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Ims 6 f

Manufactured by Cameca

The IMS 6 F is a secondary ion mass spectrometer (SIMS) manufactured by Cameca. It is designed to perform high-sensitivity, high-resolution elemental and isotopic analysis of solid samples. The IMS 6 F utilizes a focused primary ion beam to sputter material from the sample surface, and the resulting secondary ions are analyzed by a mass spectrometer to determine their elemental and isotopic composition.

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4 protocols using ims 6 f

1

Depth Profiling via SIMS Analysis

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The experiments were performed in an UHV system for secondary ion mass spectrometry (SIMS, IMS 6f, Cameca) to obtain depth composition profiles. A Cs+ primary ion beam of impact energy of 15 keV was employed to analyze the samples. The beam current was 50 nA, and the beam reached the sample through a 150 μm × 150 μm size of raster; the generated secondary ions were collected by detector through 33π μm2 size of aperture.
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2

SIMS Depth Profiling of Mn-Containing Layers

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The SIMS measurements have been performed in a Cameca IMS 6 F using either 133Cs+ or ions, and are presented in Fig. 8 for samples A, B and R. The profiles confirm the nominal thickness of the Mn-containing layers (30 nm) and are consistent with the Mn concentration established from the saturation moment at 2 K (2.4 and 2.5% for samples A and B, respectively, as given in the main text).
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3

Thermal Evaporation of Bi2S3 and Te Films

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The Bi2S3 powder (99%) and Te (99.8%) were purchased from Sigma-Aldrich and used directly as evaporation sources. Bi2S3 and Te films were deposited using the same thermal evaporator via a standard procedure. The substrate temperature was maintained at RT, and the vacuum pressure before evaporation was ~3 × 10−6 Torr. The distance between the substrate and Bi2S3/Te-loaded tungsten boat was ~20 cm. The thickness of the Bi2S3/Te film was monitored during deposition. The as-deposited samples were then annealed at different temperatures for 30 min in a N2-filled glove box. The crystal structures of the films on glass were analyzed using XRD with Cu Kα radiation (Bruker D8 ADVANCE). AFM images were obtained using a Nanoscope V Multimode 8 (Bruker, Newark, DE, United States of America) on Si substrates. Optical absorption spectra were obtained using a UV–visible spectrophotometer (V-770, JASCO). Samples for HRTEM characterization were prepared using a focused ion beam (FIB). The images and FFT patterns were obtained using HRTEM (JEOL JEM 2100 F). XPS analysis was performed using a PHI 5000 VersaProbe instrument (Ulvac-PHI, Japan). The depth element distribution was measured by SIMS (IMS 6 F, CAMECA). The Hall measurements of the films were performed in an N2-filled glove box using the van der Pauw method with a 0.51 T magnet at RT.
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4

REE Composition Analysis of Apatite and Merrillite

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The REE compositions of apatite and merrillite were determined with the Cameca IMS-6f instrument at Hokkaido University. Before measurements, the polished sections of DaG 978 were carbon-coated. The procedure was similar to that described in refs 35 , 36 . The primary beam was mass filtered 16O of –14.5 keV and irradiated on the sample surface to a diameter of ∼25 μm. The primary beam current is 10–15 nA. Kinetic energy filtering was used to reduce interferences from molecular ions by offsetting the sample acceleration voltage (–100 eV). The energy bandwidth was 20 eV. The exit slit was set to a mass resolving power of ∼500. Positive secondary ion intensities were counted for 10 s with an electron multiplier detector in magnetic peak-jumping mode. Each analysis included 15 cycles. Relative sensitivity factors between secondary ion intensity and concentration for each REE (relative to Ca) were determined using the Takashima augite, for which REE contents have been well determined by instrumental neutron activation analysis37 .
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