The fourth UltraVISTA data release

A. Moneti,H. J. McCracken, P. Hudelot, S. Rouberol, O. Herent, Y. Mellier,O. Le Fèvre,J. Fynbo, R. Bowler,K. Caputi, O. Kauffmann,C. Gonzalez-Fernandez,E. Gonzalez-Solares, M. Irwin, J. Lewis, R. Blake,N. Cross, M. Read

semanticscholar(2019)

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摘要
DR4 was built from the pre-processed UltraVISTA images from CASU (“The Cambridge Astronomy Survey Unit”1) observed at VISTA from 4 December, 2009 to 29 June, 2016 as available in early 2017. We downloaded 63,931 individual images. After quality control (which mainly is a rejection of images with FWHM > 1.0′′ or ellipticity > 0.1, see Sect. 4.1), we were left with 58,138 individual images that were used to create the 5 stacks for the 5 bands: Y , J , H, Ks, and NB118. The observation dates of all the individual images used can be found by inspecting the file names of the individual images which are recorded in the provenance tables
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