Search Results - "Saunders, Richard D"
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Bayesian modelling of clusters of galaxies from multifrequency-pointed Sunyaev–Zel'dovich observations
Published in Monthly notices of the Royal Astronomical Society (01-10-2009)“…We present a Bayesian approach to modelling galaxy clusters using multi-frequency pointed observations from telescopes that exploit the Sunyaev–Zel'dovich…”
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Very Small Array observations of the anomalous microwave emission in the Perseus region
Published in Monthly notices of the Royal Astronomical Society (01-03-2010)“…The dust complex G159.6–18.5 in the Perseus region has previously been observed with the COSMOSOMAS experiment on angular scales of ≈1°, and was found to…”
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PHYSIOLOGIC AND DOSIMETRIC CONSIDERATIONS FOR LIMITING ELECTRIC FIELDS INDUCED IN THE BODY BY MOVEMENT IN A STATIC MAGNETIC FIELD
Published in Health physics (1958) (01-06-2011)“…Movement in a strong static magnetic field induces electric fields in a human body, which may result in various sensory perceptions such as vertigo, nausea,…”
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AMI observations of northern supernova remnants at 14–18 GHz
Published in Monthly notices of the Royal Astronomical Society (11-06-2009)“…We present observations between 14.2 and 17.9 GHz of 12 reported supernova remnants (SNRs) made with the Arcminute Microkelvin Imager Small Array (AMI SA). In…”
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10C survey of radio sources at 15.7 GHz - II. First results
Published in Monthly notices of the Royal Astronomical Society (11-08-2011)“…In a previous paper (Paper I), the observational, mapping and source-extraction techniques used for the Tenth Cambridge (10C) Survey of Radio Sources were…”
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10C survey of radio sources at 15.7GHz - I. Observing, mapping and source extraction
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…ABSTRACT We have observed an area of [asymptotically =]27deg2 to an rms noise level of 0.2mJy at 15.7 GHz, using the Arcminute Microkelvin Imager Large Array…”
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Radio source calibration for the Very Small Array and other cosmic microwave background instruments at around 30 GHz
Published in Monthly notices of the Royal Astronomical Society (21-08-2008)“…Accurate calibration of data is essential for the current generation of cosmic microwave background (CMB) experiments. Using data from the Very Small Array…”
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AMI observations of Lynds dark nebulae: further evidence for anomalous cm-wave emission
Published in Monthly notices of the Royal Astronomical Society (11-12-2009)“…Observations at 14.2 to 17.9 GHz made with the Arcminute Microkelvin Imager (AMI) Small Array towards 14 Lynds dark nebulae with a resolution of ≈2 arcmin are…”
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Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-yr data: I – Spectral properties
Published in Monthly notices of the Royal Astronomical Society (01-12-2009)“…We present follow-up observations of 97 point sources from the Wilkinson Microwave Anisotropy Probe (WMAP) 3-yr data, contained within the New Extragalactic…”
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Detailed Sunyaev–Zel'dovich study with AMI of 19 LoCuSS galaxy clusters: masses and temperatures out to the virial radius
Published in Monthly notices of the Royal Astronomical Society (01-09-2012)“…ABSTRACT We present detailed 16‐GHz interferometric observations using the Arcminute Microkelvin Imager (AMI) of 19 clusters with LX > 7 × 1037 W (h50 = 1)…”
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A digital correlator upgrade for the Arcminute MicroKelvin Imager
Published in Monthly notices of the Royal Astronomical Society (21-04-2018)Get full text
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12
Sub-kpc radio jets in the brightest central galaxy of the cool-core galaxy cluster RXJ1720.1+2638
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2023)“…ABSTRACT The cool-core galaxy cluster RXJ1720.1+2638 hosts extended radio emission near the cluster core, known as a minihalo. The origin of this emission is…”
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Radio continuum observations of Class I protostellar discs in Taurus: constraining the greybody tail at centimetre wavelengths
Published in Monthly notices of the Royal Astronomical Society (01-03-2012)“…We present deep 1.8 cm (16 GHz) radio continuum imaging of seven young stellar objects in the Taurus molecular cloud. These objects have previously been…”
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Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-02-2012)“…We present an analysis of observations made with the Arcminute Microkelvin Imager (AMI) and the Canada-France-Hawaii Telescope (CFHT) of six galaxy clusters in…”
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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
Published in Monthly notices of the Royal Astronomical Society (11-12-2008)“…ABSTRACT We present interferometric imaging at 33 GHz, with the new superextended configuration of the Very Small Array (VSA), of a very deep decrement in the…”
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Sunyaev-Zel'dovich observations of galaxy clusters out to the virial radius with the Arcminute Microkelvin Imager
Published in Monthly notices of the Royal Astronomical Society (01-12-2011)“…We present observations using the Small Array of the Arcminute Microkelvin Imager (AMI; 14-18 GHz) of four Abell and three MACS clusters spanning 0.171-0.686…”
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AMI-LA radio continuum observations of Spitzer c2d small clouds and cores: Perseus region
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…We present deep radio continuum observations of the cores identified as deeply embedded young stellar objects in the Perseus molecular cloud by the Spitzer c2d…”
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Physical modelling of galaxy cluster Sunyaev–Zel’dovich data using Einasto dark matter profiles
Published in Monthly notices of the Royal Astronomical Society (01-11-2019)“…We derive a model for Sunyaev–Zel’dovich data from a galaxy cluster that uses an Einasto profile to model the cluster’s dark matter component. This model is…”
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Parametrization effects in the analysis of AMI Sunyaev-Zel'dovich observations
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…Most Sunyaev-Zel'dovich (SZ) and X-ray analyses of galaxy clusters try to constrain the cluster total mass (M T(r)) and/or gas mass (M g(r)) using parametrized…”
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G64.5+0.9: a new shell supernova remnant with unusual central emission
Published in Monthly notices of the Royal Astronomical Society (01-09-2009)“…We present observations between 1.4 and 18 GHz confirming that G64.5+0.9 is a new Galactic shell supernova remnant, using the Very Large Array and the…”
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