| Original language | English |
|---|---|
| Article number | e2211778119 |
| Pages (from-to) | 1-1 |
| Number of pages | 1 |
| Journal | Proceedings of the National Academy of Sciences of the United States of America |
| Volume | 119 |
| Issue number | 41 |
| Early online date | 3 Oct 2022 |
| DOIs |
|
| Publication status | Published - 11 Oct 2022 |
Bibliographical note
Funding Information:We thank Walker et al., as their experiments revealed a problem with a subset of our published data, and Peiyan Wu and Yongjiang Xu at Center for High Pressure Science and Technology Advanced Research (HPSTAR) and Maan Verburg at Vrije Universiteit Amsterdam for helping to perform the new series of experiments, and Shuang Xu for technical assistance on electron microprobe analyses at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau. The editor is thanked for critical comments that helped clarify this reply. This research was supported by the National Science Foundation of China (Grants U1530402 and U1930401) HPSTAR. W.v.W. acknowledges financial support from the Dutch Research Council Planetary and Exoplanetary Science program.
Funding Information:
ACKNOWLEDGMENTS. We thank Walker et al., as their experiments revealed a problem with a subset of our published data, and Peiyan Wu and Yongjiang Xu at Center for High Pressure Science and Technology Advanced Research (HPSTAR) and Maan Verburg at Vrije Universiteit Amsterdam for helping to perform the new series of experiments, and Shuang Xu for technical assistance on electron microprobe analyses at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau. The editor is thanked for critical comments that helped clarify this reply. This research was supported by the National Science Foundation of China (Grants U1530402 and U1930401) HPSTAR. W.v.W. acknowledges financial support from the Dutch Research Council Planetary and Exoplanetary Science program.
Funding
We thank Walker et al., as their experiments revealed a problem with a subset of our published data, and Peiyan Wu and Yongjiang Xu at Center for High Pressure Science and Technology Advanced Research (HPSTAR) and Maan Verburg at Vrije Universiteit Amsterdam for helping to perform the new series of experiments, and Shuang Xu for technical assistance on electron microprobe analyses at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau. The editor is thanked for critical comments that helped clarify this reply. This research was supported by the National Science Foundation of China (Grants U1530402 and U1930401) HPSTAR. W.v.W. acknowledges financial support from the Dutch Research Council Planetary and Exoplanetary Science program. ACKNOWLEDGMENTS. We thank Walker et al., as their experiments revealed a problem with a subset of our published data, and Peiyan Wu and Yongjiang Xu at Center for High Pressure Science and Technology Advanced Research (HPSTAR) and Maan Verburg at Vrije Universiteit Amsterdam for helping to perform the new series of experiments, and Shuang Xu for technical assistance on electron microprobe analyses at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau. The editor is thanked for critical comments that helped clarify this reply. This research was supported by the National Science Foundation of China (Grants U1530402 and U1930401) HPSTAR. W.v.W. acknowledges financial support from the Dutch Research Council Planetary and Exoplanetary Science program.
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