The Hidden Potential of VVV RR Lyrae Light Curves
| dc.catalogador | pau | |
| dc.contributor.author | Hajdu, Gergely | |
| dc.contributor.author | Catelan, Marcio | |
| dc.contributor.author | Dékány, István | |
| dc.contributor.author | Grebel, Eva K. | |
| dc.date.accessioned | 2024-03-05T15:15:07Z | |
| dc.date.available | 2024-03-05T15:15:07Z | |
| dc.date.issued | 2018 | |
| dc.description.abstract | We introduce a new method of determining the average magnitudes of RR Lyrae variables: in the K_{S}-band, based on robust fitting of principal components from a high-quality training sample; in the J-band, using the amplitudes of the K_{S} principal components to approximate the J-band light-curve shape in each pulsation phase. Furthermore, it has been found that the metallicity of individual RR Lyrae variables can be inferred from the K_{S}-band light curves.... | |
| dc.fuente.origen | ORCID | |
| dc.identifier.uri | https://www.pta.edu.pl/proc/v6p1 | |
| dc.identifier.uri | https://ui.adsabs.harvard.edu/abs/2018pas6.conf..295H/abstract | |
| dc.identifier.uri | https://repositorio.uc.cl/handle/11534/84112 | |
| dc.information.autoruc | Instituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556 | |
| dc.language.iso | en | |
| dc.rights | acceso restringido | |
| dc.title | The Hidden Potential of VVV RR Lyrae Light Curves | |
| dc.type | comunicación de congreso | |
| sipa.codpersvinculados | 1001556 | |
| sipa.trazabilidad | ORCID;2024-01-22 |