论文标题

Zwicky瞬态设施和球形群集:RR Lyrae Gri-Band时期 - 亮度金属性和周期 - wesenheit-Altallicity关系

Zwicky Transient Facility and Globular Clusters: The RR Lyrae gri-Band Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity Relations

论文作者

Ngeow, Chow-Choong, Bhardwaj, Anupam, Dekany, Richard, Duev, Dmitry A., Graham, Matthew J., Groom, Steven L., Mahabal, Ashish A., Masci, Frank J., Medford, Michael S., Riddle, Reed

论文摘要

基于从Zwicky瞬态设施(ZTF)收集的时间序列观察,我们得出了位于球状簇中的RR Lyrae的周期 - 轻度金属度(PLZ)和周期 - wesenheit-Atallicity(PWZ)关系。我们已经应用了各种选择标准,以有问题或虚假的光曲线排除RR Lyrae。这些选择标准使用了有关每个光曲线,幅度,颜色和残差的信息数量和/或周期 - wesenheit关系的信息。由于混合,发现球状簇中的许多RR Lyrae异常明亮,并且其ZTF光曲线的幅度很小。我们在46个球状簇中使用了〜750 RR Lyrae的最终样品,涵盖了宽的金属性范围(-2.36 <[fe/h] <-0.54 dex),以在GRI频段中得出PLZ和PWZ关系。此外,我们还得出了周期彩色金属性(PCZ),并且首次是Q-索引通过构造灭绝的PQZ关系。我们将我们的各种关系与文献中可用的经验和理论关系进行了比较,并与大多数研究发现了一个很好的共识。最后,我们将派生的PLZ关系应用于矮星系II,发现其真实距离模量应大于最新测定。

Based on time-series observations collected from Zwicky Transient Facility (ZTF), we derived period-luminosity-metallicity (PLZ) and period-Wesenheit-metallicity (PWZ) relations for RR Lyrae located in globular clusters. We have applied various selection criteria to exclude RR Lyrae with problematic or spurious light curves. These selection criteria utilized information on the number of data points per light curve, amplitudes, colors, and residuals on the period-luminosity and/or period-Wesenheit relations. Due to blending, a number of RR Lyrae in globular clusters were found to be anomalously bright and have small amplitudes of their ZTF light curves. We used our final sample of ~750 RR Lyrae in 46 globular clusters covering a wide metallicity range (-2.36 < [Fe/H] < -0.54 dex) to derive PLZ and PWZ relations in gri bands. In addition, we have also derived the period-color-metallicity (PCZ) and for the first time, the PQZ relations where the Q-index is extinction-free by construction. We have compared our various relations to empirical and theoretical relations available in literature, and found a good agreement with most studies. Finally, we applied our derived PLZ relation to a dwarf galaxy, Crater II, and found its true distance modulus should be larger than the most recent determination.

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