tag:joss.theoj.org,2005:/papers/tagged/starsJournal of Open Source Software2023-11-06T16:28:16ZJournal of Open Source Softwarehttps://joss.theoj.orgtag:joss.theoj.org,2005:Paper/46062023-11-06T16:28:16Z2023-11-07T00:00:17Zmeasr: Bayesian psychometric measurement using Stanacceptedv0.3.12023-07-14 20:06:08 UTC912023-11-06 16:28:16 UTC820235742W.JakeThompsonAccessible, Teaching, Learning, and Assessment Systems, University of Kansas0000-0001-7339-030010.21105/joss.05742https://doi.org/10.5281/zenodo.10058365R, Stan, C++https://joss.theoj.org/papers/10.21105/joss.05742.pdfbayesian-modeling, educational-assessment, psychometrics, diagnostic-modelingtag:joss.theoj.org,2005:Paper/45342023-10-03T20:07:24Z2023-10-04T00:00:41ZELK: A python package for correcting, analyzing, and diagnosing TESS integrated light curvesacceptedv0.92023-06-08 20:03:09 UTC902023-10-03 20:07:24 UTC820235605TobinM.WainerDepartment of Astronomy, University of Washington, Box 351580, Seattle, WA 98195, USA, Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA0000-0001-6320-2230TomWaggDepartment of Astronomy, University of Washington, Box 351580, Seattle, WA 98195, USA0000-0001-6147-5761VijithJacobPoovelilDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA0000-0002-9831-3501GailZasowskiDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA0000-0001-6761-935910.21105/joss.05605https://doi.org/10.5281/zenodo.8393595Python, Jupyter Notebookhttps://joss.theoj.org/papers/10.21105/joss.05605.pdfastronomy, variability, blending, star clusterstag:joss.theoj.org,2005:Paper/41612023-07-22T03:05:19Z2023-07-23T00:01:35ZBridgeStan: Efficient in-memory access to the methods of a Stan modelacceptedv.1.0.02023-01-10 21:55:16 UTC872023-07-22 03:05:19 UTC820235236EdwardA.RoualdesCalifornia State University, Chico0000-0002-8757-3463BrianWardCenter for Computational Mathematics, Flatiron Institute0000-0002-9841-3342BobCarpenterCenter for Computational Mathematics, Flatiron Institute0000-0002-2433-9688AdrianSeyboldtPyMC Labs0000-0002-4239-4541SethD.AxenCluster of Excellence Machine Learning: New Perspectives for Science, University of Tübingen0000-0003-3933-824710.21105/joss.05236https://doi.org/10.5281/zenodo.8169248R, C, Juliahttps://joss.theoj.org/papers/10.21105/joss.05236.pdfStan, Python, Rust, C++, automatic differentiationtag:joss.theoj.org,2005:Paper/35932023-05-16T22:56:11Z2023-05-18T15:30:52Zclustertools: A Python Package for Analyzing Star Cluster Simulationsacceptedv1.02022-05-06 17:00:10 UTC852023-05-16 22:56:11 UTC820234483JeremyJ.WebbDavid A. Dunlap Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON, M5S 3H4, Canada0000-0003-3613-085410.21105/joss.04483https://doi.org/10.5281/zenodo.7941851Pythonhttps://joss.theoj.org/papers/10.21105/joss.04483.pdfastronomy, star clusters, N-body simulationstag:joss.theoj.org,2005:Paper/42992023-05-05T19:12:06Z2023-05-06T00:00:59ZSTARRED: a two-channel deconvolution method with Starlet regularizationacceptedv1.02023-03-10 15:25:35 UTC852023-05-05 19:12:06 UTC820235340KevinMichalewiczInstitute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Switzerland, Department of Mathematics, Imperial College London, London SW7 2AZ, United Kingdom0000-0002-6584-2749MartinMillonInstitute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Switzerland, Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, Stanford, CA 94305, USA0000-0001-7051-497XFrédéricDuxInstitute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Switzerland0000-0003-3358-4834FrédéricCourbinInstitute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Switzerland0000-0003-0758-651010.21105/joss.05340https://doi.org/10.5281/zenodo.7900798Jupyter Notebook, Pythonhttps://joss.theoj.org/papers/10.21105/joss.05340.pdfdeconvolution, PSF, astronomytag:joss.theoj.org,2005:Paper/39272023-02-14T13:07:10Z2023-02-15T00:00:23ZX-PSI: A Python package for neutron star X-ray pulse simulation and inferenceacceptedv1.0.02022-09-26 16:31:10 UTC822023-02-14 13:07:10 UTC820234977ThomasE.RileyAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0001-9313-0493DevarshiChoudhuryAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0002-2651-5286TuomoSalmiAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0001-6356-125XSerenaVinciguerraAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0003-3068-6974YvesKiniAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0002-0428-8430BasDorsmanAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0002-9407-0733AnnaL.WattsAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1090GE Amsterdam, The Netherlands0000-0002-1009-2354DanielaHuppenkothenSRON Netherlands Institute for Space Research, Niels Bohrweg 4, NL-2333 CA Leiden, the Netherlands0000-0002-1169-7486SebastienGuillotInstitut de Recherche en Astrophysique et Planétologie, UPS-OMP, CNRS, CNES, 9 avenue du Colonel Roche, BP 44346, F-31028 Toulouse Cedex 4, France0000-0002-6449-106X10.21105/joss.04977https://doi.org/10.5281/zenodo.7632629Python, Cython, Chttps://joss.theoj.org/papers/10.21105/joss.04977.pdfastrostatistics, neutron starstag:joss.theoj.org,2005:Paper/36462023-01-29T17:26:40Z2023-01-30T00:00:39ZMSG: A software package for interpolating stellar spectra in pre-calculated gridsacceptedv1.02022-06-05 19:36:35 UTC812023-01-29 17:26:40 UTC820234602RichTownsendDepartment of Astronomy, University of Wisconsin-Madison, USA0000-0002-2522-8605AaronLopezDepartment of Astronomy, University of Wisconsin-Madison, USA10.21105/joss.04602https://doi.org/10.5281/zenodo.7559319Fortran, Pythonhttps://joss.theoj.org/papers/10.21105/joss.04602.pdfC, astronomy, spectra, stars, grids, interpolationtag:joss.theoj.org,2005:Paper/36102022-09-05T10:04:38Z2022-10-11T06:54:05ZBTE: a Python module for pandemic-scale mutation-annotated phylogenetic treesacceptedv0.8.12022-05-17 23:22:33 UTC772022-09-05 10:04:38 UTC720224433JakobMcBroomeDepartment of Biomolecular Engineering, University of California Santa Cruz. Santa Cruz, CA 95064, USA, Genomics Institute, University of California Santa Cruz, Santa Cruz, CA 95064, USA0000-0002-5002-5156YatishTurakhiaDepartment of Electrical and Computer Engineering, University of California, San Diego; San Diego, CA 92093, USA0000-0001-5600-2900RussellCorbett-DetigDepartment of Biomolecular Engineering, University of California Santa Cruz. Santa Cruz, CA 95064, USA, Genomics Institute, University of California Santa Cruz, Santa Cruz, CA 95064, USA0000-0001-6535-247810.21105/joss.04433https://doi.org/10.5281/zenodo.7036163Python, C++, Cythonhttps://joss.theoj.org/papers/10.21105/joss.04433.pdfphylogenetics, epidemiology, SARS-CoV-2tag:joss.theoj.org,2005:Paper/34572022-06-26T07:46:52Z2022-06-27T00:00:38ZA-SLOTH: Ancient Stars and Local Observables by Tracing Halosacceptedv1.02022-04-06 11:28:21 UTC742022-06-26 07:46:52 UTC720224417MattisMaggInstitut für Theoretische Astrophysik, Universität Heidelberg, Germany, International Max Planck Research School for Astronomy and Cosmic Physics, University of Heidelberg (IMPRS-HD), Germany0000-0002-9022-5136TilmanHartwigInstitute for Physics of Intelligence, The University of Tokyo, Japan, Department of Physics, The University of Tokyo, Japan, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Japan0000-0001-6742-8843Li-HsinChenInstitut für Theoretische Astrophysik, Universität Heidelberg, Germany, International Max Planck Research School for Astronomy and Cosmic Physics, University of Heidelberg (IMPRS-HD), GermanyYutaTarumiDepartment of Physics, The University of Tokyo, Japan0000-0002-9801-778810.21105/joss.04417https://doi.org/10.5281/zenodo.6683682Roff, Fortran, Pythonhttps://joss.theoj.org/papers/10.21105/joss.04417.pdfPopulation III Stars, Semi-Analyticaltag:joss.theoj.org,2005:Paper/34552022-05-26T15:09:37Z2022-05-27T00:00:56Ztomso: TOols for Models of Stars and their Oscillationsacceptedv0.1.02022-03-31 20:47:04 UTC732022-05-26 15:09:37 UTC720224343WarrickH.BallSchool of Physics & Astronomy, University of Birmingham, United Kingdom0000-0002-4773-101710.21105/joss.04343https://doi.org/10.5281/zenodo.6563220Python, AMPL, Gnuplothttps://joss.theoj.org/papers/10.21105/joss.04343.pdfastronomy