Discovering the Unexpected in Astronomical Survey Data
arXiv:1611.05570 · doi:10.1017/pasa.2016.63
Abstract
Most major discoveries in astronomy are unplanned, and result from surveying the Universe in a new way, rather than by testing a hypothesis or conducting an investigation with planned outcomes. For example, of the 10 greatest discoveries made by the Hubble Space Telescope, only one was listed in its key science goals. So a telescope that merely achieves its stated science goals is not achieving its potential scientific productivity. Several next-generation astronomical survey telescopes are currently being designed and constructed that will significantly expand the volume of observational parameter space, and should in principle discover unexpected new phenomena and new types of object. However, the complexity of the telescopes and the large data volumes mean that these discoveries are unlikely to be found by chance. Therefore, it is necessary to plan explicitly for these unexpected discoveries in the design and construction of the telescope. Two types of discovery are recognised: unexpected objects, and unexpected phenomena. This paper argues that next-generation astronomical surveys require an explicit process for detecting the unexpected, and proposes an implementation of this process. This implementation addresses both types of discovery, and relies heavily on machine-learning techniques, and also on theory-based simulations that encapsulate our current understanding of the Universe to compare with the data.
References in corpus (8)
- A bright millisecond radio burst of extragalactic origin
- Radio sources in the 6dFGS: Local luminosity functions at 1.4 GHz for star-forming galaxies and radio-loud AGN
- Deep ATLAS radio observations of the CDFS-SWIRE field
- The weirdest SDSS galaxies: results from an outlier detection algorithm
- ATLAS 1.4 GHz Data Release 2 -- II. Properties of the faint polarized sky
- Deep 610-MHz Giant Metrewave Radio Telescope observations of the Spitzer extragalactic First Look Survey field - III. The radio properties of Infrared-Faint Radio Sources
- Feature Detection in Radio Astronomy using the Circle Hough Transform
- Serendipity in Astronomy
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- Closing the loop: surveying PIs who have not published their data
- Understanding the human in the design of cyber-human discovery systems for data-driven astronomy