Introduction

Initial Upper Paleolithic in the Levant

The Initial Upper Paleolithic (IUP) was originally defined by Marks and Ferring (1988) to represent the latest phase of the Levantine Middle-Upper Paleolithic transition (thus, the earliest phase of the UP) that they proposed on the basis of the cultural stratigraphic sequence at Boker Tachtit in the Negev (Fig. 1). Specifically, the lithic assemblage from the uppermost level (Level 4) of the site was designated as the IUP. Currently, the term IUP is also applied to other assemblages (Bar-Yosef & Belfer-Cohen, 2010a, 2010b; Kuhn, 2003; Meignen, 2012), including those that have been called UP Phase 1 (Neuville, 1951), Emiran (Garrod, 1951; Rose & Marks, 2014; Shea, 2013), the MP-UP transition (Marks, 1983, 1993), the Bokerian (Leder, 2014, 2018), and the Paléolithique intermédiaire (Boëda, et al., 2015). Despite the varying nomenclature, the grouping of these lithic assemblages is broadly shared among the researchers. This study employs the term IUP in the broad sense.

Fig. 1
figure 1

Map of the Levant, showing the locations of Upper Paleolithic sites mentioned in the text

The Levantine IUP lithics are broadly characterized by technomorphological elements of both the MP and the UP. Typologically, they are characterized by UP tool types, such as end scrapers and burins, and unique types, such as Emireh points and chamfered pieces. Blank forms are dominated by robust elongated pieces, i.e., blades and points that have broad, often faceted, striking platforms indicating hard-hammer percussion (e.g., Kadowaki et al., 2019b; Kuhn et al., 2009; Marks & Kaufman, 1983; Meignen, 2012; Ohnuma, 1988; Volkman, 1983).

The term IUP is currently used not only in the Levant but also in other regions, such as Central–Southeastern Europe and Central–North Asia to represent the earliest phase of the UP (Hublin, 2015; Kuhn & Zwyns, 2014; Zwyns et al., 2019). One of the key issues in this continental-scale cultural phenomenon, broadly dated to ca. 50–40 ka, is its relationship to the concurrent human biogeographic phenomena that involved the geographic expansion of anatomically modern humans (AMHs) and the decline of archaic humans (e.g., Neanderthals and Denisovans) indicated by human fossil and genomic studies (Fu et al., 2014; Hublin et al., 2020).

Regarding this issue in the Levant, there are various explanations depending on how researchers evaluate the degree of cultural continuity and the roles of incoming AMHs in the cultural changes from the MP to the UP. One hypothesis regards the MP-UP cultural changes as the introduction of new cultural/behavioral patterns associated with incoming AMHs that replaced Neanderthals (Abadi et al., 2020; Bar-Yosef, 2007; Shea, 2007, 2008). Recently, some researchers have recognized both continuous and discontinuous cultural elements from the MP to the IUP and suggested autochthonous cultural development within indigenous populations with some influence of incoming groups (Abadi et al., 2020; Meignen, 2012, 2019; Rose & Marks, 2014). The latter views are congruent with an idea of coexistence of Neanderthals and AMHs in the Levant during the MP (Boaretto et al., 2021; Hovers, 2006; Hovers & Belfer-Cohen, 2013) that lead to the formation of polymorphic populations through interaction and interbreeding (Green et al., 2010; Sánchez-Quinto et al., 2012; Fu et al., 2014; Reich, 2018; Dennell, 2020). The intensification of such social interactions, instead of a population turnover, has recently been proposed as a driver for the cultural changes from the MP to the UP (Goring-Morris & Belfer-Cohen, 2020; Greenbaum et al., 2019; Stutz, 2020).

Another issue regarding the IUP is its variability that does not easily allow us to treat the IUP simply as a short-term event marking the beginning of the UP. Instead, the IUP variability should be explained as manifestations of cultural phenomena taking place over millennia and wide geographic regions (Kuhn & Zwyns, 2014; Marks & Rose, 2012). In the case of the Levantine IUP, its geographic variability has been known for differential distributions of Emireh points and chamfered pieces (Garrod, 1951, 1955; Nishiaki, 2018). Diachronic changes in the IUP have also been recognized from stratigraphic records at several sites, such as Boker Tachtit (Marks & Kaufman, 1983; Volkman, 1983), Tor Sadaf (Fox, 2003; Fox & Coinman, 2004), Ksar Akil (Azoury, 1986; Ohnuma, 1988; Ohnuma & Bergman, 1990), and Ücağızlı (Kuhn et al., 2009). More recently, several technological phases (Bokerian A, B, C, Jelf Ajlan, and Boker Tachtit 4) have been proposed by Leder (2014, 2016). He also examined the lithic variability of the IUP in relation to geographic locations, surrounding environment, on-site activities, and occupational intensity (Leder, 2018).

In order to contextualize the IUP in the cultural dynamics at the MP-UP transition, it is necessary to clarify its relationship with the late MP and the Ahmarian (Marks & Rose, 2012). In general, most of IUP assemblages post-date the late MP and pre-date the Ahmarian. However, Boaretto et al (2021) have recently proposed that the earliest occupations at Boker Tachtit (i.e., Levels 1–3 and AH-B) and the earliest date from Wadi Aghar Layer D2, dated to ca. 50 ka (Kadowaki et al., 2019b), overlap with the reported ages of lateMP industries from regional sites (Tor Faraj and Far’ah II). From this, they suggest that late MP groups coexisted (and probably interacted) with IUP populations in the Negev ca. 50 ka (Boaretto et al., 2021).

In addition, chrono-stratigraphic records at Kebara and Manot indicate the appearance of the Ahmarian at ca. 47–46 ka cal BP (Alex et al., 2017; Rebollo et al., 2011), preceding or overlapping the dates of the IUP occurrences at other sites, including Ksar Akil (Douka et al., 2012; Bosch et al., 2015a, 2015b), Ücağızlı (Kuhn et al., 2019), Umm el-Tlel (Boëda et al., 2015), and Wadi Aghar (Kadowaki et al., 2019b). The possible contemporaneity of the Ahmarian at Kebara/Manot and the IUP at other sites in the Levant could represent regional mosaic patterns of cultural developments that occurred at local scales (Stutz, 2020).

To provide new data relevant to the above issues, this paper presents chronological and lithic technological features of the IUP occupation at Tor Fawaz, southern Jordan. The previous studies of the site showed unique characteristics of the Upper Paleolithic assemblages (Coinman & Henry, 1995; Kerry & Henry, 2003), and the renewed investigation made a preliminary study of lithic assemblage and reported marine shells with interim radiocarbon dates (Kadowaki & Henry, 2019; Kadowaki et al., 2019a). Here, we present more detailed descriptions of the lithic assemblages and present OSL and additional radiocarbon dates along with analyses of micromorphology, phytoliths, and dung spherulites to evaluate the formation and postdepositional processes through high-resolution micro-contextual studies.

Research Background of the Site

Tor Fawaz (29° 56′ 49.44′′ N, 35° 20′ 9.03′′ E, 980 m a.s.l.) is one of several rockshelter sites in the Jebel Qalkha area, southwest Jordan (Figs. 13). The area (ca. 6 km2) is located at a northwestern corner of the Wadi Hisma basin, where extensive exposure of Paleozoic and Cretaceous sandstone beds are dissected by valleys flanked with many rockshelters (Rabb’a, 1987; Hassan, 1995). The investigation of Tor Fawaz was initiated by one of the authors (D.H.) as part of a long-term prehistoric project in which systematic surveys and excavations at numerous prehistoric sites were conducted in several study areas with different elevational, topographic, and biotic settings including the Mediterranean zone on the Ma’an Plateau, the Irano-Turanian steppe in the Judayid Basin, the Saharo-Arabian desert in the lowland of Wadi Hisma, and the Wadi Araba Rift Valley (Henry & Beaver, 2014; Henry, 1994, 1995, 2003, 2017a, 2017b). The Jebel Qalkha area (ca. 1,000 m a.s.l.) corresponds to the lower piedmont zone and is physiographically transitional between the Irano-Turanian and the Saharo-Arabian zones. The current climate of the area is hyperarid, receiving less than 50 mm of annual rainfall. More detailed descriptions about the natural settings of the Jebel Qalkha are available in previous publications (Henry, 1995, 2003).

In the Jebel Qalkha area, fourteen Paleolithic sites have been investigated (Fig. 2), and a chrono-cultural scheme from the MP and UP to the Epipaleolithic periods has been suggested on the basis of technotypological studies of lithic assemblages along with radiometric dating and sedimentological correlations of cultural deposits (Henry, 1995, 1997, 2003). Since 2016, a renewed investigation has been conducted at MP and UP sites in an effort to refine the cultural-chronology and to increase human behavioral and paleoenvironmental records in the late Pleistocene (Kadowaki & Henry, 2019). Recent results include chronological and lithic technological studies of an IUP occupation at a rockshelter site of Wadi Aghar (Kadowaki et al., 2019b). Here we present another occurrence of IUP occupation at nearby Tor Fawaz.

Fig. 2
figure 2

Topographic map of the Jebel Qalkha area, showing the locations of Middle and Upper Paleolithic sites mentioned in the text. Late Middle Paleolithic (Tor Faraj), Initial Upper Paleolithic (Tor Fawaz and Wadi Aghar), and Ahmarian (Tor Hamar, Tor Aeid, and Jebel Humeima)

In the initial excavation at Tor Fawaz in 1983 and 1984, five 1 m × 1 m squares (Units 1–5 in Fig. 4) were opened. Units 1–4 were located outside the rockshelter on the slope, while Unit 5 was near the drip line. The excavation of Units 1–4 revealed shallow deposits (10–20 cm deep), and Unit 5 exposed a thicker deposit (> 70 cm) of a compact light brown silt. From Units 1–5, Upper Paleolithic chipped stones (n = 3983) were recovered. The lithic assemblage was described as “non-Ahmarian” by Coinman and Henry (1995) due to the lack of diagnostic elements of either the Ahmarian or the Levantine Aurignacian, and they characterized it as “a blade technology that produced large, thick, bulky debitage and tools” (Coinman & Henry, 1995: 194).

Fig. 3
figure 3

Overview of Tor Fawaz, looking west towards Jebel Qalkha. Note excavation areas at the top of the slope near the shallow rockshelter

Fig. 4
figure 4

Topographic map of Tor Fawaz, showing the location of excavated areas

The following investigation in 1994 excavated a larger area (3 m × 4 m) behind the drip-line (Figs. 4 and 5) where cultural deposits accumulated more, up to 1 m in thickness. The deposits were divided into five stratigraphic layers (A, B1, B2, C, and D from the top). Layer A is a surface deposit of loose, dark grey silt including many twigs, dung, ash, and charcoal of probably recent time periods. Layer B consists of silty deposits that grade in color from grey (B1) to tan (B2). The deposits of Layer B become progressively compacted with depth, underlain by Layer C that consists of very compact yellow silt. Yellow silt of Layer C is partly underlain by red sand (Layer D) resting on bedrock. This sedimentary succession matches that seen at the nearby UP site of Jebel Humeima and follows the areal stratigraphy recognized in other Jebel Qalkha sites in which the Q3 yellow silt is associated with UP horizons, whereas the Q4 red sand holds MP horizon (Henry, 1997; Kadowaki et al., 2019b).

Fig. 5
figure 5

East stratigraphic section of the 1994 trench at Tor Fawaz, also showing the vertical distribution of lithics and the location of sediment samples. A bar graph shows the number of lithics by 10-cm-thick arbitrary levels reported by Kerry and Henry (2003). Numbers in circles are the OSL sample # associated with dates. Circles associated with Bulk 16–20 are spots of sediment samples for phytolith and fecal spherulite analyses. A rectangle labeled as MM 6 shows the location of a micromorphology sample

Kerry and Henry (2003: 74) interpreted that Layers A and B represent different degrees of disturbance and reworking of Layer C because Upper Paleolithic artifacts (n = 1314) were recovered throughout Layers A–C. The study of the lithic assemblage from the 1994 trench in combination with the 1983/84 collection suggested unique techno-typological characteristics that do not fit a conventional scheme of UP traditions, i.e., the Levantine Aurignacian or the Early Ahmarian (Kerry & Henry, 2003). A possible correlation of the Tor Fawaz assemblage to the IUP was mentioned by Belfer-Cohen and Goring-Morris (2003) and Goring-Morris and Belfer-Cohen (2018, 2020).

In 2016 and 2017, we conducted renewed fieldwork at Tor Fawaz to take samples for dating and to increase sample size of archaeological materials. Preliminary reports were published in Kadowaki and Henry (2019) and Kadowaki et al. (2019a), and here we show more detailed descriptions of the lithic assemblages and present new evidence from OSL/radiocarbon dates and micromorphological, phytolith and dung spherulites analyses, in order to make more thorough evaluations of the chrono-cultural characteristics of Tor Fawaz.

Materials and methods

Excavation and Micromorphology Sampling

In the 2017 season, we set up five 1 m × 1 m squares (Units 6–10) to the north of Units 1–5 that were excavated in the 1983/84 season (Figs. 3 and 4). The area for Units 6–10 was selected because of the high density of lithic distributions on the surface. In addition, the area is located behind the drip line of the rockshelter and near the highest part of the slope. We expected that this location may have preserved primary deposits of archaeological remains near prehistoric activity areas. Units 6 and 10 were excavated to the depth of 30–45 cm below the surface (Fig. 6), while only surface finds were collected in Units 7–9.

Fig. 6
figure 6

Stratigraphic section of Units 6 and 10 at Tor Fawaz, showing the vertical distribution of lithics and the location of sediment samples and marine shells. Bar graph shows the number of lithics by 5-cm-thick arbitrary levels. Numbers in circles are the OSL sample # associated with dates. A rectangle labeled as MM 12 shows the location of a micromorphology sample. The find spots of marine shells (JQ17-C17, C18, C19, C20, and C23) are indicated by their radiocarbon dates calibrated against the Marine20 curve in the OxCal v4.4.2 (Bronk Ramsey, 2009; Heaton et al., 2020)

The excavation was conducted by 5 cm arbitrary levels, and levels were grouped as layers according to changes in sedimentological characteristics, such as color, compactness, and grain size. Archaeological remains were collected by 5 cm level and by 50 × 50 cm quadrat (e.g., 6a, 6b, 6c, 6d) forming a quarter of one square. All of the excavated sediments were dry-sieved with a mesh of 2 mm. Finds from the excavation were predominantly chipped stone artifacts alongside several gastropod shells (Kadowaki et al., 2019a). The preservation of organic remains, such as bones and charcoal, was very poor, and these materials were difficult to find even under a microscope.

For micromorphological analyses, a large column of sediment (MM6) was collected from Layer C in the east section of the 1994 trench (Figs. 5, Online Resource Fig. 1). Another sediment block (MM12) was collected from the east section of Unit 6d covering Layers B and C (Figs. 6, Online Resource Fig. 2). The intact sediment blocks were each processed into six thin section slides by Nichika Geo-Science Material Inc. in Kyoto Japan. Following standard thin section preparation techniques, each block was thoroughly air and oven dried, then impregnated with a clear epoxy polyester resin in a vacuum environment to remove air bubbles and, once consolidated, prepared into thin section slides, each 30 µm in thickness and 3 × 5 cm in size.

OSL Dating

After the excavations of Units 6 and 10, sediment samples for OSL dating were taken by hammering light-tight plastic or metal tubes 15 cm long into the trench walls (Table 1). Five sediment samples for OSL dating were collected from the stratigraphic sections in Units 6 and 10 (Fig. 6). In addition, five more OSL samples were taken from the section in the 1994 trench (Fig. 5) that was reported by Kerry and Henry (2003). In total, four samples (OSL46, OSL47, OSL58, and OSL60) were taken from Layer B, while five samples (OSL32, OSL34, OSL45, OSL48, and OSL61) were collected from Layer C. Another sample (OSL59) was taken from the interface between Layer B and Layer C.

Table 1 Details of samples for OSL dating: sample level, water, U, Th, K, and Rb contents, and cosmic and total dose rates

Sample preparation and luminescence measurement were done at the luminescence laboratory of the Geological Survey of Japan. Samples were prepared under subdued red light to avoid affecting the luminescence signals. Sediment within 20–25 mm of the ends of the tube was removed and used for measurements of water content and dosimetry. The remaining samples were processed for luminescence measurements. They were dried, sieved to extract grains of 62–90 µm diameter, and then treated with hydrochloric acid and hydrogen peroxide to remove carbonate and organic matter. Quartz and K-feldspar grains were then separated using sodium polytungstate liquids of densities 2.70, 2.58, and 2.53 g/cm3. The 2.53–58 g/cm3 fraction was taken as K-feldspar. Quartz grains were purified by etching the fraction of 2.58–70 g/cm3 in 40% hydrofluoric acid for 1 h, followed by hydrochloric acid treatment for 1 h. Grains were mounted on stainless steel disks to form small (2 mm in diameter) aliquots for luminescence measurements with a TL-DA-20 automated Risø TL/OSL reader equipped with blue and infrared (IR) LEDs centered on wavelengths of 470 and 970 nm, respectively, for stimulation, and a 90Sr/90Y beta source for laboratory irradiation. For stimulation by blue and infrared LEDs, emitted luminescence through a Hoya U-340 filter, and a combination of Schott BG3 (3 mm thick), BG39 (2 mm), and GG400 (3 mm) filters, respectively, was measured with a photomultiplier tube.

Preliminary measurements indicated that natural quartz OSL signals showed anomalous dependency on preheat temperature, characteristics unfavorable for dating. Therefore, only post-IR IR-stimulated luminescence (post-IR IRSL, referred to here as pIRIR) signals of K-feldspar grains were further investigated. Further details of the quartz OSL measurements are provided in Online Resource Text 1 and Online Resource Fig. 4.

The modified single-aliquot regenerative (SAR) dose protocols of pIRIR measured at 150 °C (Online Resource Table 1; Buylaert et al., 2009, 2012; Thomsen et al., 2008) after a prior IRSL at 50 °C (signal referred to as pIRIR50/150) was applied to the K-feldspar grains. This measurement temperature was selected after tests of preheat plateau and dose recovery carried out for sediments at the Wadi Aghar site, 1.2 km distant from the Tor Fawaz site. Bright pIRIR signals were observed for all samples (Online Resource Fig. 5). The luminescence signal was sampled every 0.1 s for 100 s, and the intensity was derived from the integral of the first 2.0 s of signal after subtracting the average intensity during the last 20 s of signal. Preheat temperatures were set at 180 °C in all cases. Dose recovery was examined with bleaching experiments for sample gsj18208 (OSL-47) as follows. Six aliquots for each case were exposed to artificial sunlight for 4 h in a UVACUBE 400 chamber (Hönle) with a SOL 500 lamp module. After bleaching, three aliquots were dosed and then used for a dose recovery test; the remaining aliquots were used to estimate the residual dose. Dose recovery was assessed after subtracting the residual dose from the recovered dose, yielding an acceptable recovery ratio 0.95 ± 0.03.

De were determined for eight replicates per sample with five regeneration points including 0 Gy and a replicate of the first regeneration point, which was used to check whether the sensitivity correction procedure was performing adequately. No aliquot showed a recycling ratio outside 1.0 ± 0.1. For age determinations, mean De values were determined per sample by applying the Central Age Model of Galbraith et al. (1999) (Table 2). Fading tests were also carried out on aliquots measured for De to determine fading rates (expressed as g2days-value) by following the method of Auclair et al. (2003). The environmental dose rate was determined using the DRAC of Durcan et al. (2015) based on the contributions of both natural radioisotopes and cosmic radiation (Table 1). Concentrations of U, Th, and Rb were measured by inductively coupled plasma mass spectrometry (ICP-MS), and concentration of K was by ICP atomic emission spectrometry (ICP-AES). These concentrations were then converted to dose rate according to the conversion factors of Adamiec and Aitken (1998). The attenuation factors used for beta and alpha rays were based on Mejdahl (1979) and Bell (1980), respectively. We used an a-value of 0.15 ± 0.05 (Balescu & Lamothe, 1994). The internal K content of K-feldspar was assumed to be 12.5 ± 0.5% (Huntley & Baril, 1997). For water content, an error of 5% was applied to the measured value. As the excavation is located close to the rockshelter, cosmic dose rate is assumed to be 50% of the rate at an open-air site which is estimated based on Prescott and Hutton (1994) with the overburden of 1.8 g/cm3. The mean De values were divided by the environmental dose rate to obtain uncorrected ages. Fading corrections were performed for uncorrected ages based on Huntley and Lamothe (2001) and using the R Luminescence Package (Fuchs et al., 2015; Kreutzer et al., 2012). All dates are expressed relative to the present (Table 2).

Table 2 Equivalent dose (De), uncorrected age, g-value, and corrected age of OSL samples

Radiocarbon Dating of Sea Shells

Radiocarbon dating was conducted on five marine shells collected from Units 6, 9, and 10 (Fig. 6). They include three fragments of Pecten sp. (JQ17-C17, JQ17-C19, and JQ17-C20), one fragment of Conus sp. or Conomurex sp. (JQ17-C18), and one fragment of Naria sp. (JQ17-C23). Four of them (JQ17-C17, C18, C19, and C20) were found in the upper part of Layer B (Layer B1) in Unit 10 corresponding to the highest density of lithic distribution. The Naria sp. shell (JQ17-C23) was found on the surface in Unit 9 in association with abundant lithic artifacts (n = 554). Previously, we reported the taxonomic identification and preliminary radiocarbon dates of these shells (Kadowaki et al., 2019a). Here, we report the results of their re-dating.

The re-dating of three additional samples (JQ17-C18, JQ17-C20, and JQ17-C23) was conducted in Laboratory of Radiocarbon Dating at The University of Tokyo. Marine carbonates have contamination risks derived from recrystallisation or replacements in nature burial environments. Main polymorphs of original marine shells are magnesium enriched calcite or aragonite, but the secondary carbonate forms low magnesium calcite. Since the calcite reforming occurs with exogenous contamination and/or internally within shell carbonates, the degree of contamination cannot be evaluated quantitatively by only examining the calcite contents in the sample. However, observations of aragonite or calcite are helpful to choose appropriate pretreatment methods and to imply the quality of carbonate 14C data. The calcite and aragonite in the samples were detected by X-ray diffraction, and the polymorphs composition was evaluated by the direct derivation method (Rigaku MiniFrex 600). After the sample surface was cleaned by acid etching with HCl, if the sample mainly consisted of aragonite, the carbonate density separation method (CarDS; Douka et al., 2010) was performed to concentrate the sample originated carbonate, removing calcite residue. Finally, the pure CO2 extracted from the prepared sample was reduced to graphite for AMS 14C dating. The 14C measurements were performed by 0.5 MV 1.5 SDH-1 AMS system (NEC). The conversion of 14C age into a calibration date was calculated by the OxCal 4.4 program (Bronk Ramsey, 2009) with the Marine 20 (Heaton et al., 2020) calibration curve.

Phytolith and Dung Spherulites Analyses

Five sediment samples (Bulk 16–20) were taken from Layers A, B, C, and D exposed on the eastern section of the 1994 trench (Fig. 5). Phytoliths were extracted following the method of Katz et al. (2010). A weighed aliquot of ~ 40 mg of air-dried sediment was treated with 50 μl of a volume solution of 6 N HCl. Phytoliths were concentrated using 450 μl 2.4 g/ml sodium polytungstate solution [Na6(H2W12O40)]. Microscope slides were mounted with 50 μl of material. Phytoliths were examined at 200 × and 400 × magnification using a Leica DMEP optical microscope at the Department of Archaeology, University of Reading. Morphological identification was based on modern plant reference collections and standard literature (Albert et al., 2016; Brown, 1984; Mulholland & Rapp, 1992; Piperno, 1988, 2006; Rosen, 1992; Twiss, 1992; Twiss et al., 1969). The terms used to describe phytolith morphologies follow the standards of the International Code for Phytolith Nomenclature 2.0. (Neumann et al., 2019).

The methods used for the calcitic dung spherulite analysis are similar to those proposed by Canti (1999). About 1 mg of dried sediment was mounted on a microscope slide with Entellan New from Merck. Spherulites found in a known number of randomly chosen fields were counted at 400 × magnification under the optical microscope with crossed polarized light (XPL). Both dung spherulite and phytolith assemblages were compared to modern reference ethnoarchaeological datasets of modern dung remains that have followed a similar quantitative approach (Tsartsidou et al., 2008; Portillo et al., 2012, 2014, 2017, 2021; Portillo and Matthews, 2020).

Technotypological Analyses of Lithics

We analyzed the lithic artifacts from Tor Fawaz according to their technomorphological classification, primarily following the scheme used in previous studies (Coinman & Henry, 1995; Kerry & Henry, 2003) so that the new samples can be compared. The general categories include tools, debitage, and debris. The tools principally consist of retouched tools; however, the categories of Levallois-like points and Umm el-Tlel points include both retouched and unretouched pieces.

We use the term “Levallois-like points” instead of “Levallois points” because they are likely sub-products of robust blade production from single platform cores as we discuss later (see the “Discussion” section). In other words, they are similar to points from Boker Tachtit Level 4 that were described as “pointed blades that morphologically parallel the elongated Levallois points” (Volkman, 1983).

Umm el-Tlel points are characterized by a series of small elongated scars, like bladelet scars, near the butt (Boëda et al., 2015). Multiple (up to five) elongated scars from the butt end of the points have also been reported from Boker Tachtit Levels 1–3 (Volkman, 1983).

This study has another point category “pointed flake,” which is an unretouched blank form. It does not show characteristic dorsal scar patterns and has plain striking platforms. Thus, pointed flakes do not indicate standardized production methods, unlike Levallois-like points or Umm el-Tlel points.

All of other point types, such as el-Wad points and Ksar Akil points, are always retouched. According to the definition by Bergman (1981), both el-Wad points and Ksar Akil points are blades or bladelets pointed by abrupt or semi-abrupt retouch near the distal end, and the distinction between them is sometimes difficult, as discussed by Ohnuma (1988: 314–315). In this study, we differentiated between el-Wad points and Ksar Akil points on the basis of technomorphological features of blanks. More precisely, el-Wad points are made on bladelets with small butts (i.e., punctiform or linear platforms), while Ksar Akil points are made on blades with larger platforms.

The debris category consists of chips and chunks. Chips are flakes whose maximum length is smaller than 25 mm, and chunks are fragmented pieces that do not clearly show ventral or dorsal surfaces. The debitage category consists of various unretouched pieces, such as flakes, blades, primary elements, core trimming elements (CTE), and cores. A blade is defined as a flake whose length is equal to or greater than twice its width. Usually, a blade also has parallel lateral sides and ridges. We employ a definition of bladelet by Tixier (1963) to be consistent with the previous study (Kerry & Henry, 2003). A bladelet is a blade with a length < 50 mm and a width < 12 mm. Primary elements are flakes or blades that have cortex covering more than 50% of their dorsal surfaces.

The identification of Levallois products is based on the Levallois flaking concept defined by Boëda (1994) and Eren and Lycett (2012). Although we identified a few Levallois-like points/blades/flakes by observing their lateral and distal convexities as well as the platforms that show large, often facetted platforms, the Levallois flaking is primarily defined by the volumetric concept and hierarchical exploitation of cores. As we describe in the “Result” section, we did not identify genuine Levallois cores or CTEs indicative of Levallois flaking, such as éclat debordant. Thus, we use the term “Levallois-like point/blade/flake.”

CTEs are flakes or blades with distinctive morphologies, such as core tablets and crested pieces, which result from their detachment from specific parts of cores for the maintenance of core-surface morphology. Crested blades and core tablets follow the definitions by Inizan et al. (1999). In Tor Fawaz, we also found “half-crested blades” that have a ridge created by perpendicular flaking in only one direction (in contrast to two opposed directions in typical crested blades). We also include plunging flakes (or overshot flakes; Inizan et al., 1999) as CTEs although they may have been accidental results rather than intentional core-maintenance.

We conducted analyses by focusing on cores, CTEs, blank morphology, the production technology of blades/bladelets, and tool types. Cores and CTEs were analyzed by subdividing them according to their detailed technomorphological traits. Such traits for cores include the locations and the extent of the working surface that are related to the volumetric concepts in core exploitation.

We examined the morphological variations of blanks by focusing on the relative frequencies of several debitage categories including, flakes, blades, bladelets, Levallois-like flakes, Levallois-like blades, and convergent blanks that include Levallois-like points, Umm el-Tlel points, and pointed flakes.

The production technology of blades/bladelets was analyzed by observing their several attributes, including (1) dorsal-distal shapes, (2) dorsal scar patterns, (3) platform types, (4) relative platform size, and (5) overhang removals. These attributes, except for the dorsal-distal shapes, have been reported in Kadowaki et al. (2021) in comparison with those of other sites in the Jebel Qalkha area, but here we re-examined the data by separating the assemblages according to the stratigraphy (Surface, Layer B1, Layer B2, and Layer C1) that pertains to the chronological discussion.

Dorsal-distal shapes are classified into four types, including convergent blanks, pointed blades, in-betweeners, and blunt blades, primarily following the scheme by Leder (2014). This attribute is a combination of dorsal shape and distal shape defined by Marks (1976). The first three types (i.e., convergent blanks, pointed blades, and in-betweeners) commonly show a tapering form. Among them, the convergent type has the greatest width at the proximal end and has converging lateral sides, thus resembling elongated Levallois points. In contrast, the pointed-blade type has parallel lateral sides with a pointed distal end. The in-betweener type has an intermediate morphology between the former two types. The blunt category includes blades with a blunt distal end. The dorsal scar patterns of blades/bladelets were classified into unidirectional, bidirectional, crossed, and centripetal.

Regarding the platform types, we followed a standard scheme by Inizan et al. (1999), but also included a category of ‘partially faceted type’ (Kadowaki, 2017) that has been defined by Ohnuma (1988) and Ohnuma and Bergman (2013). The partially faceted butt shows multiple facets, but it is distinguished from the multi-faceted type by the location (sometimes concentration) of small facets at spots, where dorsal ridges meet the butt.

The relative platform size is defined as a ratio of the platform area (platform width x platform depth) to the cross-sectional area of the blank (width × thickness of the blank). The smaller the value is, the smaller the platform size is in comparison to the width and thickness of the blank. This measurement is similar to the ratio of platform width to width analyzed by Wiseman (1993).

Lastly, we examined the traces of overhang removals at the platform of blades/bladelets. When the removal traces are present, they were divided into coarse flaking and fine flaking (or abrasion/grinding). The latter technique is known to have increased since the Ahmarian (Kuhn et al., 2009; Ohnuma, 1988).

For the above analyses of blades/bladelets, we used only complete pieces for the surface and Layer B assemblages while we also used broken pieces retaining the relevant attributes for the Layer C assemblage to increase the sample size.

To evaluate the patterns of the above quantitative data, we used Kruskal–Wallis test and Pearson’s chi-square test according to the measurement scales.

Results

Stratigraphy and the Distributions of Lithic Artifacts

In the 2017 fieldwork, the deposits in Units 6 and 10 were excavated to the depth of 30–45 cm below the surface (Fig. 6). The upper deposits of ca. 30 cm thickness consisted of tan silt that resembled Layer B in the 1994 trench. The sediments became increasingly compact and lighter in color in the lower levels which were similar to yellowish silt of Layer C in the 1994 block. The deposits included sandstone rubble of various sizes (up to ca. 30 cm in the maximum length) throughout the excavated levels.

The archaeological finds from the deposits consisted mainly of lithic artifacts. We also collected lithic artifacts on the surface in Units 7–9. As shown in Fig. 6, lithic artifacts were most densely distributed in the upper part of Layer B (Layer B1). Although the density of lithic distribution generally decreased towards Layer C, it slightly increased in the lower part of Layer B (Layer B2). This distributional pattern partly differs from that in the 1994 trench (Fig. 5: Kerry & Henry, 2003), where the greatest density appeared in Layer A. On the other hand, the lower part of layer B (Layer B2) commonly showed a slight increase in the density of lithic distribution.

In the re-examination of the stratigraphic section of the 1994 trench, we separated Layer C into the upper and lower parts (Layer C1 and Layer C2) because of greater compactness in Layer C2 (Fig. 5). The border between Layer C1 and Layer C2 also corresponds to a few flat-lying cobbles exposed on the section. According to this subdivision of Layer C in the 1994 trench, we correlated Layer C in Units 6 and 10 to Layer C1 because its proximity to Layer B2. This layer designation is consistent with OSL dates, as we describe later.

According to the above stratigraphy and lithic distributions, we defined lithic assemblages by the surface, Layer A, Layer B1, Layer B2, Layer C1, and Layer C2. Regarding the horizontal distributions of lithic artifacts, Table 3 shows the density of lithics (number/m3) from the excavated units of the previous (Units 1–5 and the 1994 trench) and renewed investigations (Units 6 and 10). The density of lithics is distinctively high in Unit 10, followed by Units 3, 2, 4, 6, 1, and 5 in the descending order. The lithic density is the lowest in the 1994 trench. Units 1–4 are located on the slope beneath the rockshelter and exposed only shallow deposits (10–20 cm) which are considered to represent displaced re-deposition (Kerry & Henry, 2003). Units 6 and 10 are located within the rockshelter near the top of the slope. Given these locational contexts, the area around Units 6 and 10 is considered to represent the densest part of the lithic distributions at Tor Fawaz.

Table 3 Density of lithic artifacts by excavation areas in Tor Fawaz
Table 4 List of marine shells from Tor Fawaz and their radiocarbon dates

OSL Dates

Natural signals are well beneath the saturation level and De was successfully obtained from the dose–response curve (Online Resource Fig. 5), ranging from 45 to 92 Gy (Table 2). Uncorrected pIRIR50/150 ages range from 12 ± 1 to 39 ± 3 ka. g2days-values of individual samples are low and consistent (0.9–2.2%/decade), yielding slightly higher corrected ages between 14 ± 1 and 45 ± 3 ka. As shown in Table 2, corrected ages are consistent with the stratigraphic order from Layer B1 to Layer C2 with a single exception (OSL-58) in Layer B1. pIRIR signals are generally harder to bleach than quartz OSL and in some cases associated with a residual dose which leads to age overestimation. Our bleaching test for sample gsj18208 (OSL-47) indicated a residual of ~ 0.9 Gy after 4-h exposure to artificial sunlight. Samples dated here are considered of aeolian origin and likely well-bleached before burial. Thus the potential residual dose for the samples should be equivalent to, or lower than, 0.9 Gy; this leads to possible age overestimation of < 300 years for the average dose rate of the site (c. 2.9 Gy/ka). Compared to the errors of individual age estimates, this possible age overestimation is negligible.

Radiocarbon Dating of Sea Shells

According to the carbonate component of modern references, the shells of Conus sp. or Conomurex sp. (JQ17-C18) and Naria sp. (JQ17-C23) consist mainly of aragonite, and the shells of Pecten sp. (JQ17-C20) are mainly calcite. The polymorphs component estimated by XRD generally agreed with the original components, indicating that the samples including JQ17-C20 had a low probability of heavy diagenetic changes, such as the exchanges of carbonate polymorphs over 10%. CarDS was applied only to JQ17-C18 in which the calcite content was slightly recognized.

Table 4 shows the 14C ages and calibrated dates, including the previous (Beta) and new results (TKA). The additional dates approximately supported the previous ones, but the age discrepancy appeared in each duplicate measurement. For example, the JQ17-C18 and JQ17-C23, which are mostly aragonite (99%), were younger than the previous ages by more than 4800 years, and the JQ17-C20 sample, mostly calcite, was younger by 2500 years. Based on the results of the XRD analysis, the existence of exogenous contamination to explain the large offsets is not commensurate with the mass balance, at least in the additional analyses. Even if there is a laboratory offset, it is inconsistent with the fact that the relatively old JQ17-C20 sample, which can be easily affected by a laboratory offset, had a smaller age difference than the other two samples. In this way, it was difficult to specify the reasons for the age differences although they may have resulted from contamination influences or laboratory offset. Therefore, we accepted the previous and new data as the upper and lower limits, respectively.

Micromorphology

Sediment block MM6 comes from the east section of the 1994 excavation trench, located at the eastern side near the mouth of the rockshelter (Fig. 5). The six slides cut from this block represent samples from the upper portion of Layer C, i.e., Layer C1 (slides 1–3) and lower portion of Layer C, i.e., Layer C2 (slides 4–6), and the transition between them (Online Resource Fig. 1). All of these sediments are primarily aeolian in origin, although there is also clear input from in situ disintegration of the local sandstone bedrock (as evidenced by ~ 20% sand-sized fragments of sandstone) and colluvial input. Abundant secondary carbonate impregnation and nodule formation indicate significant infiltration from water (likely a combination of seasonal rainwater and location of the trench at the dripline of the rockshelter). Mineralogically, the sediments are primarily composed of well-rounded and well-sorted medium to fine sand-sized quartz grains (30–40%) derived from the local sandstone (Fig. 7). Sandstone fragments show iron-rich cementation of quartz sand and silt; the weathering of this sandstone and breakdown and ongoing weathering of the iron-enriched cement contributes to the reddish color of the groundmass. The quartz grains are generally embedded in the compact and dense groundmass to form a close porphyric c/f related distribution (Stoops, 2003) and intergrain microaggregate microstructure (Fig. 7).

Fig. 7
figure 7

Digital photomicrographs of MM6: ab a microflake of chert with carbonate coating within a carbonate impregnated sandy (quartz) clay groundmass from MM6-6 at 3 × magnification, XPL and PPL, respectively. cd Well-developed typic carbonate nodule within a carbonate impregnated sandy (quartz) clay groundmass from MM6-5 at 3 × magnification, XPL and PPL, respectively. ef A fragment of sandstone (left) within a heavily carbonate concreted fine sandy clay groundmass from MM6-5 at 3 × magnification, XPL and PPL, respectively. gh A small fragment of burnt bone (center) and unburnt bone (lower center, yellow in PPL) within a sandy clay groundmass from MM6-3 at 3 × magnification, XPL and PPL, respectively. Note in the PPL image (h) that the well-developed matrix pedofeatures, creating small carbonate aggregates and bridges between quartz grains

Secondary pedogenic features are restricted in type to intrusive pedofeatures (Fig. 7ch): (1) clay coatings around rock fragments (generally as pendants), quartz grains, and voids and (2) carbonate impregnation of the groundmass creating well-developed nodules and bridges between grains and clay aggregates and lining large planar voids and (3) calcite crystal growths and intergrowths in the groundmass. Typic and concentric nodules range from incipient to well-developed. In some cases, secondary calcite growth within the very fine silt and clay groundmass cemented the fine fraction to produce a consolidated, speckled birefringence. These types of pedofeatures are abundant and indicate persistent infiltration and movement of water through the sediment; occasional or seasonal inundation of the sediment with groundwater led to the formation of more invasive pedofeatures like nodule formation and crystal intergrowths.

Anthropogenic input is limited to small (fine sand to silt-sized) fragments and slivers of bone (5%) and shell (< 3%), and one flint flake from MM6-6 (Fig. 7ab), and these components are more common in the Layer C1 slides than the Layer C2 slides. The bone is both burnt and unburnt (Fig. 7gh). Charcoal and ash were not identified in any of the MM6 slides. The bone fragments are embedded within the groundmass and, alongside the horizontal orientation of larger fragments (sandstone and flint), indicate that the depositional structure of the sediments in Layer C2 are largely intact with minimal reworking; the more random orientation and distribution of materials in Layer C1, and the presence of burnt bone with no evidence of charcoal or ash, suggests more extensive reworking. The boundary between Layer C1 and Layer C2 is unclear and gradual in thin section and based primarily on slightly higher quantities of microartifacts in Layer C1 and a greater degree of carbonate impregnation and carbonate formation in Layer C2. There are no obvious breaks in deposition and no visible erosional unconformities.

Sediment block MM12 comes from the east section of Unit 6, located in the western portion of the rockshelter entrance, also near the dripline (Fig. 6). In general, the MM12 slides are more disaggregated and less dense than the samples from MM6 (Online Resource Fig. 2), where a spongy structure and macroscopic and microscopic laminations are visible in Layer B2 (lower part of Layer B). Slides MM12-1 to MM12-3 (top) are from Layer B2, while MM12-3 (lower) to MM12-6 are from Layer C1. Like MM6, these slides are all dominated by quartz sand and silt (30–40%) and fragments of sandstone (5%) embedded within a reddish-brown silty clay groundmass (Fig. 8). The distinction between Layers B2 and C1 are visible in the degree of carbonate impregnation, abundance of anthropogenic input, and overall microstructure; however, these differences are generally in magnitude or degree of expression of features, rather than in content. As with MM6, these slides represent largely aeolian processes with secondary carbonate formation related to water infiltration and subsurface movement.

Fig. 8
figure 8

Digital photomicrographs of MM12: ab carbonate coatings around void spaces adjacent to a sandstone fragment (bottom) within a sandy (quartz) clay groundmass from MM12-4 at 3 × magnification, XPL and PPL, respectively. cd Well-developed carbonate crystal intergrowth (left) within a carbonate impregnated sandy (quartz) clay groundmass from MM12-5 at 3 × magnification, XPL and PPL, respectively. ef A partially burnt bone fragment (left center) within a heavily carbonate concreted fine sandy clay groundmass from MM12-2 at 4.5 × magnification, XPL and PPL, respectively. Note the well-developed carbonate aggregates and bridges between quartz grains. gh A small fragment of burnt bone (center) within a sandy clay groundmass from MM12-2 at 4.5 × magnification, XPL and PPL, respectively

The Layer B2 slides are composed of well-sorted and well-rounded (and extensively weathered) coarse silt and sands-sized grains of quartz and fragments of sandstone that exhibit a double-spaced porphyric coarse/fine related distribution and vughy to granular microstructure (Fig. 8). While there are no clear orientation and distribution patterns in the coarse components, including the anthropogenic materials, the abundance of calcium carbonate within the groundmass gives the fabric a speckled to crystallic birefringence. Anthropogenic input includes small shell fragments (sand-sized, 5%), highly fragmented charcoal (5%), fine slivers and fragments of bone (5%; Fig. 8eh), and very fine ash. However, there is no evidence of in situ combustion features. There is also 5% amorphous organic tissue throughout these slides that may relate to the other clearly anthropogenic material. Like MM6, the highly fragmented and randomly distributed and oriented nature of the anthropogenic material embedded in the groundmass suggests it has been partially reworked or redeposited.

There are also differences in slides MM12-1, MM12-2, and MM12-3 (from Layer B2) as the sediments grade gradually into Layer C1. MM12-1 contains more anthropogenic material (especially shell, amorphous organic tissue, charcoal, and ash rhombs), extensive clay coatings around quartz grains (not around voids). MM12-2 exhibits a higher quartz silt content (and more extensive weathering of quartz grains) and more, larger sandstone fragments, a denser groundmass, and better-developed secondary carbonate features (layered nucleic nodule formation and coatings around voids). MM12-3 exhibits many large sandstone fragments, many with pendants of carbonate or clay coatings, and extensive carbonate impregnative pedofeatures. These differences correspond to macroscopic layering of the sediment in Layer B2 that may result from successive slopewash or colluvial events, each causing the reworking and fragmentation of microartifacts.

The Layer C1 slides are very similar to those from MM6; calcitic secondary pedofeatures (nodules, crystal growths, impregative features) are common and increase with depth from MM12-4 to MM12-6 (Fig. 8ad). These slides, however, have no charcoal or ash, no flint microflakes, and only the rare occurrence (3%) of very small fragments of bone. Taken together with the MM6 slides, Layer C1 represents continuous, ongoing aeolian activity—both erosion and deposition—such that the accumulation of sand is persistent but slow. The highly variable degree of weathering of quartz sand and silt derives from the combination of erosion of local sandstone and input from windblown sediment. Water movement through the rockshelter, especially at its entrance, and likely episodic during the rainy seasons (and perhaps also sometimes inundating), has kept vegetation growth at a minimum (voids related to plant root casts are rare), but secondary calcite features are very common. The rate of deposition increased during the accumulation of Layer B2, formed by a combination or alternation of aeolian processes and colluviation, and the comparative decrease in the expression of secondary carbonate features suggests less water input. There is little difference in the content of anthropogenic material between Layers B2 and C1, with the exception of ash and charcoal being more prominent in Layer B2. Given the proximity (0–30 cm) of Layer B to the ground surface, recent use of the rockshelter may have also contributed to less compact, more disaggregated and spongy Layer B. The range of OSL dates are consistent with long-term, continuous but slow accumulation of these deposits over time, producing a wide range of dates for the sediments in Layers C and B and consistent with the repeated deposition and reworking of the deposits over an extended period of time.

Phytolith and Dung Spherulite

Phytoliths were noted in all samples (15,000–270,000 phytoliths/g sediment, Table 5), whereas dung spherulites were only noted in the upper layers (Layer A and Layer B1). The richest sample by far corresponds to the topsoil (Layer A) including animal dung (sample 16; 0.8 million spherulites/g sediment; Table 5), which showed also high phytolith concentrations, mainly produced by dicotyledonous leaves (Fig. 9a; Table 6). This is noteworthy given that dicotyledonous plants are minor producers of phytoliths. These microfossil associations are suggested to derive from herbivorous fecal matter showing a diet that is either based on or includes a component of dicotyledonous leaves (García-Suárez et al., 2021a, 2021b; Macphail et al., 1997; Portillo et al., 2019, 2020; Rasmussen, 1993). Both microfossil abundances decrease dramatically in Layer B1 (sample 17; below 30,000/g sediment; Table 5), where associations suggest a similar composition also dominated by dicotyledonous phytoliths (Table 6), that may relate to animal dung, likely infiltration from Layer A, as noted by the excavators in the field.

Table 5 Description of samples and main phytolith and dung spherulite results from Tor Fawaz
Fig. 9
figure 9

Photomicrographs of microfossils identified in Tor Fawaz (sample 16). a tracheary phytolith from dicotyledonous leaves; b dung spherulite under crossed polarized light (XPL)

Table 6 Main phytolith morphotypes obtained from the samples with indication of plants or parts to which they are attributed based on modern reference studies (Albert & Weiner, 2001; Albert et al., 2008, 2016; Tsartsidou et al., 2008; Portillo et al., 2014)

Lastly, sediments from Layer C1 (sample 18) and Layer C2 (19) yielded 16 phytoliths in total, whereas only 4 phytoliths were noted in sample 20 from Layer D and whereas dung spherulites were completely absent in these layers (Table 5). These assemblages are dominated by wood/ bark, as well as the leaves and culms of monocotyledonous plants, which are not diagnostic of any particular grass subfamily (Table 6). These plant materials possibly relate to anthropogenic remains; however, the general low microfossil amounts along with phytoliths weathering limit what can be said of these occupations.

Technomorphological Characteristics of Lithics

Table 7 shows technomorphological inventories of chipped stone artifacts from the previous and renewed excavations. The following presents the results of the analyses focusing on cores, core trimming elements, blank morphology, blades/bladelets, and tool types.

Table 7 Inventory of lithic artifacts from Tor Fawaz

Cores and Core Trimming Elements

Table 8 shows technotypological classification of cores from Units 6–10. The cores are dominated by several types of along-axis cores for which we follow the definition by Leder (2014, 2016). Along-axis cores assume a flat overall shape consisting of two convex surfaces (i.e., flat-faced cores). Only one surface is used for the detachment of blanks, while the other is used for striking platforms, thus resembling the Levallois concept (Boëda, 1994). Along-axis cores are characterized by the dominant use of axial flaking, i.e., unidirectional or bidirectional flaking (thus, along axis), for producing elongated blanks as well as for maintaining the convex working surface. However, it is difficult to distinguish between predetermined blanks from predetermining blanks, unlike Levallois methods.

Table 8 Frequency of core types by layers and the scar shapes. The samples include cores from Units 6–10 at Tor Fawaz

In the along-axis cores from Tor Fawaz (Fig. 10ah), parallel sided types (Type 1 according to Leder, 2014) are dominant, and unipolar and bipolar types occur in similar frequencies. Along-axis cores with convergent forms are less common and show unipolar flaking scars, including both preferential (Type 2B) and recurrent (Type 3) methods.

Fig. 10
figure 10

Cores from Units 6–10 at Tor Fawaz. ac Along-axis, single platform, parallel sided, d and e along-axis, opposed platform, parallel sided, f and g along-axis, single platform, convergent preferential for point, h along-axis, single platform, convergent recurrent for blades, i volumetric, single platform, conical, j volumetric, single platform, cylindrical, k and l burin-like cores on flakes. (a, d, e, f, h, i, j, k, l) from Layer B; (b, c, g) from Layer C. Arrows on flaking scars (outlined) show flaking directions. Abbreviations: C = cortex; V = ventral surface of a flake used as a blank for core

Volumetric cores differ from along-axis cores in the overall shape, assuming prismatic or pyramidal forms. In volumetric cores, a working surface extends around a wide periphery of the striking platform (i.e., cylindrical and conical cores) or is located at a narrow front of the core (i.e., narrow-fronted cores). In the Tor Fawaz assemblages, we classified eight cores as volumetric types including parallel or convergent lateral forms (Fig. 10ij). There is one volumetric core with a narrow working surface, assuming a carinated form. All of the volumetric cores show unidirectional flaking scars. In addition, all volumetric cores appear to be made on blocks, while 26% of the along-axis cores (n = 48) are made on thick flakes.

Eight cores are made on flakes with less modification, thus largely retaining original morphology of the flakes. In such cores-on-flakes, we identified three types. The burin-core type (Fig. 10kl) has lateral sides exploited for the detachment of narrow blanks, assuming a burin-like morphology (Zwyns et al., 2012). This type of core technology is part of “bladelet-core-on-flakes” defined by Leder (2014, 2018) and occurs at several Levantine IUP sites including Boker Tachtit (especially Level 2), where multifaceted burins and nucleiform burins are reported (Demidenko et al., 2020; Marks & Kaufman, 1983). Another type of cores-on-flakes is the truncated-and-faceted type (also called Nahr Ibrahim cores). This type is usually made on flakes rather than blades, and their dorsal or ventral surfaces are exploited for the production of flakes (Henry, 2003; Hovers, 2009; Nishiaki, 1985; Solecki & Solecki, 1970). They are included as cores in this study because the final removal scars extend large portions of the exploited convex surface, resembling the Levallois concept. The third type is represented by a scraper-like core. The thickness of the flake is exploited for flake production by using the ventral surface as a striking platform.

Table 8 also shows forms of flaking scars on the working surface of the cores. The majority of the along-axis cores, volumetric cores, and burin-cores show blade/bladelet scars along with flake scars. Point scars occur on three along-axis cores. Exhausted and expedient cores are dominated by flake scars.

The four assemblages (surface, Layer B1, Layer B2, and Layer C1) are commonly characterized by the dominance of along-axis cores, particularly their single platform types. The absence of volumetric cores in Layer C1 is likely due to the small sample size. There is no statistical difference in the relative frequencies of along-axis cores, volumetric cores, and cores-on-flakes between Layer B1 and Layer B2 that have larger sample size (p value of chi-square test = 0.68).

CTEs are dominated by crested/half-crested blades and core tablets in the assemblages from surface, Layer B1, Layer B2, and Layer C1 (Fig. 11ad; Table 9). On the other hand, Layer B2 is characterized by a higher frequency of plunging blades/flakes. Although the sample size of Layer C1 is small, it is similar to other assemblages in the occurrences of half-crested blades and a core tablet. There was no CTEs indicative of Levallois flaking, such as éclat debordant in any assemblage.

Fig. 11
figure 11

Core trimming elements and blades/bladelets from Units 6–10 at Tor Fawaz. a Core tablet, bd crested blades, e bladelet with a plain platform with coarse overhang removal, f bladelet with a plain platform without overhang removal, g Levallois blade with a faceted platform and a blunt distal end, h blade with a faceted platform and a pointed distal end, i Blade with a partially faceted platform and a lateral-distal shape of the in-betweener type, j Levallois-like blade with a faceted platform and a convergent lateral-distal form. Arrows on flaking scars (outlined) show flaking directions. Abbreviations: C = cortex

Table 9 Frequency of core trimming elements from Units 6–10 at Tor Fawaz

Blank Morphology

Table 10 shows frequencies of several technomorphological groups of main blanks (unretouched and not including CTEs, primary elements, and spalls) excavated from the 1994 trench and Units 6–10. Flakes are the most dominant morphology (60–83%), and blades/bladelets (Fig. 11ej) account for about 20–40% except for Layer C2 (11%) in the 1994 trench.

Table 10 Frequency of technomorphological groups of main blanks (not including CTEs, primary elements, and spalls) from the 1994 trench and Units 6–10 at Tor Fawaz

Also notable is the occurrences of pointed blanks, including Levallois-like points (Fig. 13a–c), Umm el-Tlel points (Fig. 13de), and pointed flakes (Fig. 13hj). Their frequency is low (n = 12), but they were found in Layer B1, Layer B2, and Layer C2. In addition, Levallois-like flakes and Levallois-like blades occur in the assemblages from surface, Layer B1, Layer B2, and Layer C1.

There is no statistically significant difference (p value of chi-square test = 0.14) in the frequencies of blank types among Layer B1, Layer B2, and Layer C1 that have larger sample size.

Blades/Bladelets

The ratios of bladelets to blades range between 0.19 and 0.89 (Table 10). The lowest value (0.19) is based on the largest number of blades/bladelets (n = 409) of the Layer B1 assemblage in the Units 6–10. The ratio slightly increases in the underlying layers, i.e., Layer B2 (0.28) and Layer C1 (0.39) in the same units. Similar ratios are observable in Layer C1 (0.33) and Layer C2 (0.33) in the 1994 units. On the other hand, the highest ratio occurs in Layer A (0.89), followed by Layers B1 and B2 (both 0.5) in the 1994 trench.

Regarding the dorsal-distal shapes (Table 11), about a half of the blades/bladelets (49%) are tapering towards the distal end, including three sub-types, i.e., the convergent (Fig. 11j), the in-betweener (Fig. 11i), and the pointed form (Fig. 11h). Among the three sub-types, the pointed type was observed most frequently, followed by the in-betweener. The convergent type, which has the maximum width at the proximal end, is few (n = 4). This pattern does not differ significantly among the assemblages from the surface, Layer B1, Layer B2, and Layer C1 (p value of chi-square test = 0.38).

Table 11 Dorsal-distal shapes of blades/bladelets from Units 6–10 at Tor Fawaz

As shown in Table 12, the dorsal scar directions of blades/bladelets are dominated by the unidirectional scars, followed by the bidirectional and then the crossed pattern. This generally applies to the assemblages from the surface, Layer B1, Layer B2, and Layer C1. However, the percentage of the unidirectional scars gradually decreases from Layer C1 towards the surface, while the bidirectional pattern increases. Such differences are statistically significant (p value of chi-square test < 0.01).

Table 12 Frequency of dorsal scar patterns of blades/bladelets from Units 6–10 at Tor Fawaz

The plain platform occurs most frequently in blades/bladelets, followed by the faceted and partially faceted platforms (Table 13). The “chapeau de gendarme” platform is very rare, and the linear and punctiform platforms are almost completely absent. This pattern does not differ significantly among the assemblages from the surface, Layer B1, layer B2, and Layer C1 (p value of chi-square test = 0.40). The blades/bladelets from the surface, Layer B1, Layer B2, and Layer C1 are also similar to each other in the relative size of the platform (p value of Kruskal–Wallis test = 0.31) (Fig. 12).

Table 13 Frequency of platform types of blades/bladelets from Units 6–10 at Tor Fawaz
Fig. 12
figure 12

Relative platform size (see text for the definition) of blades/bladelets from the surface (n = 20), Layer B1 (n = 70), Layer B2 (n = 39), and Layer C1 (n = 15) in Units 6–10 at Tor Fawaz

As shown in Table 14, the overhang removal is not observable in more than half of the blades/bladelets. When the overhang is removed, it is done by coarse flaking mostly. The fine flaking/abrasion is almost completely absent. This pattern does not differ significantly among the assemblages from the surface, Layer B1, Layer B2, and Layer C1 (p value of chi-square test = 0.82).

Table 14 Frequency of overhang removals of blades/bladelets from Units 6–10 at Tor Fawaz

Tool Types

As shown in Table 7, retouched blades/flakes, which are morphologically unstandardized, constitute the dominant tool type (32–79%) in all the assemblages (Fig. 13). The occurrences of end scrapers (Fig. 13k–n) and burins (Fig. 13o–s) also generally characterize the assemblages from Tor Fawaz. The absence of end scraper from Layer C1 is likely due to the small sample size, rather than a chronological trend, as the underlying Layer C2 includes end scrapers. In contrast, side scrapers are absent or very few (0–1%) in all the assemblages.

Fig. 13
figure 13

Retouched tools, including unretouched points, at Tor Fawaz. ab Retouched Levallois-like points, c unretouched Levallois-like point, d retouched Umm el-Tlel point, e unretouched Umm el-Tlel point, f and g Ksar Akil points, h retouched point on a pointed flake, ij unretouched pointed flakes, kn end scrapers, o and r burin on truncation, p dihedral burin, q and s angle burins, tu retouched blades. All the pieces are from Units 6–10, except for (r) from the 1994 trench. Arrows on flaking scars (outlined) show flaking directions. Abbreviations: C = cortex

A few Levallois-like points were found in Layer B1, Layer B2, and Layer C2 (Fig. 13ab). In addition, Layer B1 and Layer B2 included a single piece of Umm el-Tlel point respectively (Fig. 13de). They are characterized by a series of small elongated scars, like bladelet scars, near the butt (Boëda et al., 2015). One of them has marginal retouch near the tip and on the left lateral edge (Fig. 13d). Layer B1 and B2 also yielded a single piece of Ksar Akil point, respectively (Fig. 13fg). These Ksar Akil points are made on pointed blades (not bladelets). One lateral edge near the tip is marginally retouched to enhance the acuteness of the tip. Four el-Wad points were recovered in Layer A (n = 3) and Layer B1 (n = 1) in the 1994 trench (Kerry & Henry, 2003).

Regarding the morphology of blanks of tool types, Table 15 shows that more than half of the retouched tools are made on blades (53%), followed by flakes (34%). The use of points, bladelets, and CTEs are infrequent (2–4%). Given the predominance of flakes in debitage (Table 10), the greater percentage of blades in retouched tools indicates the selective use of blades with retouch.

Table 15 Frequencies of tool types in Units 6–10 by their blank morphologies

Discussion

Technomorphological Characteristics of the Tor Fawaz lithic Assemblages

The new lithic assemblages from Units 6–10 (n = 6350) are larger than those of previous collections from Units 1–5 (n = 3983) and the 1994 trench (n = 1314), thus doubling the sample size in total (Table 7: n = 11,647). In addition, Units 6–10 were probably closer to prehistoric activity areas given their locations within the rockshelter around the highest part of the slope as well as high densities of lithic distributions on the surface and in the deposits (Fig. 4; Table 3). The depositional contexts of lithics in Units 6–10 were generally similar to those in the 1994 trench, but Layer A was not recognized in Units 6–10 where the greatest density of lithic artifacts was in Layer B1 that was exposed on the surface.

All the lithic assemblages at Tor Fawaz are commonly characterized by the occurrences of Upper Paleolithic tool types, such as end scrapers and burins, that are often made on blades (Tables 7 and 15). Tools made on bladelets, such as retouched bladelets and el-Wad points, are few. Bladelets are also a minor component in unretouched blanks that are dominated by flakes followed by blades (Table 10).

Thus, the previous and new assemblages at Tor Fawaz consistently indicate “a blade technology that produced large, thick, bulky debitage and tools,” as originally pointed out by Coinman and Henry (1995: 194). The robustness of blades/bladelets is associated with their platform traits that are large and often faceted (including dihedral, faceted, partially faceted, and chapeau de gendarme types: Table 13). In addition, overhang removals are absent or conducted by coarse flaking (Table 14). While robust blanks with large, faceted platforms are the general characteristics of Levallois products, the Tor Fawaz assemblages do not include Levallois cores but are characterized by the frequent occurrences of along-axis cores and volumetric cores with blade scars (Table 8), a finding consistent with the presence of a few Levallois-like points, blades, and flakes (Tables 7 and 10). Moreover, the CTEs are characterized by crested blades and core tables with no element indicative of Levallois methods, such as éclat debordant (Table 9).

Among the Levallois-like products, only one of them shows double patination that indicates cultural recycling of the Middle Paleolithic artifacts (Kerry & Henry, 2003). Another possibility is the post-depositional mixing of the Middle Paleolithic artifacts from the underlying layer (e.g., Layer D in the 1994 trench). However, as already pointed out by Kerry and Henry (2003), the Levallois blanks “do not seem to correlate with any stratigraphic trends,” occurring both in Layers B and C. The same result was obtained in the new assemblages from Units 6–10 (Tables 7 and 10).

Consequently, the above techno-typological characteristics at Tor Fawaz are generally in line with IUP lithic technology. We suggest that the few occurrences of Levallois-like points/blades/flakes are part of the inherent characteristics of the Tor Fawaz lithic technology affiliated with the IUP. They are not likely main products of genuine Levallois methods but more likely sub-products of sequential blade production, either from along-axis cores or volumetric cores. Given the dominance of unidirectional dorsal scar patterns (Table 12), the blade production at Tor Fawaz is similar to those at Boker Tachtit Level 4 (Marks & Kaufman, 1983; Volkman, 1983), Tor Sadaf A and B (Fox, 2003; Coinman and Fox, 2004), and Wadi Aghar C–D1 (Kadowaki et al., 2019b) in the southern Levant and Ksar Akil XXIII–XXI (Ohnuma, 1988) and Ücağızlı I–F (Kuhn et al., 2009) in the northern Levant. Although Boker Tachtit Level 4 is characterized by the absence of crested blades (Volkman, 1983), the other IUP assemblages mentioned above include crested debitage like Tor Fawaz.

The distinction of along-axis cores from Levallois cores is sometimes difficult and can vary depending on researchers. For example, Levallois point cores have been recognized in the assemblages from Boker Tachtit Levels 1–3 by original investigators (Marks & Kaufman, 1983; Marks & Rose, 2012; Volkman, 1983), while the cores from these levels are classified as along-axis cores by Leder (2018). The latter position represents one of several opinions that regard the point production technology at Boker Tachtit Levels 1–3 different from the Levallois technology by recognizing some elements of the Upper Paleolithic volumetric flaking strategy (Bar-Yosef, 2000; Belfer-Cohen & Goring-Morris, 2014; Kuhn, 2003; Meignen, 2012).

In the case of Tor Fawaz, along-axis cores, which dominate the core assemblage, should not be classified as “Levallois cores” because the dominance of “Levallois cores” would be inconsistent with the few occurrences of morphologically Levallois blanks (Table 7). In fact, cores and core reduction technology at Boker Tachtit Level 4, Tor Sadaf A/B, and Wadi Aghar C–D1 (that resemble the Tor Fawaz assemblages) are recognized as non-Levallois by original investigators of the sites (Marks, 1983; Volkman, 1983; Coinman and Fox, 2004; Kadowaki et al., 2019b).

On the other hand, the term “Levallois” is used for some cores and blanks in the reports of Ksar Akil XXIII–XXI (Ohnuma, 1988) and Ücağızlı I–F (Kuhn et al., 2009). However, Ohnuma (1988: 285) recognizes “a broad technological similarity” between Ksar Akil XXIII–XXI and Boker Tachtit Level 4, and Kuhn (2003) suggests that “IUP blank production technology already represents a significant departure from Levallois sensu stricto”.

The IUP affiliation of the Tor Fawaz assemblages is also supported by the recovery of two Umm el-Tlel points and two Ksar Akil points from Layers B1 and B2 (Fig. 13). The former type has been known from the IUP contexts at Umm el Tle and Jerf Ajla (Boëda et al., 2015; Richter et al., 2001), while the latter is known from the IUP and the Ahmarian contexts at Ksar Akil (Bergman, 1981; Ohnuma, 1988). On the other hand, it is notable that no Emireh point or chamfered piece is included in the Tor Fawaz assemblages, like Boker Tachtit Level 4, Tor Sadaf A/B, and Wadi Aghar C–D1 in the southern Levant.

The IUP affiliation of the Tor Fawaz assemblages can also be shown by three key attributes of blades/bladelets, i.e., the relative frequencies of (1) unidirectional dorsal scar pattern, (2) pointed distal forms, and (3) faceted platforms including dihedral, multiple faceted, and partially faceted types. Figure 14 compares the Tor Fawaz assemblages from Units 6–10 with Boker Tachtit Levels 1–4 (Marks & Kaufman, 1983), Ksar Akil XXV–XVI (Ohnuma, 1988), Boker A (Jones et al., 1983), and Wadi Aghar B–D1 (Kadowaki et al., 2019b). Layers B2 and C1 at Tor Fawaz are plotted near Boker Tachtit Level 4. More specifically, Layers B2 and C1 are located slightly towards Boker A (Ahmarian) because of the decrease in the frequency of faceted platforms. Tor Fawaz Layer B1 is plotted near the Wadi Aghar assemblages, and the surface collection is near Boker Tachtit Level 3 and Ksar Akil XXI. The shift from Layers B2–C1 to Layer B1/Surface is caused by the decrease in the unidirectional scar pattern and the concomitant increase in the bidirectional scar pattern (Table 12). This technological trend is apparently opposite to that at Boker Tachtit Levels 3–4 and similar to Ksar Akil XXII–XXI; however, it has to be considered with caution because of the surface collection that additionally suffers from small sample size. In addition, Layer B1 in Units 6–10 is directly exposed on the surface and is likely to have been reworked, as we discuss in the next section.

Fig. 14
figure 14

Three-dimensional scatterplot of relative frequencies of unidirectional scar patterns on blades/bladelets, pointed blades/bladelets, and faceted platforms (including multiple, dihedral, and partially faceted types) at Tor Fawaz in comparison with the IUP and Ahmarian assemblages. Abbreviations: BT = Boker Tachtit; KS = Ksar Akil; WA_B = Wadi Aghar Layer B; WA_C-D1; Wadi Aghar Layer C–D1. Chronological orders of the assemblages are indicated by arrows (solid lines for Boker Tachtit, dashed lines for Ksar Akil). See Kadowaki et al.,  2019b2019b: SOM Tables S11–S13) for data sources of Ksar Akil, Boker Tachtit, Boker A, and Wadi Aghar. Data of Tor Fawaz are from Units 6–10

Although all the Tor Fawaz assemblages generally show the IUP techno-typological features, as described above, we note some mixtures of later UP artifacts. Firstly, four el-Wad points have been found in the 1994 trench (Kerry & Henry, 2003). Three of them were found near the surface (Layer A), and another one was from the upper part of Layer B (Layer B1). Secondly, the Layer A assemblage shows a distinctively greater percentage of bladelets (18%) in blanks and a greater ratio of bladelets to blades (0.89) in comparison with the other assemblages (Table 10). However, bladelets are still minor components in the Layer A and Layer B1 assemblages. Based on these observations, we suggest some mixtures of later UP artifacts in Layer A that also infiltrated to Layer B1 in the 1994 trench. The mixed bladelet artifacts are most likely from the Ahmarian that is known at other sites in the Jebel Qalkha area, such as Jebel Humeima, Tor Aeid, and Tor Hamar (Coinman & Henry, 1995; Kerry, 1997; Williams, 1997). In contrast, we did not detect clear signatures of later lithic artifacts in Units 6–10 even in the collection from the surface where Layer B1 deposits are directly exposed.

Depositional Processes and Chronology of the Tor Fawaz Assemblages

Despite the IUP affiliation of most lithic artifacts at Tor Fawaz, the associated OSL and radiocarbon dates are widely distributed from 45 ka to 14 ka (Fig. 15). A major reason for this discrepancy is most likely the redeposition of the lithic artifacts, as exemplified by their distributions on surface and in Layer A that includes twigs and animal dung from recent use of the rockshelter as an animal pen. Thus, we discuss here the depositional processes according to the stratigraphy at Tor Fawaz by considering the results of the multiple analyses presented in this study (Table 16).

Fig. 15
figure 15

Probability distributions of OSL and radiocarbon dates according to the stratigraphy at Tor Fawaz and Wadi Aghar. All the radiocarbon dates are from marine shells (a series of JQ17 and JQ18 numbers) and have been calibrated against the Marine20 curve in the OxCal v4.4.2 (Bronk Ramsey, 2009; Heaton et al., 2020)

Table 16 Summary of the multiple analyses in this study and the reconstruction of depositional processes at Tor Fawaz

Layer A

Layer A was detected only in the 1994 trench, and it has the greatest density of lithic artifacts in this area (Fig. 5) consisting mostly of IUP lithic artifacts with some mixtures of Ahmarian artifacts. The high density and the mixture of IUP and Ahmarian artifacts are likely to have resulted from the deflation of pre-existing deposits (Layer B1 and an overlying Ahmarian deposits). The recent use of the rockshelter as an animal pen resulted in the deposition of animal dung, twigs, and ash.

Layer B1

The lithic artifacts from Layer B1 also showed IUP techno-typological characteristics. However, a single el-Wad point was included in Layer B1 of the 1994 trench, indicating the infiltration of Ahmarian artifacts from Layer A. The mixture of Layer A deposits in Layer B1 was also indicated by the results of phytoliths and dung spherulite analyses (Table 16). These analyses were conducted specifically to examine whether modern animal dung in Layer A was mixed in the underlying layers. As a result, a sample from Layer B1 (No. 17) contained a combination of dung spherulites and phytoliths of dicotyledonous leaves, indicating some mixture with Layer A.

Layer B2

Layer B2 corresponds to the second highest density of lithic distributions (Fig. 5 and 6), and the Layer B2 assemblages show IUP techno-typological characteristics with no apparent mixture of later materials. Although Layer B2 was not analyzed for dung spherulites/phytoliths, the mixture of modern animal dung from Layer A is expected be minimum, if present, considering the significant drop of the dung spherulite density from Layer A (880,000/1g) to Layer B1 (19,000/1g) and its complete absence in the underlying Layer C1.

Layers C1 and C2

The density of lithic artifacts decreases in Layer C1, but the Layer C1 assemblage also shows IUP techno-typological characteristics, particularly in blade production technology (Fig. 14), as presented above. Layer C2 was detected only in the 1994 trench, and the Layer C2 assemblage is even smaller than Layer C1 However, the Layer C2 assemblage is characterized by the occurrence of end scrapers and a few Levallois-like blanks with no Levallois core (Table 7). Thus, we suggest it also affiliated with the IUP. The absence of later lithic artifacts in Layer C is consistent with the complete absence of dung spherulite (from surface deposits) in the Layer C1/C2 samples (Table 5).

Layer D

Layer D, consisting of red sand, was only partially reached near the bedrock in the 1994 trench. The small extent of exposure yielded too few lithic artifacts to conduct techno-typological analysis. Like Layer C, no intrusion of dung spherulite from the surface was detected.

Chronology of the IUP Assemblages at Tor Fawaz

Based on the above discussion of depositional processes, we suggest that the OSL dates of Layer C2 (ca. 45–36 ka) as reliable chronological estimates for the IUP occupations at Tor Fawaz. This age partially overlaps with the OSL dates in Layer C1 and the radiocarbon dates of the marine shells associated with IUP artifacts. The younger OSL dates from Layers A–B2 likely represent the timing of redeposition. One marine shell (JQ17-C18), dated to ca. 26–21 ka cal BP, from Layer B1 probably originated from Ahmarian occupations that also left some lithic artifacts.

Spatio-temporal Distributions and Variations of the IUP in the Levant

The dates of Tor Fawaz and Wadi Aghar have greater overlap with those of the IUP layers at Ksar Akil and Ücağızlı. The latter two sites’ radiocarbon dates are distributed in the span between 46–41 ka cal BP. For example, the end of Ksar Akil Level XXI is estimated to 41.6–40.9 ka cal BP by Douka et al. (2013), and the start of Ksar Akil Level XXII is estimated to 44.9–43.6 ka cal BP by Bosch et al., (2015a, 2015b). Layers G–I at Ücağızlı are estimated to have formed between about 41.4–35 ka BP (ca. 45–40 ka cal BP) (Kuhn et al., 2009), which is similar to an estimate of 45–43 ka cal BP as a start date of Layers F–I by Douka (2013).

In southern Jordan, there are two more IUP sites, i.e., Tor Sadaf and Al-Ansab 2. The Tor Sadaf A and B assemblages are similar to each other in the production of elongated, convergent points with large striking platforms (“elongated Levallois-like points”) from single platform cores, but Tor Sadaf B (later) can be distinguished from Tor Sadaf A (earlier) by some technological aspects, such as the decline of platform faceting and the increase in core tablets (Fox, 2003; Coinman and Fox, 2004). The lithics from Al-Ansab 2 also consist of robust blades and single platform blade cores (Richter et al., 2015) and more specifically characterized by the dominance of volumetric cores and the decline of convergent blanks according to Leder (2018). Although no radiometric dates have been obtained from the two sites, a technotypological study by Leder (2018) placed them in the technological groups (Bokerian B/C and Boker Tachtit 4) that are later than Boker Tachtit 1–2.

The increase of later IUP sites in southern Jordan, dated to ca. 45–36 ka according to Wadi Aghar and Tor Fawaz, may have been facilitated by climatic amelioration as the area is currently dominated by semi-arid and arid environments. According to paleoclimatic data from the Dead Sea, a period of 45–40 ka was associated with an increase in lake level, and the lithological facies of sediment cores show a shift towards wetter conditions at least until 35 ka (Torfstein & Enzel, 2017; Torfstein et al., 2015). A palynological study of the Lake Lisan sediments suggest that the Dead Sea region was climatically stable with constant moisture availability between 62.6 and 15.4 ka, as indicated by relatively high percentages of arboreal pollen or high ratios of Artemisia/Amaranthaceae that are linked to moister conditions (Miebach et al., 2019). In addition, a study of marine pollen record in the southeastern Mediterranean suggests a humid interval at ~ 56–44 ka in the Levant (Langgut et al., 2018). According to this study, the humid interval consists of two phases corresponding to Dansgaard-Oeschger (D-O) interstadials 14 and 12, intervened by a dry spell of Heinrich event 5 (ca. 47–46 ka). The latter humid phase is temporally closer to the beginning of late IUP sites in southern Jordan.

We suggest that a time span estimated for the MP-UP transition at Kebara (49/48 to 47/46 ka: Rebollo et al., 2011) cannot be applied to other areas, where the IUP technology may have lasted until later. An exception is Manot, where the beginning of the Ahmarian was dated to 46 ka cal BP (Alex et al., 2017). Interestingly, neither Kebara nor Manot has yielded IUP assemblages to date, and the assemblages at both sites belong to the northern Ahmarian variant (Abulafia et al., (in press); Kadowaki et al., 2015). In addition, a lithic assemblage from Mughr el-Hamamah (MHM) Layer B, dated to 45–39 ka cal BP (Stutz et al., 2015), has been designated as a variant of the Ahmarian (Shea et al., 2019). Accepting these dates means the contemporaneity of the Ahmarian at Kebara/Manot/MHM and the IUP in other areas in the Levant such as southern Jordan and the Negev. In addition, our age estimate for the IUP at Tor Fawaz (ca. 45–36 ka) overlaps with the age (ca. 38 ka) of the Ahmarian occupation at Al-Ansab 1 in southern Jordan (Richter et al., 2020). Given the possible contemporaneity of the IUP and Ahmarian, Stutz (2020) proposed that they represent two alternative technologies employed by the same forager social networks that spread across areas with variable ecological productivity, population density, and residential mobility.

On the other hand, we suggest it is also important to recognize the geographic differences in the trends of diachronic technological changes. As shown in Fig. 14, the IUP assemblages at Ksar Akil and Boker Tachtit initially showed a similar trend towards an increase in a unidirectional scar pattern. However, the Ksar Akil sequence subsequently shows a decline in the unidirectional pattern from Level XXI (caused by an increase in bidirectional flaking), while at Boker Tachtit unidirectional flaking continued to increase throughout levels 1–4. The increase in bidirectional flaking in the later layers at Ksar Akil is also paralleled by the stratigraphic sequence at Ücağızlı, also located in the littoral zone of the northern Levant (Kuhn et al., 2009). This later technological trend in Ksar Akil and Ücağızlı continued into their subsequent Ahmarian assemblages, resulting in a prominent trait of the northern Ahmarian variant. In contrast, the successive rise in unidirectional flaking seen in the IUP in the southern Levant continued this progression into the southern variant of the Ahmarian represented by Boker A and BE (Jones et al., 1983), Nahal Nizzana XIII (Davidzon & Goring-Morris, 2003), the Lagama sites (Bar-Yosef & Belfer, 1977), Abu Noshra I and II (Phillips, 1988), Tor Sadaf EUP (Fox, 2003), Tor Hamar (Coinman & Henry, 1995), Tor Aeid (Williams, 1997), Jebel Humeima (Kerry, 1997), Al-Ansab 1 (Hauck, 2015; Hussain, 2015; Richter et al., 2020; Schyle, 2015), and others.

In the northern inland Levant, the IUP variant (Paléolithique intermédiaire) at Umm el-Tlel is characterized the production of elongated convergent blanks through unidirectional core flaking (Boëda & Bonilauri, 2006; Boëda et al., 2015), and the dominant employment of unidirectional flaking continued to the blade/bladelet production in the overlying UP levels (Ploux & Soriano, 2003). A similar UP blade/bladelet assemblage, dominated by unidirectional flaking, has also been found at Wadi Kharar 16R in the same area (Kadowaki, 2018; Kadowaki et al., 2015), while no assemblage similar to the northern Ahmarian has so far been found in the northern inland Levant.

Consequently, we suggest that the geographically variable technological trajectories from the late IUP to the Ahmarian (or other early UP entities) can also serve as robust evidence in discussing cultural/social dynamics at the MP-UP transition. This is because the technological trajectories based on stratigraphic evidence are less vulnerable to chronological uncertainties arising from the difficulty in accurate dating for the period in question. Thus, even if the current chronology for the IUP or the Ahmarian are to be changed or refined in future, the regionally different cultural trajectories from the late IUP to the beginning of the Ahmarian will remain stable evidence for the geographically variable pattern of cultural changes that provide important implications for the forager social networks in the Levant and our understanding in how the MP-UP cultural transition took place (Meignen, 2012; Stutz, 2020).

Conclusion

This paper presented lithic technological and chronological analyses of the Tor Fawaz assemblages along with micromorphology, phytolith and dung spherulite examinations to evaluate the formation and postdepositional processes of archaeological remains. As a result, the Tor Fawaz assemblages show general similarity to those of Boker Tachtit Level 4, Tor Sadaf A–B, and Wadi Aghar C–D1 that represent the late phase of the IUP in the southern Levant. Given the extensive redeposition/reworking in the upper layers (Layers A and B), we suggest that the OSL dates of Layer C (particularly Layer C2) as reliable chronological estimates for the IUP occupations at Tor Fawaz (ca. 45–36 ka). This overlaps with the radiocarbon dates of the marine shells (except for a single piece) associated with IUP artifacts.

Thus, Tor Fawaz IUP is temporally close to a nearby IUP occupation at Wadi Aghar C–D1 (ca. 45–40 ka), but the age of Tor Fawaz includes a younger range of post 40 ka. This chronological difference may be congruent with sedimentological and lithic technological differences between the two sites. Thus, the IUP occupations at Wadi Aghar and Tor Fawaz in the Jebel Qalkha area may represent slightly different phases that generally parallel the IUP sequence at Tor Sadaf, another IUP site in southern Jordan, and possibly post-date Boker Tachtit Level 4. This is a detailed recognition of lithic and chronological variability within the late IUP.

Based on these observations, we discussed the issue of partial contemporaneity between the Ahmarian and the late IUP assemblages, and more importantly stressed the geographically different trends in cultural changes from the late IUP to the Ahmarian. The latter phenomenon was likely linked to the formation of multiple forager communities that developed over different environmental areas, including the Mediterranean coast, the Jordan Valley, and the inland steppe. The IUP occurrences at Tor Fawaz and Wadi Aghar (and perhaps at Tor Sadaf and Al-Ansab 2) represent the exploitation of the inland semi-arid zone that was probably facilitated by humid climatic conditions. Despite the formation of multiple local communities, the boundaries between them were not likely rigid but porous with occasional interactions as there were basic common grounds in the direction of lithic technological changes from the IUP to the Ahmarian, such as the increase in bladelet production with the development of the platform preparation technique (Kadowaki et al., 2021). More accurate chronological and cultural data are required to further our understanding of the MP-UP cultural transition.