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相关论文: An Extremely Red Nucleus in an Absorbed QSO at z=0…

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The results of deep-imaging observations of a candidate of an absorbed QSO at z=0.653, AX J131831+3341, are presented. AX J131831+3341 was found during the course of optical follow-up observations of the ASCA Large Sky Survey, and has an…

We present results from XMM-Newton observations of the obscured QSO 1SAX J1218.9+2958. We find that the previously reported optical and soft X-ray counterpart positions are incorrect. However we confirm the spectroscopic redshift of 0.176.…

天体物理学 · 物理学 2009-11-10 Nicola Loaring , M. J. Page , G. Ramsay

We present K-band imaging and photometry of a sample of 52 radio loud quasars (RQs) selected from the B3 survey with flux densities above 0.5 Jy at 408 MHz. The optical completeness of the sample is 90% and the quasars cover the redshift…

天体物理学 · 物理学 2009-10-30 R. Carballo , S. F. Sanchez , J. I. Gonzalez-Serrano , C. R. Benn , M. Vigotti

The nearby Seyfert 2 Galaxy NGC 1068 was observed with speckle imaging techniques in the near-infrared H-band (1.6 microns) at the Hale 200-inch Telescope and K-band (2.2 microns) at the 10 m Keck I Telescope. Images with diffraction…

天体物理学 · 物理学 2009-10-31 A. J. Weinberger , G. Neugebauer , K. Matthews

The presence of dust in quasar absorbers, such as damped Lyman alpha (DLA) systems, may cause the background QSO to appear reddened. We investigate the extent of this potential reddening by comparing the optical-to-infrared (IR) colors of…

天体物理学 · 物理学 2008-11-26 Sara L. Ellison , Patrick B. Hall , Paulina Lira

We present deep K-band imaging at the positions of four very faint X-ray sources found in the UK ROSAT Deep Survey to have no optical counterpart brighter than R~23. Likely identifications are found within the ROSAT error circle in all four…

天体物理学 · 物理学 2015-06-24 A. M. Newsam , I. M. McHardy , L. R. Jones , K. O. Mason

We present results of near-infrared photometry (J, H, K_S) for a sample of active galactic nuclei (AGNs) obtained from hard X-ray surveys with ASCA. The sample covers the AGNs at z=0.1-1 with L(2-10keV)=10^42-10^46 erg/s with very high…

天体物理学 · 物理学 2009-11-10 Chisato Watanabe , Kouji Ohta , Masayuki Akiyama , Yoshihiro Ueda

We aim to understand the multi-wavelength properties of 2XMM J123204+215255, the source with the most extreme X-ray-to-optical flux ratio amongst a sample of bright X-ray selected EXOs drawn from a cross-correlation of the 2XMMp catalogue…

天体物理学 · 物理学 2009-11-13 A. Del Moro , M. G. Watson , S. Mateos , M. Akiyama , Y. Hashimoto , N. Tamura , K. Ohta , F. J. Carrera , G. Stewart

We report the discovery of a bright quasar (E=15.8, z=0.868) associated with the flat spectrum radio source NVSS J235953-124148. This quasar we designate QSO 2359-1241 possesses a rare combination of extreme properties that make it of…

We present XMM-Newton observations of AXJ0341.4-4453, a mildly reddened A_V<7 QSO at a redshift of z=0.672. The XMM-Newton spectrum shows a large obscuring column N_H~10^23 cm^{-2} corresponding to A_V~70, in agreement with previous results…

天体物理学 · 物理学 2008-11-26 I. Georgantopoulos , A. Georgakakis , G. C. Stewart , A. Akylas , B. J. Boyle , T. Shanks , R. E. Griffiths

Extensive calculations of the atomic data required for the spectral modelling of the K-shell photoabsorption of oxygen ions have been carried out in a multi-code approach. The present level energies and wavelengths for the highly ionized…

天体物理学 · 物理学 2009-11-10 J. Garcia , C. Mendoza , M. A. Bautista , T. W. Gorczyca , T. R. Kallman , P. Palmeri

We present J, H and K-band images and 0.9-2.5 micron spectra of the nuclear regions of Centaurus A obtained with IRIS on the AAT. While K band has a point source coincident with the nucleus, at H and J we identify diffuse structure…

天体物理学 · 物理学 2009-10-31 J. J. Bryant , R. W. Hunstead

We are currently undertaking a large survey for redshifted atomic and molecular absorption ... only one clear and one tentative detection were obtained: HI absorption at z = 0.097 in PKS 1555-140 and OH absorption at z =0.126 in PKS…

We have undertaken a search for millimetre-wave band absorption (through the CO and HCO+ rotational transitions) in the host galaxies of reddened radio sources (z = 0.405-1.802). Despite the colour selection (optical-near infrared colours…

宇宙学与河外天体物理 · 物理学 2015-05-28 S. J. Curran , M. T. Whiting , F. Combes , N. Kuno , P. Francis , N. Nakai , J. K. Webb , M. T. Murphy , T. Wiklind

We present the results of a systematic analysis of the XMM-Newton spectra of nearby optically bright QSOs. The objects have been selected from X-ray Galaxy Catalog Xgal20. It is a catalog of 1172 manually identified and classified galaxies,…

宇宙学与河外天体物理 · 物理学 2021-10-15 Lidiia Zadorozhna , Anatolii Tugay , Nadiia Pulatova , Oleh Maluy

There exists a significant population of broad line, z~2 QSOs which have heavily absorbed X-ray spectra. Follow up observations in the submillimetre show that these QSOs are embedded in ultraluminous starburst galaxies, unlike most…

宇宙学与河外天体物理 · 物理学 2015-05-28 M. J. Page , F. J. Carrera , J. A. Stevens , J. Ebrero , A. J. Blustin

A simple estimate of the photometric redshift would prove invaluable to forthcoming continuum surveys on the next generation of large radio telescopes, as well as mitigating the existing bias towards the most optically bright sources. While…

星系天体物理 · 物理学 2019-09-11 S. J. Curran , J. P. Moss

I present a study of the X-ray spectral properties of a sample containing 24 type-1 active galactic nuclei using the medium spectral resolution of ``ASCA''. The sample consists of 20 radio-quiet objects and 4 radio-loud objects. A simple…

天体物理学 · 物理学 2015-06-24 C. S. Reynolds

We present a detailed study of the X-ray and optical spectra of the luminous Seyfert galaxy Mrk 1393, which revealed variable partial obscuration of the active nucleus. The X-ray spectra obtained by XMM-Newton and Swift show moderate…

宇宙学与河外天体物理 · 物理学 2009-11-13 T. G. Wang , H. Y. Zhou , D. Grupe , W. M. Yuan , X. B. Dong , H. L. Lu

A point X-ray source located 9 arcmin northeast of the center of SN~1006 has been spectroscopically identified as a background QSO, with a redshift of 0.335. The object is moderately bright, with magnitude V=18.3. If its ultraviolet…

天体物理学 · 物理学 2009-10-30 P. Frank Winkler , Knox S. Long
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