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Capabilities and limitations of Se isotopic analysis using hydride generation coupled to MC-ICP-MS

Lana Abou-Zeid *a, Martin Wiech b and Frank Vanhaecke a
aAtomic & Mass Spectrometry – A&MS Research Unit, Department of Chemistry, Ghent University, Campus Sterre, Krijgslaan 281 – S12, 9000 Ghent, Belgium. E-mail: lana.abouzeid@ugent.be
bInstitute of Marine Research, PO Box 1870, Nordnes, 5817 Bergen, Norway

Received 17th May 2025 , Accepted 23rd June 2025

First published on 25th June 2025


Abstract

This study presents a comprehensive methodological investigation aimed at optimizing selenium (Se) isotopic analysis using MC-ICP-MS. Fundamental aspects of the plasma were revisited through spatial profiling, enabling detailed characterization of the distribution of Se+ and ArAr+/ArArH+ species within the plasma. Increasing the sampling depth (sampling further upstream in the plasma) proved more effective than the commonly employed methane addition, offering a more effective suppression of the Ar-based species, although at the cost of some loss in the sensitivity for Se. Under these conditions, precision values (expressed as 2SD) of 0.03‰ and 0.17‰ were obtained for δ82/78Se and of 0.08‰ and 0.38‰ for δ82/76Se, at 100 and 25 μg L−1, respectively. Moreover, the method proved robust, with a long-term reproducibility of 0.07‰ (2SD, n = 120) and high accuracy, even at up to 30% sample-standard concentration mismatch. However, the method's relatively high hydride formation rate (∼7 × 10−3) limits its applicability to samples with As/Se post-isolation ratios ≤0.05, beyond which mathematical corrections lead to biased results. Finally, the method was validated using the SELM-1 reference material, for which the δ82/78Se and δ82/76Se values were in excellent agreement with published data, and was subsequently applied to a set of tuna fish organs (liver, spleen, kidney, and intestine). This study demonstrates that the method that was developed, optimized and validated forms a solid basis for further investigating Se metabolic pathways in marine fish and for elucidating its role in Hg detoxification.


1. Introduction

Selenium (Se) is an essential trace element for living organisms and plays a key role in environmental systems as it is involved in several bio(geo)chemical processes. In the human body, Se is mainly incorporated into proteins and enzymes such as glutathione peroxidases (GPxs) and thioredoxin reductases (TrxRs), mainly involved in antioxidant defense and redox state regulation.1,2 Studies have shown that insufficient Se levels are associated with diseases such as cancer, diabetes, and immune disorders,2 further highlighting the importance of Se in human health. Moreover, Se plays a critical protective role against mercury (Hg) toxicity in both humans and animals3 by forming biologically inert HgSe nanoparticles, as evidenced in marine mammals4–6 and seabirds,7 making Se of great interest in marine ecotoxicology and food safety. Despite its essential role, Se can become toxic at concentrations just 3- to 5-fold above the optimal intake, and this duality defined Se as the “double-edged sword element”.8

Selenium has six stable isotopes with masses ranging from 74 to 82 amu and occurs in multiple redox states, i.e. Se(0), Se(−II), Se(IV) and Se(VI), which are involved in several environmental and biogeochemical processes.9–11 Due to their mass difference, Se isotopes participate with slight differences in the reaction rate (kinetically governed isotope fractionation) and/or in the equilibrium state (thermodynamically governed isotope fractionation) in chemical reactions, leading to isotopic fractionation.12 This makes Se isotopic analysis highly valuable for tracing Se sources in the environment and understanding its redox cycling and metabolic transformations in natural systems.13–16 Selenium isotopic analysis is typically performed using multi-collector inductively coupled plasma-mass spectrometry (MC-ICP-MS) due to the high sample throughput and high precision typically offered by this technique.17,18 However, MC-ICP-MS isotopic analysis of Se is associated with numerous challenges. First, Se has a high ionization potential (9.75 eV), resulting in a relatively poor ionization yield in the ICP source (30%)19 and therefore, a lower sensitivity compared to other elements. This poses the first challenge for precise isotope ratio measurements, as a reduced ion beam intensity can lead to higher uncertainty (counting statistics), while in most sample types, Se is present at very low concentrations only. To mitigate this lower sensitivity, Se is commonly introduced into the MC-ICP-MS unit under “dry plasma conditions” using a hydride generation (HG) system.20–23 The latter involves the reduction of Se(IV) by sodium borohydride (NaBH4), resulting in the formation of gaseous Se-hydride. This introduction system increases the Se introduction efficiency in comparison to the standard wet plasma approach using a pneumatic nebulizer and spray chamber and therefore results in an enhanced Se signal intensity. Unfortunately, HG is not Se-selective and other hydride-forming elements such as Ge and As are also converted into gaseous hydrides by NaBH4 and further introduced into the MC-ICP-MS unit, causing spectral interferences affecting the signals of the Se isotopes (overlap of the signals of 74Ge+ and 74Se+, 75AsH+ and 76Ge+ and 76Se+, and 76GeH+ and 77Se+). Moreover, the HG process is susceptible to interferences from transition metal ions from elements such as cobalt (Co), copper (Cu), nickel (Ni), and iron (Fe) if present in the sample. These elements are reported to inhibit the conversion of Se(IV) into Se-hydride form, leading to a reduction in Se ion signal intensity.24 Therefore, a chemical purification prior to HG-MC-ICP-MS measurement is necessary to separate Se from these interfering elements. This is typically accomplished using the well-established thiol cellulose powder (TCP) method, as it ensures quantitative Se recovery and provides optimal separation efficiency from these interfering elements.24 However, any Se loss during chromatographic isolation may induce isotopic fractionation, thereby compromising the accuracy of isotope ratio measurements. To address this limitation, the double-spike approach is often used, which involves adding a known mixture of enriched Se isotopes to the sample, allowing one to correct for these losses and for instrumental mass discrimination occurring at the level of the MC-ICP-MS. Despite the advantages offered by this approach, it is costly, labor-intensive and requires meticulous sample preparation, while the analysis of samples with an isotopic composition that deviates substantially from the natural one can require longer rinsing to avoid cross-over contamination due to memory effects.

Another significant challenge in Se isotope ratio measurement using MC-ICP-MS is the occurrence of spectral interferences, primarily arising from argon-based polyatomic ions, the signals of which overlap with those of most of the Se isotopes. The most important ones are argon (Ar) dimers, formed by the combination of different Ar isotopes, i.e.40Ar36Ar+ and 38Ar38Ar+ (both to a lesser extent), 40Ar38Ar+ and especially 40Ar40Ar+, the signals of which overlap with those of 76Se, 78Se and 80Se, respectively, in addition to 40Ar37Cl+, which interferes with the monitoring of 77Se. These interferences are impossible to resolve using a “traditional” MC-ICP-MS not equipped with a collision/reaction cell, as the mass resolution required exceeds the capabilities of the commercially available instrumentation.17 One of the most effective strategies reported to mitigate this problem is the introduction of methane gas (CH4) into the plasma,25,26 which has been adopted by many researchers for Se isotope ratio measurement and is typically accomplished by introducing CH4 through the hydride generation unit.21,22,27 Already an amount as low as 1–3 mL min−1 of 2% CH4 in Ar was shown to successfully decrease the signal intensity of ArAr+ and ArArH+ ions by nearly a factor of 2 and at the same time increase the Se signal intensity by approximately a factor of 1.5, resulting in an improved Se/interference ratio, and therefore, in more accurate Se isotope ratio measurements.26 However, while this solution significantly reduced the formation of Ar-based interferences, it did not eliminate them entirely, further restricting accurate Se isotope ratio measurements at low concentration levels.

Using an MC-ICP-MS equipped with a collision/reaction cell (CRC) nowadays is probably the most effective solution for eliminating Ar-based interferences affecting the Se+ signals. However, this type of instrumentation was introduced relatively recently only, such that the large majority of all MC-ICP-MS instrumentation used worldwide is not equipped with a CRC. Moreover, the MC-ICP-MS units equipped with a CRC are also substantially more expensive. Therefore, in this work, we present an alternative approach for reducing the spectral overlap of the Ar-based interferences hampering Se isotopic analysis through revisiting some fundamental aspects of the plasma using a “traditional” MC-ICP-MS unit. For this aim, radial and axial profiling of the plasma was conducted in order to elucidate the distribution of ArAr+, ArArH+ and Se+ ions. These profiles enabled the selection of an optimal torch position such that plasma regions with reduced formation of the interfering ions are extracted via the sampling cone orifice, thereby enhancing the Se/interference signal ratio. In addition, the effect of the torch position on the accuracy and precision of Se isotope ratio data was also evaluated. The results obtained under these optimized instrument settings were compared to those achieved using the widely adopted CH4 addition approach. Moreover, TCP was used for separating Se from matrix elements, ensuring quantitative Se recovery, thereby eliminating the requirement for a double-spike approach. Finally, the method was validated using the selenium-enriched yeast (SELM-1) reference material, previously characterized for its Se isotopic composition by several groups and was applied to a set of tuna fish organs as a proof-of-concept application. This method paves the way to more routine studies of the Se isotopic signature as an additional source of information for revealing the metabolic pathways of Se in fish and further elucidating its role in Hg detoxification.

2. Experimental part

2.1. Chemicals

Sodium borohydride (NaBH4), sodium hydroxide (NaOH), Sigmacell cellulose (type 20, particle size 20 μm), thioglycolic acid (98%), acetic anhydride ReagentPlus® ≥99%, glacial acetic acid ReagentPlus® ≥99% and hydrogen peroxide H2O2 9.8 M were purchased from Sigma-Aldrich (Belgium). Sulfuric acid 95–98% Primer Plus™ for trace metal analysis was purchased from Fisher scientific (France). HCl and HNO3 were supplied by Fisher Chemicals (UK) and further subjected to sub-boiling distillation in a Savillex DST purification system (Savillex, USA). Ultrapure water (18.2 MΩ cm at 25 °C, further referred to as MQ) was obtained from a Milli-Q purification system from Millipore (France). The NIST SRM 3149 Se standard was supplied by the National Institute of Standards and Technology (NIST, USA), Se standard solution (Lot Number HC44697996) was purchased from MERCK (Belgium). The Selenium-enriched yeast certified reference material (SELM-1) was purchased from the National Research Council Canada (NRC).

2.2. Samples

Atlantic bluefin tuna (ABFT) Thunnus thynnus were caught by recreational fishers with a rod and line in summer and autumn along the Norwegian coast. In this work, organ samples from one individual were analysed as a proof-of-principle application. The tuna was caught on August 21st 2020, measured 244 cm (standard fork length) and had an estimated age of 15.8 ± 2.4 years.6 The samples were obtained fresh on site when the fish was landed with clean sampling devices, and stored frozen in clean, sterile, plastic bags until analysis. All samples were homogenized before and after freeze-drying.

2.3. Sample preparation

All sample preparation was carried out in a class-10 clean lab (PicoTrace, Germany).
2.3.1. Sample digestion. Certified reference materials and samples were taken into solution via microwave-assisted acid digestion using a Multiwave 7000 unit (Anton Paar, Belgium). Depending on the Se concentration, approximately 0.1–1 g of material was weighed into a pre-cleaned TFM (modified polytetrafluoroethylene PTFE) microwave vessel. Digestion was carried out using 4 mL of 14 M HNO3 and 1 mL of 9.8 M H2O2 using the following microwave program: 0–20 min: ramp up to 220 °C at 140 bar, 20–30 min: 220 °C at 140 bar, 30–50 min: cooling down. The digest thus obtained was subsequently transferred using 2 mL MQ water into a pre-cleaned PFA (perfluoroalkoxy) beaker and further subjected to evaporation to near dryness at 60 °C. After evaporation, the sample was taken up in 6 M HCl. The beaker was subsequently closed and left on a hotplate at 110 °C for 4 hours to fully reduce Se(VI) to Se(IV).
2.3.2. Sample purification using thiol cellulose powder (TCP). TCP was synthesized according to the method described by Elwaer et al. in 2008.24 0.1 g of the synthetized TCP (0.5 mL of wet TCP) was loaded into a BioRad column with an internal diameter of 0.8 cm (Eichrom Technologies, France). The resin was washed with 2 mL MQ, followed by 2 mL of 6 M HCl, and then conditioned using 2 mL of 1 M HCl. Finally, 2 mL of sample solution in 1 M HCl was loaded onto the column. The flow rate was accelerated and controlled using a polycarbonate vacuum box (Triskem, France) and was set at approximately 7 mL min−1. The matrix was washed off with 2 mL MQ, 2 mL of 6 M HCl and 2 mL of 1 M HCl. Finally, the resin was left to dry, transferred from the column into a falcon tube and 500 μL of MQ and 500 μL of 14 M HNO3 were added. Se was extracted from TCP by heating the falcon tubes in a water bath at 95 °C for 20 min. After completing the extraction, 2 mL of MQ water was added into the falcon tube, and the latter was centrifuged at 4 rpm for 5 min. The extraction procedure was repeated once more to ensure a complete extraction of Se from the TCP. The first and the second extract were mixed (total volume V = 6 mL), and transferred into a pre-cleaned PFA beaker from which the solvent was evaporated at 60 °C. The residue was collected with 6 M HCl, subjected to a reduction step at 110 °C to ensure complete reduction of Se(VI) to Se(IV) and finally diluted to 100 μg L−1 in 2 M HCl for isotope ratio measurements using HG-MC-ICP-MS.

2.4. Instrumentation

2.4.1. Multi-collector inductively coupled plasma-mass spectrometry (MC-ICP-MS). Selenium was introduced into a Neptune XT MC-ICP-MS unit (Thermo Scientific, Germany) in the form of gaseous Se-hydride (H2Se) using a CETAC HGX 200 hydride generator unit (Teledyne CETAC Technologies, USA). The generation of Se-hydride is based on the reaction of Se(IV) with NaBH4 following eqn (1):
 
3NaBH4 + 3H2O + 3HCl + 2H2SeO3 → 3NaCl + 2H2Se + 3H3BO3 + 6H2(1)

In the hydride generation (HG) unit, the sample is first acidified with 2 M HCl solution in a mixing tee (Mixing Tee 1 in Fig. S1). Subsequently, it is mixed with NaBH4 (0.4% w/v in 0.1 M NaOH) in a second mixing tee (Mixing Tee 2), and is allowed to react with NaBH4 in a mixing loop, resulting in the reduction of Se(IV) to Se(−II), in the form of H2Se.

Selenium is then introduced into the MC-ICP-MS unit under dry conditions. For the experiments involving CH4 addition, a CH4/Ar (2/98 mol%) gas mixture (Air liquid, Belgium) was introduced in the additional gas port (Fig. S1).

The instrument settings of the HG unit and MC-ICP-MS instrument are summarized in Table 1.

Table 1 Operating parameters of the HG unit and MC-ICP-MS instrument for Se isotope ratio measurements
Hydride generation unit
Solution Composition Uptake rate
HCl 2 M 0.182 mL min−1
NaBH4 0.4% w/v in 0.1 M NaOH 0.182 mL min−1
Sample 2 M HCl 0.364 mL min−1

MC-ICP-MS cup configuration
Cup L4 L3 L2 L1 C H1 H2 H3 H4
Mass 73 75 76 77 78 80 81 82 83

MC-ICP-MS
Instrument settings Data acquisition parameters
Sampling cone Ni; Jet-type; 1.1 mm Ø orifice Integration time 4.194 s
Skimmer Ni; X-type; 0.8 mm Ø orifice Uptake time 240 s
Plasma gas flow rate 15 L min−1 Measurement 1 block, 60 cycles
Auxiliary gas flow rate 0.7 L min−1 Mass resolution Low
Carrier gas flow rate (HG) 1.2 L min−1
Additional gas flow rate (HG) 0 L min−1
RF power (W) 1200


The signal intensity was monitored at all m/z using Faraday cups connected to amplifiers equipped with 1011 Ω resistors, except at m/z = 80, at which the signal intensity was monitored using a Faraday cup connected to an amplifier equipped with a 1010 Ω resistor, which can tolerate higher currents without saturation.

Se isotope ratios were reported in the delta notation, as per mil deviation (‰), relative to the NIST SRM-3149 standard:

 
image file: d5ja00196j-t1.tif(2)
with x being 76 or 78.

The bias induced by instrumental mass discrimination was corrected for using the sample-standard bracketing approach (SSB), by measuring the NIST SRM 3149 standard before and after each sample. Interference correction will be further detailed in Section 2.4.

2.4.2. Inductively coupled plasma-tandem mass spectrometry (ICP-MS/MS). An 8800 Agilent inductively coupled plasma-tandem mass spectrometry ICP-MS/MS unit (Agilent Technologies, Japan) equipped with a MicroMist nebulizer, a Peltier cooled spray chamber, a 2 mm internal diameter injector and nickel cones was relied upon for Se quantification. Se was monitored in mass shift mode, using O2 as a reaction gas in the collision/reaction cell (CRC). Se levels were quantified by means of external calibration using Te as an internal standard (IS) to correct for potential matrix effects and signal instability. Additionally, also the potential presence of the interfering elements Fe, Co, Ni, Cu, and As was monitored. These elements were determined in mass-shift mode, with NH3 introduced into the CRC for Fe, Co, Ni, and Cu, and O2 for As. Quantification was carried out using external calibration with Ga as an internal standard. The ICP-MS/MS instrument settings and the ion products monitored are summarized in Table 2.
Table 2 ICP-MS/MS instrument settings and data acquisition parameters used for Se quantification
Plasma conditions
Plasma gas flow rate (L min−1) 15
Auxiliary gas flow rate (L min−1) 0.9
RF power (W) 1550
Nebulizer gas flow rate (L min−1) 1.0
Optional gas NA
Reaction gas flow rate – O2 (mL min−1) 0.45 (30%)
Ions monitored 80Se16O+, Co(NH3)2+, Ni(NH3)2+, Fe(NH3)2+, Cu(NH3)2+, AsO+, Te+ (IS) and Ga+ (IS)
Integration time (s) 1
Replicates 10
Sweeps 100


2.5. Interference correction for Se signals in MC-ICP-MS measurements

Several corrections were applied to correct the signals obtained for the Se isotopes for contributions from the ArAr+ ions, hydride ions (ArArH+, BrH+, and SeH+) and traces of As potentially present after TCP purification. These corrections are described below. As the Ge concentration detected in the targeted fish samples was lower than the limit of detection, Ge was not considered as a potential interferent and therefore, no Ge correction was developed or performed.
2.5.1. Evaluation of correction for the occurrence of ArAr+. To correct for Ar-based interferences, an on peak zero (OPZ) or blank subtraction is performed. For this purpose, a 2 M HCl blank sample was measured before and after each sample/standard. The average signal of the two blanks was then subtracted from the signal at the m/z values of 76, 78 and 82. For an accurate OPZ correction, the 2 M HCl blank used for the correction was derived from the same acid batch used to prepare the samples and the standards. In addition to Ar-based interferences, OPZ subtraction also allows to correct for potential trace impurities of Kr in Ar, which leads to isobaric interferences affecting 78Se, 80Se and 82Se, and to correct for 81BrH+ (Br contamination in HCl) which interferes with the monitoring of 82Se.

For obtaining the net signal for 80Se, the following calculations were performed:

After correcting for the 82Kr interference by means of OPZ subtraction, 82Se(corr) can be used to calculate the signal of 80Se using the natural abundances of the Se isotopes (eqn (3)).

 
image file: d5ja00196j-t2.tif(3)
with nat.ab = natural abundance and I = signal intensity.

Subsequently, the signal for 40Ar40Ar+ can be calculated using eqn (4).

 
40Ar40Ar(calc)+ = I(80) − 80Secalc+(4)

Using the natural abundances of the Ar isotopes, the contribution from ArAr+ ions at m/z = 76 and 78 can be calculated as described in eqn (5) and (6).

 
image file: d5ja00196j-t3.tif(5)
 
image file: d5ja00196j-t4.tif(6)

These calculated ArAr+ signals were only used to evaluate the contribution from these interferences to the signals at m/z = 76 and 78. The contribution (%) was calculated by dividing the calculated signal intensity for 76ArAr(calc)+ and 78ArAr(calc)+ by the total signal intensity at mass 76 and 78, respectively. As the occurrence of ArAr+ ions was minimized to the maximum extent (see the Results and discussion section), an OPZ subtraction was sufficient to correct for this contribution. The additional correction using these estimated signals only added errors to the final results.

2.5.2. Evaluation of correction for the occurrence of hydride ions. Se tends to form SeH+ hydride ions which overlap with the signals of the Se+ atomic ions at mass M + 1. For instance, the signals of 77SeH+ and 78Se+ overlap. In addition, As, potentially present as traces in the Se fraction after TCP purification, can also form a hydride ion (75AsH+), which interferes with the measurement of 76Se. To correct for these interferences, the hydride generation rate was calculated as shown in eqn (7):
 
image file: d5ja00196j-t5.tif(7)
with I(83)corr, the intensity at m/z = 83 corrected for the contribution from 83Kr using the OPZ subtraction.

The HG rate is typically very stable throughout a measurement session and is assumed to be the same for all Se isotopes. Therefore, the HG rate was used to correct the signal obtained at m/z = 78 for the contribution from 77SeH+ as shown in eqn (8) and (9):

 
77SeH+ = 77Se+ × HG rate(8)
 
78Secorr+ = I(78) − 77SeH+(9)
with I(78) corrected for the ArAr+ interferences using the OPZ subtraction.

In the case of As, it is assumed that the AsH+/As+ ratio is identical to 82SeH+/82Se+. Therefore, the HG rate was also used to correct the signal at m/z = 76 for the contribution from 75AsH+ as shown in eqn (10) and (11):

 
75AsH+ = 75Ascorr+ × HG rate(10)
 
76Secorr+ = I(76) − 75AsH+(11)
with 75Ascorr+, the signal at m/z = 75 corrected for the 40Ar35Cl+ contribution using the OPZ subtraction.

3. Results and discussion

3.1. Effect of plasma parameters on Ar-based interferences

It is well established that the ion beam analyzed by the mass spectrometer does not originate from a single point in the plasma, but from a cylindrical volume of plasma with a diameter of ca. 0.25 mm and a depth of ca. 2 mm (sample volume of ca. 0.14 mm3) in front of the sampling cone aperture.28 To investigate the distribution of Se+ ions and of interfering species, particularly ArAr+ and ArArH+, within the plasma, axial and radial spatial profiling were performed. For this aim, a 100 μg L−1 Se NIST elemental solution was introduced into the MC-ICP-MS unit via the HG unit and the signals at m/z = 81 (corresponding to ArArH+) and 80 (which includes contributions from both 80Se+ and 80ArAr+, calculated according to eqn (3) and (4)) were recorded at various x, y, and z torch positions (Fig. 1(a-1) to (c-1)). The same experiment was conducted using a blank solution of 2 M HCl (Fig. 1(a-2) to (c-2)) for monitoring the signal of the interfering ions in the absence of Se.
image file: d5ja00196j-f1.tif
Fig. 1 Radial (x, y) and axial (z) spatial profiling of 80ArAr+, 81ArArH+ and 80Se+ with a fixed carrier gas flow rate of 1.2 L min−1. For radial profiling, the z position was fixed at −4.0 mm.

As can be seen in Fig. 1, the profiles obtained with and without Se in solution are nearly identical, with Ar-based interference intensities remaining consistent, even when experiments were conducted on different days. This observation aligns with the findings of Pogge von Strandmann et al.,29 who used HG coupled to a sector field ICP-MS unit operated in high resolution mode to monitor the stability of Ar-based interfering signals. The authors showed that the intensity obtained for ArAr+ was identical with and without Se present in solution, and stable throughout the measurement session.29

Furthermore, as shown in Fig. 1(a-1) and (b-1), the radial profiles of ArAr+ and ArArH+ exhibit a distinct double or bimodal peak shape, in accordance with the observations of Fraser and Beauchemin.30 The profiles reveal two maxima at distinct positions: −3.23 mm and −1.5 mm on the y-axis, and −1.5 mm and 0.3 mm on the x-axis, with maximum signal intensities of approximately 25 V for 80ArAr+ and 10 V for ArArH+. At the central position between the two peaks (2.33 mm on the y-axis and −0.6 mm on the x-axis), a minimum intensity is observed for the interfering species with 0.05 V for 80ArAr+ and 2.22 V for ArArH+, being respectively 500- and 4.5-fold lower than those observed at the maxima of each peak. Moreover, a maximum contribution from the 80Se+ signal at m/z = 80 is observed at this position with an intensity of 5.70 V, making these x and y values optimal for a high Se/interference ratio. Following this observation, the y and x positions were fixed at −0.6 mm and 2.33 mm, respectively, and the z position of the torch (sampling depth or distance between the tip of the torch and the sampling cone aperture) was changed from 2.5 mm (torch at the furthest position from the sampler cone, thus sampling further downstream in the ICP), to 0 mm as the central position (medium position), and finally to −4 mm (torch at the closest position to the sampler cone, thus sampling more upstream in the ICP), as reported in Fig. 1(c-1) and (c-2). The axial profile reveals a different behavior of the Se+ and interfering ion species, respectively. For 80ArAr+, the signal exhibits a maximum of 62 V at 2.5 mm and decreases when bringing the torch closer to the sampling cone, reaching 0.27 V at −4 mm. For 80Se+, the signal displays a slight increase first, reaching a maximum of 23.83 V at 1.5 mm, before slowly decreasing to 5.47 V at −4 mm. This observation is in accordance with previous observations from Holliday and Beauchemin who stated that sampling more upstream in the plasma results in reduced signal intensity due to the short residence time of the analyte in the plasma.28 Finally, for ArArH+, an increase is first observed, reaching a maximum of 4.82 V at −2 mm after which the signal decreases to a minimum of 2.48 V at −4 mm. Based on these results, it can be concluded that a torch position of −4 mm (sampling more upstream in the ICP), seems to be the most suitable for drastically reducing the contribution from ArAr+ to the Se+ signals, with signal intensities of 0.27 V for 80ArAr+ and of 5.47 V for 80Se+. It is important to mention that the tuning parameters were shown to be very robust, with signal intensities for Se-ions and Ar-based interferences being consistent across multiple days. Only minor adjustments to the torch position (always within the predefined range) were occasionally necessary.

Although the ArAr+ signal intensity has been drastically reduced under these conditions, the signal for ArArH+ remains relatively high (2.48 V), compromising the accuracy of the signal obtained for the 77Se+ signal if not properly accounted for. According to the literature, introducing CH4 into the plasma has proven effective in reducing the occurrence of ArAr+ and, more notably, ArArH+ while also enhancing the Se signal by a factor of 1.5 due to the carbon effect.22,26,31,32 Therefore, to further suppress the contribution from ArArH+ under the optimized conditions, the impact of CH4 addition was assessed, as discussed in the following section.

3.2. Effect of methane addition

Methane gas (2% CH4 in Ar) was introduced into the ICP via the additional gas port of the HG unit (Fig. S1). Various flow rates were tested to evaluate their impact on the signal intensities for the Se+ and Ar-based ions under the previously optimized plasma conditions. The results obtained are presented in Fig. 2.
image file: d5ja00196j-f2.tif
Fig. 2 Effect of CH4 addition on 80Se+, 80ArAr+ and 81ArArH+ signal intensities, at different carrier gas flow rates.

Under the optimized conditions (carrier gas 1.2 L min−1, sampling depth of −4 mm and y and x positions of −0.6 mm and 2.33 mm), increasing the CH4 flow rate led to a nearly 2-fold decrease in the signal intensities for both Se and Ar-based interfering ions upon addition of 1 mL min−1 of CH4 gas only. Consequently, no further CH4 flow rate testing was performed under these conditions. When the carrier gas flow rate was slightly reduced to 1.1 L min−1 (Fig. 2(b)), a similar trend of signal suppression was observed. However, at 1.0 L min−1 (Fig. 2(c)), a different trend was observed. The Se signal intensity increased by a factor of 2 when the CH4 flow rate was increased to approximately 0.8–1.0 mL min−1, while the ArAr+ signal intensity decreased by a similar factor. This behavior aligns with the observation previously reported in the literature.26 Surprisingly, the ArArH+ signal intensity increased with the addition of CH4, reaching a maximum of 0.9 V at a flow rate of 1.0 mL min−1. This result contrasts with findings in the literature, where CH4 addition is reported to significantly decrease the ArArH+ intensity. This discrepancy is likely due to differences in the plasma parameters used in our study as compared to those in previously reported work. Despite this increase, the ArArH+ intensity remains approximately 2.5-fold lower than that observed under our optimized conditions without CH4 addition (Section 3.1). Beyond 1.0 mL min−1 of CH4, the signal intensities for both Se+ and the Ar-based interfering ions begin to decline, mirroring the trend observed in Fig. 2(a) and (b). In addition, the signal intensities for ArAr+ and ArArH+ observed when introducing a 2 M HCl blank solution were compared under optimized conditions (i) without CH4 addition (Fig. 3(a)) and (ii) with CH4 addition (Fig. 3(b)).


image file: d5ja00196j-f3.tif
Fig. 3 Comparison of the signal intensities for ArAr+ and ArArH+ (a) without CH4 addition, under optimized plasma conditions and (b) with CH4 addition.

The results show that optimizing the plasma settings and sampling at higher sampling depth significantly reduces the contribution from ArAr+ to the signal monitored, with only 0.27 V observed at m/z 80 for the blank. However, although CH4 addition does reduce the intensity of the signal at mass 80 as reported in the literature, the remaining contribution from the blank under optimized conditions (signal intensity of 10 V) remains relatively high – approximately 40-fold higher than the value obtained without CH4 addition. In contrast, the ArArH+ signal is significantly lower (about 3-fold lower) when CH4 is added to the plasma, compared to the conditions without CH4. Based on these observations, we prioritized the substantial reduction in the contribution from ArAr+ achieved by optimizing the instrument settings without the addition of CH4, as ArAr+ represents a major interferent affecting two of the Se isotopes, 76Se and 78Se. Consequently, these optimized conditions were selected for all subsequent analyses. Given the relatively high contribution from ArArH+ observed under these conditions, we focused on δ82/78Se and δ82/76Se and omitted δ82/77Se due to the potentially high contribution from ArArH+ at an m/z = 77. The contribution was too prominent for accurate correction using the OPZ correction only.

3.3. Effect of sampling depth on measurement accuracy and precision

After evaluating the effect of the instrument settings on the signal intensities of Se and interfering ions, their impact on the accuracy and precision of Se isotope ratio measurements was assessed. Therefore, three different z positions (sampling depths) were selected (Fig. S2): (i) a sampling depth of 1.5 mm (position far from the sampler cone, sampling more downstream in the plasma), which showed a maximum contribution from ArAr+ to the signal at m/z = 80 (Fig. 1(c)), (ii) a sampling depth of 0 mm, at which nearly equal contributions from Se+ and ArAr+ were observed and finally, (iii) a sampling depth of −4 mm (position very close to the sampling cone, sampling more upstream in the plasma), which showed a dominant contribution of 80Se+ to the signal at m/z = 80.

In order to evaluate the impact of the sampling depth on the accuracy of Se isotope ratio measurements, a Se Merck solution (LOT HC44697996), previously characterized for its Se isotopic composition,22 was measured at the three above-mentioned sampling depths and at three concentrations (25, 50, and 100 μg L−1). The bias introduced by instrumental mass discrimination was corrected for using external correction with a standard measured in a SSB approach following the application of the OPZ and hydride corrections described in the Experimental section. The final results for δ82/78Se and δ82/76Se are shown in Fig. 4.


image file: d5ja00196j-f4.tif
Fig. 4 Effect of the sampling depth (z position of the torch) on the accuracy and precision of δ82/78Se (a) and δ82/76Se (b) at 25, 50 and 100 μg L−1 of Se. The full red line represents the value of the Se Merck solution obtained by Chang et al.22 and the dotted red lines represent the corresponding ±2SD range. The dots represent the mean value of n ≥ 3 measurements and the error bars represent the 2SD.

At 1.5 mm sampling depth, the accuracy and precision of the Se isotope ratio measurement is compromised, especially at the lowest concentration levels of 25 μg L−1, with −0.48 ± 0.28‰ and +0.98 ± 2.37‰ for δ82/78Se and δ82/76Se, respectively (reference value −0.72 ± 0.07 and −1.07 ± 0.16, as reported by Chang et al. 2017[thin space (1/6-em)]22). This can be explained by the low signal intensity for the Se isotopes monitored at such a low concentration (0.689 V for 82Se) and therefore, the high contribution of the interference to the signal intensity (1.1% contribution from 78ArAr+ at m/z = 78 and 13% contribution from 76ArAr+ at m/z = 78, see the ESI). Such a contribution is too significant to be accurately accounted for using the OPZ correction. At 0 mm sampling depth, with nearly equal contributions from the Se+ and interference signals, the values were accurate and precise for δ82/78Se with −0.72 ± 0.13‰ and −0.69 ± 0.06‰ at 50 and 100 μg L−1, respectively (less than 0.5% contribution from 78ArAr+), except at 25 μg L−1 where δ82/78Se showed high 2SD values −0.78 ± 0.32‰ (0.8% contribution from 78ArAr+). In contrast, the values are inaccurate and imprecise for δ82/76Se, with −3.04 ± 0.90‰, −2.10 ± 0.24‰ and −0.92 ± 0.37 for 25, 50 and 100 μg L−1 of Se, respectively, due to the significant contribution from ArAr+ at m/z = 76 (2.7–9% contribution). Finally, at −4 mm sampling depth, the values are accurate and precise for both ratios (e.g., −0.72 ± 0.05‰ and −1.08 ± 0.04‰ for δ82/78Se and δ82/76Se, respectively, at 50 μg L−1 of Se), except at 25 μg L−1 for which the precision was degraded (ex. −0.70 ± 0.17‰ and −1.15 ± 0.38‰ for δ82/78Se and δ82/76Se, respectively) due to the low signal intensity obtained for the Se+ signals (0.157 V for 76Se, 0.4105 V for 78Se and 0.1637 V for 82Se). At this position, the contribution from 78ArAr+ to the signal at m/z = 78 ranged between 0.03% and 0.1%, only, and the contribution from 76ArAr+ to the signal at m/z = 76 ranged between 0.4 and 1.4% at 100 and 25 μg L−1 of Se, respectively. These values highlight the effective reduction of Ar-based interferences under the plasma conditions selected, resulting in improved accuracy and precision of the Se isotope ratio measurements.

3.4. Effect of standard/sample concentration mismatch

To ensure an accurate correction of instrumental mass discrimination using external calibration with a standard measured by the SSB approach, it is crucial to closely match the elemental concentration of the samples and the bracketing standard. To determine the tolerable range of concentration mismatch under the conditions selected, the NIST SRM 3149 bracketing standard was maintained at 50 μg L−1, while the Se Merck solution was prepared with concentrations deviating from −25% to +30% compared to that of the standard. The results obtained under these conditions are presented in Fig. 5.
image file: d5ja00196j-f5.tif
Fig. 5 Effect of sample-standard concentration mismatch on the accuracy of δ82/78Se and δ82/76Se. The diamond-shaped dots represent the value obtained for a single measurement and the error bars represent the 2SE (internal error).

The values obtained for δ82/78Se and δ82/76Se are accurate, even at −25% and +30% concentration mismatch between the sample and the bracketing standard. It is important to emphasize that while the amplitude of the mass bias is influenced by the analyte concentration and matrix composition, it is also systematically influenced by instrumental conditions.33 Andrén et al. (2004) showed that the torch position (sampling depth) has a significant impact on the magnitude and stability of the mass bias. They reported that when the torch is moved closer to the sampler cone, the intensity of the ion beam dropped by almost 20% and the amplitude of the mass bias increased; however, the mass bias was more stable and the precision of the isotope ratio measurement was improved.33 These findings may help explain the results presented in Fig. 5, where the mass bias appears largely unaffected by concentration mismatch. This could be attributed to the stable operating conditions and the stable mass bias achieved at a torch position of −4 mm, as similarly reported by Andrén et al. (2004). Despite this wide tolerable range of sample-standard mismatch, a maximum of 10% mismatch was adopted throughout the remainder of this study as this is the standard range used for most isotope systems in our laboratory.

3.5. Effect of As

Arsenic, potentially present in the sample, readily reacts with NaBH4 in the HG unit by forming 75AsH3 and further reaches the MC-ICP-MS unit where next to 75As+, also 75AsH+ is formed, causing spectral interference affecting 76Se+. Isolation of Se using TCP largely removes As. However, some traces might still remain (e.g., for shale rocks, the average As/Se before isolation is 13.5 and rarely exceeds 0.3 after isolation, but for some shales with an exceptionally high original As/Se ratio, the ratio post TCP chemistry might exceed this29). The spectral overlap caused by the remaining As can be corrected for mathematically, as shown in Section 2.4 of the Experimental part. However, if the occurrence of As is significant, the correction might no longer be accurate. In this section, the effect of residual As on the accuracy of Se isotope ratio measurements and the reliability of the mathematical correction were evaluated by spiking the Se Merck solution with As at As/Se ratios varying between 0 and 0.5. The results obtained for δ82/78Se and for δ82/76Se following mathematical corrections at m/z = 76 (see Section 2.4) are shown in Fig. 6.
image file: d5ja00196j-f6.tif
Fig. 6 Effect of different As/Se ratios on the accuracy of δ82/78Se and δ82/76Se values. For δ82/76Se, the values presented are obtained after applying mathematical correction at m/z = 76. The dots represent the value obtained for a single measurement and the error bars represent the 2SE (internal error).

The δ82/78Se values remain accurate regardless of the As/Se ratios, since 78Se is not affected by spectral interferences from this element. In contrast, δ82/76Se is significantly impacted, even at As/Se ratios as low as 0.1. As mentioned previously, significant spectral interference affecting the monitoring of 76Se is caused by the formation of 75AsH+. Under the conditions used, this interference can be reliably corrected for up to an As/Se ratio of 0.05, yielding a δ82/76Se value of −0.97‰ (compared to −1.87‰ without correction). However, at higher ratios, the correction is no longer fit-for-purpose. For example, for an As/Se ratio of 0.1, the uncorrected value of −2.55‰ is adjusted to −0.72‰ after correction. This trend of over-correction continues with increasing As/Se ratios, resulting in increasingly heavier values – for example, at a ratio of 0.5, the corrected δ82/76Se shifts to +0.55‰, whereas the uncorrected value is at −8‰. This contrasts with the results reported in the literature, where As/Se ratios up to 0.6 were reliably corrected for using the same mathematical correction, combined with a double-spike correction approach.23,29 This inconsistency with the results reported in the literature can be explained by the high hydride formation rate of ∼7 × 10−3 (calculated for 82SeH+/82Se+ according to eqn (7)) obtained under our experimental conditions, which is higher than the values reported in the literature (∼10−3–10−4).29 When it is assumed that the AsH+/As+ ratio is identical to 82SeH+/82Se+ (eqn (10)), the AsH+ formation under the conditions used is significant even at low As/Se ratios. This constitutes a limitation for the method, making it only suitable for samples showing an As/Se content ≤0.05 post TCP chemistry, or for samples without As. For samples with high As concentrations, a further optimization of the TCP separation conditions will be necessary to achieve lower residual As/Se ratios.

3.6. Long-term reproducibility

The long-term reproducibility of the δ82/78Se values obtained with this method was assessed by tracking the values obtained for Se Merck solution (N = 120), measured over a period of 18 months (August 2023–January 2025). The results obtained for 2 concentration levels 100 and 50 μg L−1 are summarized in Fig. 7.
image file: d5ja00196j-f7.tif
Fig. 7 δ 82/78Se values (n = 120) obtained over an 18 month period at 50 and 100 μg L−1 of Se.

The average of all δ82/78Se values obtained for the Se Merck solution is −0.71 ± 0.07 (2SD, n = 120), in accordance with the values previously reported by Chang et al.22 for the same solution (reference value −0.72 ± 0.07). This further demonstrates the method's robustness and suitability for accurate and precise Se isotope ratio measurements.

3.7. Validation and application to tuna fish organs

For validating the proposed method, the Se-enriched yeast (SELM-1) reference material, previously characterized for its Se isotopic composition by other groups, has been digested, and subjected to TCP for isolating Se from the matrix, and subsequently to MC-ICP-MS measurement under the optimized conditions. Se was quantitatively recovered upon TCP purification, thus avoiding any impact of potential fractionation effects on the final results. The Se isotopic composition measured for SELM-1 was −0.77 ± 0.11‰ (n = 3, 2SD) for δ82/78Se, and −1.16 ± 0.42‰ (n = 3, 2SD) for δ82/76Se, which is in agreement with the values reported in the literature (−0.66 ± 0.29‰,34 −0.68 ± 0.02‰,35 −0.70 ± 0.07‰[thin space (1/6-em)]36 and −0.69 ± 0.06‰[thin space (1/6-em)]37 for δ82/78Se and −0.97 ± 0.3‰[thin space (1/6-em)]34 for δ82/76Se), thus validating the method.

Finally, the validated method was applied to a set of tuna fish organs (liver, spleen, kidney, and intestine), previously characterized for their Hg concentration, speciation and isotopic composition. The aim of this kind of work is to study the role of Se in the Hg detoxification process through monitoring its concentration and isotopic composition. The different fish organs have been subjected to acid digestion and to Se isolation using the TCP method in triplicate. The Se recovery (%) and information on the elemental composition of these samples before and after isolation (represented as the X/Se ratio, with X being the element of interest) are summarized in Table 3.

Table 3 X/Se ratio before and after isolation of the samples using the TCP method; Se recovery (%) from the column (mean ± SD, n = 3)
Fe/Se Co/Se Ni/Se Cu/Se As/Se Se recovery (%)
Liver Before isolation 5.78 0.01 0.04 5.07 0.29 101 ± 3%
After isolation 0.05 0.00 0.00 0.01 0.05
Spleen Before isolation 18.25 0.00 0.00 0.01 0.02 97 ± 3%
After isolation 0.02 0.00 0.00 0.00 0.01
Kidney Before isolation 18.26 0.01 0.01 3.08 0.12 96 ± 2%
After isolation 0.03 0.00 0.00 0.01 0.02
Intestine Before isolation 4.90 0.00 0.02 0.42 0.57 98 ± 3%
After isolation 0.16 0.00 0.02 0.02 0.08


For all organs analyzed in triplicate, Se was quantitatively eluted from the column, with recovery factors ≥96% ± 2%. Moreover, critical elements known to interfere with the hydride generation process (Fe, Co, Ni, and Cu) and those causing spectral interference affecting the signals of the Se isotopes of interest (As), were efficiently removed from the matrix, with an X/Se ratio post TCP chemistry of 0 ≤ X/Se ≤ 0.16. The As/Se ratio in the sample prior to TCP was already low (≤0.57) and was further reduced following the TCP purification, now ranging between 0.01 and 0.05 (except for the intestine for which it was slightly higher). These residual As/Se ratios fall within the acceptable range for accurate mathematical correction, as previously demonstrated in Section 3.5.

Subsequently, the purified Se fractions were subjected to MC-ICP-MS measurement using the previously developed method at a Se concentration of 100 μg L−1. Throughout the sequence, the Se Merck solution was measured as a quality control solution at the beginning and at the end of the sequence and in-between every 6 samples for monitoring the accuracy of the isotope ratio measurements (δ82/78Se = −0.70 ± 0.09‰ and δ82/76Se = −1.07 ± 0.14‰, Mean ± 2SD, n = 7). Furthermore, the δ82/78Se value, obtained for the samples and the Se Merck solution, was plotted as a function of the corresponding δ82/76Se values. The three-isotope plot obtained is provided as Fig. 8.


image file: d5ja00196j-f8.tif
Fig. 8 Three-isotope plot of δ82/78Se vs. δ82/76Se of all data points for the tuna fish organs and for the different measurements of the Se Merck solution throughout the sequence.

The δ82/78Se vs. δ82/76Se three-isotope plot of Fig. 8 shows a linear trend (R2 = 0.9871), with a slope of 0.6871, which closely matches the slope of the theoretical mass-dependent fractionation of 0.6497, calculated according to Young et al. (2002), assuming thermodynamically governed fractionation.38 This confirms that our results are accurate and not affected by spectral interference. For a further interpretation of the Se isotopic composition in tuna fish organs, the δ82/78Se results were plotted together with the Se concentration found in each organ. The results are shown in Fig. 9.


image file: d5ja00196j-f9.tif
Fig. 9 Se concentration (μg g−1) and isotopic composition (δ82/78Se ‰) measured in the intestine, liver, kidney and spleen of tuna fish. The δ82/78Se values (red diamonds) represent the average value of three replicate analyses (sample preparation included) of the same sample and the error bars represent the 1SD.

As shown in Fig. 9, δ82/78Se values for all tuna fish organs display a Se isotopic composition that is heavier than that of the standard (positive δ82/78Se values). The spleen had the highest Se content and displayed the lightest Se isotopic composition +0.17 ± 0.05‰ (n = 3, 1SD), whereas the liver showed the heaviest δ82/78Se value of all organs measured: +0.57 ± 0.07‰ (n = 6, 1SD). This is consistent with the previous observations of Marchán-Moreno et al. (2024)37 and Clark & Johnson et al. (2010)39 who also reported that the liver of fish (catfish, sunfish and carp) and seabirds (giant petrels) exhibited the heaviest Se isotopic composition of all organs analysed. This was attributed to the liver being the primary site for Se intake from the diet, from which Se is redistributed to other organs for various metabolic functions. The unutilized Se tends to accumulate in the liver and becomes enriched in heavier isotopes, as lighter isotopes are preferentially involved in the metabolic processes.37 The depletion in the heavier Se isotopes in the other organs (lighter isotopic composition) shown in Fig. 9 supports the hypothesis of lighter Se isotopes being more efficiently distributed from the liver to the other tissues.

When comparing the Se isotopic composition obtained in this work with that of Hg measured in the same organs by Wiech et al. (2024),6 a similar trend is observed. The authors showed that the liver exhibited the heaviest Hg isotopic composition, followed by the intestine and the kidney, while the spleen showed the lightest δ202Hg values. This pattern was attributed to differences in Hg speciation, particularly the methylmercury (MeHg) content, which was the highest in the liver and lowest in the spleen. Since during methylation, there is a slight preference for the heavier Hg isotopes being incorporated, MeHg is enriched in the heavier isotopes compared to inorganic Hg (iHg). Moreover, Wiech et al. (2024)6 reported that the masses of both Hg and Se present in the particulate form were the highest in the spleen and kidney, suggesting that HgSe nanoparticle formation predominantly occurs in these organs. This supports the idea that the spleen and kidney might play a key role in the Hg detoxification process by Se. Although coming from one individual fish only, the Se concentration and isotopic data obtained in this study support this view: in addition to the lowest content of MeHg, the spleen and kidney exhibited the highest Se concentration and the lightest Se isotopic composition. These initial results suggest that isotopic analysis can be an additional tool for investigating whether Se is actively involved in the demethylation of MeHg. It is important to highlight that, to the best of the authors' knowledge, this work is the first reporting data on the Se isotopic composition in marine fish organs and in tuna fish particularly. As such, data interpretation remains tentative due to the very limited availability of Se isotope ratio data in biological systems, particularly in marine organisms. In fact, the only data reported for biological samples are limited to fish and plants from a Se-contaminated lake,39,40 plankton from the Pacific Ocean,41 and more recently tissues (liver, kidney, muscle and brain) of a marine top-predator seabird.37 Therefore, based on these promising initial results, Se isotopic analysis of a wider collection of tuna fish organs (higher number of individuals) can aid in better understanding of the role of Se in Hg detoxification processes in marine fish.

4. Conclusions

In this work, a detailed investigation of the distribution of Se+ and ArAr+/ArArH+ ions within the ICP was accomplished through radial and axial spatial profiling. By optimizing the torch position, particularly by sampling the ICP more upstream (sampling depth of −4 mm), Ar-based interferences affecting the Se+ signals were significantly reduced. Under optimized conditions, the contribution from 76ArAr+ and 78ArAr+ to the signals at m/z = 76 and = 78 was reduced to 0.4% and 0.03%, respectively, at a Se concentration of 100 μg L−1. This optimization enabled accurate and precise Se isotope ratio measurements, with a 2SD of 0.03‰ and 0.17‰ for δ82/78Se and of 0.08‰ and 0.38‰ for δ82/76Se, at 100 and 25 μg L−1, respectively. These results were obtained after OPZ correction and using external correction for the mass bias with the standard measured in a SSB sequence. Notably, this configuration maintained stable mass bias conditions, delivering accurate data even with up to 30% concentration mismatch between the Se concentration in the sample and bracketing standard. Despite these advantages, the method exhibits some inherent limitations, mainly related to the high hydride formation rate (∼7 × 10−3) obtained under the optimized conditions. This resulted in a low tolerance to the presence of residual As in the measured sample solution, as only for As/Se ratios ≤0.05 mathematical correction proved sufficient. Nevertheless, the method demonstrated excellent long-term reproducibility, with a standard deviation of 0.07‰ (2SD) for 120 δ82/78Se measurements across an 18-month period, highlighting its robustness. Finally, the method was validated using the SELM-1 reference material, with values in agreement with those reported in the literature, and was applied, for the first time, to a set of tuna fish organs (spleen, intestine, kidney and liver). These initial results demonstrated organ-specific Se isotopic signatures, indicating the potential of Se isotopic analysis as a powerful tool for tracing metabolic processes of this element and for potentially elucidating its role in Hg detoxification in marine fish.

Data availability

The data supporting this article have been included as part of the ESI.

Conflicts of interest

There are no conflicts to declare.

Acknowledgements

FWO-Vlaanderen is acknowledged for funding the acquisition of MC-ICP-MS instrumentation (ZW15-02 – G0H6216N). Financial support from Ghent University funding (BOF24J/2021/054) is also acknowledged for providing the grant that enabled the execution of this project. Furthermore, the work was also supported by the Norwegian Ministry of Trade, Industry and Fisheries.

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Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5ja00196j

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