Clusterix 2.0: a virtual observatory tool to estimate cluster
membership probability

J 2020

Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability

BALAGUER-NUNEZ, Lola; Mauro LOPEZ DEL FRESNO; Enrique SOLANO; David GALADI-ENRIQUEZ; Carme JORDI et. al.

Základní údaje

Originální název

Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability

Autoři

BALAGUER-NUNEZ, Lola (724 Španělsko); Mauro LOPEZ DEL FRESNO (724 Španělsko); Enrique SOLANO (724 Španělsko); David GALADI-ENRIQUEZ (724 Španělsko); Carme JORDI (724 Španělsko); Francisco JIMENEZ-ESTEBAN (724 Španělsko); Enrique MASANA (724 Španělsko); Juan CARBAJO-HIJARRUBIA (724 Španělsko) a Ernst PAUNZEN (40 Rakousko, garant, domácí)

Vydání

Monthly Notices of the Royal Astronomical Society, MALDEN, WILEY, 2020, 0035-8711

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Velká Británie a Severní Irsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 5.287

Kód RIV

RIV/00216224:14310/20:00115736

Organizační jednotka

Přírodovědecká fakulta

DOI

http://dx.doi.org/10.1093/mnras/stz3610

UT WoS

000518148000087

EID Scopus

2-s2.0-85091965822

Klíčová slova anglicky

methods: statistical; virtual observatory tools; proper motions; open clusters and associations: general; open clusters and associations: individual: NGC 2682

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 29. 4. 2021 16:11, Mgr. Marie Novosadová Šípková, DiS.

Anotace

V originále

Clusterix 2.0 is a web-based, Virtual Observatory compliant, interactive tool for the determination of membership probabilities in stellar clusters based on proper-motion data using a fully non-parametric method. In an area occupied by a cluster, the frequency function is made up of two contributions: cluster and field stars. The tool performs an empirical determination of the frequency functions from the vector point diagram without relying on any previous assumption about their profiles, Clusterix 2,0 allows us to search the appropriate spatial areas in an interactive way until an optimal separation of the two populations is obtained. Several parameters can be adjusted to make the calculation computationally feasible without interfering with the quality of the results, The system offers the possibility to query different catalogues, such as Gala, or upload a user's own data, The results of the membership determination can be sent via Simple Application Messaging Protocol (SAMP) to Virtual Observatory (VO) tools such as Tool for OPerations on Catalogues And Tables (TOPCAT), We apply Clusterix 2,0 to several open clusters with different properties and environments to show the capabilities of the tool: an area of live degrees radius around NGC 2682 (M67), an old, well-known cluster; a young cluster NGC 2516 with a striking elongated structure extended up to four degrees; NGC 1750 and NGC 1758, a pair of partly overlapping clusters; the area of NGC 1817, where we confirm a little-known cluster, Juchert 23; and an area with many clusters, where we disentangle two overlapping clusters situated where only one was previously known: Ruprecht 26 and the new CLUSTERIX 1.

Citovat

BALAGUER-NUNEZ, Lola; Mauro LOPEZ DEL FRESNO; Enrique SOLANO; David GALADI-ENRIQUEZ; Carme JORDI; Francisco JIMENEZ-ESTEBAN; Enrique MASANA; Juan CARBAJO-HIJARRUBIA a Ernst PAUNZEN. Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability. Monthly Notices of the Royal Astronomical Society. MALDEN: WILEY, 2020, roč. 492, č. 4, s. 5811-5843. ISSN 0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/stz3610.

@article{1660119,
   author = {BalaguerandNunez, Lola and Lopez del Fresno, Mauro and Solano, Enrique and GaladiandEnriquez, David and Jordi, Carme and JimenezandEsteban, Francisco and Masana, Enrique and CarbajoandHijarrubia, Juan and Paunzen, Ernst},
   article_location = {MALDEN},
   article_number = {4},
   doi = {http://dx.doi.org/10.1093/mnras/stz3610},
   keywords = {methods: statistical; virtual observatory tools; proper motions; open clusters and associations: general; open clusters and associations: individual: NGC 2682},
   language = {eng},
   issn = {0035-8711},
   journal = {Monthly Notices of the Royal Astronomical Society},
   title = {Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability},
   url = {https://academic.oup.com/mnras/article-abstract/492/4/5811/5733679?redirectedFrom=PDF},
   volume = {492},
   year = {2020}
}

TY  - JOUR
ID  - 1660119
AU  - Balaguer-Nunez, Lola - Lopez del Fresno, Mauro - Solano, Enrique - Galadi-Enriquez, David - Jordi, Carme - Jimenez-Esteban, Francisco - Masana, Enrique - Carbajo-Hijarrubia, Juan - Paunzen, Ernst
PY  - 2020
TI  - Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability
JF  - Monthly Notices of the Royal Astronomical Society
VL  - 492
IS  - 4
SP  - 5811-5843
EP  - 5811-5843
PB  - WILEY
SN  - 00358711
KW  - methods: statistical
KW  - virtual observatory tools
KW  - proper motions
KW  - open clusters and associations: general
KW  - open clusters and associations: individual: NGC 2682
UR  - https://academic.oup.com/mnras/article-abstract/492/4/5811/5733679?redirectedFrom=PDF
L2  - https://academic.oup.com/mnras/article-abstract/492/4/5811/5733679?redirectedFrom=PDF
N2  - Clusterix 2.0 is a web-based, Virtual Observatory compliant, interactive tool for the determination of membership probabilities in stellar clusters based on proper-motion data using a fully non-parametric method. In an area occupied by a cluster, the frequency function is made up of two contributions: cluster and field stars. The tool performs an empirical determination of the frequency functions from the vector point diagram without relying on any previous assumption about their profiles, Clusterix 2,0 allows us to search the appropriate spatial areas in an interactive way until an optimal separation of the two populations is obtained. Several parameters can be adjusted to make the calculation computationally feasible without interfering with the quality of the results, The system offers the possibility to query different catalogues, such as Gala, or upload a user's own data, The results of the membership determination can be sent via Simple Application Messaging Protocol (SAMP) to Virtual Observatory (VO) tools such as Tool for OPerations on Catalogues And Tables (TOPCAT), We apply Clusterix 2,0 to several open clusters with different properties and environments to show the capabilities of the tool: an area of live degrees radius around NGC 2682 (M67), an old, well-known cluster; a young cluster NGC 2516 with a striking elongated structure extended up to four degrees; NGC 1750 and NGC 1758, a pair of partly overlapping clusters; the area of NGC 1817, where we confirm a little-known cluster, Juchert 23; and an area with many clusters, where we disentangle two overlapping clusters situated where only one was previously known: Ruprecht 26 and the new CLUSTERIX 1.
ER  -

BALAGUER-NUNEZ, Lola; Mauro LOPEZ DEL FRESNO; Enrique SOLANO; David GALADI-ENRIQUEZ; Carme JORDI; Francisco JIMENEZ-ESTEBAN; Enrique MASANA; Juan CARBAJO-HIJARRUBIA a Ernst PAUNZEN. Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability. \textit{Monthly Notices of the Royal Astronomical Society}. MALDEN: WILEY, 2020, roč.~492, č.~4, s.~5811-5843. ISSN~0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/stz3610.

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