Point source detection and extraction from simulated Planck time-ordered data using optimal adaptive filters
Wavelet-related techniques have proven useful in the processing and analysis of one- and two-dimensional data sets (spectra in the former case, images in the latter). In this work we apply adaptive filters, introduced in a previous work, to optimize the detection and extraction of point sources from...
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2002 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/394112 |
| Acceso en línea: | http://hdl.handle.net/10261/394112 |
| Access Level: | acceso abierto |
| Palabra clave: | Methods: data analysis Cosmic microwave background |
| Sumario: | Wavelet-related techniques have proven useful in the processing and analysis of one- and two-dimensional data sets (spectra in the former case, images in the latter). In this work we apply adaptive filters, introduced in a previous work, to optimize the detection and extraction of point sources from a one-dimensional array of time-ordered data such as the one that will be produced by the future 30-GHz LFI28 channel of the ESA Planck mission. At a 4σ detection level, 224 sources over a flux of 0.88 Jy are detected with a mean relative error (in absolute value) of 21 per cent and a systematic bias of −7.7 per cent. The position of the sources in the sky is determined with errors inferior to the size of the pixel. The catalogue of detected sources is complete at fluxes ⩾4.3 Jy. The number of spurious detections is less than 10 per cent of the true detections. We compared the results with the ones obtained by filtering with a Gaussian filter and a Mexican Hat Wavelet of width equal to the scale of the sources. The adaptive filter outperforms the other filters in all considered cases. We conclude that optimal adaptive filters are well suited to detect and extract sources with a given profile embedded in a background of known statistical properties. In the Planck case, they could be useful to obtain a real-time preliminary catalogue of extragalactic sources, which would have a great scientific interest, e.g. for follow-up observations. |
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