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Agama reference documentation

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arxiv 1802.08255 v2 pith:ORCEBJP7 submitted 2018-02-22 astro-ph.IM astro-ph.GA

classification astro-ph.IMastro-ph.GA
keywords galaxylibraryactionagamaangledatadensitydynamics
verification ladder T0 review T1 audit T2 compute T3 formal
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Agama (Action-based Galaxy Modelling Architecture) is a software library intended for a broad range of tasks within the field of stellar dynamics. As the name suggests, it is centered around the use of action/angle formalism to describe the structure of stellar systems, but this is only one of its many facets. The library contains a powerful framework for dealing with arbitrary density/potential profiles and distribution functions (analytic, extracted from N-body models, or fitted to the data), a vast collection of general-purpose mathematical routines, and covers many aspects of galaxy dynamics up to the very high-level interface for constructing self-consistent galaxy models. This document serves two purposes. First of all, this is a detailed reference for the library itself. Second, it describes various mathematical and numerical methods that could be applicable in a broader context. These include: (1) one- and multidimensional interpolation using cubic and quintic splines; (2) penalized spline fitting of noisy data and penalized spline density estimation; (3) adaptive rejection sampling from multidimensional probability distributions; (4) computation of gravitational potentials using spherical- and azimuthal-harmonic expansions; (5) Staeckel fudge method for computing action/angle variables; (6) a general discussion about good programming practices.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Weighing the Milky Way's Satellite Galaxies Using Pulsar Accelerations

    astro-ph.GA 2025-12 conditional novelty 7.0 of 10

    The LMC weighs 4.1±1.0×10^10 M_sun within 16.6 kpc and Sagittarius 3.5±2.4×10^8 M_sun within 5 kpc, measured from pulsar accelerations alone.

  2. Dynamical Models of the Milky Way in Action Space with LAMOST DR8 and GAIA EDR3

    astro-ph.GA 2025-02 conditional novelty 6.0 of 10

    A best-fit action-based model of the Milky Way from K giant kinematics gives a virial mass of about 1.3 x 10^12 solar masses and a thicker, hotter thick disk than the 2017 model.

  3. Variable gravitational potential of Milky Way analogues in HESTIA suite

    astro-ph.GA 2024-12 conditional novelty 6.0 of 10

    The gravitational potential of Milky Way analogues at large radii is significantly shaped by the Local Group environment, so orbit models must include it.

  4. Characterizing the disruption of B\"ootes III: a missing link in the Galactic halo?

    astro-ph.GA 2026-07 accept novelty 5.5 of 10

    Extensive Gaia, CaHK, UNIONS, SDSS, and DELVE searches find no observational evidence that Boötes III is the progenitor of the Styx stream.

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