Surface electronic structure of Ni-doped Fe$_3$O$_4$(001)
<p>The main data analysis was done with Wavemetrics Igor Pro 7.08 using user-defined macros.</p><p> <strong>General Remarks</strong></p><p>The calibration factor for our electron analyzer in the laboratory source XPS measurements was determined based on the peak positions of Au 4f7/2 Ag 3d5/2, and Cu 2p3/2 acquired from freshly prepared metallic Au, Ag, and Cu samples. For a pass energy of 50 eV: </p><p>CKE=(MKE-0.58267)/0.99913</p><p>where CKE and MKE represent calibrated and measured kinetic energies, respectively.</p><p>The XPD and FSM patterns throughout this dataset are presented in a file structure: tab-separated YXZT. To obtain the patterns as they were represented in the manuscript, first plot Y vs. X in marker mode. Assign Z and T as marker size and color, respectively.</p><p> </p><p><strong>%%% Figure 1 %%%</strong></p><p> </p><p><strong>Figure 1.a and Figure 1.b</strong></p><p>The high symmetry points:</p><p>|ΓL|= √3π/a</p><p>|ΓX|= 2π/a</p><p>|ΓW|= √5π/a </p><p>|ΓK|= √3π/2a</p><p>|ΓU|= √3π/2a</p><p> <strong>Figure 1.c</strong></p><p>The SBZ boundaries for the bulk and reconstructed cell:</p><p>|ΓX|bulk= √2π/a </p><p>|ΓX|rec= π/a</p><p> <strong>Figure 1.d</strong></p><p>File: "Fig1d.tiff" </p><p>LEED Image (Energy=20 eV)</p><p><strong>Figure 1.e</strong></p><p>File: "Fig1e.txt" </p><p>File structure(Left-to-right): Tab separated YXZT</p><p>The Fermi surface of a pristine Fe3O4(001), excitation: He Ia (21.22 eV)</p><p><strong>Figure 1.f</strong></p><p>File: "Fig1f.txt" </p><p>File structure(Left-to-right): Tab separated YXZT</p><p>The Fermi surface of a pristine Fe3O4(001), excitation: He IIa (40.80 eV)</p><p> </p><p><strong>%%% Figure 2 %%%</strong></p><p> </p><p>Angular distribution maps of photoelectrons excited from their fixed initial-state energy Ei (EF, 0.22 eV, 0.43 eV, 1.29 eV, 1.49 eV and 1.70 eV) mapped versus parallel momentum.</p><p><strong>Figure 2.a </strong></p><p>Files: "Fig2a_EF.txt, Fig2a_0p22eV.txt, Fig2a_0p43eV.txt, Fig2a_1p29eV.txt, Fig2a_1p49eV.txt, Fig2a_1p70eV.txt" </p><p>File structure(Left-to-right): Tab separated YXZT</p><p>The measurements were acquired with a He Ia excitation. </p><p><strong>Figure 2.b </strong></p><p>Files: "Fig2b_EF.txt, Fig2b_0p22eV.txt, Fig2b_0p43eV.txt, Fig2b_1p29eV.txt, Fig2b_1p49eV.txt, Fig2b_1p70eV.txt" </p><p>File structure(Left-to-right): Tab separated YXZT</p><p>The simulations, which were obtained with the RSMS code, were acquired to mimic He Ia excitation. </p><p><strong>Figure 2.c </strong></p><p>Files: "Fig2c_EF.txt, Fig2c_0p22eV.txt, Fig2c_0p43eV.txt, Fig2c_1p29eV.txt, Fig2c_1p49eV.txt, Fig2c_1p70eV.txt" </p><p>File structure(Left-to-right): Tab separated YXZT</p><p>The measurements were acquired with a He IIa excitation. </p><p><strong>Figure 2.d </strong></p><p>Files: "Fig2d_EF.txt, Fig2b_0p22eV.txt, Fig2d_0p43eV.txt, Fig2d_1p29eV.txt, Fig2d_1p49eV.txt, Fig2d_1p70eV.txt" </p><p>File structure(Left-to-right): Tab separated YXZT</p><p>The simulations, which were obtained with the RSMS code, were acquired to mimic He IIa excitation. </p><p> </p><p><strong>%%% Figure 3 %%%</strong></p><p> </p><p><strong>Figure 3.a </strong></p><p>File: "Fig3a.txt" </p><p>"File structure: Tab-separated YYYX, where the first three columns (from left to right) represent spectra taken from the pristine, as-grown, and post-annealed samples, respectively. Column X (Ni 2p) denotes the binding energy.</p><p><strong>Figure 3.b </strong></p><p>File: "Fig3b.txt" </p><p>"File structure: Tab-separated YYYX, where the first three columns (from left to right) represent spectra taken from the pristine, as-grown, and post-annealed samples, respectively. Column X (Fe 2p) denotes the binding energy.</p><p><strong>Figure 3.c-e</strong></p><p>File: "Fig3c.txt, Fig3d.txt, Fig3e.txt " </p><p>File structure(Left-to-right): Tab separated YXZT</p><p> </p><p><strong>%%% Figure 4 %%%</strong></p><p> </p><p><strong>Figure 4.a </strong></p><p>File: "Fig4a_010.txt, Fig4a_110.txt, Fig4ac_kpar.txt" </p><p>File structure (Left-to-right): YY….YY (Fig4a_010.txt, Fig4a_110.txt) vs. X (Fig4ac_kpar.txt)</p><p>Parallel momentum range from k=0 Å-1 to k=1.83 Å-1.</p><p>Energy range Ebin= 0 eV to Ebin= 2.6 eV.</p><p>Plot type: MDC, Sample: Pristine Fe3O4(001), Crystal directions: [010] and [110]</p><p>Note that the data presented in the manuscript were given with a Y-offset.</p><p><strong>Figure 4.b </strong></p><p>File: "Fig4b_010.txt, Fig4b_110.txt, Fig4bd_en.txt" </p><p>File structure (Left-to-right): YY….YY (Fig4b_010.txt, Fig4b_110.txt) vs. X (Fig4bd_en.txt)</p><p>Parallel momentum range from k=0 Å-1 to k=1.83 Å-1.</p><p>Energy range Ebin= 0 eV to Ebin= 2.6 eV.</p><p>Plot type: EDC, Sample: Pristine Fe3O4(001), Crystal directions: [010] and [110]</p><p>Note that the data presented in the manuscript were given with a Y-offset.</p><p><strong>Figure 4.c </strong></p><p>File: "Fig4c_010.txt, Fig4c_110.txt, Fig4ac_kpar.txt " </p><p>File structure (Left-to-right): YY….YY (Fig4e_010.txt, Fig4e_110.txt) vs. X (Fig4ac_kpar.txt)</p><p>Parallel momentum range from k=0 Å-1 to k=1.83 Å-1.</p><p>Energy range Ebin= 0 eV to Ebin= 2.6 eV.</p><p>Plot type: MDC, Sample: Post-annealed 26-ML Ni/Fe3O4(001), Crystal directions: [010] and [110]</p><p>Note that the data presented in the manuscript were given with a Y-offset.</p><p><strong>Figure 4.d </strong></p><p>File: "Fig4d_010.txt, Fig4d_110.txt , Fig4bd_en.txt" </p><p>File structure (Left-to-right): YY….YY (Fig4d_010.txt, Fig4d_110.txt) vs. X (Fig4bd_en.txt)</p><p>Parallel momentum range from k=0 Å-1 to k=1.83 Å-1.</p><p>Energy range Ebin= 0 eV to Ebin= 2.6 eV.</p><p>Plot type: EDC, Sample: Post-annealed 26-ML Ni/Fe3O4(001), Crystal directions: [010] and [110]</p><p>Note that the data presented in the manuscript were given with a Y-offset.</p><p> </p><p><strong>%%% Figure 5 %%%</strong></p><p> </p><p><strong>Figure 5.a </strong></p><p>File: "Fig5a.txt"</p><p>File structure: Tab-separated YYX(Mg Ka) YYX(He Ia), where Y represents spectra taken from the pristine and post-annealed samples from left to right, respectively, and X denotes the binding energies.</p><p><strong>Figure 5.b </strong></p><p>File: "Fig5b.txt"</p><p>File structure : Tab separated YX-YYYX-YX</p><p>YX(Measurement) </p><p>Left-to-right (Y: The spectrum from the pristine sample, X: Binding energy)</p><p>YYYX(TDOS)</p><p>Left-to-right (Y: Spin up, Y: Spin down, Y: Spin Tot, X: Energy(X-offset: 4.943 eV) for NixFe3-xO4 (x=0))</p><p>YX(Gaussian-broadened TDOS) Broadening:0.5 eV</p><p>Left-to-right (Y: Spin Tot, X: Energy)</p><p><strong>Figure 5.c </strong></p><p>File: "Fig5c.txt"</p><p>File structure: Tab separated YX-YYYX-YX</p><p>YX(Measurement) </p><p>Left-to-right (Y: The spectrum from the post-annealed sample, X: Binding energy)</p><p>YYYX(TDOS)</p><p>Left-to-right (Y: Spin up, Y: Spin down, Y: Spin Tot, X: Energy(X-offset: 5.343 eV) for NixFe3-xO4 (x=1))</p><p>YX(Gaussian-broadened TDOS) Broadening:0.5 eV</p><p>Left-to-right (Y: Spin Tot, X: Energy)</p><p><strong>Figure 5.d </strong></p><p>File: "Fig5d.txt"</p><p>File structure: Tab separated YX-YYYX-YX</p><p>YX(Measurement) </p><p>Left-to-right (Y: XP spectrum from the post-annealed sample, X: Binding Energy)</p><p>YYYX(TDOS)</p><p>Left-to-right (Y: Spin up, Y: Spin down, Y: Spin Tot, X: Energy(X-offset: 5.593 eV) for NixFe3-xO4 (x=2))</p><p>YX(Gaussian-broadened TDOS) Broadening:0.5 eV</p><p>Left-to-right (Y: Spin Tot, X: Energy)</p><p><strong>Figure 5.e </strong></p><p>File: "Fig5e.txt"</p><p>File structure: Tab separated Y-YY-YY-X</p><p>Left-to-right (Y:Fe Total PDOS, Y: Fetet PDOS spin up, Y: Fetet PDOS spin down , Y: Feoct PDOS spin up, Y: Feoct PDOS spin down, X: Energy for for NixFe3-xO4 (x=0)) Gaussian Broadening: 0.2 eV</p><p><strong>Figure 5.f </strong></p><p>File: "Fig5f.txt"</p><p>File structure: Tab separated Y-YY-YY-YY-X</p><p>Left-to-right (Y: Ni and Fe Total PDOS, Y: Nioct PDOS spin up, Y: Nioct PDOS spin down , Y: Fetet PDOS spin up, Y: Fetet PDOS spin down, Y: Feoct PDOS spin up, Y: Feoct PDOS spin down, X: Energy(X-offset: 1.93 eV) for NixFe3-xO4 (x=1)) Gaussian Broadening: 0.2 eV</p><p><strong>Figure 5.g </strong></p><p>File: "Fig5g.txt"</p><p>File structure: Tab separated Y-YY-YY-X</p><p>Left-to-right (Y: Ni and Fe Total PDOS, Y: Nioct PDOS spin up, Y: Nioct PDOS spin down, Y: Fetet PDOS spin up, Y: Fetet PDOS spin down, X: Energy(X-offset: 2.12 eV) for NixFe3-xO4 (x=2)) Gaussian Broadening: 0.2 eV</p><p> </p><p><strong>%%% Figure 6 %%%</strong></p><p> </p><p><strong>Figure 6.a </strong></p><p>File: "Fig6a.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, X: Energy) (X-offset: 2 eV)</p><p><strong>Figure 6.b </strong></p><p>File: "Fig6b.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: Ni 2p Energy) </p><p> </p><p><strong>%%% Figure 7 %%%</strong></p><p> </p><p><strong>Figure 7.a </strong></p><p>File: "Fig7a.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: Energy) (X-offset: 2.8 eV)</p><p><strong>Figure 7.b </strong></p><p>File: "Fig7b.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: Fe 2p Energy) </p><p> </p><p><strong>%%% Figure 8 %%%</strong></p><p> </p><p><strong>Figure 8.a </strong></p><p>File: "Fig8a.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: Energy) (X-offset: 1.1 eV)</p><p><strong>Figure 8.b </strong></p><p>File: "Fig8b.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-X</p><p>(Y: (120 ML-Pristine), Y: (50 ML-Pristine), Y: (10 ML-Pristine), X: Energy) </p><p> </p><p><strong>%%% SUPLLEMENTARY INFORMATION %%%</strong></p><p> </p><p><strong>%%% Figure SI3 %%%</strong></p><p> </p><p> File: "FigSI3_pristine.txt, FigSI3_26ML_AG.txt, FigSI3_26ML_PA.txt"</p><p>File structure (Left-to-right): XY1-XY2-XY3… XY9-XY10-XY11-XY12 (AG: As-grown, PA: Post-annealed)</p><p>XY1 – XY9 (Y: Fit Peak, X: Energy) </p><p>XY10 (Y: Cumulative Fit Peak, X: Energy) </p><p>XY11 (Y: Residue, X: Energy) </p><p>XY12 (Y: Shirley BG Subtracted XPS Measurement, X: Energy) </p><p> </p><p><strong>%%% Figure SI4 %%%</strong></p><p> </p><p><strong>Figure SI4.a</strong></p><p> File: "FigSI4_oct.txt"</p><p>File structure(Left-to-right): YYYYYY1-YYYYYY2-YYYYYY3… YYYYYY4-X</p><p>YYYYYY1 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S</p><p>YYYYYY2 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S-2</p><p>YYYYYY3 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S-6</p><p>YYYYYY4 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S-8</p><p>X: Energy</p><p><strong>Figure SI4.b</strong></p><p> File: "FigSI4_tet.txt"</p><p>File structure(Left-to-right): YYYYYY1-YYYYYY2-YYYYYY3… YYYYYY4-X</p><p>YYYYYY1 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S-1</p><p>YYYYYY2 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: Interstitial Tet</p><p>YYYYYY3 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S-3</p><p>YYYYYY4 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Layer: S-7</p><p>X: Energy</p><p>Channeltron positions: 0.00 eV, 0.22 eV, 0.43 eV, 1.29 eV, 1.49 eV and 1.70 eV</p><p> </p><p><strong>%%% Figure SI5 %%%</strong></p><p> </p><p><strong>Figure SI5.a</strong></p><p>File: "FigSI5a_EF.txt, FigSI5a_0p22eV.txt, FigSI5a_0p43eV.txt, FigSI5a_1p29eV.txt, FigSI5a_1p49eV.txt, FigSI5a_1p70eV.txt "</p><p>File structure(Left-to-right): Tab separated YXZT</p><p><strong>Figure SI5.b</strong></p><p>File: "FigSI5b_EF.txt, FigSI5b_0p22eV.txt, FigSI5b_0p43eV.txt, FigSI5b_1p29eV.txt, FigSI5b_1p49eV.txt, FigSI5b_1p70eV.txt "</p><p>File structure(Left-to-right): Tab separated YXZT</p><p><strong>Figure SI5.c</strong></p><p>File: "FigSI5c_EF.txt, FigSI5c_0p22eV.txt, FigSI5c_0p43eV.txt, FigSI5c_1p29eV.txt, FigSI5c_1p49eV.txt, FigSI5c_1p70eV.txt "</p><p>File structure(Left-to-right): Tab separated YXZT</p><p> </p><p><strong>%%% Figure SI6 %%%</strong></p><p> </p><p><strong>Figure SI6.a</strong></p><p>File: "FigSI6a_EF.txt, FigSI6a_0p22eV.txt, FigSI6a_0p43eV.txt, FigSI6a_1p29eV.txt, FigSI6a_1p49eV.txt, FigSI6a_1p70eV.txt "</p><p>File structure(Left-to-right): Tab separated YXZT</p><p><strong>Figure SI6.b</strong></p><p>File: "FigSI6b_EF.txt, FigSI6b_0p22eV.txt, FigSI6b_0p43eV.txt, FigSI6b_1p29eV.txt, FigSI6b_1p49eV.txt, FigSI6b_1p70eV.txt "</p><p>File structure(Left-to-right): Tab separated YXZT</p><p><strong>Figure SI6.c</strong></p><p>File: "FigSI6c_EF.txt, FigSI6c_0p22eV.txt, FigSI6c_0p43eV.txt, FigSI6c_1p29eV.txt, FigSI6c_1p49eV.txt, FigSI6c_1p70eV.txt "</p><p>File structure(Left-to-right): Tab separated YXZT</p><p> </p><p><strong>%%% Figure SI7 %%%</strong></p><p> </p><p><strong>Figure SI7.a</strong></p><p>File: "FigSI7a.tif"</p><p>LEED Image (Energy=20 eV), Sample: Pristine Fe3O4(001)</p><p><strong>Figure SI7.b</strong></p><p>File: "FigSI7b.tif"</p><p>LEED Image (Energy=20 eV), Sample: As-grown 26 ML Ni/Fe3O4(001)</p><p> </p><p><strong>Figure SI7.c</strong></p><p>File: "FigSI7c.tif"</p><p>LEED Image (Energy=20 eV), Sample: Post-annealed 26 ML Ni/Fe3O4(001)</p><p> </p><p><strong>%%% Figure SI8 %%%</strong></p><p> </p><p>File: "FigSI8_XPS_and_UPS.txt, FigSI8_Fe3O4_DOS.txt, FigSI8_NiFe2O4_DOS.txt, FigSI8_Ni2FeO4_DOS.txt"</p><p>Experiment: FigSI8_XPS_and_UPS.txt</p><p>File structure(Left-to-right): Tab separated YYX(Mg Ka) YYX(He Ia), where Y are the spectra taken from the pristine and post-annealed sample left to right, respectively, and X donate the binding energies.</p><p>DOS (Fe3O4): FigSI8_Fe3O4_DOS.txt </p><p>File structure: YYYX(TDOS) - YX(Gaussian-broadened TDOS) Broadening:0.5 eV</p><p>(Y: Spin Tot, Y: Spin up, Y: Spin down, X: Energy) (X-offset: 4.943 eV)</p><p>(Y: Spin Tot, X: Energy) </p><p> </p><p>DOS (NiFe2O4): FigSI8_NiFe2O4_DOS.txt </p><p>File structure: YYYX(TDOS) - YX(Gaussian-broadened TDOS) Broadening:0.5 eV</p><p>(Y: Spin Tot, Y: Spin up, Y: Spin down, X: Energy) (X-offset: 5.343 eV)</p><p>(Y: Spin Tot, X: Energy)</p><p> </p><p>DOS (NiFe2O4): FigSI8_Ni2FeO4_DOS.txt </p><p>File structure: YYYX(TDOS) - YX(Gaussian-broadened TDOS) Broadening:0.5 eV</p><p>(Y: Spin Tot, Y: Spin up, Y: Spin down, X: Energy) (X-offset: 5.593 eV)</p><p>(Y: Spin Tot, X: Energy)</p><p> </p><p><strong>%%% Figure SI9 %%%</strong></p><p> </p><p><strong>Figure SI9.a</strong></p><p>File: "Fig9a.txt"</p><p>File structure: YYYYYY1-YYYYYY2-X</p><p>YYYYYY1 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Fe_oct</p><p>YYYYYY2 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Fe_tet</p><p>X: Energy</p><p><strong>Figure SI9.b</strong></p><p>File: "Fig9b.txt"</p><p>File structure: YYYYYY1-YYYYYY2-YYYYYY3-X</p><p>YYYYYY1 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Fe_oct</p><p>YYYYYY2 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Fe_tet</p><p>YYYYYY3 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Ni_oct</p><p>X: Energy</p><p><strong>Figure SI9.c</strong></p><p>File: "Fig9c.txt"</p><p>File structure(Left-to-right): YYYYYY1-YYYYYY2-X</p><p>YYYYYY1 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Fe_tet</p><p>YYYYYY2 (Y: PDOS eg down, PDOS Tot down, PDOS t2g down, PDOS eg up, PDOS Tot up, PDOS t2g up) Coordination: Ni_oct</p><p>X: Energy</p><p> </p><p><strong>%%% Figure SI10 %%%</strong></p><p> </p><p>File: "FigSI10_010.txt, FigSI10_110.txt, FigSI10_Energy.txt" </p><p>File structure(Left-to-right): YY….YY (FigSI10_010.txt, FigSI10_110.txt) vs. X (FigSI10_Energy.txt)</p><p>Parallel momentum range from k=0 Å-1 to k=1.83 Å-1.</p><p>Plot type: EDC, Sample: Pristine Fe3O4(001), Crystal directions: [010] and [110]</p><p>Note that the data presented in the manuscript were given with a Y-offset.</p><p> </p><p><strong>%%% Figure SI11 %%%</strong></p><p> </p><p><strong>Figure SI11.a </strong></p><p>File: "Fig SI11a.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, X: Energy) (X-offset: 2 eV)</p><p><strong>Figure SI11.b </strong></p><p>File: "Fig SI11b.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: Ni 2p Energy)</p><p><strong>Figure SI11.c </strong></p><p>File: "FigSI11c.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y: Pristine, X: Energy) (X-offset: 2.8 eV)</p><p><strong>Figure SI11.d </strong></p><p>File: "FigSI11d.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: Fe 2p Energy)</p><p><strong>Figure SI11.e </strong></p><p>File: "FigSI11e.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y: Pristine, X: Energy) (X-offset: 1.1 eV)</p><p><strong>Figure SI11.f </strong></p><p>File: "FigSI11f.txt"</p><p>File structure(Left-to-right): Tab separated Y-Y-Y-Y-X</p><p>(Y: 120 ML, Y:50 ML, Y: 10 ML, Y:Pristine, X: O 1s Energy)</p><p> </p>
ShareScore
32/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 4
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 8
- Engagement
- 0