An excess of emission in the dark cloud LDN 1111 with the Arcminute Microkelvin Imager (2008)
Hurley-Walker, N., Green, D. A., Davies, M. L., Grainge, K. J. B., Hobson, M. P., ...
We present observations of the Lynds' dark nebula LDN 1111 made at microwave frequencies between 14.6 and 17.2 GHz with the Arcminute Microkelvin Imager (AMI). We find emission in this frequency band...
Feroz, F., Hobson, M. P., Zwart, J. T. L., Saunders, R. D. E., Grainge, K. J. B.
We present a Bayesian approach to modelling galaxy clusters using multi-frequency pointed observations from telescopes that exploit the Sunyaev--Zel'dovich effect. We use the recently developed...
The Arcminute Microkelvin Imager (2008)
Barker, R. W., Biddulph, P., Bly, D., Boysen, R. C., Brown, A. R., ...
The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope...
Tucci, M., Rubiño-Martin, J. A., Rebolo, R., Genova-Santos, R., Watson, R. A., Battye, R. A., ...
We present an analysis of the spectral properties of the extragalactic radio sources in the nearly complete Very Small Array (VSA) sample at 33 GHz. Data from different surveys are used to study...
Tucci, M., Rubiño-Martin, J. A., Rebolo, R., Genova-Santos, R., Watson, R. A., Battye, R. A., ...
We present an analysis of the spectral properties of the extragalactic radio sources in the nearly-complete VSA sample at 33GHz. Data from different surveys are used to study source spectra between...
AMI limits on 15 GHz excess emission in northern HII regions (2007)
Scaife, A. M. M., Hurley-Walker, N., Davies, M. L., Duffett-Smith, P. J., Feroz, F., Grainge, K. J. B., ...
We present observations between 14.2 and 17.9 GHz of sixteen Galactic HII regions made with the Arcminute Microkelvin Imager (AMI). In conjunction with data from the literature at lower radio...
Rubiño-Martín, J.A., Aliaga, A.M., Barreiro, R.B., Battye, R.A., Carreira, P., Cleary, K., ...
Out of the 41 published VSA individual pointings dedicated to cosmological [cosmic microwave background (CMB)] observations, 37 are found to be consistent with Gaussianity, whereas four pointings...
Millimetric observation of the SZ effect in the Corona Borealis supercluster (2006)
Battistelli, E. S., De Petris, M., Lamagna, L., Watson, R. A., Rebolo, R., Melchiorri, F., ...
We have observed the Corona Borealis Supercluster with the Millimeter and Infrared Testa grigia Observatory (MITO), located in the Italian Alps, at 143, 214, 272, and 353 GHz. We present a...
Rajguru, N., Myers, S. T., Battye, R. A., Bond, J. Richard, Cleary, K., Contaldi, C. R., ...
We present coincident observations of the Cosmic Microwave Background (CMB) from the Very Small Array (VSA) and Cosmic Background Imager (CBI) telescopes. The consistency of the full datasets is...
Cosmological parameter estimation using Very Small Array data out to ℓ= 1500 (2004)
Rebolo, R., Battye, R.A., Carreira, P., Cleary, K., Davies, R.D., Davis, R.J., ...
We estimate cosmological parameters using data obtained by the Very Small Array (VSA) in its extended configuration, in conjunction with a variety of other cosmic microwave background (CMB) data and...
Cosmological parameter estimation using Very Small Array data out to ℓ= 1500 (2004)
Rebolo, R., Battye, R.A., Carreira, P., Cleary, K., Davies, R.D., Davis, R.J., ...
We estimate cosmological parameters using data obtained by the Very Small Array (VSA) in its extended configuration, in conjunction with a variety of other cosmic microwave background (CMB) data and...
Estimating the bispectrum of the Very Small Array data (2004)
Smith, S., Rocha, R., Challinor, A., Battye, R.A., Carreira, P., Cleary, K., ...
We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in 2002 December, and compare our results with those obtained from Gaussian...
First results from the Very Small Array - IV. Cosmological parameter estimation (2003)
Rubino-Martin, J. A., Rebolo, R., Carreira, P., Cleary, K., Davies, R. D., Davis, R. J., ...
Associated absorption in radio quasars. I. C IV absorption and the growth of radio sources (2001)
Baker, J. C., Hunstead, R. W., Athreya, R. M., Barthel, P. D., De Silva, E., Lehnert, M. D., ...
We assess the global properties of associated C IV 1548,1550 absorption lines measured in the spectra of radio-loud quasars drawn from a near-complete, low-frequency selected sample. The observations...