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[ascl:1805.019] HENDRICS: High ENergy Data Reduction Interface from the Command Shell

HENDRICS, a rewrite and update to MaLTPyNT (ascl:1502.021), contains command-line scripts based on Stingray (ascl:1608.001) to perform a quick-look (spectral-)timing analysis of X-ray data, treating the gaps in the data due, e.g., to occultation from the Earth or passages through the SAA, properly. Despite its original main focus on NuSTAR, HENDRICS can perform standard aperiodic timing analysis on X-ray data from, in principle, any other satellite, and its features include power density and cross spectra, time lags, pulsar searches with the Epoch folding and the Z_n^2 statistics, color-color and color-intensity diagrams. The periodograms produced by HENDRICS (such as a power density spectrum or a cospectrum) can be saved in a format compatible with XSPEC (ascl:9910.005) or ISIS (ascl:1302.002).

Code site:
https://github.com/StingraySoftware/HENDRICS https://hendrics.stingray.science/en/stable/
Used in:
https://ui.adsabs.harvard.edu/abs/2018ApJ...853L..21B
Bibcode:
2018ascl.soft05019B
Preferred citation method:

https://ui.adsabs.harvard.edu/abs/2015ascl.soft02021B ; if you use the cospectrum, please also refer to https://ui.adsabs.harvard.edu/abs/2015ApJ...800..109B


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ascl:1805.019
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