46 results on '"Jones, Michael E."'
Search Results
2. Detection of spectral variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
3. Characterizing the performance of high-speed data converters for RFSoC-based radio astronomy receivers
4. The C-Band All-Sky Survey: total intensity point-source detection over the northern sky
5. Resolved observations at 31 GHz of spinning dust emissivity variations in ρ Oph
6. The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
7. Gain stabilization for radio intensity mapping using a continuous-wave reference signal
8. The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region
9. The C-Band All-Sky Survey (C-BASS): digital backend for the northern survey
10. The C-Band All-Sky Survey (C-BASS): design and capabilities
11. Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz
12. C-Band All-Sky Survey: a first look at the Galaxy
13. Astronomical receiver modelling using scattering matrices
14. The C-Band All-Sky Survey (C-BASS): design and implementation of the northern receiver
15. The Cosmic Background Imager 2
16. A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
17. A 33-GHz Very Small Array survey of the Galactic plane from ℓ= 27° to 46°
18. Radio source calibration for the Very Small Array and other cosmic microwave background instruments at around 30 GHz
19. Erratum: Source subtraction for the extended Very Small Array and 33-GHz source count estimates
20. Astronomical receiver modelling using scattering matrices.
21. Non-Gaussianity in the Very Small Array cosmic microwave background maps with smooth goodness-of-fit tests
22. Cosmic microwave background observations from the Cosmic Background Imager and Very Small Array: a comparison of coincident maps and parameter estimation methods
23. Source subtraction for the extended Very Small Array and 33-GHz source count estimates
24. H0from an orientation-unbiased sample of Sunyaev-Zel'dovich and X-ray clusters
25. High-sensitivity measurements of the cosmic microwave background power spectrum with the extended Very Small Array
26. Cosmological parameter estimation using Very Small Array data out to ℓ= 1500
27. Estimating the bispectrum of the Very Small Array data
28. Searching for non-Gaussianity in the Very Small Array data
29. 9C: a survey of radio sources at 15 GHz with the Ryle Telescope
30. Measuring the Hubble constant from Ryle Telescope and X-ray observations, with application to Abell 1413
31. Detection of a cosmic microwave background decrement towards a cluster of mJy radio sources
32. Mapping of the Sunyaev—Zel'dovich effect in the cluster Cl 0016+16 with the Ryle Telescope
33. Surveying the sky with the Arcminute MicroKelvin Imager: expected constraints on galaxy cluster evolution and cosmology
34. The radio source counts at 15 GHz and their implications for cm-wave CMB imaging
35. A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters.
36. AMI observations of northern supernova remnants at 14–18 GHz.
37. A Very Small Array search for the extended Sunyaev–Zel'dovich effect in the Corona Borealis supercluster.
38. H0 from an orientation-unbiased sample of Sunyaev–Zel'dovich and X-ray clusters.
39. First results from the Very Small Array – I. Observational methods.
40. First results from the Very Small Array – III. The cosmic microwave background power spectrum.
41. First results from the Very Small Array – II. Observations of the cosmic microwave background.
42. First results from the Very Small Array – IV. Cosmological parameter estimation.
43. A measurement of H[sub 0] from Ryle Telescope,ASCA andROSAT observations of Abell 773.
44. A maximum-likelihood approach to removing radio sources from observations of the Sunyaev–Zel'dovich effect, with application to Abell 611.
45. The cosmic microwave background power spectrum out to ℓ= 1400 measured by the Very Small Array.
46. Cosmological parameter estimation and Bayesian model comparison using Very Small Array data.
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