weaver_1981 =========== J\. H\. Weaver, C\. Krafka, D\. W\. Lynch and E\. E\. Koch, Optical Properties of Metals, Part II\: Noble Metals, Aluminum, Scandium, Yttrium, the Lanthanides and the Actinides \(0\.1 \<= hv \<= 500 eV\), Physik Daten / Physics Data Nr\. 18\-2 \(Fachinformationszentrum Energie, Physik, Mathematik, Karlsruhe, 1981\), ISSN 0344\-8401 `Source record `__ · :doc:`Catalogue ` · :doc:`Review register ` No DOI is recorded. **Source kind:** compilation **Recorded technique:** A data compilation \(the companion volume, Nr\. 18\-1, has the transition metals Ti\-Ni, Zr\-Pd, Hf\-Pt\)\. For each element\: a survey table of the published work \(authors, energy range, technique, temperature, sample\: film, crystal or bulk and its preparation, data presentation, remarks\), a survey figure of the energy ranges, figures comparing the reflectance, epsilon\_1, epsilon\_2 and the absorption coefficient from the literature, and one table of the authors' choice of 'most reliable' optical constants\: E \(eV\), epsilon\_1, epsilon\_2, n, k, Im\(\-1/epsilon\) and R\(phi = 0\)\. ALUMINIUM \(pp\. 79\-86\)\: 'publication by E\. Shiles, T\. Sasaki, M\. Inokuti, and D\.Y\. Smith in Phys\. Rev\. B 22, 1612 \(1980\) based on the following tabulation', i\.e\. Shiles et al\.'s Kramers\-Kronig analysis of compiled data with sum\-rule tests \(shiles\_1980\)\. GOLD \(pp\. 64\-69\)\: 'Unpublished reflectance data for electropolished Au\(110\) by J\.H\. Weaver \(0\.2 \<= hv \<= 4 eV\) and C\.G\. Olson and D\.W\. Lynch \(~4 \<= hv \<= 30 eV\)\. Optical constants determined by Kramers\-Kronig analysis\.' **Materials in structured entries:** Al, Au **Dataset quantities:** extinction\_coefficient, permittivity\_imaginary, permittivity\_real, refractive\_index **Contents:** 12 datasets; 0 formulas. Curation notes -------------- IDENTITY AND LIBRARY\. original/source\_01 \(Cover\-2\.pdf, 28 pdf pages\) is the front matter\: title pages \(pdf pp\. 1\-2\), acknowledgements, preface, the introduction \(Definitions; Methods of Measurement and Errors; Use and Misuse of the Data; pdf pp\. 5\-24\), its 67 references \(pdf pp\. 25\-27\) and Table 1, the abbreviations \(pdf p\. 28\)\. source\_02 Ag\.pdf \(11 pages ending with the table on book pp\. 52\-53; supplement\_01\), source\_03 Al\.pdf \(pp\. 70\-86; supplement\_02\), source\_04 Au\.pdf \(pp\. 54\-69; supplement\_03\), source\_05 Bibliography\-2\.pdf \(pp\. 239\-256; supplement\_04, text only\)\. The copper chapter is not in the library \(J\. C\. Travers's scan, pp\. 32\-42, is described below\)\. The citation is the library's asserted BibTeX \(no DOI; ISSN 0344\-8401 and 'Nr\. 18 \- 2', 1981, from pdf p\. 1\)\. Page numbers below are the book's printed page numbers \('\-79\-'\)\. WHAT THE INTRODUCTION SAYS \(source\_01 pdf pages\)\. Range 25 A \<= lambda \<= 25 um, ~0\.05 \<= hv \<= 500 eV, hv \(eV\) = 12398/lambda \(A\) \(pdf p\. 5\)\. Convention exp\(\-i omega t\), epsilon = epsilon\_1 \+ i epsilon\_2, N = n \+ ik = sqrt\(epsilon\), epsilon\_1 = n^2 \- k^2, epsilon\_2 = 2nk, R = \(\(n \- 1\)^2 \+ k^2\)/\(\(n \+ 1\)^2 \+ k^2\) at normal incidence, mu = 4 pi k / lambda, loss function Im\(\-1/epsilon\) = epsilon\_2/\(epsilon\_1^2 \+ epsilon\_2^2\) \(pdf pp\. 8, 13\-14\)\. Kramers\-Kronig of the reflectance\: 'the extrapolation errors affect the magnitude of epsilon\_1 and epsilon\_2 much more than they affect the positions and shapes of spectral structures'; for Mo their dispersion\-integral results over 0\.1\-30 eV agree with photometric and ellipsometric data 'to within 10%, while an error analysis yields an estimate of possible errors of up to 50%' \(pdf p\. 17\)\. Electropolishing leaves 'a smooth, strain\-free surface, but one with an overlayer of oxide', which 'causes little error in the infrared reflectance, but above about 6 eV the 2p electrons of oxygen absorb and cause errors' \(pdf p\. 20\)\. The tabulated data 'were measured with bulk samples' and are less suitable than film data for modelling evaporated films \(pdf p\. 21\)\. UNCERTAINTY\: 'We believe that the data tabulated are good to within \+\-10% in most cases \(except near places where epsilon\_1 crosses zero, for which a relative error is meaningless\)' \(pdf p\. 22\), recorded as relative 0\.10, level not stated, on the n and k datasets of both metals\. The anomalous skin effect was ignored in obtaining epsilon \(pdf p\. 23\)\. 'We have presented room temperature or liquid helium temperature data only' \(pdf p\. 23\)\. ALUMINIUM TABLE \(pp\. 79\-86; datasets n\_Al, k\_Al primary, eps1\_Al, eps2\_Al check\)\. Supplement\_02 tables tbl\_41f659cbf54e \(p\. 79\), tbl\_41f03578c473 \(80\), tbl\_550bc2056f85 \(81\), tbl\_6b7f728e7af0 \(82\), tbl\_5937497d4313 \(83\), tbl\_7ae05093ee33 \(84\), tbl\_b1243e5e0609 \(85\), tbl\_bd839bc39e50 \(86\)\: the page order is the pdf order, each page continuing the last \(0\.190/0\.195, 1\.460/1\.480, 14\.400/14\.500, 25\.500/26\.000, 72\.400/72\.500, 111\.000/112\.000, 340\.000/350\.000 eV\)\. 447 rows, 0\.040\-1551\.000 eV, energies as printed \(1049\.999, 1099\.999 \.\.\.; 0\.002 eV steps at 0\.04\-0\.1 eV growing to 0\.05 eV at 0\.6\-1\.2 eV, 0\.02 eV over the 1\.5 eV interband peak, 0\.05 eV at 14\.5\-16 eV around the plasma edge, 0\.1 eV at 72\-74 eV at the L edge, 10\-50 eV above 200 eV and 1\-2 eV again at 1540\-1551 eV\), E, epsilon\_1, epsilon\_2, n, k, Im\(\-1/epsilon\) to three decimals and R to four; the loss function and R are kept in printed\. Each page was compared with its image\. PROVENANCE\: the book is where this tabulation was first printed\: shiles\_1980 \(the analysis\) says its full tabulation 'will be given elsewhere', citing Ref\. 12, 'E\. Shiles and D\. Y\. Smith \(unpublished\)'; so the datasets are this record's, with no reproduced\_from, and shiles\_1980 is the analysis \(compiled reflectance, ellipsometry and absorption data joined by Kramers\-Kronig and sum\-rule tests, with kappa above the L edge reduced ad hoc by 14 % to satisfy the f\-sum rule\: see that record\)\. ordal\_1983's Shiles block is a reproduction of this table \(reproduced\_from shiles\_1980 and this record\); rakic\_1995 took Shiles et al\.'s k above 14\.9 eV through Palik's Handbook \(Smith, Shiles and Inokuti\), which is why it agrees with this table from ~35 eV\. CHECKS \(2026\-09\-28\)\: in every row epsilon = N^2 holds within the bound set by the printed rounding \(worst 0\.97 of it, 0\.650 eV\), Im\(\-1/epsilon\) from epsilon within its bound \(worst 0\.99, 1\.280 eV\) and R from N within 0\.0016 \(all within the bound\) once three library misreadings are fixed in the script against the images \(1\.700 eV R \.8977 for \.8972; 27\.000 eV epsilon\_1 0\.700 for 0\.706; 134\.000 eV Im\(\-1/epsilon\) 0\.036 for 0\.038\), and one misprint is corrected by erratum \(17\.500 eV k printed 0\.036 for 0\.038\)\. k = 0\.000\: from 500 eV k prints 0\.000 in all 47 rows \(500\-1551 eV; and epsilon\_2 0\.000 from 600 eV, Im\(\-1/epsilon\) 0\.000 from 600 eV\)\: kept as printed, but these rows carry no absorption information \(k \< 0\.0005 only; k = 0 cannot be used for an absorbing model\)\: the range is cut at review\. Above ~350 eV n also rounds to 0\.996\-1\.000 \(delta = 1 \- n to one or two figures only\)\. ALUMINIUM COMPARISONS \(2026\-09\-28; interpolated in this table\)\. ordal\_1983's Shiles block \(26 points, 323\-16100 cm\-1, 0\.040\-2\.0 eV, three figures\)\: n within 0\.85 % and k within 0\.41 % \(medians 0\.01 % and 0\.05 %\), its rounding\: a faithful copy\. ordal\_1988 \(40 points, 0\.043\-1\.86 eV, their own Kramers\-Kronig with the cavity data, which uses Shiles et al\. above 320 cm\-1\)\: n 2\.1 % higher \(median; up to 3\.0 % at 1\.61 eV\), k 1\.1 % higher \(up to 1\.35 %\); e\.g\. 1\.0 eV 1\.233 \+ 12\.61i against 1\.212 \+ 12\.46i\. rakic\_1995 \(film data to 14\.9 eV, Shiles et al\.'s k above\)\: 0\.05 eV 68\.5 \+ 164\.8i against 75\.0 \+ 172\.2i \(n \-9 %, k \-4 %\), 1\.0 eV 1\.316 \+ 12\.24i against 1\.212 \+ 12\.46i, 2\.0 eV 1\.366 \+ 7\.405i against 1\.304 \+ 7\.479i, 5\-10 eV within 1\-5 % in k, at the plasma edge \(15 eV\) n 0\.151 against 0\.125 and k 0\.110 against 0\.153, from ~35 eV the same to this table's three decimals\. mcpeak\_2015's film \(200\-1700 nm\) against this table\: \|epsilon\| 21\-31 % smaller \(31 % at 200 nm, 24 % at 500 nm, 21\-22 % at 800\-1700 nm; 1550 nm\: \-197\.9 \+ 38\.1i against \-252\.6 \+ 46\.1i\)\. GOLD TABLE \(pp\. 64\-69; datasets n\_Au, k\_Au primary, eps1\_Au, eps2\_Au check\)\. Supplement\_03 tables tbl\_e1aa4a8fd3ac \(p\. 64, 49 rows\), tbl\_0099904bfe57 \(65, 57\), tbl\_3b6da8494ea6 \(66, 57\), tbl\_c59b9057cc82 \(67, 57\), tbl\_22fe363af672 \(68, 57\), tbl\_e323eaae89b9 \(69, 7\), in page order\. 284 printed rows, 0\.10\-30\.00 eV \(0\.05 eV steps to 1 eV, 0\.1 eV to 2 eV, 0\.05 eV to 2\.3 eV, 0\.02\-0\.03 eV to 3 eV, 0\.05 eV to 5 eV, 0\.1 eV to 16 eV, 0\.2 eV to 30 eV\), E, epsilon\_1, epsilon\_2, n, k, Im\(\-1/epsilon\) to two decimals and R to three \(epsilon also two decimals when large, e\.g\. \-6794\.55 at 0\.10 eV\)\. The book is now the printed source, so its rows are the primary data \(n, k to two decimals\: at 1\-1\.7 eV n = 0\.13\-0\.08 carries only one or two figures; epsilon is the more precise there\)\. CHECKS \(2026\-09\-28\)\: the library's cells were compared one by one with an independent transcription of the page images \(made before the pages entered the library, from J\. C\. Travers's scans\)\: they agree except four library misreadings, fixed in the script against the images \(2\.20 eV R \.980 for \.880; 2\.50 eV epsilon\_1 \-1\.96 for \-1\.86; 19\.40 eV k 0\.76 for 0\.78; 28\.80 eV epsilon\_2 0\.65 for 0\.85\)\. Then epsilon = N^2 holds in every row within the printed rounding \(worst 0\.93 of the bound, 15\.50 eV\) and Im\(\-1/epsilon\) within its \(worst 0\.97, 1\.90 eV\)\. The printed R is not the R of the printed n, k\: from about 2\.7 eV up, \|\(N \- 1\)/\(N \+ 1\)\|^2 exceeds the printed R by up to 0\.0064 \(24\.20 eV\: \.119 against 0\.125\), and falls below it by up to 0\.0049 elsewhere; R is presumably the measured reflectance the analysis started from \(not stated\)\. THE BOOK'S MISPRINTS \(errata; register entries for review\)\: the energy after 6\.50 eV is printed '6\.50' again \(p\. 66; the sequence and the workbook have 6\.60; row id '6\.50 \(repeat\)'\), '26\.50' is printed for 26\.60 \(p\. 68\); the 8\.40 eV row is printed twice, identically \(p\. 66\)\: the repeat, row id '8\.40 \(repeat\)', is excluded\. So 283 rows are used\. THE WORKBOOK'S COPY OF THE GOLD TABLE \(datasets sheet\_n\_Au, sheet\_k\_Au, sheet\_eps1\_Au, sheet\_eps2\_Au, all check\)\. J\. H\. Weaver's website workbook, the file behind babar\_2015 \(optical\-constantsCuAgAu\.xlsx, sheet 'JHW\-Au\-ZAED', fetched 2026\-09\-28 and attached to babar\_2015's paper in the library\)\: 217 rows, 0\.1\-30 eV, E \(eV\), R, n, k, e1, e2 \(no loss function\), on a grid of 0\.1 eV to 1 eV, 0\.2 eV to 2 eV, 0\.1 eV to 4\.4 eV, 0\.2 eV to 6 eV, 0\.1 eV to 16 eV and 0\.2 eV to 30 eV \(it leaves out 66 of the book's rows, all below 6 eV\)\. Its e1, e2 are the book's \(five figures where \|epsilon\| \>= 1000, e\.g\. \-6794\.6 for \-6794\.55\) and its n, k are sqrt\(e1 \+ i e2\) of them to five figures \(to 6\.4e\-5 relative\), not the book's two\-decimal n, k\. Against the book, now settled on the library's cells and the images\: the SHEET is wrong at 12\.2 eV \(e2 2\.02; the book 2\.03\), 17\.6 eV \(e1 0\.86, copying the 17\.8 eV row; the book 0\.85\) and 21\.4 eV \(e1 0\.23; the book 0\.27, which with the book's n = 1\.03, k = 0\.88 is consistent; the sheet's n, k there, 1\.0135, 0\.8929, are off by 1\.6 %\), and at 11\.4 eV \(R 0\.11 for the book's \.111\)\. No book erratum follows from them\: they are copying errors of Babar and Weaver's sheet\. Otherwise the sheet's n, k round to the book's except at 27 rows \(by at most 0\.0071\: the book's n, k were computed from unrounded epsilon\) and the book's loss function agrees with the sheet's epsilon but for rounding \(11 rows, 0\.009 or less\)\. The sheet's energies 6\.6 and 26\.6 confirm the two energy errata\. Against ordal\_1983's copy \(Table 3's Weaver block, 21 rows, 807\-16100 cm\-1, reproduced\_from this record\)\: the same to its three figures \(k within 0\.14 at 41\.7, 0\.3 %\)\. GOLD\: SAMPLE, TEMPERATURE\. Electropolished Au\(110\) single crystal \(p\. 64 heading\), bulk\. The Au survey table \(p\. 57, 'Au\-4'\) lists 'We Unpl, 0\.26\-4\.2 eV, Refl, 4\.2 K, X\-tal, EP, A, absorptivity measured by calorimetry'; the bibliography \(p\. 255\) gives 'We Unpub\: J\.H\. Weaver, Unpublished'\. So the 0\.2\-4 eV part of the table MAY BE LIQUID\-HELIUM\-TEMPERATURE ABSORPTIVITY \(4\.2 K\), not room temperature\. The table's heading does not state a temperature, and 'OL Unpub' \(C\. G\. Olson and D\. W\. Lynch, ~4\-30 eV\) has neither a survey\-table entry nor a bibliography entry \(the bibliography has OL81, Olson and Lynch on rare\-earth trifluorides, not this\)\. parameters\.temperature\_k is therefore not set; this should be decided before using the table as room\-temperature gold below 4 eV \(babar\_2015 used this reflectance for its room\-temperature Au analysis, its Fig\. 3\)\. Figs\. 13\-15 \(pp\. 60\-62\: R, epsilon\_1, epsilon\_2 to 30 eV\) show 'We Unpub \(~0\.2\-4 eV\) and OL Unpub \(~4\-30 eV\)' as the solid line among the other authors' data\. OTHER GOLD PAGES \(not extracted\)\. Survey table pp\. 54\-57 \(Au\-1 to Au\-4\: Sa39 to We Unpl, 49 entries\: e\.g\. JC72 = P\. B\. Johnson and R\. W\. Christy, Phys\. Rev\. B 6, 4370 \(1972\), 0\.5\-6\.5 eV films, johnson\_1972; HGK74 = H\. J\. Hagemann, W\. Gudat and C\. Kunz, DESY SR\-74/7 \(1974\), hagemann\_1974; TH70 = M\. L\. Theye, Phys\. Rev\. B 2, 3060 \(1970\), 0\.6\-6 eV uhv films; AKB80 = D\. E\. Aspnes, E\. Kinsbron and D\. D\. Bacon, Phys\. Rev\. B 21, 3290 \(1980\), 1\.5\-5\.8 eV ellipsometry; 'Hun Unpl' 1\.31\-4\.13 eV absorptivity at 4\.2 and 300 K and 'Th Pvt' \(M\. L\. Theye, private communication\), no bibliography entry for Hun Unpl\); Fig\. 12 survey \(pp\. 58\-59\); Figs\. 13\-15; Fig\. 16 absorption coefficient 30\-300 eV \(HGK75 = Hagemann, Gudat and Kunz, J\. Opt\. Soc\. Am\. 65, 742 \(1975\), hagemann\_1975; HKS68 = R\. Haensel, C\. Kunz, T\. Sasaki and B\. Sonntag, Appl\. Opt\. 7, 301 \(1968\); DFR70 = J\. Daniels, C\. v\. Festenberg, H\. Raether and K\. Zeppenfeld, Springer Tracts in Modern Physics 54, p\. 77 \(1970\); WG74 = C\. Wehenkel and B\. Gauthe, Proc\. VI Int\. Conf\. VUV Physics, Hamburg \(1974\) p\. 455\) \(pp\. 60\-63\)\. OTHER ALUMINIUM PAGES \(not extracted\)\. pp\. 70\-72\: survey table Al\-1 to Al\-3 \(Sa39 to RYE77\: e\.g\. BG68 = M\. A\. Biondi and A\. I\. Guobadia, Phys\. Rev\. 166, 667 \(1968\), and BoL70 = L\. W\. Bos and D\. W\. Lynch, Phys\. Rev\. Lett\. 25, 156 \(1970\)\: absorptivity by calorimetry at 4\.2 K on electropolished bulk, 0\.11\-1\.23 and 0\.2\-5 eV; BL75 = R\. L\. Benbow and D\. W\. Lynch, Phys\. Rev\. B 12, 5615 \(1975\), 0\.2\-3 eV single crystal at 4\.2 K; HGK75 13\-150 eV and HGK76 \(Phys\. Stat\. Sol\. B 74, 507 \(1976\)\) 30\-150 eV transmission; HKL77 = T\. Hollstein, U\. Kreibig and F\. Leis, Phys\. Stat\. Sol\. B 83, k49 \(1977\), 1\.77\-2\.95 eV ellipsometry at 1\.5 and 300 K; MM71 = A\. G\. Mathewson and H\. P\. Myers, Phys\. Scripta 4, 291 \(1971\), 0\.7\-2\.5 eV; LM62 \(R\. LaVilla and H\. Mendlowitz\), 12\-18 eV energy loss; GMS60 = A\. I\. Golovashkin, G\. P\. Motulevich and A\. A\. Shubin, Sov\. Phys\. JETP 11, 38 \(1960\)\)\. pp\. 73\-74\: Fig\. 17 survey\. p\. 75\: Fig\. 18 reflectivity 0\-30 eV \(SS80 = E\. Shiles, T\. Sasaki, M\. Inokuti and D\. Y\. Smith, Phys\. Rev\. B 22, 1612 \(1980\), solid\)\. pp\. 76\-78\: Fig\. 19 epsilon\_1, Fig\. 20 epsilon\_2 \(SS80, EPS63, MM71, LM62, HKL77, HGK75, GMS60\), Fig\. 21 absorption coefficient 75\-300 eV \(RSK69, GB70 = C\. Gahwiller and F\. C\. Brown, Phys\. Rev\. B 2, 1918 \(1970\), HGK75\)\. EPS63 and RSK69 are not found in the library's text of the bibliography\. SILVER \(Ag\.pdf, supplement\_01; not extracted\)\. Survey table and figures, then pp\. 52\-53 \(tbl\_495baf394146, tbl\_2489ab9aa2d9\)\: 'Silver\: publication by H\.J\. Hagemann, W\. Gudat, and C\. Kunz in J\. Opt\. Soc\. Am\. 65, 742 \(1975\) based on the following tabulation', 93 rows, 0\.10\-100\.00 eV, two decimals \(R three\)\. It is a two\-decimal reprint of the DESY report's silver table \(hagemann\_1974, Table 4\: three figures, 5 meV to 50 keV, with the absorption coefficient, reflectance, loss function and n\_eff\) on a subset of its energies, so it adds nothing over hagemann\_1974 and is not extracted\. Against the workbook's HGK sheet \(Hagemann et al\.'s silver, 61 common energies, 0\.1\-30 eV\)\: the same to the book's rounding except 11\.00 eV \(epsilon\_1 2\.00 against 2\.08, n 1\.52 against 1\.543\), 13\.00 eV \(epsilon\_1 2\.33 against 2\.392\) and 21\.50 eV \(epsilon\_1 1\.23 against 1\.28\), and at the edges of rounding elsewhere\. The library misreads four cells of this table \(0\.20 eV epsilon\_2 '200\.00' for 260\.00; 3\.50 eV epsilon\_2 '0\.00' for 0\.60; 4\.00 eV n '1\.01' for 1\.61; 10\.00 eV k '0\.50' for 0\.56; checked on the image\)\. The comparison with hagemann\_1974 itself is another extraction's\. COPPER \(J\. C\. Travers's scan Cu\.pdf, pp\. 32\-42; not in the library, not extracted\)\. pp\. 32\-34\: survey table Cu\-1 to Cu\-3 \(Sa39 to We Unpl\: e\.g\. Bio56 = M\. A\. Biondi, Phys\. Rev\. 102, 964 \(1956\), and BG68 absorptivity at 4\.2 K; JC72 and JC75 \(Johnson and Christy, Phys\. Rev\. B 11, 1315 \(1975\)\) 0\.5\-6\.5 eV films; HGK74 13\-150 eV; SeS70 = D\. H\. Seib and W\. E\. Spicer, Phys\. Rev\. B 2, 1676 \(1970\), 0\.5\-11\.8 eV electropolished bulk; 'Ben Unpl' 0\.16\-4\.3 eV and 'We Unpl' 0\.2\-1\.8 eV absorptivity by calorimetry at 4\.2 K on chemically polished bulk\)\. pp\. 35\-36\: Fig\. 2 survey\. pp\. 37\-40\: Figs\. 3\-6\. pp\. 41\-42\: the table, 'Copper\: publication by H\.J\. Hagemann, W\. Gudat, and C\. Kunz in J\. Opt\. Soc\. Am\. 65, 742 \(1975\) based on the following tabulation', 0\.10 eV \(\-4240\.00, 4250\.00, 29\.69, 71\.57, R \.980\) to 17\.00 eV on p\. 41 \(49 rows\) and 18\.00\-61\.00 eV on p\. 42; the scan ends at 61 eV with a row cut off\. The book's copper table is Hagemann et al\.'s \(hagemann\_1974\), not Weaver's own\. RELATED RECORDS\. babar\_2015 used this gold reflectance for its Au analysis \(its Fig\. 3 caption\); its website Au epsilon\_2 is 2\-3 % above this table at 2\-15 eV\. ordal\_1988 cites the book \(its Ref\. 2\) for Shiles et al\.'s aluminium; ordal\_1983 reproduces the aluminium \(Shiles block\) and the gold \(Weaver block\) with reproduced\_from naming this record\. **Recorded bibliographic identity status:** ASSERTED. This concerns identification of the source; it does not establish the scientific correctness of its contents. Datasets -------- weaver\_1981/n\_Al ~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "n_Al", "material": "Al", "file": "Al/weaver_1981__n_Al.csv", "table": "tbl_41f659cbf54e", "quantity": "refractive_index", "abscissa_unit": "eV", "use": "primary", "uncertainty": { "relative": 0.1, "level": "not stated" }, "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of compiled data with sum-rule adjustment (Shiles et al. 1980)" } } Aluminium table, pp\. 79\-86 \(supplement\_02, tbl\_41f659cbf54e \.\.\. tbl\_bd839bc39e50, eight pages in order\)\: n of Shiles, Sasaki, Inokuti and Smith's recommended tabulation, 0\.040\-1551\.000 eV, 447 rows, three decimals as printed; first printed here \(shiles\_1980's Ref\. 12\: 'unpublished'\), so no reproduced\_from\. From 500 eV k prints 0\.000 \(47 rows\) and from about 600 eV epsilon\_2 0\.000\: those rows carry no absorption information \(see notes\)\. weaver\_1981/k\_Al ~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "k_Al", "material": "Al", "file": "Al/weaver_1981__k_Al.csv", "table": "tbl_41f659cbf54e", "quantity": "extinction_coefficient", "abscissa_unit": "eV", "use": "primary", "uncertainty": { "relative": 0.1, "level": "not stated" }, "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of compiled data with sum-rule adjustment (Shiles et al. 1980)" } } Aluminium table, pp\. 79\-86 \(supplement\_02, tbl\_41f659cbf54e \.\.\. tbl\_bd839bc39e50, eight pages in order\)\: k of Shiles, Sasaki, Inokuti and Smith's recommended tabulation, 0\.040\-1551\.000 eV, 447 rows, three decimals as printed; first printed here \(shiles\_1980's Ref\. 12\: 'unpublished'\), so no reproduced\_from\. From 500 eV k prints 0\.000 \(47 rows\) and from about 600 eV epsilon\_2 0\.000\: those rows carry no absorption information \(see notes\)\. weaver\_1981/eps1\_Al ~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "eps1_Al", "material": "Al", "file": "Al/weaver_1981__eps1_Al.csv", "table": "tbl_41f659cbf54e", "quantity": "permittivity_real", "abscissa_unit": "eV", "use": "check", "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of compiled data with sum-rule adjustment (Shiles et al. 1980)" } } Aluminium table, pp\. 79\-86 \(supplement\_02, tbl\_41f659cbf54e \.\.\. tbl\_bd839bc39e50, eight pages in order\)\: epsilon\_1 of Shiles, Sasaki, Inokuti and Smith's recommended tabulation, 0\.040\-1551\.000 eV, 447 rows, three decimals as printed; first printed here \(shiles\_1980's Ref\. 12\: 'unpublished'\), so no reproduced\_from\. From 500 eV k prints 0\.000 \(47 rows\) and from about 600 eV epsilon\_2 0\.000\: those rows carry no absorption information \(see notes\)\. A check\: it repeats n and k \(epsilon = N^2\)\. weaver\_1981/eps2\_Al ~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "eps2_Al", "material": "Al", "file": "Al/weaver_1981__eps2_Al.csv", "table": "tbl_41f659cbf54e", "quantity": "permittivity_imaginary", "abscissa_unit": "eV", "use": "check", "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of compiled data with sum-rule adjustment (Shiles et al. 1980)" } } Aluminium table, pp\. 79\-86 \(supplement\_02, tbl\_41f659cbf54e \.\.\. tbl\_bd839bc39e50, eight pages in order\)\: epsilon\_2 of Shiles, Sasaki, Inokuti and Smith's recommended tabulation, 0\.040\-1551\.000 eV, 447 rows, three decimals as printed; first printed here \(shiles\_1980's Ref\. 12\: 'unpublished'\), so no reproduced\_from\. From 500 eV k prints 0\.000 \(47 rows\) and from about 600 eV epsilon\_2 0\.000\: those rows carry no absorption information \(see notes\)\. A check\: it repeats n and k \(epsilon = N^2\)\. weaver\_1981/n\_Au ~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "n_Au", "material": "Au", "file": "Au/weaver_1981__n_Au.csv", "table": "tbl_e1aa4a8fd3ac", "quantity": "refractive_index", "abscissa_unit": "eV", "use": "primary", "excluded_rows": { "8.40 (repeat)": "The book prints the 8.40 eV row twice (p. 66), identically." }, "uncertainty": { "relative": 0.1, "level": "not stated" }, "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } Gold table, pp\. 64\-69 \(supplement\_03, tbl\_e1aa4a8fd3ac \.\.\. tbl\_e323eaae89b9, six pages in order\)\: n of electropolished Au\(110\), 0\.10\-30\.00 eV, 284 printed rows \(283 used\: the repeated 8\.40 eV row is excluded\), two decimals as printed; energies 6\.50 \(repeat\) and 26\.50 corrected to 6\.60 and 26\.60 by errata\. Temperature not stated\: the 0\.2\-4 eV part may be at 4\.2 K \(the survey table, p\. 57; see notes\)\. weaver\_1981/k\_Au ~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "k_Au", "material": "Au", "file": "Au/weaver_1981__k_Au.csv", "table": "tbl_e1aa4a8fd3ac", "quantity": "extinction_coefficient", "abscissa_unit": "eV", "use": "primary", "excluded_rows": { "8.40 (repeat)": "The book prints the 8.40 eV row twice (p. 66), identically." }, "uncertainty": { "relative": 0.1, "level": "not stated" }, "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } Gold table, pp\. 64\-69 \(supplement\_03, tbl\_e1aa4a8fd3ac \.\.\. tbl\_e323eaae89b9, six pages in order\)\: k of electropolished Au\(110\), 0\.10\-30\.00 eV, 284 printed rows \(283 used\: the repeated 8\.40 eV row is excluded\), two decimals as printed; energies 6\.50 \(repeat\) and 26\.50 corrected to 6\.60 and 26\.60 by errata\. Temperature not stated\: the 0\.2\-4 eV part may be at 4\.2 K \(the survey table, p\. 57; see notes\)\. weaver\_1981/eps1\_Au ~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "eps1_Au", "material": "Au", "file": "Au/weaver_1981__eps1_Au.csv", "table": "tbl_e1aa4a8fd3ac", "quantity": "permittivity_real", "abscissa_unit": "eV", "use": "check", "excluded_rows": { "8.40 (repeat)": "The book prints the 8.40 eV row twice (p. 66), identically." }, "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } Gold table, pp\. 64\-69 \(supplement\_03, tbl\_e1aa4a8fd3ac \.\.\. tbl\_e323eaae89b9, six pages in order\)\: epsilon\_1 of electropolished Au\(110\), 0\.10\-30\.00 eV, 284 printed rows \(283 used\: the repeated 8\.40 eV row is excluded\), two decimals as printed; energies 6\.50 \(repeat\) and 26\.50 corrected to 6\.60 and 26\.60 by errata\. Temperature not stated\: the 0\.2\-4 eV part may be at 4\.2 K \(the survey table, p\. 57; see notes\)\. A check\: it repeats n and k \(epsilon = N^2\)\. weaver\_1981/eps2\_Au ~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "eps2_Au", "material": "Au", "file": "Au/weaver_1981__eps2_Au.csv", "table": "tbl_e1aa4a8fd3ac", "quantity": "permittivity_imaginary", "abscissa_unit": "eV", "use": "check", "excluded_rows": { "8.40 (repeat)": "The book prints the 8.40 eV row twice (p. 66), identically." }, "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } Gold table, pp\. 64\-69 \(supplement\_03, tbl\_e1aa4a8fd3ac \.\.\. tbl\_e323eaae89b9, six pages in order\)\: epsilon\_2 of electropolished Au\(110\), 0\.10\-30\.00 eV, 284 printed rows \(283 used\: the repeated 8\.40 eV row is excluded\), two decimals as printed; energies 6\.50 \(repeat\) and 26\.50 corrected to 6\.60 and 26\.60 by errata\. Temperature not stated\: the 0\.2\-4 eV part may be at 4\.2 K \(the survey table, p\. 57; see notes\)\. A check\: it repeats n and k \(epsilon = N^2\)\. weaver\_1981/sheet\_n\_Au ~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "sheet_n_Au", "material": "Au", "file": "Au/weaver_1981__sheet_n_Au.csv", "table": "data/optical-constantsCuAgAu.xlsx", "quantity": "refractive_index", "abscissa_unit": "eV", "use": "check", "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } The website workbook's sheet 'JHW\-Au\-ZAED' \(Babar and Weaver's copy of the gold table\)\: n, 0\.1\-30 eV, 217 rows, five figures\. Its epsilon is the book's except 12\.2 eV \(e2 2\.02 for 2\.03\) and 17\.6 and 21\.4 eV \(e1 0\.86 for 0\.85, 0\.23 for 0\.27\); its n and k are sqrt\(e1 \+ i e2\) of its own epsilon\. A check on the book's datasets, not data to fit beside them\. weaver\_1981/sheet\_k\_Au ~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "sheet_k_Au", "material": "Au", "file": "Au/weaver_1981__sheet_k_Au.csv", "table": "data/optical-constantsCuAgAu.xlsx", "quantity": "extinction_coefficient", "abscissa_unit": "eV", "use": "check", "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } The website workbook's sheet 'JHW\-Au\-ZAED' \(Babar and Weaver's copy of the gold table\)\: k, 0\.1\-30 eV, 217 rows, five figures\. Its epsilon is the book's except 12\.2 eV \(e2 2\.02 for 2\.03\) and 17\.6 and 21\.4 eV \(e1 0\.86 for 0\.85, 0\.23 for 0\.27\); its n and k are sqrt\(e1 \+ i e2\) of its own epsilon\. A check on the book's datasets, not data to fit beside them\. weaver\_1981/sheet\_eps1\_Au ~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "sheet_eps1_Au", "material": "Au", "file": "Au/weaver_1981__sheet_eps1_Au.csv", "table": "data/optical-constantsCuAgAu.xlsx", "quantity": "permittivity_real", "abscissa_unit": "eV", "use": "check", "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } The website workbook's sheet 'JHW\-Au\-ZAED' \(Babar and Weaver's copy of the gold table\)\: e1, 0\.1\-30 eV, 217 rows, five figures\. Its epsilon is the book's except 12\.2 eV \(e2 2\.02 for 2\.03\) and 17\.6 and 21\.4 eV \(e1 0\.86 for 0\.85, 0\.23 for 0\.27\); its n and k are sqrt\(e1 \+ i e2\) of its own epsilon\. A check on the book's datasets, not data to fit beside them\. weaver\_1981/sheet\_eps2\_Au ~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "sheet_eps2_Au", "material": "Au", "file": "Au/weaver_1981__sheet_eps2_Au.csv", "table": "data/optical-constantsCuAgAu.xlsx", "quantity": "permittivity_imaginary", "abscissa_unit": "eV", "use": "check", "parameters": { "form": "bulk", "technique": "Kramers-Kronig analysis of reflectance (absorptivity below 4 eV)" } } The website workbook's sheet 'JHW\-Au\-ZAED' \(Babar and Weaver's copy of the gold table\)\: e2, 0\.1\-30 eV, 217 rows, five figures\. Its epsilon is the book's except 12\.2 eV \(e2 2\.02 for 2\.03\) and 17\.6 and 21\.4 eV \(e1 0\.86 for 0\.85, 0\.23 for 0\.27\); its n and k are sqrt\(e1 \+ i e2\) of its own epsilon\. A check on the book's datasets, not data to fit beside them\. Formulas -------- No formulas are recorded. Corrections ----------- .. code-block:: text [ { "dataset": "k_Al", "row": "17.500", "column": "value", "printed": "0.036", "corrected": "0.038", "reason": "A misprint of k at 17.500 eV (p. 82): the row's epsilon_1 = 0.269, epsilon_2 = 0.040 and n = 0.520 give k = Im sqrt(epsilon) = 0.0385 (0.038-0.039 over epsilon's rounding) and 2nk = 0.0374 against the printed epsilon_2 0.040; the printed loss function 0.537 agrees with epsilon (0.540), and the neighbours print k = 0.040 (17.250 eV) and 0.036 (17.750 eV). The image prints 0.036 (the library reads it so).", "evidence": "Supplement_02 table tbl_6b7f728e7af0 (book p. 82) and its image; every other of the 447 rows satisfies epsilon = N^2 within the printed rounding." }, { "dataset": "n_Au", "row": "6.50 (repeat)", "column": "x", "printed": "6.50", "corrected": "6.60", "reason": "The energy after 6.50 eV is printed '6.50' again (p. 66) where the 0.1 eV sequence (6.40, 6.50, -, 6.70) and the workbook's copy (6.6) have 6.60; the row's values (0.61, 2.56, 1.27, 1.01) lie between the 6.50 and 6.70 rows.", "evidence": "Supplement_03 table tbl_3b6da8494ea6 (book p. 66) and its image (the digit reads 5, as the library has it); the workbook sheet JHW-Au-ZAED row 6.6 holds the same epsilon, 0.61 and 2.56." }, { "dataset": "n_Au", "row": "26.50", "column": "x", "printed": "26.50", "corrected": "26.60", "reason": "The energy is printed '26.50' (p. 68) between 26.40 and 26.80 eV in a 0.2 eV sequence; the workbook's copy has 26.6 with the same values (0.46, 0.86).", "evidence": "Supplement_03 table tbl_22fe363af672 (book p. 68) and its image; the workbook sheet JHW-Au-ZAED row 26.6." }, { "dataset": "k_Au", "row": "6.50 (repeat)", "column": "x", "printed": "6.50", "corrected": "6.60", "reason": "The energy after 6.50 eV is printed '6.50' again (p. 66) where the 0.1 eV sequence (6.40, 6.50, -, 6.70) and the workbook's copy (6.6) have 6.60; the row's values (0.61, 2.56, 1.27, 1.01) lie between the 6.50 and 6.70 rows.", "evidence": "Supplement_03 table tbl_3b6da8494ea6 (book p. 66) and its image (the digit reads 5, as the library has it); the workbook sheet JHW-Au-ZAED row 6.6 holds the same epsilon, 0.61 and 2.56." }, { "dataset": "k_Au", "row": "26.50", "column": "x", "printed": "26.50", "corrected": "26.60", "reason": "The energy is printed '26.50' (p. 68) between 26.40 and 26.80 eV in a 0.2 eV sequence; the workbook's copy has 26.6 with the same values (0.46, 0.86).", "evidence": "Supplement_03 table tbl_22fe363af672 (book p. 68) and its image; the workbook sheet JHW-Au-ZAED row 26.6." }, { "dataset": "eps1_Au", "row": "6.50 (repeat)", "column": "x", "printed": "6.50", "corrected": "6.60", "reason": "The energy after 6.50 eV is printed '6.50' again (p. 66) where the 0.1 eV sequence (6.40, 6.50, -, 6.70) and the workbook's copy (6.6) have 6.60; the row's values (0.61, 2.56, 1.27, 1.01) lie between the 6.50 and 6.70 rows.", "evidence": "Supplement_03 table tbl_3b6da8494ea6 (book p. 66) and its image (the digit reads 5, as the library has it); the workbook sheet JHW-Au-ZAED row 6.6 holds the same epsilon, 0.61 and 2.56." }, { "dataset": "eps1_Au", "row": "26.50", "column": "x", "printed": "26.50", "corrected": "26.60", "reason": "The energy is printed '26.50' (p. 68) between 26.40 and 26.80 eV in a 0.2 eV sequence; the workbook's copy has 26.6 with the same values (0.46, 0.86).", "evidence": "Supplement_03 table tbl_22fe363af672 (book p. 68) and its image; the workbook sheet JHW-Au-ZAED row 26.6." }, { "dataset": "eps2_Au", "row": "6.50 (repeat)", "column": "x", "printed": "6.50", "corrected": "6.60", "reason": "The energy after 6.50 eV is printed '6.50' again (p. 66) where the 0.1 eV sequence (6.40, 6.50, -, 6.70) and the workbook's copy (6.6) have 6.60; the row's values (0.61, 2.56, 1.27, 1.01) lie between the 6.50 and 6.70 rows.", "evidence": "Supplement_03 table tbl_3b6da8494ea6 (book p. 66) and its image (the digit reads 5, as the library has it); the workbook sheet JHW-Au-ZAED row 6.6 holds the same epsilon, 0.61 and 2.56." }, { "dataset": "eps2_Au", "row": "26.50", "column": "x", "printed": "26.50", "corrected": "26.60", "reason": "The energy is printed '26.50' (p. 68) between 26.40 and 26.80 eV in a 0.2 eV sequence; the workbook's copy has 26.6 with the same values (0.46, 0.86).", "evidence": "Supplement_03 table tbl_22fe363af672 (book p. 68) and its image; the workbook sheet JHW-Au-ZAED row 26.6." } ] Formula corrections, where recorded, appear with their formulas above. Curation notes may also discuss corrections or unresolved interpretation. Consult the :doc:`review register ` for the checks and decisions.