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spelling ftdatacite:10.48550/arxiv.1407.5237 2023-05-15T18:10:50+02:00 The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes Sharp, R. Allen, J. T. Fogarty, L. M. R. Croom, S. M. Cortese, L. Green, A. W. Nielsen, J. Richards, S. N. Scott, N. Taylor, E. N. Barnes, L. A. Bauer, A. E. Birchall, M. Bland-Hawthorn, J. Bloom, J. V. Brough, S. Bryant, J. J. Cecil, G. N. Colless, M. Couch, W. J. Drinkwater, M. J. Driver, S. Foster, C. Goodwin, M. Gunawardhana, M. L. P. Ho, I. -T. Hampton, E. J. Hopkins, A. M. Jones, H. Konstantopoulos, I. S. Lawrence, J. S. Leslie, S. K. Lewis, G. F. Liske, J. Lopez-Sanchez, A. R. Lorente, N. P. F. McElroy, R. Medling, A. M. Mahajan, S. Mould, J. Parker, Q. Pracy, M. B. Obreschkow, D. Owers, M. S. Schaefer, A. L. Sweet, S. M Thomas, A. Tonini, C. Walcher, C. J. 2014 https://dx.doi.org/10.48550/arxiv.1407.5237 https://arxiv.org/abs/1407.5237 unknown arXiv https://dx.doi.org/10.1093/mnras/stu2055 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM Astrophysics of Galaxies astro-ph.GA FOS Physical sciences article-journal Article ScholarlyArticle Text 2014 ftdatacite https://doi.org/10.48550/arxiv.1407.5237 https://doi.org/10.1093/mnras/stu2055 2022-04-01T12:53:05Z We present a methodology for the regularisation and combination of sparse sampled and irregularly gridded observations from fibre-optic multi-object integral-field spectroscopy. The approach minimises interpolation and retains image resolution on combining sub-pixel dithered data. We discuss the methodology in the context of the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) Galaxy Survey underway at the Anglo-Australian Telescope. The SAMI instrument uses 13 fibre bundles to perform high-multiplex integral-field spectroscopy across a one degree diameter field of view. The SAMI Galaxy Survey is targeting 3000 galaxies drawn from the full range of galaxy environments. We demonstrate the subcritical sampling of the seeing and incomplete fill factor for the integral-field bundles results in only a 10% degradation in the final image resolution recovered. We also implement a new methodology for tracking covariance between elements of the resulting datacubes which retains 90% of the covariance information while incurring only a modest increase in the survey data volume. : 17 pages, 10 figures, Accepted MNRAS September 2014 Text sami DataCite Metadata Store (German National Library of Science and Technology)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Instrumentation and Methods for Astrophysics astro-ph.IM
Astrophysics of Galaxies astro-ph.GA
FOS Physical sciences
spellingShingle Instrumentation and Methods for Astrophysics astro-ph.IM
Astrophysics of Galaxies astro-ph.GA
FOS Physical sciences
Sharp, R.
Allen, J. T.
Fogarty, L. M. R.
Croom, S. M.
Cortese, L.
Green, A. W.
Nielsen, J.
Richards, S. N.
Scott, N.
Taylor, E. N.
Barnes, L. A.
Bauer, A. E.
Birchall, M.
Bland-Hawthorn, J.
Bloom, J. V.
Brough, S.
Bryant, J. J.
Cecil, G. N.
Colless, M.
Couch, W. J.
Drinkwater, M. J.
Driver, S.
Foster, C.
Goodwin, M.
Gunawardhana, M. L. P.
Ho, I. -T.
Hampton, E. J.
Hopkins, A. M.
Jones, H.
Konstantopoulos, I. S.
Lawrence, J. S.
Leslie, S. K.
Lewis, G. F.
Liske, J.
Lopez-Sanchez, A. R.
Lorente, N. P. F.
McElroy, R.
Medling, A. M.
Mahajan, S.
Mould, J.
Parker, Q.
Pracy, M. B.
Obreschkow, D.
Owers, M. S.
Schaefer, A. L.
Sweet, S. M
Thomas, A.
Tonini, C.
Walcher, C. J.
The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
topic_facet Instrumentation and Methods for Astrophysics astro-ph.IM
Astrophysics of Galaxies astro-ph.GA
FOS Physical sciences
description We present a methodology for the regularisation and combination of sparse sampled and irregularly gridded observations from fibre-optic multi-object integral-field spectroscopy. The approach minimises interpolation and retains image resolution on combining sub-pixel dithered data. We discuss the methodology in the context of the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) Galaxy Survey underway at the Anglo-Australian Telescope. The SAMI instrument uses 13 fibre bundles to perform high-multiplex integral-field spectroscopy across a one degree diameter field of view. The SAMI Galaxy Survey is targeting 3000 galaxies drawn from the full range of galaxy environments. We demonstrate the subcritical sampling of the seeing and incomplete fill factor for the integral-field bundles results in only a 10% degradation in the final image resolution recovered. We also implement a new methodology for tracking covariance between elements of the resulting datacubes which retains 90% of the covariance information while incurring only a modest increase in the survey data volume. : 17 pages, 10 figures, Accepted MNRAS September 2014
format Text
author Sharp, R.
Allen, J. T.
Fogarty, L. M. R.
Croom, S. M.
Cortese, L.
Green, A. W.
Nielsen, J.
Richards, S. N.
Scott, N.
Taylor, E. N.
Barnes, L. A.
Bauer, A. E.
Birchall, M.
Bland-Hawthorn, J.
Bloom, J. V.
Brough, S.
Bryant, J. J.
Cecil, G. N.
Colless, M.
Couch, W. J.
Drinkwater, M. J.
Driver, S.
Foster, C.
Goodwin, M.
Gunawardhana, M. L. P.
Ho, I. -T.
Hampton, E. J.
Hopkins, A. M.
Jones, H.
Konstantopoulos, I. S.
Lawrence, J. S.
Leslie, S. K.
Lewis, G. F.
Liske, J.
Lopez-Sanchez, A. R.
Lorente, N. P. F.
McElroy, R.
Medling, A. M.
Mahajan, S.
Mould, J.
Parker, Q.
Pracy, M. B.
Obreschkow, D.
Owers, M. S.
Schaefer, A. L.
Sweet, S. M
Thomas, A.
Tonini, C.
Walcher, C. J.
author_facet Sharp, R.
Allen, J. T.
Fogarty, L. M. R.
Croom, S. M.
Cortese, L.
Green, A. W.
Nielsen, J.
Richards, S. N.
Scott, N.
Taylor, E. N.
Barnes, L. A.
Bauer, A. E.
Birchall, M.
Bland-Hawthorn, J.
Bloom, J. V.
Brough, S.
Bryant, J. J.
Cecil, G. N.
Colless, M.
Couch, W. J.
Drinkwater, M. J.
Driver, S.
Foster, C.
Goodwin, M.
Gunawardhana, M. L. P.
Ho, I. -T.
Hampton, E. J.
Hopkins, A. M.
Jones, H.
Konstantopoulos, I. S.
Lawrence, J. S.
Leslie, S. K.
Lewis, G. F.
Liske, J.
Lopez-Sanchez, A. R.
Lorente, N. P. F.
McElroy, R.
Medling, A. M.
Mahajan, S.
Mould, J.
Parker, Q.
Pracy, M. B.
Obreschkow, D.
Owers, M. S.
Schaefer, A. L.
Sweet, S. M
Thomas, A.
Tonini, C.
Walcher, C. J.
author_sort Sharp, R.
title The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
title_short The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
title_full The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
title_fullStr The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
title_full_unstemmed The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
title_sort sami galaxy survey: cubism and covariance, putting round pegs into square holes
publisher arXiv
publishDate 2014
url https://dx.doi.org/10.48550/arxiv.1407.5237
https://arxiv.org/abs/1407.5237
genre sami
genre_facet sami
op_relation https://dx.doi.org/10.1093/mnras/stu2055
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1407.5237
https://doi.org/10.1093/mnras/stu2055
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