VISTA Science Verification — The Galactic and Extragalactic Mini-surveys

Author(s)
M. Arnaboldi, M. Petr-Gotzens, M. Rejkuba, M. Neeser, T. Szeifert, V. D. Ivanov, W. Hummel, M. Hilker, N. Neumayer, P. Møller, K. Nilsson, B. Venemans, E. Hatziminaoglou, G. Hussain, T. Stanke, P. Teixeira, S. Ramsay, J. Retzlaff, R. Slijkhuis, F. Comerón, J. Melnick, M. Romaniello, J. Emerson, W. Sutherland, M. Irwin, J. Lewis, S. Hodgkin, E. Gonzales-Solares
Abstract

The Visible and Infrared Survey Telescope for Astronomy (VISTA) will be mostly dedicated to the execution of ESO public surveys, requiring large amounts of service observing time. VISTA Science Verification (SV) thus differs from that usually implemented for other VLT instruments. VISTASV consisted of two self-contained mini-surveys: a Galactic mini-surveyin the region around the Orion Belt stars; and a deep extragalactic mini-survey of the nearby spiral galaxy NGC 253. ESO astronomers used these mini-surveys as benchmarks to optimise the survey operation procedures, minimise overheads, and experience the full end-to-end process of survey data acquisition. The raw data and associated calibrations from both mini-surveys were released in December 2009, and the reduced images and catalogues will soon be available, enabling the first exciting science with VISTA.

Organisation(s)
Department of Astrophysics
External organisation(s)
Queen Mary University of London, University of Cambridge, European Southern Observatory (Germany), Joint ALMA Observatory
Journal
The Messenger
Volume
139
Pages
6-11
ISSN
0722-6691
Publication date
03-2010
Austrian Fields of Science 2012
103004 Astrophysics
Portal url
https://ucrisportal.univie.ac.at/en/publications/65ca5348-f4bf-46e2-99ca-ced69a482ab0