activity
19992018
most citedThe Arcminute Microkelvin Imager

246 citations · 2.1k across the 57 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

12 papers · 1 filter

astro-ph.GA2018

9C spectral-index distributions and source-count estimates from 15 to 93 GHz - a re-assessment

E. M. Waldram, R. C. Bolton, J. M. Riley +1

In an earlier paper (2007), we used follow-up observations of a sample of sources from the 9C survey at 15.2 GHz to derive a set of spectral-index distributions up to a frequency o…

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.GA2016★ 19 cited

10C continued: a deeper radio survey at 15.7 GHz

I. H. Whittam, J. M. Riley, D. A. Green +5

We present deep 15.7-GHz observations made with the Arcminute Microkelvin Imager Large Array in two fields previously observed as part of the Tenth Cambridge (10C) survey. These ob…

astro-ph.GA2013★ 21 cited

Deep 20-GHz survey of the Chandra Deep Field South and SDSS Stripe 82: source catalogue and spectral properties

T. M. O. Franzen, E. M. Sadler, R. Chhetri +6

We present a source catalogue and first results from a deep, blind radio survey carried out at 20 GHz with the Australia Telescope Compact Array, with follow-up observations at 5.5…

astro-ph.GA2012★ 60 cited

AMI Galactic Plane Survey at 16 GHz: I -- Observing, mapping and source extraction

AMI Consortium, :, Yvette C. Perrott +18

The AMI Galactic Plane Survey (AMIGPS) is a large area survey of the outer Galactic plane to provide arcminute resolution images at milli-Jansky sensitivity in the centimetre-wave…

astro-ph.GA2011★ 3 cited

AMI observations of unmatched Planck ERCSC LFI sources at 15.75 GHz

AMI Consortium, :, Yvette C. Perrott +17

The Planck Early Release Compact Source Catalogue includes 26 sources with no obvious matches in other radio catalogues (of primarily extragalactic sources). Here we present observ…

astro-ph.GA2011★ 19 cited

AMI-LA radio continuum observations of Spitzer c2d small clouds and cores: Perseus region

Anna M. M. Scaife, Jennifer Hatchell, Matthew Davies +15

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 programme at a wavel…

astro-ph.GA2010★ 13 cited

AMI Large Array radio continuum observations of Spitzer c2d small clouds and cores

Anna M. M. Scaife, Emily I. Curtis, Matthew Davies +15

We perform deep 1.8 cm radio continuum imaging towards thirteen protostellar regions selected from the Spitzer c2d small clouds and cores programme at high resolution (25") in orde…

astro-ph.GA2009★ 21 cited

High resolution AMI Large Array imaging of spinning dust sources: spatially correlated 8 micron emission and evidence of a stellar wind in L675

Anna M. M. Scaife, David A. Green, Guy G. Pooley +15

We present 25 arcsecond resolution radio images of five Lynds Dark Nebulae (L675, L944, L1103, L1111 & L1246) at 16 GHz made with the Arcminute Microkelvin Imager (AMI) Large Array…

astro-ph.GA2009★ 37 cited

AMI observations of Lynds Dark Nebulae: further evidence for anomalous cm-wave emission

Anna M. M. Scaife, Natasha Hurley-Walker, David A. Green +13

Observations at 14.2 to 17.9 GHz made with the AMI Small Array towards fourteen Lynds Dark Nebulae with a resolution of 2' are reported. These sources are selected from the SCUBA o…

astro-ph.GA2009★ 7 cited

G64.5+0.9, a new shell supernova remnant with unusual central emission

AMI Consortium, :, Natasha Hurley-Walker +15

We present observations between 1.4 and 18 GHz confirming that G64.5+0.9 is new Galactic shell supernova remnant, using the Very Large Array and the Arcminute Microkelvin Imager. T…

astro-ph.GA2009★ 35 cited

AMI observations of northern supernova remnants at 14-18 GHz

Natasha Hurley-Walker, A. M. M. Scaife, D. A. Green +12

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 conjunction with data…