From d4954d47f8a702bd51d5e4f93c83a8b0272cb359 Mon Sep 17 00:00:00 2001 From: Dan F-M Date: Sat, 1 Jun 2024 16:58:34 -0400 Subject: [PATCH] Small edits for JOSS review --- paper/paper.bib | 2 +- paper/paper.md | 6 +++--- 2 files changed, 4 insertions(+), 4 deletions(-) diff --git a/paper/paper.bib b/paper/paper.bib index 2b13e7a..39a5de6 100644 --- a/paper/paper.bib +++ b/paper/paper.bib @@ -205,7 +205,7 @@ @article{dyson @article{drasco, author = {{Drasco}, Steve and {Hughes}, Scott A.}, title = "{Gravitational wave snapshots of generic extreme mass ratio inspirals}", - journal = {\prd}, + journal = {Physical Review D}, keywords = {04.70.-s, 97.60.Lf, Physics of black holes, Black holes, General Relativity and Quantum Cosmology, Astrophysics}, year = 2006, month = jan, diff --git a/paper/paper.md b/paper/paper.md index 3a14970..127ba59 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -43,15 +43,15 @@ version of the parameters used to define a Keplerian orbit (eccentricity, semi-l Bound geodesics also possess fundamental frequencies since their radial, azimuthal, and polar motions are periodic. `KerrGeoPy` is a Python package which computes both stable and plunging timelike geodesics in Kerr spacetime using the -analytic solutions to the geodesic equation derived in [@fujita] and -[@dyson]. It mirrors and builds upon much of the functionality of the `KerrGeodesics` [@kerrgeodesics] Mathematica library. +analytic solutions to the geodesic equation derived in @fujita and +@dyson. It mirrors and builds upon much of the functionality of the `KerrGeodesics` [@kerrgeodesics] Mathematica library. Geodesic solutions are written in terms of Legendre elliptic integrals, which are evaluated using `SciPy`. Users can construct a geodesic by providing the initial position and four-velocity, or by providing either the constants of motion or the Keplerian parameters described above. `KerrGeoPy` provides methods for computing the four-velocity, fundamental frequencies, and constants of motion associated with a given geodesic and also implements the algorithm described -in [@stein] for finding the location of the last stable orbit, known as the separatrix. The package also +in @stein for finding the location of the last stable orbit, known as the separatrix. The package also includes several methods for visualizing and animating geodesics. `KerrGeoPy` is a part of the [Black Hole Perturbation Toolkit](https://bhptoolkit.org). The source code