Data for: New magnetobiostratigraphic results from the Ladinian of the Dolomites and implications for the Triassic geomagnetic polarity timescale

Supplementary Table S1: ChRM components from Rio Nigra and Rio Frommer stratigraphic sections. Data are in core, in situ, and tilt-corrected coordinates. Legend of the header is at the end of the table.
Supplementary Table S2: Ages and durations of the chrons of the GPTS. The name of the chrons refers to the name of the magnetozones of origin. The mean polarity reversal rates for Early, Middle and Late Triassic (reversal/Myr) have been obtained through linear regression.
Figure S1: Anisotropy of Magnetic Susceptibility carried out on the samples from Rio Nigra and Rio Frommer sections.
Figure S2: Detail of the Middle Triassic interval of the GPTS/Age plot showing the error bars of the U-Pb zircon ages from Seceda (Wotzlaw et al., 2018) and Rio Nigra (Mietto et al., 2012).

补充表 S1：来自里奥尼格拉和里奥弗罗默地层剖面中的磁化率组分。数据以岩心、原位和倾斜校正的坐标表示。表头图例位于表格末尾。
补充表 S2：GPTS 时代地层周期的年代和持续时间。地层周期的名称参照原磁性地层的名称。早、中、晚三叠世的平均极性反转速率（反转/百万年）通过线性回归获得。
图 S1：对里奥尼格拉和里奥弗罗默剖面样品进行的磁化率各向异性测量。
图 S2：GPTS/年代图上中三叠世间隔的细节展示，其中包含来自塞切达（Wotzlaw 等人，2018年）和里奥尼格拉（Mietto 等人，2012年）的 U-Pb 锆石年龄误差棒。