The completeness and reliability of threshold and false-discovery-rate source extraction algorithms for compact continuum sources
arXiv:1112.1168 · doi:10.1071/AS11026
Abstract
The process of determining the number and characteristics of sources in astronomical images is so fundamental to a large range of astronomical problems that it is perhaps surprising that no standard procedure has ever been defined that has well understood properties with a high degree of statistical rigour on completeness and reliability. There are now a large number of commonly used software tools for accomplishing this task, typically with different tools being used for images acquired using different technologies. Despite this, there have been relatively few quantitative analyses of the robustness or reliability of individual tools, or the details of the techniques they implement. We have an opportunity to redress this omission in the context of surveys planned with the Australian Square Kilometre Array Pathfinder (ASKAP). The Evolutionary Map of the Universe (EMU) survey with ASKAP, a continuum survey of the Southern Hemisphere up to declination +30 deg, aims to utilise an automated source identification and measurement approach that is demonstrably optimal, to maximise the reliability, utility and robustness of the resulting radio source catalogues. A key stage in source extraction methods is the background estimation (background level and noise level) and the choice of a threshold high enough to reject false sources yet not so high that the catalogues are significantly incomplete. In this analysis we present results from testing such algorithms as implemented in the SExtractor, Selavy (Duchamp), and sfind tools on simulated data. In particular the effects of background estimation, threshold and false-discovery rate settings are explored. For parameters that give similar completeness, the false-discovery rate method employed by sfind results in a more reliable catalogue compared to the peak threshold methods of SExtractor and Selavy.
17 pages, 13 figures, accepted by PASA
References in corpus (4)
Cited by in corpus (16)
- Source finding in the era of the SKA (precursors): Aegean 2.0
- The Caltech-NRAO Stripe 82 Survey (CNSS) Paper I: The Pilot Radio Transient Survey In 50 deg
- Radio Continuum Surveys with Square Kilometre Array Pathfinders
- ATLAS - I. Third Release of 1.4 GHz Mosaics and Component Catalogues
- Sensitive Search For Radio Variables And Transients In The Extended Chandra Deep-Field South
- The ASKAP/EMU Source Finding Data Challenge
- Deep 3 GHz Observations of the Lockman Hole North with the Very Large Array - 1. Source extraction and uncertainty analysis
- The ATLAS 5.5 GHz Survey of the Extended Chandra Deep Field South: The Second Data Release
- Automated detection of extended sources in radio maps: progress from the SCORPIO survey
- The ATLAS 5.5 GHz survey of the Extended Chandra Deep Field South: Catalogue, Source Counts and Spectral Indices
- The Co-Ordinated Radio and Infrared Survey for High-Mass Star Formation. V. The CORNISH-South Survey and Catalogue
- The ATLAS 9.0 GHz Survey of the Extended Chandra Deep Field South: The Faint 9.0 GHz Radio Population
- Hydra I: An extensible multi-source-finder comparison and cataloguing tool
- Astroinformatics Challenges from Next-generation Radio Continuum Surveys
- Point Proposal Network: Accelerating Point Source Detection Through Deep Learning
- Ca2+ transient detection and segmentation with the Astronomically motivated algorithm for Background Estimation And Transient Segmentation (Astro-BEATS)