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相关论文: QSO 2359-1241: A Bright, Highly Polarized, Radio-M…

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We present the discovery of the radio-loud quasar PSO J352.4034-15.3373 at z=5.84 pm 0.02. This quasar is the radio brightest source known, by an order of magnitude, at z~6 with a flux density in the range of 8-100 mJy from 3GHz to 230MHz…

HE 0141-3932 (zem = 1.80) is a bright blue radio-quite quasar with an unusually weak Ly-alpha emission line. Large redshift differences (Delta z = 0.05) are observed between high ionization and low ionization emission lines. Absorption…

天体物理学 · 物理学 2009-11-10 D. Reimers , E. Janknecht , C. Fechner , I. I. Agafonova , S. A. Levshakov , S. Lopez

We present the results of XMM-Newton observations of four high-z quasars, two radio-loud and two radio-quiet. One of the radio-loud objects, PKS 2126-158, clearly shows absorption in excess of the galactic value as claimed before from ASCA…

天体物理学 · 物理学 2011-05-23 E. Ferrero , W. Brinkmann

We present the discovery of PSO J191.05696$+$86.43172 (hereafter PSO J191$+$86), a new powerful radio-loud quasar (QSO) in the early Universe (z = 5.32). We discovered it by cross-matching the NRAO VLA Sky Survey (NVSS) radio catalog at 1.4…

星系天体物理 · 物理学 2023-01-25 S. Belladitta , A. Moretti , A. Caccianiga , D. Dallacasa , C. Spingola , M. Pedani , L. P. Cassarà , S. Bisogni

We have discovered two low-ionization broad absorption line quasars in programs to obtain optical spectra for radio-selected quasar candidates from the VLA FIRST Survey (Becker, White, & Helfand 1995). Both belong to the extremely rare…

We present results of a new, large survey for high-redshift radio-loud quasars, which targets quasars with z>4. The survey is based on the PMN and NVSS radio surveys, optically identified using digitised UKST B, R and I plates. Six new z>4…

天体物理学 · 物理学 2009-11-07 I. M. Hook , R. G. McMahon , P. A. Shaver , I. A. G. Snellen

HE0141-3932 (zem=1.80) is a bright blue radio-quite quasar which reveals an emission line spectrum with an unusually weak Ly-alpha line. In addition, large redshift differences (Delta z=0.05) are observed between high ionization and low…

天体物理学 · 物理学 2009-11-11 S. A. Levshakov , I. I. Agafonova , D. Reimers , C. Fechner , E. Janknecht , S. Lopez

Few high-redshift, radio-loud quasars are known to date. The extremely luminous, radio-bright quasar, SDSS J013127.34-032100.1 was recently discovered at a redshift of $z=5.18$. We observed the source with high resolution very long baseline…

高能天体物理现象 · 物理学 2015-11-23 K. E. Gabanyi , D. Cseh , S. Frey , Z. Paragi , L. I. Gurvits , T. An , Y. K. Zhang

Only very few z>5 quasars discovered to date are radio-loud, with a radio-to-optical flux ratio (radio-loudness parameter) higher than 10. Here we report the discovery of an optically luminous radio-loud quasar, SDSS J013127.34-032100.1…

From examination of only 4 deg^2 of sky in the NOAO Deep Wide-Field Survey (NDWFS) region, we have identified the first radio-loud quasar at a redshift z>6. The object, FIRST J1427385+331241, was discovered by matching the FLAMEX IR survey…

天体物理学 · 物理学 2011-02-11 Ian D. McGreer , Robert H. Becker , David J. Helfand , Richard L. White

We report the near-IR detection of a prominent CIV absorption in the rest-frame UV spectrum of the most distant known QSO, SDSS J104433.04-012502.2, at z=5.80. This QSO was recently observed with XMM-Newton and it was found to be notably…

天体物理学 · 物理学 2009-11-06 R. Maiolino , F. Mannucci , C. Baffa , S. Gennari , E. Oliva

We present optical spectroscopic data for a complete sample of 161 S_5GHz >= 0.2 Jy, flat-spectrum radio sources. The sources were observed as part of a survey for high redshift, radio-loud quasars, and were selected for spectroscopic…

天体物理学 · 物理学 2015-06-24 I. M. Hook , R. G. McMahon , M. J. Irwin , C. Hazard

We present results from Keck I high resolution spectroscopy of the radio loud quasar PKS 0123+257 ($z_e$=2.364, V=17.5). In this object we detect Ly$\alpha$, N V 1238,1242, Si IV 1393,1402, and C IV 1548,1550 in an absorption system at a…

天体物理学 · 物理学 2014-10-13 Thomas A. Barlow , W. L. W. Sargent

SDSS J1634+2049 is a local (z = 0.1293) infrared-luminous quasar with LIR= 10^11.91 Lsun. We present a detailed multiwavelength study of both the host galaxy and the nucleus. The host galaxy demonstrates violent, obscured star formation…

We present an analysis of the absorption-line system in the Very Large Telescope/Ultraviolet and Visual Echelle Spectrograph spectrum at a redshift of $z_{\rm a}={3.1448}$ associated with the quasar SDSS J122040.23+092326.96, whose…

星系天体物理 · 物理学 2025-01-03 Qiguo Tian , Lei Hao , Yipeng Zhou , Xiheng Shi , Tuo Ji , Peng Jiang , Lin Lin , Zhenya Zheng , Hongyan Zhou

In this letter we report the detection of a strong and extremely blueshifted X-ray absorption feature in the 1 Ms Chandra spectrum of CXO CDFS J033260.0-274748, a quasar at z = 2.579 with L_2-10keV ~ 4x10^44 ergs/s. The broad absorption…

We present observations of an optically-faint quasar, RD J114816.2+525339, discovered from deep multi-color observations of the field around the z = 6.42 quasar SDSS J1148+5251. The two quasars have a projected separation of 109 arcsec and…

天体物理学 · 物理学 2009-11-13 A. Mahabal , D. Stern , M. Bogosavljevic , S. G. Djorgovski , D. Thompson

We have analyzed the broad absorption line system of the bright (V=16.5) high-redshift (z=2.361) QSO SBS1542+541 using UV spectra from the HST FOS along with optical data from the MMT and the Steward Observatory 2.3m telescope. These…

天体物理学 · 物理学 2009-10-30 Randal C. Telfer , Gerard A. Kriss , Wei Zheng , Arthur F. Davidsen , Richard F. Green

A statistical study is presented of (a) the frequency of narrow CIV lambda 1549 absorption lines in 1.5 <~ z <~ 3.6 radio-quiet and radio-loud quasars, and of (b) the UV and radio properties of the absorbed quasars. The quasar sample is…

天体物理学 · 物理学 2009-11-10 M. Vestergaard

We report the correct classification of an overlooked Fanaroff-Riley class II radio-loud quasar with broad absorption lines, only the second such object so identified. The rare properties of this quasar, LBQS 1138-0126, are twice…

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