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Detection, size, measurement, and structural analysis limits for the 2MASS, UKIDSS-LAS, and VISTA VIKING surveys

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Kelvin_2014_ASA_Detection.pdf (4.361Mb)
Date
01/01/2013
Author
Andrews, S.K.
Kelvin, L.S.
Driver, S.P.
Robotham, A.S.G.
Keywords
Galaxies: fundamental parameters
Infrared: galaxies
Surveys
QB Astronomy
QC Physics
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Abstract
The 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.
Citation
Andrews , 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.2013.41
Publication
Publications of the Astronomical Society of Australia
Status
Peer reviewed
DOI
https://doi.org/10.1017/pasa.2013.41
ISSN
1323-3580
Type
Journal article
Rights
Copyright © Astronomical Society of Australia 2014
Description
SKA 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..
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  • Physics & Astronomy Research
  • University of St Andrews Research
URI
http://hdl.handle.net/10023/5439

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