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http://hub.abes.fr/oup/periodical/mnras/2002/volume_331/issue_4/101046j13658711200205255x/authorship/5
http://hub.abes.fr/oup/periodical/mnras/2009/volume_400/issue_2/101111j13652966200915673x/authorship/9
http://hub.abes.fr/oup/periodical/mnras/2009/volume_398/issue_1/101111j13652966200915078x/authorship/6
http://hub.abes.fr/oup/periodical/mnras/2004/volume_353/issue_3/101111j13652966200408102x/authorship/12
http://hub.abes.fr/oup/periodical/mnras/2004/volume_353/issue_3/101111j13652966200408206x/authorship/11
http://hub.abes.fr/oup/periodical/mnras/2009/volume_400/issue_3/101111j13652966200915542x/authorship/8
http://hub.abes.fr/oup/periodical/mnrasl/2010/volume_403/issue_1/101111j17453933201000812x/authorship/7
http://hub.abes.fr/oup/periodical/mnras/2003/volume_341/issue_4/101046j13658711200306354x/authorship/9
http://hub.abes.fr/oup/periodical/mnras/2006/volume_369/issue_2/101111j13652966200610341x/authorship/14
http://hub.abes.fr/oup/periodical/mnrasl/2006/volume_369/issue_1/101111j17453933200600151x/authorship/24
http://hub.abes.fr/oup/periodical/mnras/2007/volume_382/issue_1/101111j13652966200712169x/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2003/volume_341/issue_4/101046j13658711200306564x/authorship/11
http://hub.abes.fr/oup/periodical/mnras/2003/volume_341/issue_4/101046j13658711200306494x/authorship/10
http://hub.abes.fr/oup/periodical/mnras/2008/volume_391/issue_3/101111j13652966200813985x/authorship/10
http://hub.abes.fr/oup/periodical/mnras/2003/volume_341/issue_4/101046j13658711200306563x/authorship/10
http://hub.abes.fr/oup/periodical/mnrasl/2007/volume_377/issue_1/101111j17453933200700305x/authorship/11
http://hub.abes.fr/oup/periodical/mnras/2004/volume_352/issue_3/101111j13652966200407885x/authorship/14
http://hub.abes.fr/oup/periodical/mnras/2008/volume_388/issue_4/101111j13652966200813515x/authorship/11
http://hub.abes.fr/oup/periodical/mnras/2003/volume_341/issue_4/101046j13658711200306493x/authorship/9
http://hub.abes.fr/oup/periodical/mnras/2004/volume_349/issue_3/101111j13652966200407578x/authorship/12
http://hub.abes.fr/oup/periodical/mnras/2005/volume_363/issue_4/101111j13652966200509519x/authorship/13
http://hub.abes.fr/oup/periodical/mnras/2009/volume_396/issue_1/101111j13652966200914583x/authorship/7
http://hub.abes.fr/oup/periodical/mnras/2009/volume_400/issue_2/101111j13652966200915518x/authorship/9
http://hub.abes.fr/oup/periodical/mnrasl/2010/volume_406/issue_1/101111j17453933201000878x/authorship/8
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First results from the Very Small Array — II. Observations of the cosmic microwave background
Searching for non-Gaussianity in the Very Small Array data
Estimating the bispectrum of the Very Small Array data
Microwave observations of spinning dust emission in NGC6946
Cosmological parameter estimation and Bayesian model comparison using Very Small Array data
High-significance Sunyaev-Zel'dovich measurement: Abell 1914 seen with the Arcminute Microkelvin Imager
High-resolution AMI Large Array imaging of spinning dust sources: spatially correlated 8 µm emission and evidence of a stellar wind in L675
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
Harmonic analysis of cosmic microwave background data — II. From ring-sets to the sky
Non-Gaussianity in the Very Small Array cosmic microwave background maps with smooth goodness-of-fit tests
Constraints on spinning dust towards Galactic targets with the Very Small Array: a tentative detection of excess microwave emission towards 3C396
G64.5+0.9: a new shell supernova remnant with unusual central emission
Cosmology with the Planck cluster sample
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
AMI observations of northern supernova remnants at 14-18 GHz
High-sensitivity measurements of the cosmic microwave background power spectrum with the extended Very Small Array
Radio source calibration for the Very Small Array and other cosmic microwave background instruments at around 30 GHz
Cosmic microwave background observations from the Cosmic Background Imager and Very Small Array: a comparison of coincident maps and parameter estimation methods
AMI observations of Lynds dark nebulae: further evidence for anomalous cm-wave emission
First results from the Very Small Array — IV. Cosmological parameter estimation
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