Search Results - "Scaife, Anna M. M."
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Practical galaxy morphology tools from deep supervised representation learning
Published in Monthly notices of the Royal Astronomical Society (02-05-2022)“…ABSTRACT Astronomers have typically set out to solve supervised machine learning problems by creating their own representations from scratch. We show that deep…”
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Bright radio emission from an ultraluminous stellar-mass microquasar in M 31
Published in Nature (London) (10-01-2013)“…A new ultraluminous X-ray source has been discovered in M 31, whose variability and associated bright, compact radio emission identify it as a stellar-mass…”
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CS-ROMER: a novel compressed sensing framework for Faraday depth reconstruction
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT The reconstruction of Faraday depth structure from incomplete spectral polarization radio measurements using the RM synthesis technique is an…”
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A GMRT survey of regions towards the Taurus molecular cloud at 323 and 608 MHz
Published in Monthly notices of the Royal Astronomical Society (01-11-2016)“…We present observations of three active sites of star formation in the Taurus molecular cloud complex taken at 323 and 608 MHz (90 and 50 cm, respectively)…”
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Fanaroff–Riley classification of radio galaxies using group-equivariant convolutional neural networks
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT Weight sharing in convolutional neural networks (CNNs) ensures that their feature maps will be translation-equivariant. However, although conventional…”
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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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KAT-7 detection of radio halo emission in the Triangulum Australis galaxy cluster
Published in Monthly notices of the Royal Astronomical Society (21-08-2015)“…We report the presence of high significance diffuse radio emission from the Triangulum Australis cluster using observations made with the KAT-7 telescope and…”
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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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Attention-gating for improved radio galaxy classification
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT In this work, we introduce attention as a state-of-the-art mechanism for classification of radio galaxies, using convolutional neural networks. We…”
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Quantifying uncertainty in deep learning approaches to radio galaxy classification
Published in Monthly notices of the Royal Astronomical Society (22-02-2022)“…ABSTRACT In this work we use variational inference to quantify the degree of uncertainty in deep learning model predictions of radio galaxy classification. We…”
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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 Galaxy Zoo: using semi-supervised learning to leverage large unlabelled data sets for radio galaxy classification under data set shift
Published in Monthly notices of the Royal Astronomical Society (21-06-2022)“…ABSTRACT In this work, we examine the classification accuracy and robustness of a state-of-the-art semi-supervised learning (SSL) algorithm applied to the…”
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IONONEST—A Bayesian approach to modeling the lower ionosphere
Published in Radio science (01-08-2016)“…Obtaining high‐resolution electron density height profiles for the D region of the ionosphere as a well‐sampled function of time is difficult for most methods…”
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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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Structured variational inference for simulating populations of radio galaxies
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT We present a model for generating postage stamp images of synthetic Fanaroff–Riley Class I and Class II radio galaxies suitable for use in simulations…”
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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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A broad-band flux scale for low-frequency radio telescopes
Published in Monthly notices of the Royal Astronomical Society. Letters (01-06-2012)“…ABSTRACT We present parametrized broad-band spectral models valid at frequencies between 30 and 300 MHz for six bright radio sources selected from the 3C…”
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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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Galaxy Zoo DESI: Detailed morphology measurements for 8.7M galaxies in the DESI Legacy Imaging Surveys
Published in Monthly notices of the Royal Astronomical Society (10-10-2023)“…ABSTRACT We present detailed morphology measurements for 8.67 million galaxies in the DESI Legacy Imaging Surveys (DECaLS, MzLS, and BASS, plus DES). These are…”
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