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Reply to Walker et al.: Rock melting? Oxygen matters

Research output: Contribution to JournalComment / Letter to the editorAcademic

Original languageEnglish
Article numbere2211778119
Pages (from-to)1-1
Number of pages1
JournalProceedings of the National Academy of Sciences of the United States of America
Volume119
Issue number41
Early online date3 Oct 2022
DOIs
Publication statusPublished - 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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