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20012011
most citedThe RMS Survey: CO observations of candidate massive YSOs in the northern Galactic plane

73 citations · 342 across the 19 of their papers we have counts for

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astro-ph2008★ 73 cited

The RMS Survey: CO observations of candidate massive YSOs in the northern Galactic plane

J. S. Urquhart, A. L. Busfield, M. G. Hoare +9

Context: The Red MSX Source (RMS) survey is an ongoing multi-wavelength observational programme designed to return a large, high-resolution mid-infrared colour-selected sample of m…

astro-ph2008★ 11 cited

Disentangling the Galaxy at low Galactic latitudes

M. Cignoni, M. Tosi, A. Bragaglia +2

We have used the field stars from the open cluster survey BOCCE, to study three low-latitude fields imaged with the Canada-France-Hawaii telescope (CFHT), with the aim of better un…

astro-ph2007★ 59 cited

Galaxy redshift surveys selected by neutral hydrogen using FAST

Alan R. Duffy, Richard A. Battye, Rod D. Davies +2

We discuss the possibility of performing a substantial spectroscopic galaxy redshift survey selected via the 21cm emission from neutral hydrogen using the Five-hundred metre Apertu…

astro-ph2004★ 55 cited

The HDF-North SCUBA Super-map II: Multi-wavelength properties

C. Borys, D. Scott, S. C. Chapman +3

We present radio, optical and X-ray detected counterparts to the sub-mm sources found using SCUBA in the Hubble Deep Field North region (GOODS-N). A new counterpart identification…

astro-ph2004★ 51 cited

The nature of a gravitationally lensed sub-millimetre arc in MS0451.6-0305: two interacting galaxies at z~2.9?

C. Borys, S. C. Chapman, M. Donahue +6

We present a new SCUBA image of the cluster MS0451.6-0305, which exhibits strong, extended sub-mm flux at 850 microns. The most striking feature in the map is an elongated region o…

astro-ph2003★ 2 cited

Giant pulses in Millisecond Pulsars

B. C. Joshi, M. Kramer, A. G. Lyne +2

Giant pulses (GPs), occasional individual pulses with an intensity 100 times the average intensity, have been detected in four pulsars todate. Their origin is not well understood,…