Geology and mineralogy of the Au-As ( Ag-Pb-Zn-Cu-Sb ) polymetallic deposit of Valiña-Azúmara ( Lugo , NW Spain )

Valiña-Azúmara is a polymetallic Au-As (Ag-Pb-Zn-Cu-Sb) deposit, located in the province of Lugo (NW Spain), that was mined for arsenic at the beginning of the 20th century. The mineralization is hosted in a Variscan thrust fault with a dip direction of N247-261oE, and N-S and NE-SW Late-Variscan faults. These structures are hosted in black slates, Cambrian in age. To a lesser extent, the mineralization also occurs disseminated within narrow, weakly silicified and sericited selvages. Mineralization is divided into two hypogene stages. The first consists of quartz, calcite, rutile, sericite, arsenopyrite and pyrite. Two types of pyrite (Py-I and Py-II) are defined according to their chemical and textural characteristics. Py-II occurs as overgrowth of previous Py-I crystals. Py-II is As-rich (≤1.7 wt.%) and often contains traces of Te, Zn, Cu, Bi, Sb and Au. The mineralized drill core sections show a significant correlation between Au and As. This is due to Au occurring as invisible Au within the Py-II grains, with contents of up to 176 ppm. The Au/As ratios of Py-II indicate that Au was deposited as Au, as solid solution within the pyrite structure. The second stage of mineralization is enriched in Ag-Pb-Zn-Cu-Sb, replacing the first stage, and consists of quartz, calcite, chlorite, sphalerite, jamesonite, Ag-rich tetrahedrite, freibergite, chalcopyrite, pyrrhotite and galena. Although jamesonite shows traces of Ag, the Cu-Ag sulfosalts are the main carriers of the Ag mineralization in the deposit, with contents that vary from 13.7 to 23.9 wt.% of Ag. In the most superficial levels of the area, secondary Fe oxide and hydroxide, scorodite and anglesite developed due to the oxidation of the ore.


Introduction
The polymetallic deposit of Valiña-Azúmara is located in the central sector of the recently discovered Vilalba gold district (Martínez-Abad et al., 2015a), which is situated 25 km southeast of the city of Vilalba (province of Lugo, NW Spain) (Fig. 1A).In addition to Valiña-Azúmara, the district is composed of the W/Au skarn of Castro de Rei and the As-Au (Ag-Pb-Zn-Cu-Sb) polymetallic mineralization of Arcos (Martínez-Abad et al., 2015b).All these deposits are hosted in Cambrian rocks, controlled by Variscan and Late-Variscan structures and spatially related to felsic dikes.Martínez-Abad et al. (2015a) proposed the model of intrusion-related gold systems to explain the mineralization of the Vilalba gold district.In this model, the Castro de Rei skarn and the Valiña-Azúmara mineralization represent a proximal and a distal deposit, respectively, relative to an unexposed post-tectonic calc-alkaline granitoid situated at depth (Fig. 1B).
The mineralization of Valiña-Azúmara was first recognized by Schulz (1835).This author indicated the presence of several old mining works where As-rich pyrite and Sb-bearing galena were extracted.At the beginning of the 20th century a local mining company carried out underground mining works in the area, in the so-called "arsenic mine of Azúmara".According to Amor Meilán (2005), in addition to As, low amounts of Ag and Au were recovered in the calcining kiln of the mine.The Valiña-Azúmara mineralization is classified as a vein-type deposit on the metallogenic map of Spain at the scale of 1:1.500.000(Au;IGME, 1972), whereas on sheet number 8 (Lugo) of the metallogenic map of Spain at the scale of 1:200.000(IGME, 1975), two mineralizations with unknown morphology are indicated in the area, one of Au (n° 30) and the other composed of pyrite, Pb and Ag (n°29).Later, González Lodeiro et al. (1982) made a first description of the ore present in the arsenic mine of Azúmara, identifying löllingite, jamesonite, galena, tetrahedrite and pyrite.In 1998, the Outokumptu mining company started to operate in the area, executing a number of exploration works, including several drill holes.In addition, this company carried out multi-element analysis (Au, As, Ag, Pb, Zn, Cu, Sb, Bi, Mo, Te, and Tl) of the mineralized sections of the drill cores.
This paper describes the mineral paragenesis and the structural controls of the Valiña-Azúmara deposit.Moreover, it provides a detailed petrographical, mineralogical, compositional and textural description of the metallic minerals present in the deposit.The electron microprobe analyzer (EMPA) and the scanning electron microscope (SEM) were employed for the compositional and textural description of the mineral phases, allowing us to recognize that Au mineralization occurs as refractory Au in As-rich pyrite and Cu and Pb sulfosalts bear the silver mineralization in the deposit.Finally, the multi-element analysis carried out in the mineralized sections of the drill cores permit us to geochemically characterize the mineralization of Valiña-Azúmara as well as define correlations between the analyzed elements.

Geological setting
The Valiña-Azúmara deposit is located in the Mondoñedo Nappe Domain of the West Asturian-Leonese Zone (WALZ), within the Iberian Massif (Fig. 1A).In this Domain, the sedimentary rocks consist of a thick preorogenic sequence mainly composed of Cambrian and Ordovician rocks and, to a lesser extent, Silurian rocks (Martínez Catalán, 1985;Pérez-Estaún et al., 1990).
Variscan granitic intrusions are abundant in the western part of the Mondoñedo Nappe Domain (Fig. 1A).They are grouped in a N-S trending thermal metamorphic belt called the Lugo Dome.Based on their composition and their relation with the Variscan stages of deformation, the Variscan granitic intrusions are divided into three main groups: syntectonic calc-alkaline granites, aluminous leucogranites and post-tectonic calc-alkaline granites (Capdevila, 1969, Bellido Mulas et al., 1987, Corretgé et al., 1990).The Valiña-Azúmara deposit is located in the eastern zone of the Lugo Dome, where post-tectonic calcalkaline granites like that of Lugo and Castroverde (287 Ma;Cocherie, 1978) dominate.

Sampling and analytical methods
The samples were taken from outcrops and drill cores in ore-bearing zones and barren zones at the Valiña-Azúmara area.They were studied by transmitted and reflected light microscopy, SEM (MEB JEOL-6610LV) and EPMA (Cameca SX100) at the University of Oviedo.In the electron microprobe analyses, the standard deviation of results is less than 0.1%.The composition of the metallic minerals was determined at 20 kV accelerating potential, 20 nA beam current and an acquisition time of between 10 and 20 s for X-ray peak and background.Natural and synthetic certified standards were used to calibrate the quantitative analyses.Moreover, more than 170 selected analyses were performed on potential Au-bearing pyrite and arsenopyrite with the following lower limits of detection: 140 ppm Au, 100 ppm Te, 80 ppm Zn, 460 ppm Bi, 150 ppm Co, 60 ppm Cu, 80 ppm Sb, 100 ppm Ag and 80 ppm Ni (95% confidence), using the Cameca SX100 with the following operating conditions: 20 kV accelerating potential, 200 nA beam current, and acquisition times of 60 (Co and Zn), 120 (Sb, Te, Ni, Ag, Cu and Bi), 180 (Se) or 240 (Au) s for X-ray peak and background.
The multi-element analyses provided by the mining company were carried out on 1m in thick mineralized sections of the drill cores CA-18, CA-1, VAL-1 y VAL-2 (Fig. 1B and 1C).The analyses were carried out in the OMAC laboratory (Galway, Ireland).The analyzed trace elements were Au, As, Ag, Pb, Zn, Cu, Sb, Bi, Mo, Te, and Tl.Samples were digested in aqua regia and then analyzed by inductively coupled plasma optical emission spectrometry (ICP-OES).

Local Geology
The sedimentary rocks in the area of Valiña-Azúmara belong to the Lower Quartzite Fm. and the Limestone and Slate Fm. (Lower Cambrian, Walter, 1966).These rocks were affected by the Variscan regional metamorphism in the grade of the biotite.The Quartzite Fm. consists of quartzite, sandstone and slate.The Limestone and Slate Fm. can be divided into two members (Fig. 1B).The lower one hosts the whole of the mineralization in Valiña-Azúmara.It consists of black slates, 150 m in thickness.Under the microscope, they have a lepidoblastic texture and consist of quartz, biotite and minor organic matter and calcite.The upper member is formed by green sandstone and slate.Alluvial quaternary rocks fill the alluvial plain of the Azúmara river.
The Valiña-Azúmara deposit is hosted in the inverted limb of the recumbent and overturned syncline of Real developed during the first Variscan phase (D 1 ).The associated cleavage (S 1 ) has a dip direction of N222-250°E and dips between 5° and 25°.During the second phase, a thrust-fault with a dip direction of N247-261°E and a dip of 35° affected the inverted limb of the syncline (Fig. 1B and 1C).This structure cut the black slates of the Limestone and Slate Fm.Later, all these structures were crosscut by N-S, E-W and NE-SW trending Late-Variscan faults.The N-S trending faults have a dip direction of N266-285°E and dip between 70° and 90°.
Estudios Geológicos, 71(2), julio-diciembre 2015, e040, ISSN-L: 0367-0449.doi: http://dx.doi.org/10.3989/egeol.42059.369 The south sector of the study area is affected by a E-W fault with a dip direction of N172°E and a dip of 70°.The NE-SW faults occur in the north section of the study area.They show a dip direction of N300-309°E and dip between 55° and 68°.One of these faults hosts a subvolcanic felsic dike, which was already identified by González Lodeiro et al. (1979).The dike is of up to 5 m in thickness and extends almost 1 km to the northeast, crossing the village of Castro de Rei.Geochemically, this subvolcanic rock is high-K, calc-alkaline and peraluminous, classified as rhyolite (Martínez-Abad et al., 2015a).It consists of quartz, plagioclase, K-feldspar and biotite with amphibole, monazite, allanite, apatite and zircon as accessory minerals.According to these authors, it represents the evolved facies of an unexposed post-tectonic calc-alkaline granite located at depth in the Castro de Rei surroundings (Fig. 1B).

Mineralization
The mineralization in Valiña-Azúmara is structurally controlled.It is mainly associated with the thrust fault (D 2 ).In this structure, the ore occurs cementing the fault breccias and, to a lesser extent, disseminated in weakly silicified and sericitized metasedimentary host rocks (fault breccias and narrow selvages around the structure) (Fig. 2).Based on the old mining works and the drill holes carried out in the area by the mining company, it is estimated that the mineralized structure is at least 720 m long, reaches 75 m in depth and up to 5 m in thickness (Fig. 1C).To a lesser extent, the mineralization in the area is also found filling hydrothermal veins of up to 5 cm in thickness that seal fractures of the N-S and NE-SW Late-Variscan faults.On some occasions, these veins spread laterally a few centimeters (up to 4 cm) along S 1 cleavage planes.In addition to filling the veins, the ore also occurs disseminated in fault breccias and narrow selvages of up to 4 cm in thickness that are weakly hydrothermally altered (silicified and sericitized) (Fig. 2B, 2C and 2D).
The mineralization developed in two hypogene stages.The first is characterized by a Au-As metal association whereas the second shows a Ag-Pb-Zn-Cu-Sb metal association.Eventually, widespread weathering affected the superficial levels of the area.A supergenic stage consisting of secondary minerals was formed during the weathering and oxidation of the ore. Figure 3 shows the paragenetic sequence of the Valiña-Azúmara deposit.

Lithogeochemistry
The multi-element analyses show that the mineralized sections of drill core contain variable amounts of Au, As, Ag, Pb, Zn, Cu and Sb (Table 1).These samples have contents in Au of up to 2.06 ppm, in As up to 12.7%; in Ag up to 487 ppm; in Pb up to 4.4%; in Cu up to 600 ppm; in Zn up to 1.5% and in Sb up to 3600 ppm (Table 1).In all the analyzed samples, the content of Mo, Bi, Te and Tl was below the minimum limit of detection.
Geochemically, Au shows a low but significant correlation with As (R 2 =0.66;Fig. 4A).One analysis was omitted in the estimation of the correlation coefficient between both elements due to its strong dispersion compared to the rest of the analyses.Au shows no correlation with the rest of analyzed elements.With regard to the Ag, it shows a strong correlation with Cu (R 2 =0.9) (Fig. 4B).Similar to Au, Ag shows no significant correlation with the rest of analyzed elements.

First stage of mineralization (Au-As)
This stage of mineralization consists of arsenopyrite and minor pyrite.The ore occurs filling fractures and cementing fault breccias as well as disseminated in the hydrothermally altered metasedimentary host rocks (Fig. 2).Sealing veins and fault breccias, arsenopyrite and pyrite occur together with quartz and minor calcite.In the hydrothermally altered zones, sulfides occur isolated or forming aggregates of a few crystals appearing along S 1 cleavage planes (Fig. 5A).These aggregates often occur as pseudomorphic replacements of the previous grains of biotite, evidencing sulfidation processes.Thus, the biotite is altered to muscovite together with rutile and fine-grained pyrite and arsenopyrite (Fig. 5B).
Arsenopyrite is the main ore mineral of this stage of mineralization.It occurs disseminated in the hydrothermally altered metasedimentary host-rocks as isolated grains or forming aggregates of a few grains together with the pyrite.In the altered zones, Estudios Geológicos, 71(2), julio-diciembre 2015, e040, ISSN-L: 0367-0449.doi: http://dx.doi.org/10.3989/egeol.42059.369 the arsenopyrite is subhedral to anhedral in shape, with diameter that commonly varies between 5 and 100 µm (Fig. 5B), and rarely reach 500 µm.When arsenopyrite occurs as a filling phase in veins and fault breccias, it forms subhedral crystals, up to 1mm in diameter, that are isolated or in aggregates of several grains intergrown with the pyrite and the gangue minerals.The EMPAs performed on the arsenopyrite indicate that the As content of this mineral varies from 43.45 to 46.9 wt.% (30.8 to 34.1 at.%).The arsenopyrite crystals commonly display an oscillatory zoning in As, showing an As-poor core with respect to the rims.Moreover, arsenopyrite often shows impurities of Sb (of up to 0.17 wt.%) and Cu (≤195 ppm), and on some occasions of Ni (≤116 ppm) (Table 2).It should be noted that in the 49 EMPAs performed on this mineral, the Au concentration was always below the minimum limit of detection.
Pyrite is less abundant and commonly of smaller size than arsenopyrite.According to its textural characteristics under optical microscopy and BSE images, in addition to its chemical composition (Table 3), pyrite has been divided into two types: Py-I and Py-II.1B).Weathering affected the sample, producing the supergene alteration of the primary ore.The main secondary minerals recognized are iron oxides and hydroxides (reddish crust) and scorodite (pale green crust).B. Sample of veins composed mainly of arsenopyrite, quartz and minor pyrite hosted in weakly silicified and sericitized black slates.The ore mineralization is also disseminated in the host rock along S 1 cleavage planes.C. Subvertical Late Variscan fault sealed by hydrothermal veins located in the north sector of Valiña-Azúmara ("SAB" in the map of Fig. 1B).D. Sample taken from the N-S Late-Variscan fault of photo "C".The ore mineralization occurs filling the N-S fractures as well as disseminated in the adjacent hydrothermally altered black slate.In the sample, tension gashes mainly filled by quartz are also observed.
Estudios Geológicos, 71(2), julio-diciembre 2015, e040, ISSN-L: 0367-0449.doi: http://dx.doi.org/10.3989/egeol.42059.369 Py-I occurs intergrown with quartz and calcite grains filling veins and fault breccias as well as disseminated in the hydrothermally altered metasedimentary host rocks.It forms subhedral to anhedral grains of porous appearance and of up to 500 μm in diameter (Fig. 5C and 5D).Py-I is normally intergrown with the arsenopyrite, evidencing its coeval precipitation (Fig. 5B).Py-I commonly forms a core overgrown and partially corroded by the other type of pyrite that will be described later.Chemically, the EMPAs carried out on Py-I indicate that it is poor in As (< 0.2 wt.%), and often contains impurities of Cu (≤ 117 ppm) and, on some occasions, of Te (≤ 598 ppm) and Zn (≤ 412 ppm) (Table 3).
Py-II forms polygonal bands enriched in As, overgrowing and partially corroding the previous Py-I (Fig. 5C and 5D).On some occasions, both pyrites occur separated by a narrow band of gangue minerals.Py-II was formed after both arsenopyrite and Py-I precipitation, representing the last ore mineral of the first stage of mineralization.Chemically, Py-II is characterized by an enrichment in As from 0.8 to 1.7 wt.% (Table 3).Apart from As, impurities of other trace elements are commonly present, with Zn reaching 271 ppm, Cu reaching 124 ppm and Sb reaching 265 ppm.In addition, Py II can occasionally contain trace amounts of Bi (≤0.19 wt.%), Ni (≤100 ppm) and Te (≤200 ppm).Moreover, in this pyrite traces of Au, with concentrations of up to 176 ppm, have also been detected (Table 3, Fig. 5).This fact would explain the correlation between Au and As obtained in the multi-element analyses carried out on the mineralized sections of drill cores (Fig. 4A).

Refractory Au in pyrite
In accordance with the EMPAs previously shown, Au in Valiña-Azúmara occurs as refractory or invisible Au within As-rich pyrite grains (Py-II).According to Deditious et al. (2014), the presence of refractory Au in pyrite has been observed in numerous types of Au deposit including Carlin type, porphyry Cu, epithermal Au, orogenic Au, volcanogenic massive sulfide, iron oxide Cu-Au and paleoplacer Au deposits.Within NW Spain, in addition to the Vilalba gold district, refractory Au has been identified in the deposits  of Salave (Martín-Izard & Rodríguez-Terente, 2009), Salamón (Paniagua et al., 1996;Crespo et al., 2000;Fadón Loro, 2007), El Valle-Boinás (Cepedal et al., 2008) and Ibias (Villa et al., 1993) (Fig. 1A).Similar to Valiña-Azúmara, in all these deposits Au appears within As-rich pyrites that often contain traces of other elements.Furthermore, in all these deposits the presence of refractory Au within arsenopyrite grains is also common.However, as previously mentioned, Au was not detected in the arsenopyrite of Valiña-Azúmara.
In agreement with Bakken et al. (1989), Friedl et al. (1995), Simon et al. (1999a,b), Cabri et al. (2000), Palenik et al. (2004) and Reich et al. (2005), Au in As-rich pyrite and arsenopyrite occurs as solid solution (Au +1 ) and as nanoparticles of native Au (Au 0 ).Reich et al. (2005) defined the empirical solid solubility of Au in As-pyrite as C Au =0.02×CAs +4×10 −5 for a range of temperatures between 150-250 °C, in which C Au and C As represent the concentration of Au and As expressed as an atomic percentage (at.%)(Fig. 6).The line established by this equation describes the solubility limit of Au in pyrite.The points falling below this line contain Au +1 while the points falling above it contain Au 0 .The Au-As stage of mineralization in Valina-Azúmara took place at temperatures over 355 °C (Martínez-Abad et al., 2015a).However, Deditious et al. (2014) recently studied Au-bearing As-rich pyrites from different hydrothermal deposit styles (porphyry Cu, orogenic gold, metamorphic VMS and IOCG) that formed at higher temperatures than 250 °C (up to 400 °C).These authors concluded that the line of solubility of Au proposed by Reich et al. (2005) barely changes except in the case of metamorphic VMS and orogenic gold deposits, where the solubility limit can be altered as a result of complex recrystallization histories, high temperature alteration or cooling, leading to Au remobilization and growth of post-depositional Au, not observed in Valiña-Azúmara.In addition, these authors observed that the As-rich pyrites from high temperature deposits are generally plotted under the line of solubility of Au, indicating they were formed from solutions that were not saturated in Au.

Second stage of mineralization (Ag-Pb-Zn-Cu-Sb)
This stage of mineralization consists of chlorite, quartz and minor calcite in addition to metallic minerals such as sphalerite, jamesonite (Pb 4 FeSb 6 S 14 ), Cu-Ag sulfosalts (tetrahedrite-freibergite series) and minor chalcopyrite, pyrrhotite and galena (Fig. 7).These minerals occur as a second generation of filling in the structures previously described, suggesting reopening of the preexisting fractures, encompassing and partially replacing the minerals of the previous mineralization stage.The earlier deposited pyrite and arsenopyrite frequently reveal microfractures sealed by gangue and metallic minerals from this stage (Fig. 7D).Sphalerite is the most abundant ore mineral of this stage.It occurs as anhedral dark red grains, usually below 1 mm in diameter (Fig. 7C, 7E and 7F).The Fe content of the sphalerite varies between 4.2 and 7.2 wt.% (Table 4).The sphalerite usually occurs intergrown with Cu-Ag sulfosalts and jamesonite.In addition, these last two minerals and, especially pyrrhotite and chalcopyrite, may occur within the sphalerite, forming inclusions and small elongated patches (<30 μm) along perpendicular crystallographic directions ("chalcopyrite disease") (Fig. 7F).
Jamesonite forms aggregates of tabular grains with a diameter of up to 500 μm.It occurs isolated as well as intergrown with Cu-Ag sulfosalts and sphalerite (Fig. 7B and 7C).Furthermore, on occasions it forms small inclusions within the sphalerite grains.Chemically, it should be noted that on some occasions jamesonite contains traces of Ag (of up to 0.22 wt.%;Table 4) .
The Cu-Ag sulfosalts form subhedral to anhedral grains of up to 1 mm in diameter.They are normally intergrown with jamesonite (Fig. 7A and 7B) and, on some occasions, occur as small inclusions within the sphalerite grains.The Cu-Ag sulfosalts of Valiña-Azúmara belong to the tetrahedrite-freibergite solid solution series.Chemically, they have contents in Cu ranging from 22.3 to 29.4 wt.%.Together with the chalcopyrite, they are the main Cu-bearing minerals in the deposit.In addition, these sulfosalts show significant contents in Ag, ranging from 13.05 to 23.9 wt.% (Table 4).In agreement with Moëlo et al. (2008), the Cu-Ag sulfosalts of Valiña-Azúmara have been differentiated into two different phases on the basis of their chemical composition.The variety with Ag over 4 a.p.f.u has been classified as freibergite, whereas the variety with Ag below 4 a.p.f.u has been classified as Ag-rich tetrahedrite (Table 4, Fig. 8).According to these authors, due to Cu being substituted by Ag, the Ag concentration seems to be inversely correlated to the Cu concentration in the tetrahedrite-freibergite solid solution series (Fig. 8).Although, as we mentioned before, jamesonite may contain traces of Ag, the main bearers of the Ag mineralization within the Valiña-Azúmara deposit are the Ag-rich tetrahedrite and freibergite.This fact explains the strong correlation between Cu and Ag obtained in the multi-element analyses carried out on the mineralized sections of drill cores (Fig. 4B).
Chalcopyrite, galena and pyrrhotite are the least abundant ore minerals of the second stage of mineralization.They normally occur filling small hollows  Sp) and jamesonite partially encompass arsenopyrite grains from the first stage of mineralization.Jamesonite also occurs filling small hollows within the arsenopyrite (RL).D. Ag-rich tetrahedrite sealing a microfracture that crosscuts an arsenopyrite grain from the first stage of mineralization (RL).E. Sphalerite crystals encompassing and partially replacing arsenopyrite grains from the first stage of mineralization.In the photo it is also possible to observe the presence of abundant chlorite crystals in equilibrium with the sphalerite grains (PPL).F. Sphalerite grain with inclusions and small elongated patches (<30 μm) of pyrrhotite and minor chalcopyrite along perpendicular crystallographic directions (chalcopyrite disease).

Supergene alteration
Widespread weathering affected the superficial levels of the area, producing the supergene alteration of the primary ore.The secondary minerals recognized in the deposit are iron oxides and hydroxides, scorodite (FeAsO 4 •2H 2 O) and anglesite (PbSO 4 ).
The iron oxides and hydroxides are the most abundant secondary minerals in the deposit.They occur disseminated in the supergene-altered samples, forming thin reddish crusts (Fig. 2A).Scorodite and anglesite occur associated with the iron oxides and hydroxides.The scorodite replaces the arsenopyrite, forming thin pale green crusts, whereas anglesite replaces the Pb-bearing minerals (jamesonite and minor galena), forming thin yellowish crusts (Fig. 2A).The oxidation of the As-rich pyrite (Py-II) must have produced the liberation of the refractory Au contained within this mineral.However, native Au has not been recognized in any of the supergene altered samples studied for this work.

Discussion
Valiña-Azúmara together with the W/Au skarn of Castro de Rei and the polymetallic mineralization of Arcos constitute the Vilalba gold district (Martínez-Abad et al., 2015a).The Valiña-Azúmara mineralization is structurally and, to a lesser degree, lithologically controlled.As previously mentioned, Variscan thrust fault (D 2 ) and N-S, NE-SW Late-Variscan faults hosted the mineralization.The occurrence of a NE-SW trending felsic dike in the north sector of the area (Fig. 1B) indicates these Late-Variscan faults allowed the intrusion of post-tectonic igneous rocks in addition to the migration of the mineralizing fluids.The felsic dike outcropping in the area has been interpreted as part of the dike suite of a post-tectonic granitoid lying beneath the Castro de Rei area, where the occurrence of contact aureole hornfels and the skarn mineralization, with maximum temperatures of formation of between 520 and 560 °C, evidences the presence of a blind granitic body (Martínez-Abad et al., 2015a).Igneous rocks of a similar type have also been observed forming dikes and sills at the deposit of Arcos, located around 6 km to the south of Valiña-Azúmara (Martínez-Abad et al., 2015b).
The mineralization of Valiña-Azúmara occurs cementing fault breccias and forming veins and, to a lesser extent, as dissemination in the altered host rocks, which mainly consist of black slates.
Contrary to what is observed in the nearby area of Castro de Rei, the black slates show no evidence of being affected by contact metamorphism.Hydrothermal alteration of host-rocks produced sericitization in the selvages of veins and fault breccias, rarely pervasive.The biotite of the slates was altered to muscovite together with rutile and fine-grained sulfides and sulfoarsenides, evidencing sulfidation processes.Silicification also occurs but, unlike the polymetallic mineralization of Arcos, where silicification is locally pervasive and develops jasperoids (Martínez-Abad et al., 2015b), the presence of lesscarbonated rocks in Valiña-Azúmara implies this type of hydrothermal alteration is not well-developed.This type of hydrothermal alteration indicates the presence of an acid ore-forming fluid that barely reacts with the pelitic rocks of Valiña-Azúmara but reacts strongly with the alkaline limestones of Arcos.
The metallic paragenesis of Valiña-Azúmara, consisting of a first stage of mineralization with arsenopyrite and pyrite and a second stage with base metal sulfides and Pb-Sb-Ag sulfosalts, reflects the geochemistry signature of the area.If we compare the multielemental analysis carried out on drill-core mineralized samples from the Valiña-Azúmara and the Castro de Rei skarn (Bi up to 1310 ppm; Te up to 41 ppm; Mo up to 247 ppm; W up to 431 ppm; Au up to 6.4 ppm; As >2%; Ag up to 28 ppm; Sb up to 3175 ppm; Cu up to 1851 ppm; Pb up to 7000 ppm; and Zn up to 3590 ppm; Martínez-Abad, 2013), the former is enriched in As, Ag, Pb, Zn and Sb with respect to Castro de Rei, whereas the Castro de Rei skarn is enriched in W, Bi, Te, Cu, Au and Mo with respect to Valiña-Azúmara.
The deposition of gold in Valiña-Azúmara took place during the first stage of mineralization, since the only gold detected was in EMPAs of As-rich pyrites (Py-II).The Au/As ratios of Py-II suggest it formed from solutions that were not saturated in Au.Sulfidation processes, such as the one observed in Valiña-Azúmara, are proposed as the principal mechanism of deposition of invisible Au in Carlin Type and epithermal ore deposits, where it is generally accepted that Au is transported as a bisulfide complex.According to Reich et al. (2005), in solutions not saturated in Au such as Valiña-Azúmara, the decrease in H 2 S produced by sulfidation strongly favors the formation of arsenian pyrite and incorporation of Au  (Moëlo et al., 2008), within the freibergite-tetrahedrite series the mineral with Ag content above 4 a.p.f.u. is classified as freibergite (grey square), whereas that below 4 a.p.f.u.should be called Ag-rich tetrahedrite (white circle).
Estudios Geológicos, 71(2), julio-diciembre 2015, e040, ISSN-L: 0367-0449.doi: http://dx.doi.org/10.3989/egeol.42059.369as solid solution.It may therefore be reasonable to deduce that in the altered rocks of Valiña-Azúmara the hydrothermal solution transporting Au as bisulfide complexes reacted with liberated iron from the previous Fe-bearing minerals (biotite) in the rock and precipitated Au together with As-bearing iron sulfides.Martínez-Abad et al. (2015a) proposed an intrusion-related gold system model (IRGS, Lang & Baker, 2001) for the mineralizations of the Vilalba gold district.According to Lang and Baker (2001), the IRGSs comprise a group of magmatic-hydrothermal gold deposits hosted primarily within intrusions or in adjacent wall rocks.Based on their spatial relationship to intrusions, these deposits can be separated into the following three categories: Intrusionhosted deposits comprising auriferous vein deposits (Au-Bi±Te±As±Mo±W); proximal deposits located adjacent to the intrusion, within the metamorphic aureole, and including W±Cu±Au and Cu-Bi-Au±W skarns and Au-As veins; distal deposits located beyond the outer limit of hornfels and having a typical metal signature of Au-As-Sb-Hg±Ag-Pb-Zn (Au).They normally include mesothermal to epithermal auriferous quartz-sulfide veins along steep faults, base-metal veins enriched in Ag±Au, and Au disseminations in calcareous and carbonaceous sedimentary rocks (Lang & Baker, 2001).The Ag-Pb-Zn-(Au) metal association may form individual veins or representing the youngest stage of mineralization within other deposit types, and may include pyrrhotite, galena, sphalerite, Pb-Sb sulfosalts and Ag-bearing sulfosalts such as tetrahedrite and freibergite as ore minerals.
According to Martínez-Abad et al. (2015a), the W/Au skarn of Castro de Rei and the polymetallic mineralization of Valiña-Azúmara constitute an IRGS.The skarn represents a proximal deposit with respect to an unexposed granitoid, and the Valiña-Azúmara represents a distal deposit developed in the peripheral or distal zones with respect to the granitic body, outside the contact aureole.Furthermore, these deposits show the characteristic metal signature of the IRGSs, with metals such as W, Mo, Bi and Te precipitated in the high-temperature proximal deposit of Castro de Rei, while distal and cooler areas like Valiña-Azúmara are enriched in elements such as As-Ag-Pb and Zn.
Finally, Valiña-Azúmara shows many similarities with the polymetallic deposit of Arcos, which shows the same geochemical signature Au-As (Ag-Pb-Zn-Cu-Sb) and has also been interpreted as a distal deposit from an IRGS.In both deposits, the ore appears filling fractures and the paragenesis starts with an early Au-As stage of mineralization, with Au occurring mainly as invisible Au.Arsenopyrite and pyrite are the main sulfide minerals during this stage and sericitization, silicification and sulfidation are the main hydrothermal alteration processes.Unlike Arcos, the area of Valiña-Azúmara lacks reactive calcareous rocks, which implies a significantly lesser volume of hydrothermally altered rocks and, therefore, disseminated mineralization.Both deposits contain a second stage of mineralization dominated by sphalerite and Pb-Sb-Ag sulfosalts that, as previously mentioned, are characteristic of the Ag-Pb-Zn-(Au) metal association of the IRGS.In contrast to Valiña-Azúmara, tetrahedrite (up to 4.3 wt% of Ag) and accessory electrum (up to 27.7 wt% of Ag) are the main Ag-bearing minerals in Arcos.These deposits show similarities with the deposits of Salamón (Crespo et al., 2000) in the NW Iberian Massif, and Brevery Creek (Diment & Craig, 1998) in Yukon (Canada), considered by Lang & Baker (2001) to be good examples of IRGS distal deposits.

Conclusions
The mineralization of Valiña-Azúmara is structurally controlled.It is mainly hosted in a Variscan thrust fault (D 2 ) with a dip direction of N247-261°E and a dip of 35°, that affects Lower Cambrian black slates.To a lesser extent, it also occurs filling Late Variscan N-S faults with a dip direction of N266-285°E and dip between 70° and 90°, and Late Variscan NE-SW, with a dip direction of N300-309°E and dip between 55° and 68°.The mineralization occurs cementing fault breccias and forming hydrothermal veins.To a lesser extent, it also occurs disseminated in weakly sericitized and silicified fault breccias and fracture walls of up to 4 cm in thickness.
The mineral paragenesis is divided into two hypogene stages.The first is characterized by a Au-As metal association and consists of arsenopyrite and pyrite as ore minerals and quartz, rutile, sericite and minor calcite as gangue minerals.The arsenopyrite crystals commonly display an oscillatory zoning in As (43.45 to 46.9 wt.% in As), showing As-poor cores with respect to the rims.They often contain impurities of Sb, Cu and Ni.However, no traces in Au were detected in this mineral.Two different types of pyrites (Py-I and Py-II) were differentiated.Py-I commonly forms a core overgrown and partially corroded by Py-II.While Py-I is poor in As and lacks of traces of other elements, Py-II is As-rich (≤1.7 wt.%) and often contains traces of other elements such as Te, Zn, Cu, Bi, Sb and Au.Gold occurs as refractory Au within the As-rich pyrite (Py-II), showing concentrations of up to 176 ppm.The Au/As ratios of Py-II suggest that Au is present as solid solution (Au +1 ) within this sulfide and, therefore, that the hydrothermal ore-forming fluid was not saturated with respect to Au.
The second stage of mineralization is characterized by a Ag-Pb-Zn-Cu-Sb metal association.It replaces the first stage (Au-As) and consists of sphalerite, jamesonite, Ag-rich tetrahedrite, freibergite, chalcopyrite, pyrrhotite and galena as ore minerals and quartz, calcite and chlorite as gangue minerals.This stage is sealing open spaces as cavities and microfractures that crosscut the ore minerals of the first stage (Au-As) of mineralization.Sphalerite shows contents in Fe of up to 7.2 wt.%.The main bearers of the Ag mineralization in the deposit are the Ag-tetrahedrite (from 13.05 to 21.02 wt.% in Ag) and the freibergite (up to 23.9 wt.% in Ag), although jamesonite on occasions also contains trace amounts of Ag (≤0.22 wt.%).
Eventually, secondary Fe oxide and hydroxide, scorodite and anglesite developed due to the oxidation of the ore in the most superficial areas.The oxidation of the As-rich pyrite (Py-II) must have produced the liberation of the refractory Au contained within this mineral, though, native Au has not been recognized in the altered samples.

Fig. 2 .
Fig. 2.-A.Fault breccia sample taken from an old mining work in the Valiña-Azúmara area (VAL-TOX in the map of Fig.1B).Weathering affected the sample, producing the supergene alteration of the primary ore.The main secondary minerals recognized are iron oxides and hydroxides (reddish crust) and scorodite (pale green crust).B. Sample of veins composed mainly of arsenopyrite, quartz and minor pyrite hosted in weakly silicified and sericitized black slates.The ore mineralization is also disseminated in the host rock along S 1 cleavage planes.C. Subvertical Late Variscan fault sealed by hydrothermal veins located in the north sector of Valiña-Azúmara ("SAB" in the map of Fig.1B).D. Sample taken from the N-S Late-Variscan fault of photo "C".The ore mineralization occurs filling the N-S fractures as well as disseminated in the adjacent hydrothermally altered black slate.In the sample, tension gashes mainly filled by quartz are also observed.

Fig. 5 .
Fig. 5.-A.Photomicrograph under plane polarized light (PPL) of the metallic minerals of the first stage of mineralization.They are hosted in a vein together with quartz and disseminated in the weakly sericitized slaty host rock along S 1 cleavages planes.B. Photomicrograph, under reflected light (RL), of arsenopyrite (Apy) and pyrite (Py) of the first stage of mineralization.These minerals are associated with rutile (Rt) crystals.C. BSE image of a zoned pyrite constituted by a core of porous As-poor pyrite (Py-I) overgrown and partially replaced by As-rich pyrite (Py-II).The grain contains small inclusions of sphalerite (Sp) and galena (Gn).The position of EMPAs and gold concentration (ppm) is indicated.D. BSE image of an aggregate of several zoned pyrite grains constituted by As-poor cores of Py-I overgrown by As-rich Py-II.

Fig. 6 .
Fig. 6.-Au-As plot of Au-bearing Py-II.The solubility limit for Au proposed by Reich et al. (2005) is represented by the curve C Au =0.02×CAs +4×10 −5 , where C Au and C As , represent the concentration of Au and As in atomic percent (at.%).Above this line, Au is in the form of nanoparticles of native gold whereas, below it, Au is considered to be present in solid solution.l.d.: limit of detection of Au (140 ppm) for the analyses carried out in Valiña-Azúmara Py-II (dashed line).Also included in the diagram are the analyses of Au-bearing pyrites from other Au deposits of NW Spain.

Fig. 7 .
Fig. 7.-Photomicrographs of metallic assemblages from the second, Ag-Pb-Zn-Cu-Sb stage of mineralization.A. Cavity sealed by quartz (Qz) and opaque grains in a fault breccia (Cross polarized light, CPL).B. Detail of the opaque grains of photomicrograph "a" under reflected light.The Ag-rich tetrahedrite (Ttr) is intergrown with jamesonite.The arsenopyrite (Apy) was deposited earlier, during the first stage of mineralization, and occurs disseminated in the fault breccia.C. Grains of sphalerite (Sp) and jamesonite partially encompass arsenopyrite grains from the first stage of mineralization.Jamesonite also occurs filling small hollows within the arsenopyrite (RL).D. Ag-rich tetrahedrite sealing a microfracture that crosscuts an arsenopyrite grain from the first stage of mineralization (RL).E. Sphalerite crystals encompassing and partially replacing arsenopyrite grains from the first stage of mineralization.In the photo it is also possible to observe the presence of abundant chlorite crystals in equilibrium with the sphalerite grains (PPL).F. Sphalerite grain with inclusions and small elongated patches (<30 μm) of pyrrhotite and minor chalcopyrite along perpendicular crystallographic directions (chalcopyrite disease).