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Author
of
Planck early results. V. The Low Frequency Instrument data processing
Planck intermediate results
Planck 2015 results
Planck 2013 results. I. Overview of products and scientific results
Planck intermediate results
Planck 2015 results
Planck 2015 results
Planck 2015 results
Planck 2015 results
First results from the Very Small Array — II. Observations of the cosmic microwave background
Searching for non-Gaussianity in the Very Small Array data
Infrared-correlated 31-GHz radio emission from Orion East
Estimating the bispectrum of the Very Small Array data
COSMOSOMAS observations of the cosmic microwave background and Galactic foregrounds at 11 GHz: evidence for anomalous microwave emission at high Galactic latitude
Cosmological parameter estimation and Bayesian model comparison using Very Small Array data
A 33-GHz Very Small Array survey of the Galactic plane from ℓ= 27° to 46°
Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters
A measurement at the first acoustic peak of the cosmic microwave background with the 33-GHz interferometer
Cosmic microwave background observations with the Jodrell Bank-IAC interferometer at 33 GHz
First results from the Very Small Array — III. The cosmic microwave background power spectrum
The cosmic microwave background power spectrum out to ℓ= 1400 measured by the Very Small Array
Cosmological parameter estimation using Very Small Array data out to ℓ= 1500
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-yr data: I - Spectral properties
Very Small Array observations of the anomalous microwave emission in the Perseus region
Studies of cosmic microwave background structure at Dec. = + 40° - II. Analysis and cosmological interpretation
Non-Gaussianity in the Very Small Array cosmic microwave background maps with smooth goodness-of-fit tests
Galactic synchrotron emission at high frequencies
Constraints on spinning dust towards Galactic targets with the Very Small Array: a tentative detection of excess microwave emission towards 3C396
Source subtraction for the extended Very Small Array and 33-GHz source count estimates
Studies of cosmic microwave background structure at Dec. = + 40° −1. The performance of the Tenerife experiments
A multifrequency maximum-entropy joint analysis of COBE and Tenerife data
Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian cosmic microwave background cold spot
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-yr data: II - Flux density variability
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