Abstract
Devonian/Carboniferous conodonts from the Chelcheli section in the Alborz Mountains were investigated. Although conodonts are generally less abundant in the entire section, important zonal index taxa of the widely applied conodont standard zonation could be used for a precise conodont zonation. Forty-seven conodont species belonging to fifteen genera were identified and led to the discrimination of fifteen conodont zones, ranging from the Palmatolepis minuta minuta Zone into the Scaliognathus anchoralis-Doliognathus latus Zone. At the Devonian/Carboniferous boundary (DCB), characteristic lithologies such as black shales and massive sandstones represent equivalents of the Hangenberg Black Shale and Hangenberg Sandstone. Close to the DCB, there is a small stratigraphic hiatus in the conodont record which might be a result of facies (shallow-water succession with no conodont record and siliciclastic rocks) rather than a period of non-deposition as the sedimentological record seems continuous. Similar to other DCB sections in shallow-water facies in Iran the two biostratigraphically important species Protognathodus kockeli and Protognathodus kuehni do not occur.
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Introduction
The Alborz range in northern Iran is an active fold-and-thrust belt (Berberian 1983; Alavi 1996) and is situated about 200–500 km to the north of the Neo-Tethyan suture. The closure of the Palaeotethys between the Iran Plate as a part of Gondwana and the Turan Plate (Laurussia) occurred in the early Late Triassic and was accomplished during the Early/earliest Mid Jurassic (Golonka 2002). During the Palaeozoic, Iran was situated at the northern margin of Gondwana (Berberian and King 1981; Scotese 2001). In the mid-Palaeozoic, most of Iran was located about 20°–25° south of the palaeoequator. During the Mississippian, the Alborz Basin was positioned at a palaeolatitude of approximately 45–50° S (Vachard 1996; Torsvik and Cocks 2004, 2013; Muttoni et al. 2009). Devonian and Carboniferous rocks are most widespread in central and eastern Alborz but they belong to different structural units, some of which are separated by suture zones (Stöcklin 1968; Alavi 1991; Davoudzadeh 1997). The most important structural units in Iran are summarized in Fig. 1. During the last decades, a number of sections in eastern Alborz were studied due to their high fossil content and excellent preservation (e.g. Bozorgnia 1973; Brice et al. 1974; Ahmadzadeh-Heravi 1975; Jenny 1977; Coquel et al. 1977; Ashouri 1990, 2006; Wendt et al. 2005; Ghavidel-Syooki and Owens 2007; Hashemi 2011; Falahatgar and Mosaddegh 2012; Falahatgar et al. 2018; Abadi et al. 2015, 2017; Pour et al. 2018; Valeryi et al. 2018; Parvizi et al. 2021). Recently, Devonian/Carboniferous boundary (DCB) sections became a focus of international research (Aretz et al. 2013; Corradini et al. 2016). First results on DCB sections in Iran are shortly summarized in Königshof et al. (2021). The fundamental importance to study this interval is linked with one of the major extinction events (Hangenberg Crisis) in Earth’s history. Based on the ecological severity index by McGhee et al. (2013) the end-Devonian extinction is known as the seventh severe mass extinction in Phanerozoic. This first-order mass extinction eliminated nearly 20% of marine invertebrate genera and reduced the long-term biodiversity of all vertebrates by about 50% (Sepkoski 1996; Walliser 1996; Sandberg et al. 2002). The D/C transition is characterized by several transgressive/regressive cycles and widespread ocean anoxia have been recognized along continental margins or epicontinental basins known as the Hangenberg Black Shale Event (HBS). Close to the DCB a major sea-level fall (Hangenberg Sandstone Event, HSS) of assumed more than 100 m (Kaiser et al. 2011; Myrow et al. 2014 see review summary in Kaiser et al. 2016) which is associated with the glaciation on Gondwana (e.g. Isaacson et al. 1999, 2008; Streel et al. 2000, 2001; Caputo et al. 2008; Brezinski et al. 2010; Lakin et al. 2016) can be recognized in many sections around the world. The deposition of these black shales and sandstones is known as the early and middle phase of the Hangenberg Crisis as defined by Kaiser et al. (2016) and Becker et al. (2016). Depending on facies setting equivalents of the regressive Hangenberg Sandstone can also be recognized as an unconformity and/or reworked sediments (see; Cole et al. 2015; Bábek et al. 2016; Kaiser et al. 2016). Stratigraphical gaps and non-deposition related to this major regression are also known from eastern Iran as it was shown by Bahrami et al. (2011). It is noteworthy that most DCB sections worldwide are described from hemipelagic and pelagic successions. To get a more comprehensive picture of one of the most interesting time slices in Earth’s history it is necessary to study DCB sections in different depositional settings such as in shallow-water environments. Most of the DCB sections from the central and eastern Alborz Mountains have been deposited in a shallow-water, carbonate ramp setting (Königshof et al. 2021). However, in contrast to other DCB sections in Iran (Habibi et al. 2008; Bahrami et al. 2011), the Chelcheli section exhibits “characteristic rock” types around the DCB such as black shale and sandstone. In this study, we have sampled conodonts from the Khoshyeilagh Formation and the overlying Mobarak Formation of the Chelcheli section with a special focus on the DCB. Herein, we present an improved conodont-based stratigraphical record around the DCB in neritic facies which is an important contribution to the ongoing discussion about a potential new definition of the DCB.
Geological setting and study area
Several sections in the eastern Alborz have repeatedly been studied in the past and have contributed considerably to the knowledge of the sedimentary record of the Devonian/Mississippian in northern Iran (e.g. Bozorgnia 1973; Brice et al. 1974, 1978; Stampfli 1978; Hamdi and Janvier 1981; Weddige 1984; Ashouri 1990, 1994, 2006; Ghavidel-Syooki 1994; Königshof et al. 2021). For the present study, we examined the Chelcheli section with a focus around the DCB. The section (Figs. 1 and 2) is located close to the Chahar-Bagh village of the Chelcheli Wildlife conservation area at the northern end of the N–S striking Chelcheli mountain range (about 70 km northwest of Shahrud city between Shahrud and Gorgan, sheet H4 Gorgan, 1: 250.000, see Salehirad et al. (1991); WGS coordinates: base of the section: 36° 36′ 15.54″ N; 54° 32′ 55.57″ E, top of the section: 36° 36′ 15.89″ N; 54° 32′ 48.49″ E).
The Chelcheli section is exposed along a steep cliff in the higher mountain range and has a thickness of about 1300 m. Rocks are mainly composed of neritic sediments of Mid-Devonian to Pennsylvanian age. This conodont study deals with samples from the Khoshyeilagh Formation and the overlying Mobarak Formation with a special focus on the DCB (Fig. 3a). Both formations are widely distributed in central and eastern parts of the Alborz Mountains and were studied intensively in the last decades due to their rich fossil content. However, there are still some uncertainties as detailed (bio-) stratigraphic investigations on the Khoshyeilagh Formation are still lacking (e.g. Bozorgnia 1973; Ashouri 1990, 1994, 2006).
The Khoshyeilagh Formation is mainly composed of limestone, shale and marl and thick-bedded sandstone close to the DCB. In the central Alborz Mountains, the Mobarak Formation conformably overlies the Upper Devonian Jeirud Formation (Abadi et al. 2015). This formation is an equivalent to the Upper Devonian Khoshyeilagh Formation in eastern Alborz Mountains (Königshof et al. 2021: fig. 8). In the Chelcheli section, the Mobarak Formation conformably overlies the Khoshyeilagh Formation. Whereas the base of this formation is defined, the top of the formation varies in age from the Tournaisian–early Visean? in the southern part of the Alborz Mountains to late Visean in the northern part of the Alborz Mountains (Bozorgnia 1973; Wendt et al. 2005; Brenckle et al. 2009). The age discrepancy might be a result of variable uplift across the southern Alborz Mountains during the late Visean until the Cisuralian (Bozorgnia 1973; Lasemi 2001; Wendt et al. 2005) and/or by a progressive drop in sea level linked to glacial episodes between the latest Visean–Serpukhovian and early Moscovian (Fielding et al. 2008; Haq and Schutter 2008; Rygel et al. 2008; Brenckle et al. 2009). The characteristic sediments of this formation are dark grey shale and thin-bedded limestone in the lower parts, which grade into thick to massively bedded limestones with abundant skeletal and non-skeletal fragments in the upper parts (Mosaddegh 2000; Lasemi 2001; Fig. 3). According to several authors (e.g. Webster et al. 2003, 2011; Torsvik and Cocks 2004; Wendt et al. 2005; Golonka 2007; Bagheri and Stampfli 2008; Brenckle et al. 2009) the Mobarak Formation represents the most extensive carbonate cycle along the northern margin of Gondwana which was deposited after the Palaeo-Tethys rift opening.
Lithology of the section
The Khoshyeilagh Formation of the Chelcheli section is 182 m thick and was subdivided into five lithological units (Figs. 3 and 4). The lowermost succession (Unit 1, samples Ch1–Ch4-1, thickness 37 m) contains black thin to medium-bedded limestone, with intercalated shale and marl layers. This unit is very fossiliferous and contains trilobites, brachiopods, gastropods, and micro-vertebrate remains. The overlaying unit (Unit 2, samples Ch5–Ch9-1, thickness 65 m) is mainly composed of shale, marl, and medium-bedded limestone. This succession is overlain by thin-bedded limestone followed by alternating medium-bedded limestone with dark-grey shale and marl (Unit 3, samples Ch10–Ch14, thickness 60 m). Distinct horizons, rich in brachiopods (samples Ch10–Ch11), occur in the middle part of this unit. Furthermore, based on both the conodont stratigraphy (Bispathodus aculeatus aculeatus Zone) as well as the lithology of the rocks (dark-grey shales) the interval around sample Ch12 may correspond to the interval of the Late Devonian Dasberg Crisis (compare Hartenfels 2011). Unit 4 (samples Ch15–Ch16, thickness 15 m) is composed of thick shale layers with alternating thin-bedded limestone and a very thin sandstone layer. Frequently, brachiopods and corals occur in some distinct horizons. Interestingly, the black shale represents not one single layer but is composed of three layers of several cm thickness (see Fig. 3d). This succession is covered by a massive quartzitic, coarsening-upward sandstone sequence of about 10 m thickness (Unit 5). The sediments of Unit 4 and Unit 5 are most probably equivalent to the Drewer Sandstone (regressive Hangenberg prelude episode) with intercalated transgressive black shale layers equivalent to the transgressive Hangenberg Black Shale (HBS) and finally the overlying regressive Hangenberg Sandstone (HSS). The Khoshyeilagh Formation is continuously overlain by the Lower Mississippian Mobarak Formation (thickness 215 m) which is composed of an alternation of nodular medium-bedded limestone and shale. This interval is less fossiliferous and only a limited number of macrofossils such as gastropods and brachiopods were found (Unit 6, samples Ch17–Ch18, thickness 20 m). The overlying unit exhibits green thick shale with some limestone layers (Unit 7, samples Ch19–Ch20, thickness 12 m). The succession grades upwards into thin-bedded limestone (Unit 8, samples Ch21–Ch22, thickness 10 m) which is covered by shale and thin limestone (Unit 9, sample Ch22-1–Ch23, thickness 8 m). This unit yielded only some conodonts (Fig. 4). The uppermost part of the Chelcheli section was subdivided into two units (Unit 10, samples Ch24–Ch26 and Unit 11, samples Ch26-1–Ch35) which have a thickness of 165 m. This succession is composed of an alternation of limestone (nodular and thin-bedded), shale and marl. Some distinct horizons are very fossiliferous and contain bivalves, trilobites, gastropods, fish remains, and corals.
Materials and methods
Thirty-nine conodont samples of approximately 4–5 kg each were taken from carbonate rock and processed by standard processing methods (see Jeppsson and Anehus (1995)). The overall number of conodont elements is relatively low as it was shown in other shallow-water sections for instance by Bahrami et al. (2018, 2019), Munkhjargal et al. (2021) and Königshof et al. (2021). However, a total of 338 conodonts were obtained from the residues of which a reasonable number of species is biostratigraphically important. The conodont collection is stored at the Department of Geology (sample numbers: EUIC), University of Isfahan, I.R. Iran. Repository numbers of the figured specimens are given in the explanations of plates (Figs. 5, 6, 7 and 8).
Conodont distribution
338 conodont elements from the Chelcheli section around the DCB lead to the discrimination of 15 biostratigraphical intervals (Fig. 4; Table 1) and to the identification of 47 species and subspecies within fifteen genera: Alternognathus, Bispathodus, Branmehla, Clydagnathus, Gnathodus, Icriodus, Mehlina, Palmatolepis, Polygnathus, Protognathodus, Pseudopolygnathus, Scaliognathus, Doliognathus, Siphonodella and Scaphignathus utilized to establish the biostratigraphical framework for the studied section (Table 1). Overall, the preservation of the conodont elements is good, but a number of broken elements also collected were not identified. The Color Alteration Index (CAI) of conodonts (Epstein et al. 1977) is 4–4.5. In this report we use the revised conodont zonation published by Spalletta et al. (2017) until the first occurrence of Siphonodella praesulcata, then we continue to apply the conodont zonation published in Kaiser et al. (2009) which means praesulcata Zone (= old Lower praesulcata Zone), ckI (extinction-based costatus-kockeli Interregnum), kockeli Zone (= old Upper praesulcata Zone), and sulcata/kuehni Zone (= old sulcata Zone). This was done for two reasons, first Spalletta et al. (2017) substituted the praesulcata Zone, and their ultimus Zone includes the praesulcata Zone and the ckI, and second, we have not found biostratigraphically significant Protognathodus species (such as Protognathodus kockeli or Protognathodus kuehni) in this section. The occurring Protognathodus fauna is mainly represented by Protognathodus meischneri and Protognathodus collinsoni.
The conodont zonation for the Mississippian utilized was proposed by Sandberg et al. (1978), Kaiser et al. (2009) and Becker et al. (2016). The zonation, proposed as preliminary standard conodont zonation by Lane et al. (1980), was applied for the biostratigraphic analysis of the upper Tournaisian conodont zonation. The Tournaisian conodont biozones nearly always indicated by the markers, some species of the genera Gnathodus, Pseudoplygnathus, Scaliognathus, Doliognathus and Siphonodella were utilized in recognizing the biozones.
The basal part of the section (sample Ch1) yielded only a few icriodid specimens (Icriodus alternatus alternatus, Icriodus alternatus helmsi and Icriodus cornutus). Due to the lack of index conodont fauna, the precise position of this succession cannot be determined (Table 1).
Palmatolepis minuta minuta Zone (sample Ch2)
The lower limit of this zone is recognized by the entry of Palmatolepis minuta minuta Branson and Mehl, 1934, ranging from the Palmatolepis minuta minuta Zone to the Pseudopolygnathus granulosus Zone (Spalletta et al. 2017) which corresponds to the former Upper triangularis—Upper trachytera zones (Ji and Ziegler 1993) of Ziegler and Sandberg (1990). Icriodus alternatus alternatus, Icriodus alternatus helmsi and Icriodus cornutus are the accompanying conodont species.
Palmatolepis crepida Zone (sample Ch3)
Polygnathus nodocostatus nodocostatus Branson and Mehl, 1934 was found in sample Ch3. This species ranges from the Palmatolepis crepida Zone to the Palmatolepis gracilis expansa Zone (Spalletta et al. 2017) and was found in various samples from Ch3 up to Ch11. Polygnathus communis communis, Icriodus alternatus alternatus, Icriodus alternatus helmsi and Icriodus cornutus are additional conodont species in this sample.
Palmatolepis termini Zone to Palmatolepis glabra prima Zone (sample Ch4)
The entry of Polygnathus semicostatus Branson and Mehl, 1934 in sample Ch4 lead to the attribution of this sample to the Palmatolepis termini Zone. This species first appears in the lower Palmatolepis termini Zone (Ji and Ziegler 1993; Spalletta et al. 2017). Palmatolepis minuta minuta, Icriodus alternatus alternatus and Icriodus cornutus are the other associated species. There are no condodonts diagnostic for the Palmatolepis glabra prima Zone.
Palmatolepis glabra pectinata Zone to Palmatolepis rhomboidea zones interval (sample Ch4-1)
Sample Ch4-1 yielded Palmatolepis quadrantinodosalobata Sannemann, 1955a M1 Sandberg and Ziegler, 1973 and Polygnathus padovanii Perri and Spalletta, 1990, both have their first occurrence within the Palmatolepis glabra pectinata Zone (Spalletta et al. 2017). No other conodonts were found in this interval.
Palmatolepis gracilis gracilis Zone to Palmatolepis marginifera utahensis Zone (samples Ch5–Ch6)
The index conodont species Palmatolepis gracilis gracilis Branson and Mehl, 1934 ranges from the Upper rhomboidea Zone (Klapper and Ziegler 1980; Ji and Ziegler 1993), the Palmatolepis gracilis gracilis Zone of Spalletta et al. (2017). The presence of Palmatolepis gracilis gracilis in sample Ch5 allows the attribution of the level of this sample to the Palmatolepis gracilis gracilis Zone. Polygnathus triphyllatus Helms, 1961 which range starts within the basal part of the Palmatolepis gracilis gracilis Zone is also present in sample Ch5. The upper limit of the interval was defined by the entry of Scaphignathus velifer velifer in sample Ch7. Polygnathus padovanii, Polygnathus semicostatus, Polygnathus nodocostatus nodocostatus, Polygnathus communis communis, Palmatolepis minuta minuta, and Icriodus cornutus are the associated species in this interval.
Scaphignathus velifer velifer Zone (sample Ch7)
The entry of the index species Scaphignathus velifer velifer Helms, 1959 is the marker for the lower limit of this zone, the conodont species Alternognathus regularis regularis Ziegler and Sandberg, 1984 also has its first occurrence at the base of the Scaphignathus velifer velifer Zone (Spalletta et al. 2017). Palmatolepis minuta minuta, Palmatolepis gracilis gracilis, Polygnathus padovanii, Branmehla bohlenana bohlenana, Polygnathus semicostatus, Polygnathus communis communis, Polygnathus nodocostatus nodocostatus and Icriodus cornutus are present in this sample, too.
Palmatolepis rugosa trachytera Zone (sample Ch8)
The entry of zonal index species Palmatolepis rugosa trachytera Ziegler, 1960 in sample Ch8 is the marker of the lower limit of the zone (Ji and Ziegler 1993; Spalletta et al. 2017). Scaphignathus velifer velifer, Palmatolepis minuta minuta, Palmatolepis gracilis gracilis, Polygnathus padovanii, Alternognathus regularis regularis, Branmehla bohlenana bohlenana, Polygnathus semicostatus, Polygnathus communis communis, Polygnathus nodocostatus nodocostatus, and Icriodus cornutus are the other species found in this sample.
Pseudopolygnathus granulosus Zone to Palmatolepis gracilis manca Zone (samples Ch9–Ch10)
The base of this interval can be recognized by the entry of Palmatolepis gracilis sigmoidalis Ziegler, 1962. The last occurrence of Palmatolepis minuta minuta Branson and Mehl, 1934 and Icriodus cornutus Sannemann, 1955b was utilized to identifying the Pseudopolygnathus granulosus Zone. Spalletta et al. (2017) considered Palmatolepis gracilis sigmoidalis as a useful taxon for the identification of the Pseudopolygnathus granulosus Zone. Polygnathus granulosus, Bispathodus stabilis vulgaris, Branmehla ampla, Branmehla inornata can be observed at the top of this interval. The indicative species of the Polygnathus styriacus and Palmatolepis gracilis manca zones are missing. Scaphignathus velifer velifer, Palmatolepis gracilis gracilis, Polygnathus padovanii, Branmehla bohlenana bohlenana, Polygnathus semicostatus, Polygnathus communis communis, Polygnathus nodocostatus nodocostatus, Mehlina strigosa and Alternognathus regularis regularis are also present in these samples.
Palmatolepis gracilis expansa Zone (sample Ch11)
The entry of zonal index species Palmatolepis gracilis expansa Sandberg and Ziegler, 1979 in Ch11 defines the base of this zone. Bispathodus jugosus (Branson and Mehl, 1934) is also a good marker for this zone (Ziegler and Sandberg 1984; Ji and Ziegler 1993; Spalletta et al. 2017). Bispathodus bispathodus, Bispathodus stabilis stabilis, Branmehla inornata, Bispathodus stabilis vulgaris, Polygnathus granulosus, Branmehla ampla, Palmatolepis gracilis sigmoidalis, Mehlina strigosa, and Alternognathus regularis regularis are some associated species. Alternognathus regularis regularis ends at the top of the Palmatolepis gracilis manca Zone (Spalletta et al. 2017), but at the Chelcheli section it is possible to extend the range.
Bispathodus aculeatus aculeatus Zone (sample Ch12)
This zone corresponds to the lower part of the former Middle expansa Zone and is equivalent to the lower subzone of the Bispathodus aculeatus aculeatus Zone of Hartenfels (2011). The lower limit can be defined by the first occurrence of zonal index species Bispathodus aculeatus aculeatus (Branson and Mehl, 1934). This species extends into the Visean (texanus Zone; Lane et al. 1980; Spalletta et al. 2017). Palmatolepis gracilis expansa, Bispathodus bispathodus, Bispathodus jugosus, Polygnathus granulosus, Palmatolepis gracilis sigmoidalis, Palmatolepis gracilis gracilis, Polygnathus semicostatus and Polygnathus communis communis are the associated species.
Bispathodus costatus Zone (sample Ch13)
This new proposed zone (Spalletta et al. 2017) is equivalent to the upper part of the Middle expansa Zone, and to the Lower costatus Zone of Ziegler (1962). It is the same as proposed by Corradini et al. (2016) and corresponds to the Bispathodus costatus Subzone of Hartenfels (2011). The first entry of marker species Bispathodus costatus (Branson, 1934) M1 and Bispathodus costatus (Branson, 1934) M2 defines the lower limit of this zone. In addition, Bispathodus spinulicostatus, Clydagnathus plumulus, Bispathodus aculeatus aculeatus, Bispathodus stabilis stabilis, Bispathodus jugosus, Palmatolepis gracilis sigmoidalis, Palmatolepis gracilis gracilis, Polygnathus semicostatus and Polygnathus communis communis and some other species were found in this sample.
Bispathodus ultimus Zone (Ch14–Ch16 and Ch16-1)
This relatively large new defined ultimus Zone (Spalletta et al. 2017) is equivalent to the Upper expansa, Lower and Middle praesulcata zones of Ziegler and Sandberg (1984), as well as to the Upper expansa and praesulcata zones and the costatus–kockeli Interregnum of Kaiser et al. (2009); (see comments at the beginning of “Conodont distribution”). Although the base of the costatus-kockeli Interregnum (ckI) is linked with a global and sudden extinction of a number of conodonts, such as the Bi. costatus—ultimus Group, among others, the collected samples did not yield the index conodont species Bispathodus ultimus, the association with Protognathodus meischneri Ziegler, 1969, Protognathodus collinsoni Ziegler, 1969, Palmatolepis gracilis gonioclymeniae Müller, 1956 and Siphonodella praesulcata Sandberg et al., 1978, most likely suggests the Bispathodus ultimus Zone. Lithologically, the Bispathodus ultimus Zone corresponds to rocks of the upper part of unit 3 and unit 4 of the succession, in which shale, marl and limestone gradually change to very tiny alternation of platy black shales with intercalated sandstones (Fig. 3d). This succession is overlain by thick-bedded quartzitic sandstone. This characteristic lithology represents most likely equivalents of both, the Hangenberg Black Shale (HBS) and the Hangenberg Sandstone (HSS).
?Protognathodus kockeli Zone to L. Siphonodella crenulata Zone (sample Ch17–Ch25)
Although the zonal marker species Protognathodus kockeli, Protognathodus kuehni and Siphonodella sulcata were not found in the collected samples, the association of Polygnathus inornatus, Polygnathus longiposticus, Clydagnathus cavusformis, Pseudopolygnathus primus M2, Protognathodus meischneri, Protognathodus collinsoni and the entry of Siphonodella obsoleta in the level of sample Ch24 lead to the attribution of this interval to the latest Famennian/Early Mississippian ?Pr. kockeli to L. Si. crenulata zones. Pr. meischneri and Pr. collinsoni are atypical forms, as they do not correspond in detail to the original diagnosis. The sedimentological changes from the white quartzitic sandstone (HSS) to the micritic limestone at the base of sample Ch17 is considered as the DCB, thus, more research on that specific point is necessary.
Siphonodella isosticha—U. Siphonodella crenulata Zone and Gnathodus typicus Zone (samples Ch26–Ch26-1)
The lower limit of this interval is well defined by the first entry of Gnathodus semiglaber Bischoff, 1957, Gnathodus cuneiformis Mehl and Thomas, 1947 and Gnathodus punctatus Cooper, 1939 in sample Ch26. All species have their first occurrences at the base of the isosticha to Upper crenulata Zone and range into the Lower typicus Zone (Lane et al. 1980) and/or into the anchoralis—latus Zone (Voges 1959) or even higher into the Visean.
Scaliognathus anchoralis—Doliognathus latus Zone (samples Ch27–Ch35)
This zone is characterized in the upper part of the studied section by the entry of the zonal marker species Scaliognathus anchoralis europensis Lane and Ziegler, 1983 and Doliognathus latus Branson and Mehl, 1941 Morphotype 2 in sample Ch27. Gnathodus pseudosemiglaber Thompson and Fellows, 1970 and Pseudopolygnathus cf. pinnatus Voges, 1959 also have their first occurrences at the base of this zone (Lane et al. 1980).
Conclusion
Late Palaeozoic Upper Devonian to Mississippian rocks in shallow-water facies were studied in the Chelcheli section. The major finding can be summarized as follows:
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The more or less complete section ranges from the Palmatolepis minuta minuta into the Scaliognathus anchoralis-Doliognathus latus Zone.
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Due to the overall shallow-water palaeoenvironment the conodont record is not excellent but most conodont zones from the Late Devonian to the Mississippian can be distinguished.
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Close to the DCB there is a small hiatus which might be a result of facies (shallow-water succession with no conodont record and siliciclastic rocks) rather than the period of non-deposition as the sedimentological record seems continuous.
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In contrast to other DCB sections described from Iran (Königshof et al. 2021), the Chelcheli section exhibits a characteristic lithology around the DCB known from many other places around the world.
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The black shales and the superimposed thick-bedded quartzitic sandstones represent equivalents of the Hangenberg Black Shale (HBS) and the Hangenberg Sandstone (HSS), respectively.
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The conodont association around the DCB provides important information in the frame of the recent discussion on a revision of this boundary.
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Iliana Boncheva, Claudia Spalletta, Mehdi Yazdi, and the Editor-in-Chief Mike Reich are thanked for constructive reviews of the submitted manuscript. The authors are grateful to Office of Vice Chancellor for Research and Technology at the University of Isfahan for financial and technical support. This study was undertaken at the University of Isfahan in cooperation with the Senckenberg Research Institute and Natural History Museum, Frankfurt. This is a contribution to the International Geoscience Programme IGCP 652 and IGCP 700. One of the authors (P.K.) acknowledges funding by the Deutsche Forschungsgemeinschaft (DFG; KO 1622/16-1).
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Bahrami, A., Königshof, P., Hartkopf-Fröder, C. et al. Late Devonian–Mississippian conodont biostratigraphy of the Chelcheli section, NE Shahrud (Eastern Alborz, North Iran). PalZ 96, 449–469 (2022). https://doi.org/10.1007/s12542-021-00575-6
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DOI: https://doi.org/10.1007/s12542-021-00575-6