A Simultaneous Stacking and Deblending Algorithm for Astronomical Images
arXiv:0911.1592 · doi:10.1088/0004-6256/139/4/1592
Abstract
Stacking analysis is a means of detecting faint sources using a priori position information to estimate an aggregate signal from individually undetected objects. Confusion severely limits the effectiveness of stacking in deep surveys with limited angular resolution, particularly at far infrared to submillimeter wavelengths, and causes a bias in stacking results. Deblending corrects measured fluxes for confusion from adjacent sources; however, we find that standard deblending methods only reduce the bias by roughly a factor of two while tripling the variance. We present an improved algorithm for simultaneous stacking and deblending that greatly reduces bias in the flux estimate with nearly minimum variance. When confusion from neighboring sources is the dominant error, our method improves upon RMS error by at least a factor of three and as much as an order of magnitude compared to other algorithms. This improvement will be useful for Herschel and other telescopes working in a source confused, low signal to noise regime.
accepted to The Astronomical Journal. 18 pages, 6 figures
References in corpus (10)
- The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
- The LABOCA Survey of the Extended Chandra Deep Field South
- The Large APEX Bolometer Camera LABOCA
- AzTEC Millimetre Survey of the COSMOS Field: I. Data Reduction and Source Catalogue
- Signals from the Noise: Image Stacking for Quasars in the FIRST Survey
- The star-formation history of K-selected galaxies
- A Public, K-Selected, Optical-to-Near-Infrared Catalog of the Extended Chandra Deep Field South (ECDFS) from the MUltiwavelength Survey by Yale-Chile (MUSYC)
- AEGIS20: a radio survey of the Extended Groth Strip
- Star formation rates in Lyman break galaxies: radio stacking of LBGs in the COSMOS field and the sub-Jy radio source population
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- V. Submillimetre properties of near-infrared--selected galaxies in the Subaru/XMM--Newton deep field
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