Reliability of BEs in NIST Tables
NOTE:  There are No actual spectra in NIST database, only BEs that are based on Calibration BEs below 400 eV (No Cu (2p3).

 



 

Philosophy of Data Reliability for Data in
The International XPS Database & The XPS Library

Our philosophy is to collect spectra under analysis conditions that are practical, readily reproduced, and typically used in laboratories that use monochromatic X-ray sources and work under real world practical analysis conditions. We have assumed that the most XPS laboratories need practical reference spectra and will not spend the time or money to produce and to analyze pure, clean surfaces under ultimate energy resolution conditions.

These spectra are designed to assist engineers, scientists, analysts, theoreticians, and teachers who use XPS on an everyday basis under practical working conditions. We believe that these spectra will help XPS users to analyze industrial problems, gather reference data, perform basic research, test theories, and teach others. These spectra are designed to be practical tools for everyday use and were obtained under practical working conditions. No attempt was made to produce research grade spectra, but many of the spectra are actually research grade spectra because of the self-consistent methods used.

The elements have been analyzed under conditions that have maximized the accuracy of the binding energies. The binding energies for the pure elements are referenced to the reference energies recommended by the National Physical Laboratory in the UK. Please refer to section “Energy Scale Reference Energies and Calibration Details” for more details about calibration.

If the element is part of insulating chemical compound, then a C (1s) spectrum is also provided to allow the user to correct for sample charging. All narrow scan spectra are peak-fitted to reveal FWHM, peak asymmetry, and peak separation for spin-orbit pairs. The strong signals observed in the wide scan survey spectra are labeled and tabulated together with rough BE values of those strong signals. The details of the experimental protocol used to produce each these spectra are provided in the “Instrument and Analysis Details” section. All pure elements, except for Silicon and Selenium, were ion etched prior to analysis.

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Statistical Analysis of NIST BEs

 

 



 

 

Statistical Analysis of Binding Energies in NIST XPS Database of BEs

Be careful using NIST BEs.  Be sure to study the range of BEs and the energy scale calibration used in the original paper.

 

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Histogram Plots of NIST BEs

for the Elements and Various Common Chemical Compounds

 



 

Reliability and Problems in NIST SRD-20 XPS Data-bank – No Spectra

This data-bank suffers from most, if not all, of the systematic and random errors that trouble many old sources of BE numbers. This occurs because the database incorporated data measured by using different calibration energies, different charge referencing values for the C 1s hydrocarbon moiety, various charge control methods and various analysis conditions on many different instruments. The degree of these problems is partially revealed by the data shown in the Periodic Table.

The biggest problems include: publication usually gives only one calibration BE at <400 eV (no Cu (2p3) BE) and never tells data of last check of BE calibration.

Each data-file in the NIST numerical data-bank includes a category called “Energy Uncertainty”. A random review of 50 files revealed that only half of the files had an Energy Uncertainty value, and there is no indication as to whether the value is the total range or half of the range of uncertainty.

Under the category called “Energy Scale Evaluation”, the system uses the term “Reliable”. The definition, as it is written, i.e. “…within 300 eV of a reference point on the energy scale…” suggests that any BE outside of that 300 eV span should be suspect and may have a large degree of uncertainty especially since most of the measured BEs are referenced to low calibration energies for Ag 3d5/2 (~368 eV) and Au 4f7/2 (~84 eV).  Therefore, BEs above 700 eV are more uncertain.

Under the definition for “Energy Scale Evaluation”, the sentence begins with: “Literature data will not ordinarily be included unless correspondence with at least one point on this energy scale can be determined…” The indirect double negative wording reveals that some data will be included even if it does not have “…at least one point on this energy scale “.

The “General Information” category in this database is said to report the “overall energy resolution”. A random review of 30 data-files for pure elements gave a null result. And, regrettably, the definitions on the “Data Field Definitions” page do not include a definition of “overall energy resolution”.

Another random review of 30 data-files from conductors and insulators indicates that authors seldom report more than one calibration energy and they reported either the Au 4f7/2 or C 1s BE as the sole source of energy calibration. This tendency, if pervasive, greatly increases the uncertainty in BEs greater than 285 eV, the BE for C 1s.

Under the “Charge Reference” category, the database reports that gold (Au) deposition is accepted as a method for charge referencing insulators. Unfortunately, work reported by Kohiki  shows that the use of gold (Au) decoration for charge referencing is not reliable since data derived from this method of charge referencing was found to produce a large degree of uncertainty.

A literature source that defines the justification for using C 1s BE = 284.8 eV for the adventitious hydrocarbon moiety is not provided even though it is used to charge reference thousands of BEs from non-conductive materials. Any government institute for standards (e.g. NIST) should provide a series of references to significant literature work that justifies the use of this value, along with an appropriate uncertainty value. Unfortunately, this sort of supporting documentation is missing.

The NIST use of the term “adventitious hydrocarbon” implies the presence of a chemical compound that is a pure hydrocarbon. Based on this author’s experience, “adventitious carbon” materials are always accompanied by an oxygen-bearing component. A more correct phrase is “adventitious hydrocarbon moieties or components” which better reflects the true nature of “adventitious carbon”.

Version 4.1 of the NIST database provides a list of “Elemental Referenced Data” including a category called “Recommended binding energies for principal photoelectron lines (85 elements)”. These recommended BEs were compared to the mean BEs derived from the BEs of all available pure element BEs listed in v3.4 – v4.1 of the SRD-20 NIST XPS Database. Approximately 40% of the difference values shown in the chart are ≥0.15 eV, which is significantly larger (7X) than the ≤0.02 eV uncertainty attributed to the calibrant BEs listed in the Method of Energy-Scale Calibration.

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Chart showing differences between “Recommended BEs” and “Mean BEs Derived from NIST SRD-20 Database” for pure metals. Derived from analyzing v3.4 of NIST SRD-20.

 

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Histogram showing differences between “Recommended BEs” and “Mean BEs Derived from NIST SRD-20 Database” for pure metals. Derived from analyzing v3.4 of NIST SRD-20.

Based on this fact, it is difficult to understand how to use the BEs of pure conductive elements provided in the NIST SRD-20 XPS database.

A publication by Dr. Powell (NIST) reports a detailed comparison of the BEs of pure elements originally published by JEOL, PHI, Crist and Martensson that provides extensive inter-comparisons of those BEs and a mean BE derived from those BEs. The comparison produced mean differences of 0.02 and a standard deviation of 0.06. Based on the number of professional contributors, this result would make a useful addition to the Recommended BEs section.

Despite the problems and missing features, this dedicated numerical data-bank is useful as a guide for making chemical state assignments.

If statistical analyses or histogram plots that indicate which BE is “most” accurate or most likely, were included then the usefulness of the BEs in this data-bank would be clear. Otherwise, the user of this data-bank needs to be cautious.

This website includes a collection of Histogram Plots from the BEs listed in the NIST Database.

 



 

 

Examples of Histogram Plots using Calibration Metals (Ag, Au, Cu)

 

Silver (Ag) Gold (Au) Copper (Cu)

 

 

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Set of 100+ Histograms for Metals and Oxides in NIST database

 



 

Critical Review of NIST Database of XPS BEs – in Literature

 



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List of XPS experimental details that should be reported with XPS spectra,
but are often not reported in NIST database because
publication references are very old and not complete.

1) Instrument Name: (for example) Thermo K-Alpha, Thermo NEXSA, Kratos Axis Ultra, Kratos Axis Supra, Surface Science Laboratories S-Probe, PHI Quantum 2000, PHI Quantera, Ulvac-PHI Quantes, Ulvac-PHI VersaProbe III, VG ESCALAB 250
2) X-ray Source: (for example)  monochromatic Al Kalpha 1487 eV, achromatic Mg Kalpha, beta 1253 eV, He(I), He(II), synchrotron, with an X-ray angle of incidence: 35 deg (45 deg)
3) X-ray Power:  (for example)  XX mA and XX kV, 210 W (= 15mA x 14 kV)
4) Spectrometer Energy Calibration Details:  (Version #1 example) When peak maximum BEs from high energy resolution spectra of Cu 2p3/2 and Au 4f7/2 were found to deviate outside the accepted error range, the instrument energy scale (work function) was adjusted (calibrated) to give the desired Calibration binding energies (BEs) at 83.96 eV for the Au 4f7/2 line for freshly ion etched metallic gold and the spectrometer dispersion was adjusted to give a BE of 932.62 eV for the Cu 2p3/2 line of freshly ion etched metallic copper. (Version #2 example) On the same day that each sample was analyzed by XPS, the BEs for Cu (2p3/2) and Au (4f7/2) were measured. When the BEs deviated by >0.2 eV from the true BE values, the spectrometer energy scale was adjusted to produce the true BEs for Cu and Au with an error <0.2 eV.
5) Spot (Beam) Size, or Area of Analysis:  (for example)  300 micron spot, 300×700 micron beam size (area of analysis) with an X-ray angle of incidence: 35 deg (45 deg)
6) Charge Neutralizer (electron flood gun) Use: (for example)  The instrument’s on-board charge compensation system was used on all non-conducting samples.  A low voltage beam of electrons from an electron flood gun was operated at ‘X.X’ eV and ‘XX‘ mA settings. The gun included a beam of low voltage Ar ions. The XY positions were adjusted to give the most intense signal with the most narrow FWHM. (HDPE or PP can be used to check these)
7) Effectiveness of Neutralizer: (for example) XY beam position was adjusted until the charge neutralization was deemed to have been fully achieved by monitoring the FWHM and BE of the O 1s signal or C (1s) signal for the hydrocarbon signal of adventitious carbon.  The XY positions of the flood gun were adjusted to give the most intense signal with the most narrow FWHM.
8) Charge Correction (Reference) Procedures(for example) Spectra have been charge corrected (referenced) to force the main (hydrocarbon) signal of the carbon 1s spectrum (adventitious carbon) to appear at 285.0 eV (or 284.6 eV) for all non-conductive specimen samples.  The voltage difference (delta eV) used to charge correct the carbon (1s) was used to charge correct (reference) all other signals from that same sample. A thick gold dot can also be used.  (Note: Very thin deposited films of Gold are not reliable.)
9) Instrument Base Pressure: (for example) 8 x 10-10 Torr (with no samples inside).
10) Instrument Operating Pressure: 5 x 10-8 Torr (with sample inside) or 2 x 10-7 torr when Argon is used with a flood gun or an ion gun.
11) Scan Details, Pass Energy, Number of Sweeps, Step Size, Scan Window: (for example) The C 1s spectra were taken with a minimum of 10 scans with a scan window of 278-295 eV using a 0.05 eV step and 20 eV pass energy.
12) Electron Collection Lens: (for example) Electron take-off angle is 0 degrees with respect to the collection lens (produces max sampling depth). The electron collection angle is 60 degrees.  (Note:  very old XPS used a 6-7 degree electron collection angle.)
13) Spectrometer Resolution Details: (for example) Ag 3d5/2 line FWHM at 10 eV pass energy was 0.48 eV (after ion cleaning).  Ag 3d5/2 line FWHM at 50 eV pass energy was 0.65 eV. Ultimate source resolution for monochromatic Al K(alpha) X-rays is ~0.16-0.21 eV which is broadened by the electron energy analyzer.  The instrumental resolution was determined to be 0.35 eV at 10 eV pass energy using the Fermi edge of the valence band for metallic silver. Ultimate FWHM energy resolution with charge compensation system turned on is <0.68 eV for the FWHM of clean. scraped PET.
14) Software Used for Curve-Fitting: (for example) SDP v8.0, CasaXPS v2.3.35, XPSPeak, Vision 2 Processing Software
15) Peak-shape Fitting Details: (for example)  80% Gaussian/20% Lorentzian, Asymmetric line-shape, XX% Voigt, GHM and LHM, Convolved Voigt
16) Background Used for Curve-Fitting: (for example)  Linear, Iterated Shirley, Sherwood-Proctor, Castle-Vegh, Tougaard
17) Other Curve-Fitting Details as used: (for example)  FWHM, constraints, doublet separations, peak-area ratios controlled, peak BE differences controlled


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Publications about NIST BEs

Search for Greg Grezinski

 



 

Charge Compensation of Insulating Materials (not discussed in NIST database)

Charge compensation of insulating materials was normally handled by using the patented SSI mesh-screen together with a low voltage flood gun of electrons which used an acceleration voltage that was adjusted to 3-4 eV for optimum results. The mesh-screen device uses a 90% transmission electro-formed mesh made of nickel metal that is supported above the surface of the sample by mounting the mesh on a conductive metal frame that is grounded to the sample mount. To achieve good charge compensation the mesh-screen is positioned so that the distance between the mesh and the surface of the sample is between 0.5 – 1.0 mm. When the distance between the mesh-screen and the surface of the sample is greater than 1.2 mm, the usefulness of the mesh screen flood gun system was normally null.

The mesh-screen is understood to function as an electron cut-off lens with some tendency to allow incoming flood gun electrons to focus onto the area being irradiated with monochromatic X-ray beam. This occurs because the X-ray beam does not have a uniform flux density over the area of the beam. In effect, the mesh-screen produces a nearly uniform electric potential at the surface of the sample and allows incoming flood-gun electrons to pass through whenever they are needed (on demand).

The mesh-screen was used on every insulating material except for a few materials that were analyzed before the flood gun mesh-screen method was developed.

 

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