Video/Audio Open Access
Dévora-Pajares, Martín; Francisco J. Pozuelos; Juan C. Suárez; GARANAT Team
{ "files": [ { "links": { "self": "https://zenodo.org/api/files/7eeb8d48-5ceb-4cbe-b71b-d8294f971513/The%20SHERLOCK%20PIPEline.webm" }, "checksum": "md5:0caf16f9b75f3e3cfefab6c9f6f9eea4", "bucket": "7eeb8d48-5ceb-4cbe-b71b-d8294f971513", "key": "The SHERLOCK PIPEline.webm", "type": "webm", "size": 7860800 } ], "owners": [ 258026 ], "doi": "10.5281/zenodo.5554325", "stats": { "version_unique_downloads": 21.0, "unique_views": 73.0, "views": 84.0, "version_views": 84.0, "unique_downloads": 21.0, "version_unique_views": 73.0, "volume": 172937600.0, "version_downloads": 22.0, "downloads": 22.0, "version_volume": 172937600.0 }, "links": { "doi": "https://doi.org/10.5281/zenodo.5554325", "conceptdoi": "https://doi.org/10.5281/zenodo.5554324", "bucket": "https://zenodo.org/api/files/7eeb8d48-5ceb-4cbe-b71b-d8294f971513", "conceptbadge": "https://zenodo.org/badge/doi/10.5281/zenodo.5554324.svg", "html": "https://zenodo.org/record/5554325", "latest_html": "https://zenodo.org/record/5554325", "badge": "https://zenodo.org/badge/doi/10.5281/zenodo.5554325.svg", "latest": "https://zenodo.org/api/records/5554325" }, "conceptdoi": "10.5281/zenodo.5554324", "created": "2021-10-07T10:58:39.811764+00:00", "updated": "2021-10-28T16:08:24.308857+00:00", "conceptrecid": "5554324", "revision": 4, "id": 5554325, "metadata": { "access_right_category": "success", "doi": "10.5281/zenodo.5554325", "description": "<p>The arrival of space missions such as Kepler/K2 and TESS has revolutionized exoplanets' detection, producing a vast amount of data that scientists need to analyze. This situation will keep increasing shortly thanks to the ESA PLATO mission, mainly devoted to finding Earth-like planets orbiting Sun-like stars, which will be launched in 2025-2026 (Rauer et al. 2014). This poster presents SHERLOCK, a robust and easy-to-use end-to-end pipeline to search for planet candidates, vet signals, perform a statistical validation, bayesian fit, and compute observational windows from ground-based facilities to trigger a follow-up campaign. All these steps are executed with just a few lines of code, which makes SHERLOCK an optimal ready-to-use code for any planetary search program.</p>", "license": { "id": "CC-BY-4.0" }, "title": "The SHERLOCK PIPEline: Searching for Hints of Exoplanets fRom Lightcurves Of spaCe-based seeKers", "relations": { "version": [ { "count": 1, "index": 0, "parent": { "pid_type": "recid", "pid_value": "5554324" }, "is_last": true, "last_child": { "pid_type": "recid", "pid_value": "5554325" } } ] }, "communities": [ { "id": "plato2021" } ], "keywords": [ "exoplanets", "pipeline", "transits" ], "publication_date": "2021-10-07", "creators": [ { "affiliation": "Dpto. F\u00edsica Te\u00f3rica y del Cosmos. Universidad de Granada. 18071. Granada, Spain", "name": "D\u00e9vora-Pajares, Mart\u00edn" }, { "affiliation": "Astrobiology research unit, University of Li\u00e8ge", "name": "Francisco J. Pozuelos" }, { "affiliation": "Dpto. F\u00edsica Te\u00f3rica y del Cosmos. Universidad de Granada. 18071. Granada, Spain", "name": "Juan C. Su\u00e1rez" }, { "affiliation": "Dpto. F\u00edsica Te\u00f3rica y del Cosmos. Universidad de Granada. 18071. Granada, Spain", "name": "GARANAT Team" } ], "access_right": "open", "resource_type": { "type": "video", "title": "Video/Audio" }, "related_identifiers": [ { "scheme": "doi", "identifier": "10.5281/zenodo.5554324", "relation": "isVersionOf" } ] } }
All versions | This version | |
---|---|---|
Views | 84 | 84 |
Downloads | 22 | 22 |
Data volume | 172.9 MB | 172.9 MB |
Unique views | 73 | 73 |
Unique downloads | 21 | 21 |