@article{c6e1c083417e45dfa79981d313843c8a,
title = "Depth profiling and standardization from the back side of a sample for accurate analyses: Emphasis on quantifying low-fluence, shallow implants in diamond-like carbon",
abstract = "Rationale: Back-side thinning of wafers is used to eliminate issues with transient sputtering when analyzing near-surface element distributions. Precise and accurate calibrated implants are created by including a standard reference material during the implantation. Combining these methods allows accurate analysis of low-fluence, shallow features even if matrix effects are a concern. Methods: Implanted Na (<2.0 × 1011 ions/cm2, peaking <50 nm) in diamond-like carbon (DLC) film on silicon (solar wind returned by NASA's Genesis mission) was prepared for measurement as follows. Implanted surfaces of samples were epoxied to wafers and back-side-thinned using physical or chemical methods. Thinned samples were then implanted with reference ions for accurate quantification of the solar wind implant. Analyses used a CAMECA IMS 7f-GEO SIMS in depth-profiling mode. Results: Back-side-implanted reference ions reduced the need to change sample mounts or stage position and could be spatially separated from the solar wind implant even when measuring monoisotopic ions. Matrix effects in DLC were mitigated and the need to find an identical piece of DLC for a reference implant was eliminated. Accuracy was only limited by the back-side technique itself. Conclusions: Combining back-side depth profiling with back-side-implanted internal standards aides quantification of shallow mono- and polyisotopic implants. This technique helps mitigate matrix effects and keeps measurement conditions consistent. Depth profile acquisition times are longer, but if sample matrices are homogeneous, procedural changes can decrease measurement times.",
author = "Rieck, {Karen D.} and Jurewicz, {Amy J.G.} and Hervig, {Richard L.} and Peter Williams and Olinger, {Chad T.} and Wiens, {Roger C.} and Ogliore, {Ryan C.}",
note = "Funding Information: This work has been supported in large part by National Aeronautics and Space Administration (NASA) Laboratory Analysis of Returned Samples grants. Specifically, support at ASU and Caltech was provided by 80NSSC22K0589 (A.J.G.J.) and NNX09AC35G (D. S. Burnett and A.J.G.J.). Support at LANL was provided by NASA awards NNH15AZ67I and NNH09ZDA001N (R.C.W. and K.D.R.). Support at NMC and LANL was provided by 80NSSC19K1239 (K.D.R. and R.C.W.). This work has also been supported by the NASA Earth and Space Science Fellowship: PLANET14R-0012 (NASA Earth and Space Science Fellowship 2012-13, 2013-14, and 2014-15; R.L.H. and K.D.R.; ASU). SIMS analyses performed at the Arizona State University National SIMS Facility were supported by the National Science Foundation's (NSF) Division of Earth Sciences (EAR0622775). Use of the Center for Nanoscale Materials at Argonne National Laboratory was supported by the US Department of Energy, Office of Science, Office of Basic Energy Sciences (Contract DE-AC02-06CH11357). Special thanks to the Genesis curation team at Johnson Space Center, the Secondary Ion and Mass Spectrometry Lab (ASU), the Center for Meteorite Studies (ASU), the W. M. Keck Foundation Laboratory for Environmental Biogeochemistry (ASU), the Caltech Microanalysis Center, the UCLA MegaSIMS Laboratory, the LeRoy Eyring Center for Solid State Science (ASU), the NanoSIMS Facility (ASU), the Secondary Ion and Mass Spectrometry Lab (WUSTL), Leonard Kroko Inc., D. S. Burnett, F. Stevie, V. Heber, I. V. Veryovkin, C. Miller, and C. Jones. Funding Information: SIMS analyses performed at the Arizona State University National SIMS Facility were supported by the National Science Foundation's (NSF) Division of Earth Sciences (EAR0622775). Use of the Center for Nanoscale Materials at Argonne National Laboratory was supported by the US Department of Energy, Office of Science, Office of Basic Energy Sciences (Contract DE‐AC02‐06CH11357). Funding Information: This work has been supported in large part by National Aeronautics and Space Administration (NASA) Laboratory Analysis of Returned Samples grants. Specifically, support at ASU and Caltech was provided by 80NSSC22K0589 (A.J.G.J.) and NNX09AC35G (D. S. Burnett and A.J.G.J.). Support at LANL was provided by NASA awards NNH15AZ67I and NNH09ZDA001N (R.C.W. and K.D.R.). Support at NMC and LANL was provided by 80NSSC19K1239 (K.D.R. and R.C.W.). This work has also been supported by the NASA Earth and Space Science Fellowship: PLANET14R‐0012 (NASA Earth and Space Science Fellowship 2012‐13, 2013‐14, and 2014‐15; R.L.H. and K.D.R.; ASU). Publisher Copyright: {\textcopyright} 2022 The Authors. Rapid Communications in Mass Spectrometry published by John Wiley & Sons Ltd.",
year = "2023",
month = mar,
day = "30",
doi = "10.1002/rcm.9454",
language = "English (US)",
volume = "37",
journal = "Rapid Communications in Mass Spectrometry",
issn = "0951-4198",
publisher = "John Wiley and Sons Ltd",
number = "6",
}