dc.contributor.author | Tasse, C. | |
dc.contributor.author | Hugo, B. | |
dc.contributor.author | Mirmont, M. | |
dc.contributor.author | Smirnov, O. | |
dc.contributor.author | Atemkeng, M. | |
dc.contributor.author | Bester, L. | |
dc.contributor.author | Bonnassieux, E. | |
dc.contributor.author | Hardcastle, M. J. | |
dc.contributor.author | Lakhoo, R. | |
dc.contributor.author | Girard, J.H.V. | |
dc.contributor.author | Makhathini, S. | |
dc.contributor.author | Perkins, S. | |
dc.contributor.author | Shimwell, Timothy W. | |
dc.date.accessioned | 2018-06-07T16:14:12Z | |
dc.date.available | 2018-06-07T16:14:12Z | |
dc.date.issued | 2018-03-01 | |
dc.identifier.citation | Tasse , C , Hugo , B , Mirmont , M , Smirnov , O , Atemkeng , M , Bester , L , Bonnassieux , E , Hardcastle , M J , Lakhoo , R , Girard , J H V , Makhathini , S , Perkins , S & Shimwell , T W 2018 , ' Faceting for direction-dependent spectral deconvolution ' , Astronomy & Astrophysics , vol. 611 , A87 . https://doi.org/10.1051/0004-6361/201731474 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1712.02078v1 | |
dc.identifier.uri | http://hdl.handle.net/2299/20160 | |
dc.description | Reproduced with permission from Astronomy & Astrophysics, © 2018 ESO. Content in the UH Research Archive is made available for personal research, educational, and non-commercial purposes only. Unless otherwise stated, all content is protected by copyright, and in the absence of an open license, permissions for further re-use should be sought from the publisher, the author, or other copyright holder. | |
dc.description.abstract | The new generation of radio interferometers is characterized by high sensitivity, wide fields of view and large fractional bandwidth. To synthesize the deepest images enabled by the high dynamic range of these instruments requires us to take into account the direction-dependent Jones matrices, while estimating the spectral properties of the sky in the imaging and deconvolution algorithms. In this paper we discuss and implement a wideband wide-field spectral deconvolution framework (ddfacet) based on image plane faceting, that takes into account generic direction-dependent effects. Specifically, we present a wide-field co-planar faceting scheme, and discuss the various effects that need to be taken into account to solve for the deconvolution problem (image plane normalization, position-dependent Point Spread Function, etc). We discuss two wideband spectral deconvolution algorithms based on hybrid matching pursuit and sub-space optimisation respectively. A few interesting technical features incorporated in our imager are discussed, including baseline dependent averaging, which has the effect of improving computing efficiency. The version of ddfacet presented here can account for any externally defined Jones matrices and/or beam patterns. | en |
dc.format.extent | 2092327 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy & Astrophysics | |
dc.subject | Instrumentation: adaptive optics | |
dc.subject | Instrumentation: interferometers | |
dc.subject | Methods: data analysis | |
dc.subject | Techniques: interferometric | |
dc.subject | Astronomy and Astrophysics | |
dc.subject | Space and Planetary Science | |
dc.title | Faceting for direction-dependent spectral deconvolution | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
dc.identifier.url | http://www.scopus.com/inward/record.url?scp=85045518380&partnerID=8YFLogxK | |
rioxxterms.versionofrecord | 10.1051/0004-6361/201731474 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |