{"id":15735707,"url":"https://github.com/simonrw/window-function","last_synced_at":"2026-01-08T09:06:53.255Z","repository":{"id":27602852,"uuid":"31086323","full_name":"simonrw/window-function","owner":"simonrw","description":"For computing a transiting planet window function","archived":false,"fork":false,"pushed_at":"2015-03-03T10:07:42.000Z","size":480,"stargazers_count":0,"open_issues_count":0,"forks_count":0,"subscribers_count":2,"default_branch":"master","last_synced_at":"2025-02-06T08:45:16.716Z","etag":null,"topics":[],"latest_commit_sha":null,"homepage":"","language":"Makefile","has_issues":true,"has_wiki":null,"has_pages":null,"mirror_url":null,"source_name":null,"license":"mit","status":null,"scm":"git","pull_requests_enabled":true,"icon_url":"https://github.com/simonrw.png","metadata":{"files":{"readme":"README.md","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":"2015-02-20T21:35:59.000Z","updated_at":"2015-03-03T10:07:42.000Z","dependencies_parsed_at":"2022-09-02T22:51:57.092Z","dependency_job_id":null,"html_url":"https://github.com/simonrw/window-function","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/simonrw%2Fwindow-function","tags_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonrw%2Fwindow-function/tags","releases_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonrw%2Fwindow-function/releases","manifests_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/simonrw%2Fwindow-function/manifests","owner_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/owners/simonrw","download_url":"https://codeload.github.com/simonrw/window-function/tar.gz/refs/heads/master","host":{"name":"GitHub","url":"https://github.com","kind":"github","repositories_count":246413237,"owners_count":20773053,"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":"2024-10-04T01:14:46.119Z","updated_at":"2026-01-08T09:06:53.162Z","avatar_url":"https://github.com/simonrw.png","language":"Makefile","funding_links":[],"categories":[],"sub_categories":[],"readme":"# Period window function\n\nBy using basic weather statistics (or assumptions), available python astronomy libraries, the Fressin et. al. (2013) occurrence rates compute the predicted sensitivity as a function of orbital period for a transiting survey, for example [NGTS](http://www.ngtransits.org/). \n\nExample output: [http://nbviewer.ipython.org/github/mindriot101/window-function/blob/master/Output.ipynb](http://nbviewer.ipython.org/github/mindriot101/window-function/blob/master/Output.ipynb)\n\n## Requirements\n\nSee the included `requirements.conda.txt` and `requirements.txt` files.\n\n## Running the code\n\nJust type `make`, which uses [`runipy`](https://github.com/paulgb/runipy) to run the simulation on the command line. Alternatively just run the notebook!\n\n## Todo\n\n* The histogram should be number of detections per planet\n","project_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Fsimonrw%2Fwindow-function","html_url":"https://awesome.ecosyste.ms/projects/github.com%2Fsimonrw%2Fwindow-function","lists_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Fsimonrw%2Fwindow-function/lists"}