.. image:: ./SCOUSE_LOGO.png :align: center :width: 750 | ******** scousepy ******** Multi-component spectral line decomposition with ``scousepy``. ``scousepy`` is a package for the analysis of spectral line data. A detailed description of the method (and the original `IDL version `_ of the code) can be found in `Henshaw et al. 2016 `_. In the following pages you will find a :ref:`brief introduction ` to the method as well as a :ref:`tutorial `. The `source code `_ is available on GitHub and comments and contributions are very welcome. Documentation ~~~~~~~~~~~~~ .. toctree:: :maxdepth: 4 installation.rst description.rst tutorial_v2.0.0.rst stats.rst tutorial_v1.0.0.rst license.rst Reporting issues and getting help ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Please help to improve this package by reporting `issues `_ via GitHub. Alternatively, if you have any questions or if you are having any problems getting set up you can get in touch `here `_. Developers ~~~~~~~~~~ This package was developed by: * Jonathan Henshaw Contributors include: * Adam Ginsburg * Manuel Riener Citing scousepy ~~~~~~~~~~~~~~~ If you make use of this package in a publication, please consider the following acknowledgements...:: @ARTICLE{Henshaw19, author = {{Henshaw}, J.~D. and {Ginsburg}, A. and {Haworth}, T.~J. and {Longmore}, S.~N. and {Kruijssen}, J.~M.~D. and {Mills}, E.~A.~C. and {Sokolov}, V. and {Walker}, D.~L. and {Barnes}, A.~T. and {Contreras}, Y. and {Bally}, J. and {Battersby}, C. and {Beuther}, H. and {Butterfield}, N. and {Dale}, J.~E. and {Henning}, T. and {Jackson}, J.~M. and {Kauffmann}, J. and {Pillai}, T. and {Ragan}, S. and {Riener}, M. and {Zhang}, Q.}, title = "{`The Brick' is not a brick: a comprehensive study of the structure and dynamics of the central molecular zone cloud G0.253+0.016}", journal = {\mnras}, archivePrefix = "arXiv", eprint = {1902.02793}, keywords = {turbulence, stars: formation, ISM: clouds, ISM: kinematics and dynamics, ISM: structure, galaxy: centre}, year = 2019, month = may, volume = 485, pages = {2457-2485}, doi = {10.1093/mnras/stz471}, adsurl = {http://adsabs.harvard.edu/abs/2019MNRAS.485.2457H}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } @ARTICLE{Henshaw2016, author = {{Henshaw}, J.~D. and {Longmore}, S.~N. and {Kruijssen}, J.~M.~D. and {Davies}, B. and {Bally}, J. and {Barnes}, A. and {Battersby}, C. and {Burton}, M. and {Cunningham}, M.~R. and {Dale}, J.~E. and {Ginsburg}, A. and {Immer}, K. and {Jones}, P.~A. and {Kendrew}, S. and {Mills}, E.~A.~C. and {Molinari}, S. and {Moore}, T.~J.~T. and {Ott}, J. and {Pillai}, T. and {Rathborne}, J. and {Schilke}, P. and {Schmiedeke}, A. and {Testi}, L. and {Walker}, D. and {Walsh}, A. and {Zhang}, Q.}, title = "{Molecular gas kinematics within the central 250 pc of the Milky Way}", journal = {\mnras}, keywords = {stars: formation, ISM: clouds, ISM: kinematics and dynamics, ISM: structure, Galaxy: centre, galaxies: ISM, Astrophysics - Astrophysics of Galaxies}, year = 2016, month = apr, volume = {457}, number = {3}, pages = {2675-2702}, doi = {10.1093/mnras/stw121}, archivePrefix = {arXiv}, eprint = {1601.03732}, primaryClass = {astro-ph.GA}, adsurl = {https://ui.adsabs.harvard.edu/abs/2016MNRAS.457.2675H}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } Citations courtesy of `ADS `__. Please also consider acknowledgements to the required packages in your work. Papers using scousepy ~~~~~~~~~~~~~~~~~~~~~ * Hu, Lazarian, & Wang 2021, MNRAS, submitted * Henshaw et al. 2021, MNRAS, 509, 4758 * Liu, Hu, & Lazarian 2021, MNRAS, 501, 4952 * Barnes et al. 2021, MNRAS, 503, 4601 * Callanan et al. 2021, MNRAS, 505, 4310 * Yue et al. 2021, RAA, 21, 24 * Cosentino et al. 2020, MNRAS, 499, 1666 * Henshaw et al. 2020, Nat. Ast. 4, 1064 * Henshaw et al. 2019, MNRAS, 485, 2457 * Cosentino et al. 2018, MNRAS, 474, 3760 * Henshaw, Longmore, Kruijssen, 2016, MNRAS, 463L, 122 * Henshaw et al. 2016, MNRAS, 457, 2675 Recipe ~~~~~~ Recipe for a fine Liverpudlian `Scouse pie `_.