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[ascl:2301.028] special: SPEctral Characterization of directly ImAged Low-mass companions

special (SPEctral Characterization of directly ImAged Low-mass companions) characterizes low-mass (M, L, T) dwarfs down to giant planets at optical/IR wavelengths. It can also be used more generally to characterize any type of object with a measured spectrum, provided a relevant input model grid, regardless of the observational method used to obtain the spectrum (direct imaging or not) and regardless of the format of the spectra (multi-band photometry, low-resolution or medium-resolution spectrum, or a combination thereof). It analyzes measured spectra, calculating the spectral correlation between channels of an IFS datacube and empirical spectral indices for MLT-dwarfs. It fits input spectra to either photo-/atmospheric model grids or a blackbody model, including additional parameters such as (extra) black body component(s), extinction and total-to-selective extinction ratio, and can use emcee (ascl:1303.002), nestle (ascl:2103.022), or UltraNest (ascl:1611.001) samplers infer posterior distributions on spectral model parameters in a Bayesian framework, among other tasks.

Code site:
https://github.com/VChristiaens/special
Used in:
https://ui.adsabs.harvard.edu/abs/2022A%26A...664A.139D https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.6117C
Described in:
https://ui.adsabs.harvard.edu/abs/2022JOSS....7.4456C
Bibcode:
2023ascl.soft01028C
Preferred citation method:

Please see citation in formation here: https://github.com/VChristiaens/special#acknowledgements


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ascl:2301.028
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