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Non-parametric spherical Jeans mass estimation with B-splines

Monthly Notices of the Royal Astronomical Society (2022) 511(4) 5536-5549
DOI: 10.1093/mnras/stac400
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Abstract

Spherical Jeans modelling is widely used to estimate mass profiles of systems from star clusters to galactic stellar haloes to clusters of galaxies. It derives the cumulative mass profile, M(

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Rehemtulla, N., Valluri, M., & Vasiliev, E. (2022). Non-parametric spherical Jeans mass estimation with B-splines. Monthly Notices of the Royal Astronomical Society, 511(4), 5536–5549. https://doi.org/10.1093/mnras/stac400

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