REVIEW 4 cited by
Agama reference documentation
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
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.
Forward citations
Cited by 4 Pith papers
-
Weighing the Milky Way's Satellite Galaxies Using Pulsar Accelerations
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.
-
Dynamical Models of the Milky Way in Action Space with LAMOST DR8 and GAIA EDR3
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.
-
Variable gravitational potential of Milky Way analogues in HESTIA suite
The gravitational potential of Milky Way analogues at large radii is significantly shaped by the Local Group environment, so orbit models must include it.
-
Characterizing the disruption of B\"ootes III: a missing link in the Galactic halo?
Extensive Gaia, CaHK, UNIONS, SDSS, and DELVE searches find no observational evidence that Boötes III is the progenitor of the Styx stream.
Discussion (0). Continue with ORCID to comment.