Fossati , G. Tagliaferri , A. Treves

We present results on the X-ray spectra of the radio-loud, high-polarization quasar, PKS 1510-089, based on new data obtained using ASCA, and from archival ROSAT data. The X-ray spectrum obtained by ASCA is unusually hard, with the photon…

天体物理学 · 物理学 2009-10-30 K. P. Singh , C. R. Shrader , I. M. George

We report here the results of high-resolution and spectral imaging X-ray observations, with both the ROSAT HRI and PSPC, of the field surrounding the nearby Seyfert galaxy IC4329A. Many point sources are detected, the brightest being…

天体物理学 · 物理学 2007-05-23 A. M. Read , W. Pietsch

A database of radio-quiet quasars detected with ROSAT is presented containing 846 quasars seen in the All-Sky Survey and/or in pointed PSPC observations. About 70% of the objects have been detected in X-rays for the first time. We present…

天体物理学 · 物理学 2008-11-26 W. Yuan , W. Brinkmann , J. Siebert , W. Voges

We present an analysis of the \rosat and \asca spectra of 21 broad line AGN (QSOs) with $z\sim 1$ detected in the 2-10 keV band with the \asca \gis. The summed spectrum in the \asca band is well described by a power-law with…

天体物理学 · 物理学 2009-11-06 A. Pappa , G. C. Stewart , I. Georgantopoulos , R. E. Griffiths , B. J. Boyle , T. Shanks
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