Pith. sign in

REVIEW 2 cited by

ADIPLS -- the Aarhus adiabatic oscillation package

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

arxiv 0710.3106 v1 pith:V45I7UER submitted 2007-10-16 astro-ph

classification astro-ph
keywords codedevelopmentpackageaarhusadiabaticbeenactionadipls
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Development of the Aarhus adiabatic pulsation code started around 1978. Although the main features have been stable for more than a decade, development of the code is continuing, concerning numerical properties and output. The code has been provided as a generally available package and has seen substantial use at a number of installations. Further development of the package, including bringing the documentation closer to being up to date, is planned as part of the HELAS Coordination Action.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. Numerical simulations of oscillations for axisymmetric solar backgrounds with differential rotation and gravity

    astro-ph.SR 2025-08 accept novelty 6.0 of 10

    An axisymmetric HDG solver for stellar oscillation equations with gravity and differential rotation is validated by matching observed solar mode-splitting coefficients.

  2. Asteroseismology of solar-type stars

    astro-ph.SR 2019-06 unverdicted novelty 2.0 of 10

    This review summarizes the development, techniques, and open questions in asteroseismology of solar-type stars whose oscillations are stochastically excited by surface convection.

Pith tools