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dc.contributor.authorPerrott, Y.
dc.contributor.authorScaif, A.
dc.contributor.authorGreen, D.
dc.contributor.authorGrainge, K.
dc.contributor.authorHurley-Walker, Natasha
dc.contributor.authorJin, T.
dc.contributor.authorRumsey, C.
dc.contributor.authorTitterington, D.
dc.date.accessioned2017-01-30T12:42:09Z
dc.date.available2017-01-30T12:42:09Z
dc.date.created2016-01-12T20:00:21Z
dc.date.issued2015
dc.identifier.citationPerrott, Y. and Scaif, A. and Green, D. and Grainge, K. and Hurley-Walker, N. and Jin, T. and Rumsey, C. et al. 2015. AMI galactic plane survey at 16 GHz - II. Full data release with extended coverage and improved processing. Monthly Notices of the Royal Astronomical Society. 453 (2): pp. 1396-1403.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/24310
dc.identifier.doi10.1093/mnras/stv1728
dc.description.abstract

The Arcminute Microkelvin Imager Galactic Plane Survey provides mJy-sensitivity, arcminute-resolution interferometric images of the northern Galactic plane at ≈16 GHz. The first data release covered 76° < ≈ l < ≈ 170° between latitudes of |b| < ≈ 5°; here we present a second data release, extending the coverage to 53° < ≈ l < ≈ 193° and including high-latitude extensions to cover the Taurus and California giant molecular cloud regions, and the recently discovered large supernova remnant G159.6+7.3. The total coverage is now 1777 deg2 and the catalogue contains 6509 sources. We also describe the improvements to the data processing pipeline which improves the positional and flux density accuracies of the survey.

dc.titleAMI galactic plane survey at 16 GHz - II. Full data release with extended coverage and improved processing
dc.typeJournal Article
dcterms.source.volume453
dcterms.source.number2
dcterms.source.startPage1396
dcterms.source.endPage1403
dcterms.source.issn0035-8711
dcterms.source.titleMonthly Notices of the Royal Astronomical Society
curtin.note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved

curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


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