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dc.contributor.authorWright, A. H.
dc.contributor.authorRobotham, A. S G
dc.contributor.authorBourne, N.
dc.contributor.authorDriver, S. P.
dc.contributor.authorDunne, L.
dc.contributor.authorMaddox, S. J.
dc.contributor.authorAlpaslan, M.
dc.contributor.authorAndrews, S. K.
dc.contributor.authorBauer, A. E.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorBrough, S.
dc.contributor.authorBrown, M. J. I.
dc.contributor.authorClarke, C.
dc.contributor.authorCluver, M.
dc.contributor.authorDavies, L. J. M.
dc.contributor.authorGrootes, M. W.
dc.contributor.authorHolwerda, B. W.
dc.contributor.authorHopkins, A. M.
dc.contributor.authorJarrett, T. H.
dc.contributor.authorKafle, P. R.
dc.contributor.authorLange, R.
dc.contributor.authorLiske, J.
dc.contributor.authorLoveday, J.
dc.contributor.authorMoffett, A. J.
dc.contributor.authorNorberg, P.
dc.contributor.authorPopescu, C. C.
dc.contributor.authorSmith, M.
dc.contributor.authorTaylor, E. N.
dc.contributor.authorTuffs, R. J.
dc.contributor.authorWang, L.
dc.contributor.authorWilkins, S. M.
dc.date.accessioned2016-08-04T14:30:07Z
dc.date.available2016-08-04T14:30:07Z
dc.date.issued2016-07-21
dc.identifier.citationWright , A H , Robotham , A S G , Bourne , N , Driver , S P , Dunne , L , Maddox , S J , Alpaslan , M , Andrews , S K , Bauer , A E , Bland-Hawthorn , J , Brough , S , Brown , M J I , Clarke , C , Cluver , M , Davies , L J M , Grootes , M W , Holwerda , B W , Hopkins , A M , Jarrett , T H , Kafle , P R , Lange , R , Liske , J , Loveday , J , Moffett , A J , Norberg , P , Popescu , C C , Smith , M , Taylor , E N , Tuffs , R J , Wang , L & Wilkins , S M 2016 , ' Galaxy And Mass Assembly : accurate panchromatic photometry from optical priors using LAMBDAR ' Monthly Notices of the Royal Astronomical Society , vol. 460 , no. 1 , pp. 765-801 . https://doi.org/10.1093/mnras/stw832en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 244761492
dc.identifier.otherPURE UUID: d03ba558-d2e3-4a63-914d-9db5a50a5886
dc.identifier.otherScopus: 84979059335
dc.identifier.urihttp://hdl.handle.net/10023/9260
dc.descriptionAHW and SKA are supported by the Australian Government’s Department of Industry Australian Postgraduate Award (APA). SB acknowledges funding support from the Australian Research Council through a Future Fellowship (FT140101166). LD and SJM acknowledge support from the ERC in the form of the Advanced Investigator Program, COSMICISM, and the ERC Consolidator Grant CosmicDust. NB acknowledges funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 312725.en
dc.description.abstractWe present the Lambda Adaptive Multi-Band Deblending Algorithm in R (LAMBDAR), a novel code for calculating matched aperture photometry across images that are neither pixel- nor PSF-matched, using prior aperture definitions derived from high-resolution optical imaging. The development of this program is motivated by the desire for consistent photometry and uncertainties across large ranges of photometric imaging, for use in calculating spectral energy distributions. We describe the program, specifically key features required for robust determination of panchromatic photometry: propagation of apertures to images with arbitrary resolution, local background estimation, aperture normalization, uncertainty determination and propagation, and object deblending. Using simulated images, we demonstrate that the program is able to recover accurate photometric measurements in both high-resolution, low-confusion, and low-resolution, high-confusion, regimes. We apply the program to the 21-band photometric data set from the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR; Driver et al. 2016), which contains imaging spanning the far-UV to the far-IR. We compare photometry derived from LAMBDAR with that presented in Driver et al. (2016), finding broad agreement between the data sets. None the less, we demonstrate that the photometry from LAMBDAR is superior to that from the GAMA PDR, as determined by a reduction in the outlier rate and intrinsic scatter of colours in the LAMBDAR data set. We similarly find a decrease in the outlier rate of stellar masses and star formation rates using LAMBDAR photometry. Finally, we note an exceptional increase in the number of UV and mid-IR sources able to be constrained, which is accompanied by a significant increase in the mid-IR colour-colour parameter-space able to be explored.
dc.format.extent37
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://dx.doi.org/10.1093/mnras/stw832en
dc.subjectAstronomical data bases: miscellaneousen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: generalen
dc.subjectGalaxies: photometryen
dc.subjectTechniques: photometricen
dc.subjectQB Astronomyen
dc.subjectSpace and Planetary Scienceen
dc.subjectAstronomy and Astrophysicsen
dc.subjectDASen
dc.subject.lccQBen
dc.titleGalaxy And Mass Assembly : accurate panchromatic photometry from optical priors using LAMBDARen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stw832
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/1604.01923v2
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84979059335&partnerID=8YFLogxK


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