{"id":18620564,"url":"https://github.com/simonsobs/so_noise_models","last_synced_at":"2025-04-11T02:31:15.311Z","repository":{"id":45176934,"uuid":"226378985","full_name":"simonsobs/so_noise_models","owner":"simonsobs","description":"Simons Observatory N(ell) noise models for public release","archived":false,"fork":false,"pushed_at":"2022-01-03T16:10:31.000Z","size":8171,"stargazers_count":8,"open_issues_count":0,"forks_count":6,"subscribers_count":30,"default_branch":"master","last_synced_at":"2025-03-25T08:11:38.994Z","etag":null,"topics":[],"latest_commit_sha":null,"homepage":null,"language":"Python","has_issues":true,"has_wiki":null,"has_pages":null,"mirror_url":null,"source_name":null,"license":"bsd-2-clause","status":null,"scm":"git","pull_requests_enabled":true,"icon_url":"https://github.com/simonsobs.png","metadata":{"files":{"readme":"README.rst","changelog":null,"contributing":null,"funding":null,"license":"LICENSE","code_of_conduct":null,"threat_model":null,"audit":null,"citation":null,"codeowners":null,"security":null,"support":null}},"created_at":"2019-12-06T17:34:35.000Z","updated_at":"2025-02-11T14:13:15.000Z","dependencies_parsed_at":"2022-07-22T13:32:03.838Z","dependency_job_id":null,"html_url":"https://github.com/simonsobs/so_noise_models","commit_stats":null,"previous_names":[],"tags_count":0,"template":false,"template_full_name":null,"repository_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonsobs%2Fso_noise_models","tags_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonsobs%2Fso_noise_models/tags","releases_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonsobs%2Fso_noise_models/releases","manifests_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonsobs%2Fso_noise_models/manifests","owner_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/owners/simonsobs","download_url":"https://codeload.github.com/simonsobs/so_noise_models/tar.gz/refs/heads/master","host":{"name":"GitHub","url":"https://github.com","kind":"github","repositories_count":248329558,"owners_count":21085559,"icon_url":"https://github.com/github.png","version":null,"created_at":"2022-05-30T11:31:42.601Z","updated_at":"2022-07-04T15:15:14.044Z","host_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub","repositories_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories","repository_names_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repository_names","owners_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/owners"}},"keywords":[],"created_at":"2024-11-07T04:06:55.410Z","updated_at":"2025-04-11T02:31:10.299Z","avatar_url":"https://github.com/simonsobs.png","language":"Python","funding_links":[],"categories":[],"sub_categories":[],"readme":"===============\nso_noise_models\n===============\n\nThis repository hosts publicly released N(ell) noise curve projection\ncode for the `Simons Observatory \u003chttps://simonsobservatory.org\u003e`__.\nThe intention is that the full history of noise models will be\navailable here, to supplement published projections and simulations.\n\nThis main home of the repository is:\nhttps://github.com/simonsobs/so_noise_models.\n\nThe noise model was originally described and applied in the\npublication:\n\n  Simons Observatory Collaboration.  \"The Simons Observatory: science\n  goals and forecasts\".  JCAP 1902 (2019) 056.  arxiv:1808.07455\n\nThe paper may be found at the following links:\n\n- https://dx.doi.org/10.1088/1475-7516/2019/02/056\n- https://arxiv.org/abs/1808.07445\n\nNote that only code and results marked with version code *v3.0.0* will\ncorrespond exactly to the results shown in the paper.  For the LAT\ncomponent-separated noise spectra (LAT_comp_sep_noise/v3.1.0/), this\nrepository contains only the results for the *v3.1.0* noise model.\nThe v3.1.x model incorporates a fix to the low-ell noise.\n\nThis repository is organized as follows:\n\n- ``so_models_v3/``: Python 3 package providing the noise model code\n  used in publications and publicly released simulations.  This\n  consists of several independent sub-modules, representing each\n  version of the noise code.  The usage of the models can vary\n  substantially from version to version -- please consult code in\n  ``demos/`` for typical usage patterns.\n- ``demos/``: Code that demonstrates usage of the noise models, such\n  as by producing noise curve plots.\n- ``LAT_comp_sep_noise/`` - Effective noise power spectra for SO LAT\n  component-separated CMB T, E, B, and Compton-y maps.  See dedicated\n  README within.\n- ``LAT_lensing_noise/`` - Lensing noise curves from SO LAT\n  component-separated CMB T, E, B maps.  See dedicated\n  README files within.\n\nThe ``so_models_v3`` package is pure python and thus can be imported\nfrom the root level of this repository.  But you might want to install\nit into your Python environment.  Conda users can simply run::\n\n  pip3 install .\n\nIf you're not using Conda and want to install the package to your\nlocal user package folder, run::\n\n  python3 setup.py install --user\n","project_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Fsimonsobs%2Fso_noise_models","html_url":"https://awesome.ecosyste.ms/projects/github.com%2Fsimonsobs%2Fso_noise_models","lists_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Fsimonsobs%2Fso_noise_models/lists"}