3.2. μ-Raman Spectroscopy
In the case of the µ-Raman measurements, ultramarine was found in all samples (
Figure 3 a). Aside from the main band, around 546 cm
-1, several spectra also featured its first overtone (2ν
1) at 1093-1096 cm
−1 [
12]. The excellent spectrum, presented in
Figure 3 a from H_b, also shows the bands at 258 cm
−1 (S
3− ν
2 symmetric S-S bending), 585cm
−1 (S
2− ν
1 symmetric S-S stretching) and 805 cm
−1 (S
3− ν
1+ν
2 overtone). In the same spectrum, a very weak peak appears at 835 cm
-1 (stretching ν1) [
11], indicating that Aman also used chrome yellow in “Hora de peste Olt”.
In the case of T_g, a better spectrum for chrome yellow was obtained, with 2 vibration bands at 358 cm
-1 (ν
4 symmetric bending ) and at 839 cm
-1 (ν
1 stretching) [
11] being observable (
Figure 3 a). The previously mentioned characteristic Raman bands of vermillion were observed in spectra recorded for H_b, T_r, and T_g. Goethite (α-FeOOH), the compound responsible for the yellow color in yellow ochre, was observed in only one analysis point in H_b (
Figure 3 b), and due to the high fluorescence of the spectrum, only the main band at 387 cm
-1, characteristic of the B
3g phonon [
13], appeared as a very weak peak. On the same sample 2, spectra of hematite (Fe
2O
3), the Fe oxide that gives red ochre its distinct color, were recorded (
Figure 3 b). This compound was identified based on its characteristic vibration modes at 228 cm
−1(A
1g), 248 cm
−1 (E
g), 294 cm
−1 (E
g), 298 cm
−1 (Eg), 412 cm
−1 (E
g), 500 cm
−1 (A
1g), and 610 cm
−1 (E
g) (
Figure 3 b) [
14]. The Raman measurements showed the presence of pararealgar (As
4S
4), the degradation product of the realgar pigment, with an identical chemical composition, in H_b. However, due to the fluorescence and noise of the spectrum, only one band centered around 234 cm
-1 was observed instead of the main doublet at 230 cm
-1 and 236 cm
-1, while the rest of the bands were not present [
15].
In regard to organic molecules based pigments, carbon black (
Figure 3 c) was observed in all samples, with the distinctive features of the D band around 1355-1365 cm
-1 and G band at 1582- 1587 cm
-1 being present [
16]. Prussian blue (
Figure 3 c) was identified solely on samples from “Hora de peste Olt”, with over a dozen µ-Raman spectra showing the characteristic doublet at 2098 cm
-1 and 2152 cm
-1 (C≡N stretching) [
10].
One highly fluorescent spectrum collected from H_b presented bands at 1385 cm
-1, 1430 cm
-1 and 1624 cm
-1 (
Figure 2 c). Reference literature indicates that, in the case of Indian yellow, a natural mixture of the magnesium and calcium salts of euxanthic acid (eux) derived from the urine of cows fed on a diet of mango leaves used until the early 20
th century, it is very difficult to obtain Raman spectra using a 785 cm
-1 wavelength laser [
17]. At this wavelength, the bands are weak and the main ones, in order of intensity, appear at 1626 cm
-1(ν(C-C)eux + δ(C-H)eux + δ(O-H)(C-8)), 1425 cm
-1(ν(C-C)eux + δ(C-H)eux), 1441 cm
-1(ν(C-C)eux + δ(C-H)eux), 1346 cm
-1(δ(C-H)eux + δ(O-H)(C-3′) + ν(C-HC)eux) and 1368 cm
-1(δ(C-H)eux + δ(O-H)(C-3′) + ν(C-HC)eux), respectively [
17]. In the spectrum presented in
Figure 2 c, the weaker bands are not present, while the doublet at 1425 cm
-1, and 1441 cm
-1 appears as a broad shoulder at 1430 cm
-1, and only the main 1624 cm
-1 band is sharp. While other painting materials present bands close to 1624 cm
-1, they also have more intense bands in the region of 1500 cm
-1-1700 cm
-1, which makes their assignment inadequate or were not available at the time of the creation of the works of art. For the band at 1385 cm
-1, the most likely source is a very disordered graphite grain located in the vicinity of the Indian yellow. Disordered graphite with a very intense D band and a low G band has been documented at similar wavelengths [
18], and its presence is probably associated with carbon black.
3.3. XRD
The minerals present in the 4 samples were identified based on their XRD patterns with their most important peaks highlighted (
Figure 4) and the complete list of entries for each sample being presented in supporting information (
Figure S1-4). The peaks of hydrocerrusite overlap with most of the cerussite peaks, and as such, it was chosen to highlight the peaks of hydrocerrusite, highlighting only the distinctive cerrusite peak at 25.47.
For quartz, whose main peak at 2θ=26.64 overlaps with the second most intense peak of cinnabar, it was chosen to indicate the position of this peak.
The analysis of the diffraction pattern shows that all samples contain both hydrocerussite and cerussite, the two main components of the lead white pigment. Their presence can be attributed to both the use of lead white as a pigment in itself and as a component in the preparation layer of the canvas.
For “Teleleice în Harem”, XRD analysis showed the presence of kaolinite in both samples. Impurities of kaolin, such as muscovite, were found T_g, while quartz was identified in T_r. The presence of quartz cannot be solely attributed to the use of kaolin, as cinnabar and red ochre, other minerals identified by XRD and Raman spectroscopy, are also known to contain quartz impurities.
The identification of cinnabar, the mineral from which the red pigment vermilion is produced, in both “Teleleice în Harem” samples, while other pigments identified via Raman or EDS spectroscopy were not found, is likely due to its higher crystallinity rather than the amount used in the artwork.
For “Hora de peste Olt”, the XRD investigations were able to identify only the materials used in the preparation layer of the painting. As such, alongside the hydrocerussite and cerussite, previously mentioned barite, calcite and dolomite were also encountered. The presence of barite can be attributed to the use of barium white pigment, while calcite and dolomite are components of chalk.
3.4. OM and SEM-EDS
SEM-EDS measurements of the samples proved difficult as they were very brittle, and simple handling in order to mount them with conductive double adhesive tape on Al stubs resulted in them breaking apart. As such, fractured grains were investigated for the T_r, H_band H_g samples. Section investigations were possible for a T_g, as handling resulted in a clean break, and for H_g a grain was encased in resin and sectioned. Elemental compositions of the investigated areas are presented in
Table 2.
Prior to SEM-EDS investigations, OM was performed on the samples chosen for analysis and areas with different color grains were recorded in order to determine the materials used by the painter by correlating feature observed in OM with ones notices in SEM.
Red grains, designated as 1, 2, 3 and 4 in the OM investigations (
Figure 5 a, b, c) of T_r, were analyzed by EDS (
Figure 5 d, e, f, g). The investigations showed that significant amounts of Fe and Hg were present (
Table 2, lines 1-4). The presence of Hg can be straightforwardly attributed to the use of vermillion, HgS, which has a bright intense red color. The rather low amounts of Hg compared to Fe are due to the fact that vermillion has high tinting power, and generally, even a small amount allows for developing the required shade.
The presence of Fe in these red grains can be correlated to the use of red ochres, which was observed in the μ-Raman investigations. Ni is found in most cases in reduced amounts in the area of the red grains, and its presence can be correlated to Ni being an impurity in iron-bearing ores that contain hematite [
19]. The investigations also showed the presence of As (
Table 2, line 5), however, its identification in only one analysis point indicates that the painter made little use of realgar, As₄S₄.
The investigation of several grains that were dislodged from the original sample upon mounting on Al stubs (table 2 lines 5-7,
Figure S5) further confirms the use of red ochre and vermillion, with atomic percentages reaching 26.41% for Fe and 13.61% for Hg. In most analysis points, Pb is found in significant amounts, indicating that Aman made extensive use of the lead white pigment. Its presence also greatly influenced the quantification of S due to the overlap of the Mα
1 at 2,345.5 of Pb, which is intense due to the high amount of Pb, and the Kα
1 at 2,307.84, Kα
2 at 2,306.64 and Kβ
1 at 2,464.04 of S. Due to this, the stoichiometry for both realgar and vermillion is not respected in the atomic percentages. The analysis of these grains also showed important amounts of Zn and Cr, which can be correlated to the use of zinc yellow (4ZnCrO₄·K₂O·3H₂O). Other elements that were encountered include Al, Si, Ca,K, Mg, which can be correlated to the presence of alkali feldspars and kaolin.
Table 2.
Atomic concentrations of elements, as determined by EDS measurements from various analysis points in the investigated samples.
Table 2.
Atomic concentrations of elements, as determined by EDS measurements from various analysis points in the investigated samples.
| No |
C |
N |
O |
Mg |
Al |
Si |
S |
K |
Ca |
Cr |
Fe |
Ni |
Cu |
Zn |
Pd |
Ba |
Au |
Hg |
Pb |
As |
| 1 |
19.63 |
0.81 |
39.65 |
0.56 |
3.89 |
6.14 |
0 |
0.31 |
0.48 |
0.41 |
8.36 |
1.06 |
0.44 |
0.57 |
0.54 |
0.26 |
4.02 |
1.23 |
11.64 |
|
| 2 |
46.82 |
1.16 |
38.86 |
0.52 |
2.03 |
1.85 |
0.01 |
0.18 |
0.54 |
0.23 |
3.21 |
0.19 |
0.05 |
0.28 |
0.1 |
0.04 |
0.79 |
0.09 |
3.04 |
|
| 3 |
51.44 |
0.43 |
35.85 |
0.64 |
1.42 |
1.33 |
0.3 |
0.23 |
1.07 |
0.17 |
3.36 |
0.21 |
0.04 |
0.27 |
0.12 |
0.04 |
0.61 |
0.08 |
2.4 |
|
| 4 |
36.36 |
1.2 |
38.8 |
0.37 |
2.53 |
8.37 |
0 |
0.1 |
0.35 |
0.11 |
3.61 |
0.58 |
0.26 |
0.34 |
0.28 |
0.1 |
2.45 |
0.62 |
3.55 |
|
| 5 |
43.86 |
0.88 |
35.6 |
0.05 |
2.87 |
2.66 |
0 |
0.15 |
0.16 |
|
1.48 |
0.66 |
|
0.25 |
0.43 |
|
1.74 |
0.16 |
7.64 |
1.42 |
| 6 |
56.76 |
1.16 |
17.77 |
0.19 |
2.44 |
0.44 |
1.09 |
0.4 |
0.67 |
1 |
5.1 |
0.69 |
0.62 |
2.27 |
0.24 |
0.15 |
3.93 |
2.52 |
2.59 |
|
| 7 |
31.44 |
0.64 |
8.34 |
0.15 |
1.41 |
0.24 |
1.44 |
0.63 |
0.81 |
1.12 |
26.14 |
1.01 |
0.86 |
3.72 |
0.21 |
0.31 |
6.58 |
13.61 |
1.32 |
|
| 8 |
8.43 |
0.18 |
29.32 |
0.67 |
5.1 |
9.39 |
0 |
1.24 |
0.91 |
0.28 |
23.77 |
1.49 |
1.08 |
0.62 |
0.41 |
0.48 |
6.39 |
2.88 |
7.24 |
|
| 9 |
43.23 |
0.66 |
26.42 |
0.38 |
1.38 |
1.67 |
0 |
1.18 |
0.77 |
3.71 |
4.54 |
0.93 |
0.56 |
5.15 |
0.16 |
|
2.41 |
0.73 |
6.12 |
|
| 10 |
54.08 |
1.29 |
27.33 |
0.25 |
0.84 |
0.75 |
0 |
0.11 |
0.4 |
1.01 |
3.3 |
0.5 |
1.4 |
2.15 |
0.08 |
|
1.92 |
0.46 |
4.14 |
|
| 11 |
11 |
|
56.99 |
3.36 |
1.13 |
2.15 |
1.72 |
0.09 |
9.85 |
0.01 |
0.44 |
|
|
0.06 |
0.31 |
4.25 |
1.45 |
0.05 |
7.14 |
|
| 12 |
34.27 |
|
47.94 |
2.05 |
0.72 |
0.86 |
0.28 |
0.05 |
7.09 |
0.02 |
0.68 |
|
|
0.05 |
0.16 |
1.41 |
1.03 |
0.12 |
3.29 |
|
| 13 |
18.68 |
|
50.5 |
6.34 |
0.43 |
0.71 |
0.07 |
0.15 |
14.62 |
0.09 |
0.6 |
|
|
0.17 |
0.2 |
1.19 |
1.31 |
0.14 |
4.21 |
|
| 14 |
11.86 |
|
54.53 |
0.99 |
0.67 |
1.03 |
4.73 |
0.04 |
5.45 |
0 |
0.33 |
|
|
0.03 |
0.11 |
6.09 |
0.64 |
0.08 |
3.42 |
|
| 15 |
46.83 |
|
30.93 |
0.55 |
5.12 |
1.09 |
2.09 |
0.31 |
0.9 |
0.42 |
5.31 |
|
|
0.65 |
0.37 |
0.23 |
1.7 |
0.8 |
2.72 |
|
| 16 |
7.23 |
|
54.14 |
2.39 |
2.34 |
3.81 |
1.36 |
0.14 |
8.86 |
0.02 |
0.77 |
|
|
0.14 |
0.46 |
4.61 |
2.06 |
0.12 |
11.56 |
|
| 17 |
34.66 |
|
27.98 |
0.41 |
1.35 |
0.89 |
0 |
0.61 |
6.09 |
0.91 |
5.04 |
|
|
0.61 |
0.75 |
1.17 |
5.8 |
0.85 |
12.87 |
|
OM investigations of the section of the T_g grain showed that the stratigraphy of the painting consists of a white preparation layer, followed by a red underlayer on top of which the final pigment and oil layer is situated (
Figure 6). In the EDS mapping of the section for Pb, Al, Si and Fe, we have highlighted two distinct areas A and B that correspond to the white preparation layer and the red underlayer. In area A, there are higher amounts of Pb as opposed to B, while Fe is completely missing, and Al and Si are found on only two to three random grains. This indicates that the preparation layer was made exclusively with lead white. In area B, we find that Pb, Al, Si, and Fe are present, indicating that the red underlayer was composed of lead white, with the addition of red ochre. The kaolin identified in the XRD measurements likely comes from this layer as red ochre is based on siliceous clays, such as kaolin, rich in hematite (Fe
2O
3). The difference in the composition of the layer is obvious when looking at individual grains. As such, the most obvious is grain 3 highlighted in
Figure 6 e) and h), where Pb is completely absent, and the EDS mapping of Fe shows a large, well-defined grain. For the grain indicated with 1 in
Figure 6 d), e), f), g) and i), again we see a depletion of Pb well-defined edges appear for O, Al, Si and K, indicating the presence of a K feldspar, which is a common impurity in kaolin. Another impurity of kaolin quartz was observed due to the presence of Si (
Figure 6 g) and absence of other elements in grains numbered 6 and 7. The grain highlighted with 2 in
Figure 6 d), e), i), j) and k) provided conclusive evidence of the use of the use of zinc yellow, in use since the beginning of the 19
th century, as in that area we observe a depletion of Pb and instead O, K, Zn and Cr are high. In the grains highlighted with 5 and 4 in
Figure 6 e), l) and m), we observe low Pb while Hg and S are high, indicating the presence of vermillion on the very surface within the oil layer of the painting which is high in C and O. The EDS mapping also showed the presence of several Cu-rich grains, highlighted with 8, 9 and 10, which we could not correlate with any particular pigment, as they were not noticed during OM, and the presence of C and O in the binder and in the oil makes it impossible to attribute them to blue or green or other colored pigments, such as azurite, malachite, copper resinate, etc. Only a few random individual analysis points were also recorded in the section, and only the most important ones are presented (
Table 2, lines 9, 10). Their composition mirrors the one in the EDS mapping, with high amounts of Fe from red ochre and significant amounts of Zn, Cr, and K from zinc yellow (4ZnCrO₄·K₂O·3H₂O). Both in the measurements for the red grains and the green grains, the stoichiometry of the zinc yellow is not respected, as Zn is in higher amount, indicating that an excess of ZnO was used in the manufacture of the pigment. Since no blue grains were clearly observed by OM, and ultramarine is a silicate mineral, its presence could not be clearly confirmed.
In the case of the H_b grain chosen for OM and EDS analysis, the sample cracked when handling, and the two largest pieces were then collected in order to be analyzed. Unfortunately, again, during mounting on Al stubs for EDS measurements, the samples cracked, and as such, no correlation with OM images could be performed. The investigations (
Table 2, lines 11, 12, 13, 14) showed that the most abundant metals are Ca, Ba, Pb and Mg. The presence of Ca can be correlated with calcite, and that of Mg in dolomite, both found in chalk. Distinct analysis points where Ca is in very high amounts, 14.62 and 9.85, contain only much smaller amounts of S, indicating that CaCO
3 is present and not gypsum, CaSO
4. Ba and Pb, on the other hand, can be attributed to barium white and lead white, respectively. While Ba is also found in lithopone (a mixture of BaSO
4 and ZnS), the small amounts of Zn in the analysis point indicate that this pigment is not present. Al and Si were found in several areas, indicating the presence of aluminosilicate impurities in the white pigments. In an area (
Table 2, line 15), Fe is encountered in large quantities (5.04), but its presence cannot be clearly attributed to any specific pigment as OM analysis provides no support for the color of the individual analysis point, and Raman analysis proved the presence of Prussian blue, red ochre, and yellow ochre. Other elements are generally in small abundance, and no clear correlations can be made to their presence.
The analysis of H_g grains, mounted on Al stubs, showed a similar composition to the blue ones (
Table 2 lines 16, 17). Again, the most abundant metals are Pb, Ca, Ba, and Mg that can be correlated to the use of lead white, barium white and chalk. The analysis of the green sample encased in resin and sectioned (
Figure 7) showed that the stratigraphy of the painting consists of only the preparation layer (highlighted area in
Figure 7 e, f, g, j, k) and the paint layer. The paint layer could not be highlighted as the encasing resin has a similar composition to the oil rich in C and O. The EDS mapping of the sectioned grain clearly confirms previous results, indicating that in the preparation layer Aman used a mixture of white lead, barium white and chalk (calcite with dolomite impurities).
Unfortunately, the paint layer was very thin and no pigments could be observed. Several distinct grains associated with impurities are observed, and the one highlighted as 1 (
Figure 7 h) contains high amounts of Si. This is obviously a grain of quartz, even though in some areas the EDS mapping shows Ba and Ca. This indicates that the grain is not on the surface, but just below, and Si was detected, as EDS is a volume technique that can reach up to several μm in depth. The same can be said for the grains highlighted as 2 in the Al EDS mapping (
Figure 7 j), which are likely feldspars. Distinct grains containing Fe were noticed (
Figure 7 l), and their presence can be simply attributed to ochre residues on the paint brush when the artist created the preparation layer. Noticeably, no distinct grains of Hg (
Figure 7 m) and Cr (
Figure 7 n) are absent, indicating that in the section, no pigments associated with red or yellow are present in the analyzed area.
3.5. ATR-FTIR Spectroscopy
ATR-FTIR spectroscopy provided complementary molecular information to that obtained by other analytical techniques, contributing to an improved understanding of the materials’ composition and the execution technique. The infrared spectra of the samples are presented in
Figure 8, while the individual assignments of the absorption bands for the T_r, T_g_1, T_g_2, T_g_3, H_b, H_g_1, H_g_2, and H_g_3 samples can be found in
Table S1(ESI). In addition to the information regarding the degradation processes (aging of the drying oil, formation of degradation products), the identified absorption bands were mainly assigned by referring to the absorption bands of the pigments previously detected by Raman, XRD, and EDS spectroscopies.
In all studied samples, the FTIR spectra revealed the presence of the absorption bands associated with the vibrational modes of the carbonate groups from cerussite, including symmetric (between 1058-1061 cm
-1) and antisymmetric (between 1397 – 1401 cm
-1) stretching modes, in-plane (between 676 – 680 cm
-1) and out-of-plane (between 828-838 cm
-1) deformation modes of the CO₃²⁻ anion, as well as of the ν
1 and ν
4 combination bands of CO₃²⁻ (between 1734 – 1739 cm
-1) [
20]. In addition, the presence of the characteristic absorption bands attributed to O–H stretching modes (between 3531 – 3535 cm
-1) and distinct vibrations of Pb–OH bonds (937 cm
-1) of hydrocerusite was observed. The co-existence of these types of bands reflects the mixed nature of the white lead pigment, consisting of variable proportions of cerussite and hydrocerussite [
21], and confirms its extensive use as a white pigment in the analyzed pictorial layers. The presence of quartz in the T_g_1, T_g_2, and H_b FTIR spectra was evidenced by the attendance of the characteristic absorption bands corresponding to Si-O symmetrical bending (691-696 cm
-1), Si-O symmetrical (777 cm
-1, 793 – 800 cm
-1), and asymmetrical stretching (1170 cm
-1) vibrations [
22,
23]. In addition to its usual association with red ochre, quartz frequently appears as an associated material with a range of black (black chalk/graphite), white (calcium carbonate, lead white, kaolin), colored (cinnabar, green earth) pigmentsor texturing agents (clay minerals) [
24].
Kaolinite, present in the T_g_2 sample, exhibits four active IR hydroxyl stretching bands centered at 3689, 3667, 3652, and 3620 cm⁻¹, which originate from distinct types of hydroxyl groups. The three higher-frequency absorption bands belong to the stretching vibrations of the hydroxyl groups located on the inner surface, above the aluminum-oxygen layer, while the lower frequency band from 3620 cm⁻¹ corresponds to the internal hydroxyl group located below the aluminum atoms. In addition, the other two absorption bands from 937 and 910 cm⁻¹ are attributed to the in-plane bending vibrations of the hydroxyl groups from the inner and internal surfaces, respectively. Other absorption bands can be found at 1115 cm
-1 (symmetric Si-O stretching, longitudinal), 1028 and 1002 cm
-1 (in-plane anti-symmetric Si–O stretching), 937 cm
-1 (OH deformation of inner-surface hydroxyl group), 910 cm
-1 (OH deformation of inner hydroxyl groups), 785 cm
-1 (OH translations), and 749 and 692 cm
-1 (Si–O, perpendicular), respectively [
25].
The absorption bands of chrome yellow (PbCrO
4), found in the FTIR spectra of T_g_1, T_g_3, H_b, H_g_1, and H_g_3 samples, were located between 841 – 851 cm
-1 and 751 – 756 cm
-1, corresponding to Cr-O asymmetric and symmetric stretching modes, respectively [
26].
The historic Indian yellow pigment, renowned for its vibrant color derived from the complex euxanthic acid molecule, a conjugate of euxanthone and a glucuronate derivative, holds a significant place in art history. Its identification in the FTIR spectra of T_r, T_g_3, H_b, and H_g_2 samples relies on a set of characteristic absorption bands, as defined by de Faria et al. [
27]. The FTIR spectrum of Indian yellow displays several key diagnostic regions. These include bands between 1622-1627 cm⁻¹ (C–C stretch and C–H/OH bend of the euxanthic ring), 1580-1584 cm⁻¹ (asymmetric COO⁻ stretching combined with O–H bending), and between 1445-1459 cm⁻¹ (resulting from the superposition of C-C/C-H stretching/bending of the euxanthic ring, O-H bending, and asymmetric C-O-C stretching). Other absorption bands can be found at 1545–1550 cm⁻¹ (C–C stretch & C–H bend with C–O–C asym. stretch), 1365-1368 cm⁻¹ (C–H bend, C–C stretch & OH bend), 1235 cm⁻¹ (complex band involving C–C modes, C–O–C bend, and C(euxanthic)–O(glucuronic) stretch), between 1107–1115 cm⁻¹ and 1076–1081 cm⁻¹ (C–O–C asym. stretch and bend modes from the glucuronic ring), 1058–1061 cm⁻¹ (C–O–C asym. stretch from glucuronic ring), and 981–983 cm⁻¹ (C–C/C–H bending from both rings and O–H bend). The clear detection of other reported bands, notably those around 1487, 1423, 1345, 1258, and 1016 cm⁻¹ (see
Table S1 ESI), was hindered by significant spectral overlap with the intense, broad absorption bands of the aged linseed oil binder.
Zinc yellow pigment was identified in T_g_2 and H_b samples. The identification was based on the detection of the characteristic vibrations of the chromate group (CrO₄²⁻) located between 1075 – 1077, 937 – 948, 780-787 cm
-1 (Cr-O asymmetric stretching), 872 -874 cm
-1 (Cr-O symmetric stretching), and between 705 – 711 cm
-1 (O-Cr-O bending), respectively [
28,
29]. The presence of dolomite in T_r, T_g_1, and H_b samples was confirmed by the identification of thecharacteristic set of carbonate ion absorption bands. These bands appear at positions specific to dolomite, i.e., the in-plane bending (ν₄) at 721–729 cm⁻¹, the out-of-plane bending (ν₂) at 873–877 cm⁻¹, the symmetric stretching (ν₁) at 1095–1096 cm⁻¹, and the asymmetric stretching band (ν₃) at 1452–1459 cm⁻¹. The presence of calcite was also evidenced in the T_r, T_g_1, and H_b samples. Differentiation from dolomite is based on two key FTIR criteria, namely the characteristic shift of the ν4 band and the splitting of the ν3 band. In calcite, the ν4 band appears at a lower frequency, observed at 711 cm⁻¹ (compared to 721–729 cm⁻¹ domain for dolomite) [
30]. This difference is a classic spectral marker to distinguish calcium carbonate from calcium-magnesium carbonate. Also, the broad asymmetric stretching band (ν₃) shows a complex structure, with a distinct component at around 1445 cm⁻¹, which can be attributed to calcite, along with the contribution of dolomite at higher frequencies. Thus, the FTIR spectra suggest the presence of a mixture of dolomite and calcite, identifiable by careful analysis of the shape and position of the ν₄ and ν₃ bands. While in XRD calcite and dolomite do not appear in T_r and T_g samples, their presence in the FTIR speactra can be attributed to to the fact that they are likely impurities found in kaolinite.
Following FTIR analysis, the presence of Prussian blue pigment could not be detected, suggesting that this pigment was not present at the analysis points. In addition, the vermilion and realgar pigments have no characteristic absorption bands in the studied range (4000–600 cm−1).
Interpretation of the FTIR spectra indicates that all analyzed samples consist of a complex mixture of aged linseed oil, mineral pigments, and metallic soaps. This complexity significantly limits the clear identification of any specific natural resin. The carbonyl region (1700–1750 cm⁻¹) is dominated by overlapping signals from aged linseed oil (oxidized carboxylic acids, ketones, and esters) and lead white pigments (cerussite/hydrocerussite), effectively masking any resin-specific bands. Similarly, the 1200–1000 cm⁻¹ region is mostly dominated by vibrations belonging to inorganic pigments (e.g., Si–O from kaolinite and ultramarine, SO₄²⁻ from gypsum and barium white, Cr-O from zinc yellow, CO₃²⁻ from calcite, C-C, C-H, O-C, and OH from Indian yellow) and broad contributions from the aged oil (C–O, C–O–C), preventing unambiguous assignment of diagnostic C–O or C–O–C bands from a resin. In the C–H stretching region (3000–2800 cm⁻¹), the observed signals are characteristic of long aliphatic chains, compatible with aged linseed oil, zinc soaps, andother organic materials, like resins and proteinaceous materials [
31]. Consequently, although FTIR confirms the presence of a highly oxidized organic phase and chemical interactions (e.g., soap formation), it does not provide robust evidence for a specific resin, as the predominant components and advanced aging processes dominate the spectra in this region. However, a comparative analysis with reference spectra for natural resins [
32] suggests that the presence of sandarac resin, especially in spectrum H_g_3, cannot be excluded and is, in fact, plausible. This tentative assignment is based on the coincidence of most of the characteristic absorption bands of sandarac resin. The observed minor shifts in 3 of the 19 characteristic absorption bands (e.g., from 1497 to 1510 cm⁻¹, from 1213 to 1205 cm⁻¹, and from 789-792 to 779-785 cm⁻¹) and the masking of the one from around 3079 cm⁻¹ by the large O–H absorption band are phenomena consistent with the behavior of an old organic material (aged sandarac resin) embedded in a complex and degraded matrix, where molecular interactions and oxidation state can slightly modify the vibrational frequencies.
The main absorption bands in the regions 3337-3349 cm⁻¹ (combined N–H/O–H stretching), 1660–1663 cm⁻¹ (amide I, C=O stretching), 1545–1550 cm⁻¹ (amide II, combination of C=O stretching and NH bending), and between1234–1235 cm⁻¹ (amide III, CH bending), together with the absorption bands in the domains 2970-2979 cm⁻¹ (asymmetric stretching of CH₃), 2901-2908 cm⁻¹ (asymmetric stretching of CH₂ and/or CH₃) and 2860-2875 cm⁻¹ (symmetric stretching of CH₃) and 1440-1447 cm⁻¹ (scissoring bending of the CH₂/CH₃ groups), constitute the evidence for the characteristic signature of a proteinaceous binder (animal glue) in case of 4_1 and 4_4 samples [
33,
34]. Due to the spectral overlap and very close positions of the fundamental absorption bands for all types of animal glues, conventional FTIR analysis does not allow identification of the specific type of animal source (e.g., distinguishing between rabbit skin, bone, or hide glues).
Even though ultramarine and barium white were identified by other techniques and their characteristic absorption bands are present in the FTIR spectra the overlap with other bands that belong to other compounds makes their identification problematic. The band assignment is presented in Tab S1 and ESI.