Detection, Size, Measurement, and Structural Analysis Limits for the 2MASS, UKIDSS-LAS, and VISTA VIKING Surveys

Author:

Andrews Stephen K.,Kelvin Lee S.,Driver Simon P.,Robotham Aaron S. G.

Abstract

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.

Publisher

Cambridge University Press (CUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Galaxy and Mass Assembly (GAMA): variation in galaxy structure across the green valley;Monthly Notices of the Royal Astronomical Society;2018-04-14

2. ProFound: Source Extraction and Application to Modern Survey Data;Monthly Notices of the Royal Astronomical Society;2018-02-23

3. Searching for Extragalactic Sources in the VISTA Variables in the Vía Láctea Survey;The Astronomical Journal;2018-01-03

4. ProFit: Bayesian profile fitting of galaxy images;Monthly Notices of the Royal Astronomical Society;2016-11-23

5. Hyper-luminous dust-obscured galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE;Publications of the Astronomical Society of Japan;2015-07-12

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