galstreams: A library of Milky Way stellar stream footprints and tracks
Resumen:
Nearly a hundred stellar streams have been found to date around the Milky Way and the number keeps growing at an ever faster pace. Here we present the galstreams library, a compendium of angular position, distance, proper motion, and radial velocity track data for nearly a hundred (95) Galactic stellar streams. The information published in the literature has been collated and homogenized in a consistent format and used to provide a set of features uniformly computed throughout the library: e.g. stream length, end points, mean pole, stream’s coordinate frame, polygon footprint, and pole and angular momentum tracks. We also use the information compiled to analyse the distribution of several observables across the library and to assess where the main deficiencies are found in the characterization of individual stellar streams, as a resource for future follow-up efforts. The library is intended to facilitate keeping track of new discoveries and to encourage the use of automated methods to characterize and study the ensemble of known stellar streams by serving as a starting point. The galstreams library is publicly available as a PYTHON package and served at the galstreams GitHub repository.
2023 | |
ANII: FCE_1_2021_1_167524 | |
Astronomical databases Catalogues-Software Public release–Galaxy Halo – Galaxy Structure. |
|
Inglés | |
Universidad de la República | |
COLIBRI | |
https://hdl.handle.net/20.500.12008/42366 | |
Acceso abierto | |
Licencia Creative Commons Atribución (CC - By 4.0) |
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---|---|
author | Mateu, Cecilia |
author_facet | Mateu, Cecilia |
author_role | author |
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collection | COLIBRI |
dc.contributor.filiacion.none.fl_str_mv | Mateu Cecilia, Universidad de la República (Uruguay). Facultad de Ciencias. Instituto de Física. |
dc.creator.none.fl_str_mv | Mateu, Cecilia |
dc.date.accessioned.none.fl_str_mv | 2024-02-05T15:09:21Z |
dc.date.available.none.fl_str_mv | 2024-02-05T15:09:21Z |
dc.date.issued.none.fl_str_mv | 2023 |
dc.description.abstract.none.fl_txt_mv | Nearly a hundred stellar streams have been found to date around the Milky Way and the number keeps growing at an ever faster pace. Here we present the galstreams library, a compendium of angular position, distance, proper motion, and radial velocity track data for nearly a hundred (95) Galactic stellar streams. The information published in the literature has been collated and homogenized in a consistent format and used to provide a set of features uniformly computed throughout the library: e.g. stream length, end points, mean pole, stream’s coordinate frame, polygon footprint, and pole and angular momentum tracks. We also use the information compiled to analyse the distribution of several observables across the library and to assess where the main deficiencies are found in the characterization of individual stellar streams, as a resource for future follow-up efforts. The library is intended to facilitate keeping track of new discoveries and to encourage the use of automated methods to characterize and study the ensemble of known stellar streams by serving as a starting point. The galstreams library is publicly available as a PYTHON package and served at the galstreams GitHub repository. |
dc.description.sponsorship.none.fl_txt_mv | ANII: FCE_1_2021_1_167524 |
dc.format.extent.es.fl_str_mv | 34 h. |
dc.format.mimetype.es.fl_str_mv | application/pdf |
dc.identifier.citation.es.fl_str_mv | Mateu, C. "galstreams: A library of Milky Way stellar stream footprints and tracks". Monthly Notices. [en línea] 2023, 520(4): 5225–5258. 34 h. DOI: 10.1093/mnras/stad321 |
dc.identifier.doi.none.fl_str_mv | 10.1093/mnras/stad321 |
dc.identifier.issn.none.fl_str_mv | 1365-2966 |
dc.identifier.uri.none.fl_str_mv | https://hdl.handle.net/20.500.12008/42366 |
dc.language.iso.none.fl_str_mv | en eng |
dc.publisher.es.fl_str_mv | Royal Astronomical Society |
dc.relation.ispartof.es.fl_str_mv | Monthly Notices, 2023, 520(4): 5225–5258. |
dc.rights.license.none.fl_str_mv | Licencia Creative Commons Atribución (CC - By 4.0) |
dc.rights.none.fl_str_mv | info:eu-repo/semantics/openAccess |
dc.source.none.fl_str_mv | reponame:COLIBRI instname:Universidad de la República instacron:Universidad de la República |
dc.subject.es.fl_str_mv | Astronomical databases Catalogues-Software Public release–Galaxy Halo – Galaxy Structure. |
dc.title.none.fl_str_mv | galstreams: A library of Milky Way stellar stream footprints and tracks |
dc.type.es.fl_str_mv | Artículo |
dc.type.none.fl_str_mv | info:eu-repo/semantics/article |
dc.type.version.none.fl_str_mv | info:eu-repo/semantics/publishedVersion |
description | Nearly a hundred stellar streams have been found to date around the Milky Way and the number keeps growing at an ever faster pace. Here we present the galstreams library, a compendium of angular position, distance, proper motion, and radial velocity track data for nearly a hundred (95) Galactic stellar streams. The information published in the literature has been collated and homogenized in a consistent format and used to provide a set of features uniformly computed throughout the library: e.g. stream length, end points, mean pole, stream’s coordinate frame, polygon footprint, and pole and angular momentum tracks. We also use the information compiled to analyse the distribution of several observables across the library and to assess where the main deficiencies are found in the characterization of individual stellar streams, as a resource for future follow-up efforts. The library is intended to facilitate keeping track of new discoveries and to encourage the use of automated methods to characterize and study the ensemble of known stellar streams by serving as a starting point. The galstreams library is publicly available as a PYTHON package and served at the galstreams GitHub repository. |
eu_rights_str_mv | openAccess |
format | article |
id | COLIBRI_aa0cbf0adb1bfb544fa4b7fb8cf70fe2 |
identifier_str_mv | Mateu, C. "galstreams: A library of Milky Way stellar stream footprints and tracks". Monthly Notices. [en línea] 2023, 520(4): 5225–5258. 34 h. DOI: 10.1093/mnras/stad321 1365-2966 10.1093/mnras/stad321 |
instacron_str | Universidad de la República |
institution | Universidad de la República |
instname_str | Universidad de la República |
language | eng |
language_invalid_str_mv | en |
network_acronym_str | COLIBRI |
network_name_str | COLIBRI |
oai_identifier_str | oai:colibri.udelar.edu.uy:20.500.12008/42366 |
publishDate | 2023 |
reponame_str | COLIBRI |
repository.mail.fl_str_mv | mabel.seroubian@seciu.edu.uy |
repository.name.fl_str_mv | COLIBRI - Universidad de la República |
repository_id_str | 4771 |
rights_invalid_str_mv | Licencia Creative Commons Atribución (CC - By 4.0) |
spelling | Mateu Cecilia, Universidad de la República (Uruguay). Facultad de Ciencias. Instituto de Física.2024-02-05T15:09:21Z2024-02-05T15:09:21Z2023Mateu, C. "galstreams: A library of Milky Way stellar stream footprints and tracks". Monthly Notices. [en línea] 2023, 520(4): 5225–5258. 34 h. DOI: 10.1093/mnras/stad3211365-2966https://hdl.handle.net/20.500.12008/4236610.1093/mnras/stad321Nearly a hundred stellar streams have been found to date around the Milky Way and the number keeps growing at an ever faster pace. Here we present the galstreams library, a compendium of angular position, distance, proper motion, and radial velocity track data for nearly a hundred (95) Galactic stellar streams. The information published in the literature has been collated and homogenized in a consistent format and used to provide a set of features uniformly computed throughout the library: e.g. stream length, end points, mean pole, stream’s coordinate frame, polygon footprint, and pole and angular momentum tracks. We also use the information compiled to analyse the distribution of several observables across the library and to assess where the main deficiencies are found in the characterization of individual stellar streams, as a resource for future follow-up efforts. The library is intended to facilitate keeping track of new discoveries and to encourage the use of automated methods to characterize and study the ensemble of known stellar streams by serving as a starting point. The galstreams library is publicly available as a PYTHON package and served at the galstreams GitHub repository.Submitted by Pintos Natalia (nataliapintosmvd@gmail.com) on 2024-02-01T17:16:13Z No. of bitstreams: 2 license_rdf: 24251 bytes, checksum: 71ed42ef0a0b648670f707320be37b90 (MD5) 10.1093.mnras.stad321.pdf: 4311929 bytes, checksum: d1bd8c64ebf121bdc7e3de210a977237 (MD5)Approved for entry into archive by Faget Cecilia (lfaget@fcien.edu.uy) on 2024-02-05T12:17:50Z (GMT) No. of bitstreams: 2 license_rdf: 24251 bytes, checksum: 71ed42ef0a0b648670f707320be37b90 (MD5) 10.1093.mnras.stad321.pdf: 4311929 bytes, checksum: d1bd8c64ebf121bdc7e3de210a977237 (MD5)Made available in DSpace by Seroubian Mabel (mabel.seroubian@seciu.edu.uy) on 2024-02-05T15:09:21Z (GMT). No. of bitstreams: 2 license_rdf: 24251 bytes, checksum: 71ed42ef0a0b648670f707320be37b90 (MD5) 10.1093.mnras.stad321.pdf: 4311929 bytes, checksum: d1bd8c64ebf121bdc7e3de210a977237 (MD5) Previous issue date: 2023ANII: FCE_1_2021_1_16752434 h.application/pdfenengRoyal Astronomical SocietyMonthly Notices, 2023, 520(4): 5225–5258.Las obras depositadas en el Repositorio se rigen por la Ordenanza de los Derechos de la Propiedad Intelectual de la Universidad de la República.(Res. Nº 91 de C.D.C. de 8/III/1994 – D.O. 7/IV/1994) y por la Ordenanza del Repositorio Abierto de la Universidad de la República (Res. Nº 16 de C.D.C. de 07/10/2014)info:eu-repo/semantics/openAccessLicencia Creative Commons Atribución (CC - By 4.0)Astronomical databasesCatalogues-SoftwarePublic release–GalaxyHalo – GalaxyStructure.galstreams: A library of Milky Way stellar stream footprints and tracksArtículoinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionreponame:COLIBRIinstname:Universidad de la Repúblicainstacron:Universidad de la RepúblicaMateu, CeciliaLICENSElicense.txtlicense.txttext/plain; charset=utf-84267http://localhost:8080/xmlui/bitstream/20.500.12008/42366/5/license.txt6429389a7df7277b72b7924fdc7d47a9MD55CC-LICENSElicense_urllicense_urltext/plain; charset=utf-844http://localhost:8080/xmlui/bitstream/20.500.12008/42366/2/license_urla0ebbeafb9d2ec7cbb19d7137ebc392cMD52license_textlicense_texttext/html; charset=utf-820555http://localhost:8080/xmlui/bitstream/20.500.12008/42366/3/license_textc3353adb4b970603e3b1fce8a9e67d6cMD53license_rdflicense_rdfapplication/rdf+xml; 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- Universidad de la Repúblicafalse |
spellingShingle | galstreams: A library of Milky Way stellar stream footprints and tracks Mateu, Cecilia Astronomical databases Catalogues-Software Public release–Galaxy Halo – Galaxy Structure. |
status_str | publishedVersion |
title | galstreams: A library of Milky Way stellar stream footprints and tracks |
title_full | galstreams: A library of Milky Way stellar stream footprints and tracks |
title_fullStr | galstreams: A library of Milky Way stellar stream footprints and tracks |
title_full_unstemmed | galstreams: A library of Milky Way stellar stream footprints and tracks |
title_short | galstreams: A library of Milky Way stellar stream footprints and tracks |
title_sort | galstreams: A library of Milky Way stellar stream footprints and tracks |
topic | Astronomical databases Catalogues-Software Public release–Galaxy Halo – Galaxy Structure. |
url | https://hdl.handle.net/20.500.12008/42366 |