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dc.contributor.authorAndrews, S.K.
dc.contributor.authorKelvin, L.S.
dc.contributor.authorDriver, S.P.
dc.contributor.authorRobotham, A.S.G.
dc.date.accessioned2014-09-17T11:01:01Z
dc.date.available2014-09-17T11:01:01Z
dc.date.issued2013-01-01
dc.identifier.citationAndrews , S K , Kelvin , L S , Driver , S P & Robotham , A S G 2013 , ' Detection, size, measurement, and structural analysis limits for the 2MASS, UKIDSS-LAS, and VISTA VIKING surveys ' , Publications of the Astronomical Society of Australia , vol. 31 , no. 1 , e004 . https://doi.org/10.1017/pasa.2013.41en
dc.identifier.issn1323-3580
dc.identifier.otherPURE: 149113053
dc.identifier.otherPURE UUID: 7e7dbf62-d074-40d7-8280-f9df893d2e96
dc.identifier.otherScopus: 84891813082
dc.identifier.urihttps://hdl.handle.net/10023/5439
dc.descriptionSKA is supported by a summer scholarship provided by the School of Physics at UWA. LSK is supported by the Austrian Science Foundation FWF under grantSKA is supported by a summer scholarship provided by the School of Physics at UWA. LSK is supported by the Austrian Science Foundation FWF under grant P23946..en
dc.description.abstractThe 2MASS, UKIDSS-LAS, and VISTA VIKING surveys have all now observed the GAMA 9hr region in the Ks band. Here we compare the detection rates, photometry, basic size measurements, and single-component GALFIT structural measurements for a sample of 37 591 galaxies. We explore the sensitivity limits where the data agree for a variety of issues including: detection, star-galaxy separation, photometric measurements, size and ellipticity measurements, and Sérsic measurements. We find that 2MASS fails to detect at least 20% of the galaxy population within all magnitude bins, however for those that are detected we find photometry is robust (± 0.2 mag) to 14.7 AB mag and star-galaxy separation to 14.8 AB mag. For UKIDSS-LAS we find incompleteness starts to enter at a flux limit of 18.9 AB mag, star-galaxy separation is robust to 16.3 AB mag, and structural measurements are robust to 17.7 AB mag. VISTA VIKING data are complete to approximately 20.0 AB mag and structural measurements appear robust to 18.8 AB mag.
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australiaen
dc.rightsCopyright © Astronomical Society of Australia 2014en
dc.subjectGalaxies: fundamental parametersen
dc.subjectInfrared: galaxiesen
dc.subjectSurveysen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleDetection, size, measurement, and structural analysis limits for the 2MASS, UKIDSS-LAS, and VISTA VIKING surveysen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1017/pasa.2013.41
dc.description.statusPeer revieweden


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