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相关论文: Image Deconvolution of the Radio Ring PKS 1830-211

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We discuss BIMA (Berkeley Illinois Maryland Association) data and present new high quality optical and near-IR Keck images of the bright radio ring PKS 1830-211. Applying a powerful new deconvolution algorithm we have been able to identify…

天体物理学 · 物理学 2007-05-23 B. L. Frye , F. Courbin , T. Broadhurst , W. J. W. Welch , C. Lidman , P. Magain , M. Pahre , S. G. Djorgovski

Optical and near-IR Hubble Space Telescope and Gemini-North adaptive optics images, further improved through deconvolution, are used to explore the gravitationally lensed radio source PKS 1830-211. The line of sight to the quasar at z=2.507…

天体物理学 · 物理学 2009-11-07 F. Courbin , G. Meylan , J. P. Kneib , C. Lidman

We report on the spectroscopic identification and the long awaited redshift measurement of the heavily obscured, gravitationally lensed radio source PKS 1830-211, which was first observed as a radio Einstein ring. The NE component of the…

天体物理学 · 物理学 2009-10-31 C. Lidman , F. Courbin , G. Meylan , T. Broadhurst , B. Frye , W. J. W. Welch

We report on new high-resolution near-infrared images of the gravitationally lensed radio source PKS1830-211, a quasar at z=2.507. These adaptive optics observations, taken with the Very Large Telescope (VLT), are further improved through…

天体物理学 · 物理学 2009-11-11 G. Meylan , F. Courbin , C. Lidman , J. -P. Kneib , L. E. Tacconi-Garman

PKS1830-211 is an unusually radio-loud gravitationally lensed quasar. In the radio, the system appears as two compact, dominant features surrounded by relatively extended radio emission which forms an Einstein Ring. As the line of sight to…

天体物理学 · 物理学 2016-08-30 Smita Mathur , Sunita Nair

Measurements of the properties of gravitational lenses have the power to tell us what sort of universe we live in. The brightest known radio Einstein ring/gravitational lens PKS 1830-211 (Jauncey et al., 1991), whilst obscured by our Galaxy…

We present optical and/or near-IR images of 128 ultra steep spectrum (USS) radio sources. Roughly half of the objects are identified in the optical images (R <~ 24), while in the near-IR images, >94% are detected at K<~ 22. The mean…

天体物理学 · 物理学 2009-11-07 Carlos De Breuck , Wil van Breugel , Adam Stanford , Huub Rottgering , George Miley , Daniel Stern

A search for radio recombination lines near 20 cm at z=0.193 and z=0.886 towards the gravitational lens system PKS 1830-211 has yielded upper limits on the line optical depth of 5 x 10^{-5} and 5 x10^{-4} at the two redshifts respectively.…

天体物理学 · 物理学 2007-05-23 Niruj R. Mohan , K. R. Anantharamaiah , W. M. Goss

We have compiled a sample of 234 ultra-steep-spectrum (USS) selected radio sources in order to find high-redshift radio galaxies. The sample covers the declination range -40deg < DEC < -30deg in the overlap region between the 1400-MHz NRAO…

宇宙学与河外天体物理 · 物理学 2009-11-13 J. J. Bryant , J. W. Broderick , H. M. Johnston , R. W. Hunstead , B. M. Gaensler , C. De Breuck

The remarkably strong radio gravitational lens PKS 1830-211 consists of a one arcsecond diameter Einstein ring with two bright compact (milliarcsecond) components located on opposite sides of the ring. We have obtained 22 GHz VLBA data on…

We present new observations of the gravitational lens system CLASS B0128+437. HST observations detect a very faint, extended object in I-band with no emission from the lensed images visible; no detection at all is made in V-band. The lens…

天体物理学 · 物理学 2007-05-23 A. D. Biggs , I. W. A. Browne , N. J. Jackson , T. York , M. A. Norbury , J. P. McKean , P. M. Phillips

(Abridged) A new technique for the spatial deconvolution of spectra is applied to near-IR (0.95 - 2.50 micron) NTT/SOFI spectra of the lensed, radio-quiet quasar HE 1104-1805. The continuum of the lensing galaxy is revealed between 1.5 and…

天体物理学 · 物理学 2007-05-23 F. Courbin , C. Lidman , G. Meylan , J. -P. Kneib , P. Magain

The Combined EIS-NVSS Survey Of Radio Sources (CENSORS) is a 1.4 GHz radio survey selected from the NRAO VLA Sky Survey (NVSS) and complete to a flux-density of 7.2mJy. It targets the ESO Imaging Survey (EIS) Patch D, which is a 3 by 2…

天体物理学 · 物理学 2009-11-11 M. H. Brookes , P. N. Best , R. Rengelink , H. J. A. Rottgering

Compact symmetric objects (CSOs) are thought to be short-lived radio sources with two lobes of emission that are separated by less than a kpc in projection. However, studies of such systems at high redshift is challenging due to the limited…

星系天体物理 · 物理学 2025-10-10 J. P. McKean , C. Spingola , D. M. Powell , S. Vegetti

We investigate the nature of the faintest radio sources detected in 3 VLA surveys, to faint limits 8 microJy at 8.5 GHz. Using the Keck Low Resolution Imaging Spectrograph in BRI and the Near Infra Red Camera in K, we image 51 radio…

天体物理学 · 物理学 2009-11-07 Nathan Roche , James Lowenthal , David Koo

We present optical spectroscopy of 62 objects selected from several samples of ultra steep spectrum (USS) radio sources. 46 of these are from our primary catalog, consisting of 669 sources with radio spectral indices alpha < -1.30 (S_nu ~…

We report the discovery of a new gravitationally lensed radio source. Radio maps of MG0751+2716 show four lensed images, which, at higher resolution, are resolved into long arcs of emission. A group of galaxies is present in optical images,…

Ultra-steep spectrum (USS) radio sources are good tracers of powerful radio galaxies at $z > 2$. Identification of even a single bright radio galaxy at $z > 6$ can be used to detect redshifted 21cm absorption due to neutral hydrogen in the…

We present a source and lens reconstruction for the optical Einstein ring gravitational lens system RXS J1131-1231. We resolve detail in the source, which is the host galaxy of a $z=0.658$ quasar, down to a resolution of 0.045 arc seconds…

天体物理学 · 物理学 2009-11-13 Brendon J. Brewer , Geraint F. Lewis
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