论文标题

漫画萤火虫增值目录:已解决的10,010个星系的恒星种群

The MaNGA FIREFLY Value-Added-Catalogue: resolved stellar populations of 10,010 nearby galaxies

论文作者

Neumann, Justus, Thomas, Daniel, Maraston, Claudia, Hill, Lewis, Nanni, Lorenza, Wenman, Oliver, Lian, Jianhui, Comparat, Johan, Gonzalez-Perez, Violeta, Westfall, Kyle B., Yan, Renbin, Chen, Yanping, Stringfellow, Guy S., Bershady, Matthew A., Brownstein, Joel R., Drory, Niv, Schneider, Donald P.

论文摘要

我们介绍了漫画萤火虫增值库(VAC) - 从漫画调查的最终数据发布中,在附近的10,010个星系中,在空间解决的恒星人口属性约为370万个目录。全频谱拟合代码萤火虫用于得出参数,例如恒星年龄,金属性,恒星和残余质量,恒星形成历史,恒星形成率和尘埃衰减。除了Voronoi-bined测量值外,我们的VAC还提供了全球性能,例如中心值和径向梯度。可以使用VAC的两个变体:使用M11英里和新型Mastar恒星种群模型呈现拟合的结果。 Mastar允许限制整个漫画波长范围内的拟合度,扩展年龄金属参数空间,并使用与漫画同一仪器的经验光谱。采用乳腺模型的拟合平均年龄略年轻,大量加权金属性和较小的颜色过剩。当匹配波长范围和收敛模板网格时,这些差异会减少。我们进一步报告说,萤火虫恒星质量系统地比漫画PCA和Pipe3D Vacs的质量系统地低约0.3个DEX,但与NSA最佳的质量相匹配,只有〜0.1 DEX差异。最后,我们表明萤火虫恒星年龄与光谱指数年龄指标H $Δ_A$和$ d_n $(4000)相关,尽管具有明显的额外金属依赖性。

We present the MaNGA FIREFLY Value-Added-Catalogue (VAC) - a catalogue of ~3.7 million spatially resolved stellar population properties across 10,010 nearby galaxies from the final data release of the MaNGA survey. The full spectral fitting code firefly is employed to derive parameters such as stellar ages, metallicities, stellar and remnant masses, star formation histories, star formation rates and dust attenuation. In addition to Voronoi-binned measurements, our VAC also provides global properties, such as central values and radial gradients. Two variants of the VAC are available: presenting the results from fits using the M11-MILES and the novel MaStar stellar population models. MaStar allows to constrain the fit over the whole MaNGA wavelength range, extends the age-metallicity parameter space, and uses empirical spectra from the same instrument as MaNGA. The fits employing MaStar models find on average slightly younger ages, higher mass-weighted metallicities and smaller colour excesses. These differences are reduced when matching wavelength range and converging template grids. We further report that FIREFLY stellar masses are systematically lower by ~0.3 dex than masses from the MaNGA PCA and Pipe3D VACs, but match masses from the NSA best with only ~0.1 dex difference. Finally, we show that FIREFLY stellar ages correlate with spectral index age indicators H$δ_A$ and $D_n$(4000), though with a clear additional metallicity dependence.

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