Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 421, Issue 3, Pages 1825-1837Publisher
WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2011.19813.x
Keywords
methods: data analysis; techniques: image processing; techniques: photometric
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Funding
- ESA [PECS 98073]
- Hungarian Academy of Sciences
- HATNet project
- NASA [NNG04GN74G, NNX08AF23G]
- SAO IRD
- NASA [102326, NNX08AF23G] Funding Source: Federal RePORTER
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In this paper we describe the main features of the software package named fitsh, intended to provide a standalone environment for analysis of data acquired by imaging astronomical detectors. The package both provides utilities for the full pipeline of subsequent related data-processing steps (including image calibration, astrometry, source identification, photometry, differential analysis, low-level arithmetic operations, multiple-image combinations, spatial transformations and interpolations) and aids the interpretation of the (mainly photometric and/or astrometric) results. The package also features a consistent implementation of photometry based on image subtraction, point spread function fitting and aperture photometry and provides easy-to-use interfaces for comparisons and for picking the most suitable method for a particular problem. The set of utilities found in this package is built on top of the commonly used UNIX/POSIX shells (hence the name of the package); therefore, both frequently used and well-documented tools for such environments can be exploited and managing a massive amount of data is rather convenient.
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