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19962023
most citedBlazars in the Fermi Era: The OVRO 40-m Telescope Monitoring Program

549 citations · 5.8k across the 130 of their papers we have counts for

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Showing 2017Show all

12 papers · 1 filter

astro-ph.GA2017★ 2 cited

AMI-LA Observations of the SuperCLASS Super-cluster

C. J. Riseley, K. J. B. Grainge, Y. C. Perrott +21

We present a deep survey of the SuperCLASS super-cluster - a region of sky known to contain five Abell clusters at redshift - performed using the Arcminute Microkelvin I…

astro-ph.GA2017★ 2 cited

AMI-CL J0300+2613: a Galactic anomalous-microwave-emission ring masquerading as a galaxy cluster

Yvette C. Perrott, Therese M. Cantwell, Steve H. Carey +17

The Arcminute Microkelvin Imager (AMI) carried out a blind survey for galaxy clusters via their Sunyaev-Zel'dovich effect decrements between 2008 and 2011. The first detection, kno…

astro-ph.IM2017★ 86 cited

A Digital Correlator Upgrade for the Arcminute MicroKelvin Imager

Jack Hickish, Nima Razavi-Ghods, Yvette C. Perrott +18

The Arcminute Microkelvin Imager (AMI) telescopes located at the Mullard Radio Astronomy Observatory near Cambridge have been significantly enhanced by the implementation of a new…

physics.ins-det2017★ 1 cited

Stabilized Modulated Photonic Signal Transfer Over 186 km of Aerial Fiber

David Gozzard, Sascha Schediwy, Bruce Wallace +2

Aerial suspended optical-fiber links are being considered as economical alternatives to buried links for long-distance transfer of coherent time and frequency signals. We present s…

astro-ph.CO2017★ 7 cited

AMI SZ observation of galaxy-cluster merger CIZA J2242+5301: perpendicular flows of gas and dark matter

Clare Rumsey, Yvette C. Perrott, Malak Olamaie +5

AMI observations towards CIZA J2242+5301, in comparison with observations of weak gravitational lensing and X-ray emission from the literature, are used to investigate the behaviou…

astro-ph.CO2017★ 11 cited

Free-form modelling of galaxy clusters: a Bayesian and data-driven approach

Malak Olamaie, Michael P. Hobson, Farhan Feroz +5

A new method is presented for modelling the physical properties of galaxy clusters. Our technique moves away from the traditional approach of assuming specific parameterised functi…