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19952014
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 12k across the 138 of their papers we have counts for

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Showing 1998Show all

7 papers · 1 filter

astro-ph1998★ 5 cited

Deep optical imaging of the field of PC1643+4631A&B, I: Spatial distributions and the counts of faint galaxies

Toby Haynes, Garret Cotter, Joanne C. Baker +4

We present deep optical images of the PC1643+4631 field obtained at the WHT. This field contains two quasars at redshifts z=3.79 & 3.83 and a cosmic microwave background (CMB) decr…

astro-ph1998

Cosmological Evolution of the Submillimetre Luminosity of High-Redshift Radio Galaxies

D. H. Hughes, J. S. Dunlop, E. N. Archibald +2

A systematic survey measuring the submillimetre continuum luminosity in radio galaxies between redshifts z ~ 0.1 - 5 is currently in progress. The first results from observations w…

astro-ph1998★ 322 cited

The Nature and Evolution of Classical Double Radio Sources from Complete Samples

Katherine M. Blundell, Steve Rawlings, Chris J. Willott

We present a study of the trends in luminosity, linear size, spectral index, and redshift of classical double radio sources from three complete samples selected at successively fai…

astro-ph1998★ 19 cited

IRAS F10214+4724: the inner 100pc

Mark Lacy, Steve Rawlings, Stephen Serjeant

We use new near-infrared spectroscopy and our published optical spectroscopy of the gravitationally-lensed Seyfert-2 galaxy F10214+4724 to study both the links between the starburs…

astro-ph1998★ 9 cited

A radio-jet -- galaxy interaction in 3C441

Mark Lacy, Steve Rawlings, Katherine M. Blundell +1

Multi-wavelength imaging and spectroscopy of the z=0.708 radio galaxy 3C441 and a red aligned optical/infrared component are used to show that the most striking aspect of the radio…

astro-ph1998★ 27 cited

A spectroscopic study of IRAS F10214+4724

Stephen Serjeant, Steve Rawlings, Mark Lacy +4

The z=2.286 IRAS galaxy F10214+4724 remains one of the most luminous galaxies in the Universe, despite its gravitational lens magnification. We present optical and near-infrared sp…