Y. A.

Non-Gaussianity in the Very Small Array cosmic microwave background maps with smooth goodness-of-fit tests (2006)

We have used the Rayner and Best smooth tests of goodness-of-fit to study the Gaussianity of the Very Small Array (VSA) data. These tests are designed to be sensitive to the presence of `smooth'...

Cosmic microwave background observations from the Cosmic Background Imager and Very Small Array: a comparison of coincident maps and parameter estimation methods (2005)

  • Rajguru,
  • N.,
  • Myers,
  • S.T.,
  • Battye,
  • R.A.,
  • ...

WWe 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 data sets is...

Women’s Employment and Family Stability In Nigeria: A Survey of Working Women In Ibadan Metropolis (2004)

The study examined the experiences of working women in Ibadan metropolis and its impact on family stability. A total of 156 working women, both in the formal and informal sectors of the economy,...

Cosmological parameter estimation using Very Small Array data out to l= 1500 (2004)

  • Rebolo,
  • R.,
  • Battye,
  • R.A.,
  • Carreira,
  • P.,
  • ...

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,
  • G.,
  • Challinor,
  • A.,
  • ...

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...

High-sensitivity measurements of the cosmic microwave background power spectrum with the extended Very Small Array (2004)

  • Dickinson,
  • C.,
  • Battye,
  • R.A.,
  • Carreira,
  • P.,
  • ...

We present deep Ka-band (ν~ 33 GHz) observations of the cosmic microwave background (CMB) made with the extended Very Small Array (VSA). This configuration produces a naturally weighted...

Searching for non-Gaussianity in the Very Small Array data (2004)

  • Savage,
  • R.,
  • Battye,
  • R.A.,
  • Carreira,
  • P.,
  • ...

We have tested Very Small Array (VSA) observations of three regions of sky for the presence of non-Gaussianity, using high-order cumulants, Minkowski functionals, a wavelet-based test and a Bayesian...

 
Additional Information

Publishing period:

2001 - 2006 (8)

Co-authors: