{"id":32154213,"url":"https://github.com/rvspectml/scalpels.jl","last_synced_at":"2025-10-21T11:52:30.510Z","repository":{"id":56618459,"uuid":"298467023","full_name":"RvSpectML/Scalpels.jl","owner":"RvSpectML","description":"Scalpels algorithm","archived":false,"fork":false,"pushed_at":"2023-08-16T06:17:52.000Z","size":415,"stargazers_count":5,"open_issues_count":0,"forks_count":2,"subscribers_count":1,"default_branch":"main","last_synced_at":"2025-10-06T19:41:06.371Z","etag":null,"topics":["astrostatistics","cross-correlation-function","exoplanets","radial-velocities","spetroscopy","time-series-analysis"],"latest_commit_sha":null,"homepage":"https://rvspectml.github.io/RvSpectML-Overview/","language":"Julia","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/RvSpectML.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,"governance":null}},"created_at":"2020-09-25T04:27:34.000Z","updated_at":"2025-01-30T21:31:09.000Z","dependencies_parsed_at":"2022-08-15T22:01:02.145Z","dependency_job_id":"e1b787d4-1745-4878-81d0-3006f6b520da","html_url":"https://github.com/RvSpectML/Scalpels.jl","commit_stats":{"total_commits":25,"total_committers":5,"mean_commits":5.0,"dds":"0.43999999999999995","last_synced_commit":"25e79019042ae93a55e0f2f62b9a65e029ed8b6b"},"previous_names":[],"tags_count":3,"template":false,"template_full_name":null,"purl":"pkg:github/RvSpectML/Scalpels.jl","repository_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/RvSpectML%2FScalpels.jl","tags_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/RvSpectML%2FScalpels.jl/tags","releases_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/RvSpectML%2FScalpels.jl/releases","manifests_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/RvSpectML%2FScalpels.jl/manifests","owner_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/owners/RvSpectML","download_url":"https://codeload.github.com/RvSpectML/Scalpels.jl/tar.gz/refs/heads/main","sbom_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/RvSpectML%2FScalpels.jl/sbom","scorecard":null,"host":{"name":"GitHub","url":"https://github.com","kind":"github","repositories_count":280256223,"owners_count":26299342,"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","status":"online","status_checked_at":"2025-10-21T02:00:06.614Z","response_time":58,"last_error":null,"robots_txt_status":"success","robots_txt_updated_at":"2025-07-24T06:49:26.215Z","robots_txt_url":"https://github.com/robots.txt","online":true,"can_crawl_api":true,"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":["astrostatistics","cross-correlation-function","exoplanets","radial-velocities","spetroscopy","time-series-analysis"],"created_at":"2025-10-21T11:52:28.847Z","updated_at":"2025-10-21T11:52:30.496Z","avatar_url":"https://github.com/RvSpectML.png","language":"Julia","funding_links":[],"categories":[],"sub_categories":[],"readme":"# Scalpels [![Stable](https://img.shields.io/badge/docs-stable-blue.svg)](https://RvSpectML.github.io/Scalpels.jl/stable)  [![Build Status](https://github.com/RvSpectML/Scalpels.jl/workflows/CI/badge.svg)](https://github.com/RvSpectML/Scalpels.jl/actions) [![Coverage](https://codecov.io/gh/RvSpectML/Scalpels.jl/branch/master/graph/badge.svg)](https://codecov.io/gh/RvSpectML/Scalpels.jl)\n\nThis Julia package implements the core Self-Correlation Analysis of Line Profiles for Extracting Low-amplitude Shifts (Scalpels) algorithm from \n\"Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain\" A. Collier Cameron, E.B. Ford, S. Shahaf et al. (2020) submitted to *MNRAS*.\n\n","project_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Frvspectml%2Fscalpels.jl","html_url":"https://awesome.ecosyste.ms/projects/github.com%2Frvspectml%2Fscalpels.jl","lists_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Frvspectml%2Fscalpels.jl/lists"}