000000085 001__ 85 000000085 005__ 20230824003254.0 000000085 0247_ $$a10.7936/ax18-0528$$2DOI 000000085 037__ $$aRDM 000000085 041__ $$aeng 000000085 245__ $$aGamma-CaSO4 with Abnormally High Stability from Hyperarid Region on Earth and from Mars 000000085 269__ $$a2021-09-01 000000085 270__ $$malianw@levee.wustl.edu$$pWang, Alian 000000085 336__ $$aDataset 000000085 520__ $$aThe raw data of different spectra used in the “Gamma-CaSO4 with Abnormally High Stability from Hyperarid Region on Earth and from Mars ”, including (1) Raman spectra of Atacamaγ-CaSO4 and MIL03346, 168 γ-CaSO4 presented in Figure 8. Four standard Ca-sulfates are present in supplement materials. (2) EDXS spectra from the Atacamaγ-CaSO4 and MIL03346, 168 γ-CaSO4 displayed in Figure 4 and Figure 5 in the main text. (3) EELS spectra of MIL03346, 168 γ-CaSO4 shown as Figure 6 in the main text. (4) XRD patterns of standard bassanite and standard γ-CaSO4 presented in supplement materials. For more detailed information please reading section 2 (part of experiments) in the main text. 000000085 536__ $$c201806220274$$oChina Scholarship Council$$qhttps://ror.org/04atp4p48 000000085 536__ $$aMcDonnell Center for the Space Sciences Special Fund$$c94351A$$oWashington University in St. Louis$$qhttps://ror.org/01yc7t268 000000085 536__ $$cZR2019MD008$$oNatural Science Foundation of Shandong Province 000000085 536__ $$cU1931211$$oNational Natural Science Foundation of China$$qhttps://ror.org/01h0zpd94 000000085 536__ $$c41972322$$o National Natural Science Foundation of China$$qhttps://ror.org/01h0zpd94 000000085 536__ $$c11941001$$o National Natural Science Foundation of China$$qhttps://ror.org/01h0zpd94 000000085 536__ $$cD020102$$oChina National Space Administration$$qhttps://ror.org/004vanv95 000000085 540__ $$aCreative Commons Attribution (CC BY) 4.0 International$$uhttps://creativecommons.org/licenses/by/4.0/ 000000085 650__ $$aPhysical sciences 000000085 6531_ $$aRaman 000000085 6531_ $$aElectron energy loss spectroscopy 000000085 6531_ $$aEnergy-dispersive X-ray spectroscopy 000000085 6531_ $$aX-ray Powder Diffraction 000000085 655__ $$aTabular 000000085 7001_ $$aWang, Alian$$1https://orcid.org/0000-0002-0726-2869$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR 000000085 7001_ $$aLing, Zongcheng$$1https://orcid.org/0000-0002-9260-5765$$uShandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University 000000085 7001_ $$aShi, Erbin$$1https://orcid.org/0000-0002-8890-9723$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR 000000085 7001_ $$aLi, Huafang$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR 000000085 7001_ $$aOgliore, Ryan$$1https://orcid.org/0000-0001-8165-6252$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR 000000085 8564_ $$9fa8ea093-853f-4cc3-a259-fe9b22133dc2$$s8222$$uhttps://data.library.wustl.edu/record/85/files/doi107936ax180528_wang_readme.txt$$ePublic$$23f2f6858bd2d9e3e9cfd3a880e85213e$$01 000000085 8564_ $$945ecd7f1-a0be-421e-904b-a3e5b54ce138$$s825662$$uhttps://data.library.wustl.edu/record/85/files/doi107936ax180528wang_dip.zip$$ePublic$$28c095bd77af47339b6a24a930171e7f9$$01 000000085 904__ $$azcling@sdu.edu.cn 000000085 904__ $$airvingshi@epsc.wustl.edu 000000085 904__ $$ahli40@wustl.edu 000000085 904__ $$arogliore@wustl.edu 000000085 909CO $$ooai:data.library.wustl.edu:85$$pdataset 000000085 974__ $$aMars 000000085 980__ $$aWashU Researcher Data