activity
19982004
most citedEstimating the bispectrum of the Very Small Array data

19 citations · 19 across the 1 of their papers we have counts for

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astro-ph200736 cited

Constraints on spinning dust towards Galactic targets with the VSA: a tentative detection of excess microwave emission towards 3C396

Anna Scaife, David A. Green, Richard A. Battye +18

We present results from observations made at 33 GHz with the Very Small Array (VSA) telescope towards potential candidates in the Galactic plane for spinning dust emission. In the…

astro-ph200747 cited

CBI limits on 31 GHz excess emission in southern HII regions

C. Dickinson, R. D. Davies, L. Bronfman +5

We have mapped four regions of the southern Galactic plane at 31 GHz with the Cosmic Background Imager. From the maps, we have extracted the flux densities for six of the brightest…

astro-ph200419 cited

Estimating the bispectrum of the Very Small Array data

Sarah Smith, Graca Rocha, Anthony Challinor +30

We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in December 2002, and compare our results to those obtaine…

astro-ph1999

A 33 GHz interferometer for CMB observations on Tenerife

S. J. Melhuish, S. Dicker, R. D. Davies +5

We describe a new high sensitivity experiment for observing cosmic microwave background (CMB) anisotropies. The instrument is a 2-element interferometer operating at 33 GHz with a…

astro-ph1999

Cosmic Microwave background map making with data between 10 and 90GHz

A. W. Jones, A. N. Lasenby, P. Mukherjee +5

We use data from the Tenerife 10, 15 and 33 GHz beamswitching experiments along with the COBE 53 and 90 GHz data to separate the cosmic microwave background (CMB) signal from the G…

astro-ph1998

Synchrotron Emission from the Galaxy

R. D. Davies, A. Wilkinson

Galactic synchrotron emission is a potentially confusing foreground, both in total power and in polarization, to the Cosmic Microwave Background Radiation. It also contains much ph…