Multiwavelength astronomy and big data
Two major characteristics of modern astronomy are multiwavelength (MW) studies (fromγ-ray to radio) and big data (data acquisition, storage and analysis). Present astronomical databases and archives contain billions of objects observed at various wavelengths, both galactic and extragalactic, and the...
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Veröffentlicht in: | Astronomy reports 2016-09, Vol.60 (9), p.857-877 |
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description | Two major characteristics of modern astronomy are multiwavelength (MW) studies (fromγ-ray to radio) and big data (data acquisition, storage and analysis). Present astronomical databases and archives contain billions of objects observed at various wavelengths, both galactic and extragalactic, and the vast amount of data on them allows new studies and discoveries. Astronomers deal with big numbers. Surveys are the main source for discovery of astronomical objects and accumulation of observational data for further analysis, interpretation, and achieving scientific results. We review the main characteristics of astronomical surveys, compare photographic and digital eras of astronomical studies (including the development of wide-field observations), describe the present state of MW surveys, and discuss the Big Data in astronomy and related topics of Virtual Observatories and Computational Astrophysics. The review includes many numbers and data that can be compared to have a possibly overall understanding on the Universe, cosmic numbers and their relationship to modern computational facilities. |
doi_str_mv | 10.1134/S1063772916090043 |
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subjects | Astronomical bodies Astronomy Computational astrophysics Data acquisition Data management Digital Observations and Techniques Physics Physics and Astronomy Sky surveys (astronomy) Studies Universe Wavelengths |
title | Multiwavelength astronomy and big data |
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