pith. sign in

Rod D. Davies

Identifiers

  • name variant Rod D. Davies 0.60 · backfill

Papers (20)

  1. The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30$^{\circ}$,0$^{\circ}$) astro-ph.GA · 2014 · author #13
  2. Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: II - Flux-density variability astro-ph.CO · 2009 · author #3
  3. Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: I - Spectral properties astro-ph.CO · 2009 · author #3
  4. Radio source calibration for the VSA and other CMB instruments at around 30 GHz astro-ph · 2008 · author #2
  5. Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot astro-ph · 2008 · author #6
  6. Constraints on spinning dust towards Galactic targets with the VSA: a tentative detection of excess microwave emission towards 3C396 astro-ph · 2007 · author #4
  7. Non-Gaussianity in the Very Small Array CMB maps with Smooth-Goodness-of-fit tests astro-ph · 2006 · author #7
  8. A VSA search for the extended Sunyaev-Zel'dovich Effect in the Corona Borealis Supercluster astro-ph · 2005 · author #5
  9. Source subtraction for the extended Very Small Array and 33-GHz source count estimates astro-ph · 2004 · author #6
  10. High sensitivity measurements of the CMB power spectrum with the extended Very Small Array astro-ph · 2004 · author #4
  11. Cosmological parameter estimation using Very Small Array data out to l=1500 astro-ph · 2004 · author #5
  12. Estimating the bispectrum of the Very Small Array data astro-ph · 2004 · author #7
  13. Neutral hydrogen surveys for high redshift galaxy clusters and proto-clusters astro-ph · 2004 · author #2
  14. Searching for non-Gaussianity in the VSA data astro-ph · 2003 · author #5
  15. Cosmological parameter estimation and Bayesian model comparison using VSA data astro-ph · 2002 · author #4
  16. The CMB power spectrum out to l=1400 measured by the VSA astro-ph · 2002 · author #4
  17. First results from the Very Small Array -- III. The CMB power spectrum astro-ph · 2002 · author #4
  18. First results from the Very Small Array -- II. Observations of the CMB astro-ph · 2002 · author #4
  19. First results from the Very Small Array -- IV. Cosmological parameter estimation astro-ph · 2002 · author #5
  20. First results from the Very Small Array -- I. Observational methods astro-ph · 2002 · author #4

Mentions

  • 1403.3327 #13 · backfill · confidence 0.70 Rod D. Davies
  • 0907.3843 #3 · backfill · confidence 0.70 Rod D. Davies
  • 0907.3707 #3 · backfill · confidence 0.70 Rod D. Davies
  • 0804.2853 #2 · backfill · confidence 0.70 Rod D. Davies
  • 0804.0199 #6 · backfill · confidence 0.70 Rod D. Davies

Frequent Coauthors