Mark Lipson1, Anna Szécsényi-Nagy2, Swapan Mallick1,3, Annamária Pósa2, Balázs Stégmár2, Victoria Keerl4, Nadin Rohland1, Kristin Stewardson1,5, Matthew Ferry1,5, Megan Michel1,5, Jonas Oppenheimer1,5, Nasreen Broomandkhoshbacht1,5, Eadaoin Harney1,5, Susanne Nordenfelt1, Bastien Llamas6, Balázs Gusztáv Mende2, Kitti Köhler2, Krisztián Oross2, Mária Bondár2, Tibor Marton2, Anett Osztás2, János Jakucs2, Tibor Paluch7, Ferenc Horváth7, Piroska Csengeri8, Judit Koós8, Katalin Sebők9, Alexandra Anders9, Pál Raczky9, Judit Regenye10, Judit P Barna11, Szilvia Fábián12, Gábor Serlegi2, Zoltán Toldi13, Emese Gyöngyvér Nagy14, János Dani14, Erika Molnár15, György Pálfi15, László Márk16,17,18,19, Béla Melegh18,20, Zsolt Bánfai18,20, László Domboróczki21, Javier Fernández-Eraso22, José Antonio Mujika-Alustiza22, Carmen Alonso Fernández23, Javier Jiménez Echevarría23, Ruth Bollongino4, Jörg Orschiedt24,25, Kerstin Schierhold26, Harald Meller27, Alan Cooper6,28, Joachim Burger4, Eszter Bánffy2,29, Kurt W Alt30,31,32, Carles Lalueza-Fox33, Wolfgang Haak6,34, David Reich1,3,5. 1. Department of Genetics, Harvard Medical School, Boston, Massachusetts 02115, USA. 2. Institute of Archaeology, Research Centre for the Humanities, Hungarian Academy of Sciences, Budapest 1097, Hungary. 3. Medical and Population Genetics Program, Broad Institute of MIT and Harvard, Cambridge, Massachusetts 02142, USA. 4. Institute of Organismic and Molecular Evolution, Johannes Gutenberg University Mainz, Mainz 55128, Germany. 5. Howard Hughes Medical Institute, Harvard Medical School, Boston, Massachusetts 02115, USA. 6. Australian Centre for Ancient DNA, School of Biological Sciences, University of Adelaide, Adelaide, South Australia 5005, Australia. 7. Móra Ferenc Museum, Szeged 6720, Hungary. 8. Herman Ottó Museum, Miskolc 3529, Hungary. 9. Institute of Archaeological Sciences, Eötvös Loránd University, Budapest 1088, Hungary. 10. Laczkó Dezso˝ Museum, Veszprém 8200, Hungary. 11. Balaton Museum, Keszthely 8360, Hungary. 12. Department of Archaeological Excavations and Artefact Processing, Hungarian National Museum, Budapest 1088, Hungary. 13. Jósa András Museum, Nyíregyháza 4400, Hungary. 14. Déri Museum, Debrecen 4026, Hungary. 15. Department of Biological Anthropology, Szeged University, Szeged 6726, Hungary. 16. Department of Biochemistry and Medical Chemistry, University of Pécs, Pécs 7624, Hungary. 17. Imaging Center for Life and Material Sciences, University of Pécs, Pécs 7624, Hungary. 18. Szentágothai Research Center, University of Pécs, Pécs 7624, Hungary. 19. PTE-MTA Human Reproduction Research Group, Pécs 7624, Hungary. 20. Department of Medical Genetics and Szentágothai Research Center, University of Pécs, Pécs 7624, Hungary. 21. Dobó István Castle Museum, Eger 3300, Hungary. 22. Department of Geography, Prehistory, and Archaeology, University of the Basque Country, Investigation Group IT622-13, Vitoria-Gasteiz 01006, Spain. 23. CRONOS SC, Burgos 09007, Spain. 24. Department of Prehistoric Archaeology, Free University of Berlin, Berlin 14195, Germany. 25. Curt-Engelhorn-Centre Archaeometry gGmbH, Mannheim 68159, Germany. 26. Commission for Westphalian Antiquities, Westphalia-Lippe Regional Association, 48157 Münster, Germany. 27. State Office for Heritage Management and Archaeology Saxony-Anhalt and State Heritage Museum, Halle 06114, Germany. 28. Environment Institute, University of Adelaide, Adelaide, South Australia 5005, Australia. 29. Romano-Germanic Commission, German Archaeological Institute, Frankfurt am Main 60325, Germany. 30. Center of Natural and Cultural History of Man, Danube Private University, Krems-Stein 3500, Austria. 31. Department of Biomedical Engineering, University of Basel, Allschwil 4123, Switzerland. 32. Institute for Integrative Prehistory and Archaeological Science, University of Basel, Basel 4055, Switzerland. 33. Institute of Evolutionary Biology (CSIC-UPF), Barcelona 08003, Spain. 34. Department of Archaeogenetics, Max Planck Institute for the Science of Human History, Jena 07745, Germany.
Abstract
Ancient DNA studies have established that Neolithic European populations were descended from Anatolian migrants who received a limited amount of admixture from resident hunter-gatherers. Many open questions remain, however, about the spatial and temporal dynamics of population interactions and admixture during the Neolithic period. Here we investigate the population dynamics of Neolithization across Europe using a high-resolution genome-wide ancient DNA dataset with a total of 180 samples, of which 130 are newly reported here, from the Neolithic and Chalcolithic periods of Hungary (6000-2900 bc, n = 100), Germany (5500-3000 bc, n = 42) and Spain (5500-2200 bc, n = 38). We find that genetic diversity was shaped predominantly by local processes, with varied sources and proportions of hunter-gatherer ancestry among the three regions and through time. Admixture between groups with different ancestry profiles was pervasive and resulted in observable population transformation across almost all cultural transitions. Our results shed new light on the ways in which gene flow reshaped European populations throughout the Neolithic period and demonstrate the potential of time-series-based sampling and modelling approaches to elucidate multiple dimensions of historical population interactions.
Ancient DNA studies have established that Neolithic European populations were descended from Anatolian migrants who received a limited amount of admixture from resident hunter-gatherers. Many open questions remain, however, about the spatial and temporal dynamics of population interactions and admixture during the Neolithic period. Here we investigate the population dynamics of Neolithization across Europe using a high-resolution genome-wide ancient DNA dataset with a total of 180 samples, of which 130 are newly reported here, from the Neolithic and Chalcolithic periods of Hungary (6000-2900 bc, n = 100), Germany (5500-3000 bc, n = 42) and Spain (5500-2200 bc, n = 38). We find that genetic diversity was shaped predominantly by local processes, with varied sources and proportions of hunter-gatherer ancestry among the three regions and through time. Admixture between groups with different ancestry profiles was pervasive and resulted in observable population transformation across almost all cultural transitions. Our results shed new light on the ways in which gene flow reshaped European populations throughout the Neolithic period and demonstrate the potential of time-series-based sampling and modelling approaches to elucidate multiple dimensions of historical population interactions.
The population dynamics of the Neolithization process are of great importance for understanding European prehistory[10-13]. The first quantitative model of the Neolithic transition to integrate archaeological and genetic data was the demic diffusion hypothesis[10], which posited that growing population densities among Near Eastern farmers led to a range expansion that spread agriculture to Europe. Ancient DNA analysis has validated major migrations from populations related to Neolithic Anatolians as driving the introduction of farming in Europe[1-8], but the demic diffusion model does not account for the complexities of the interactions between farmers and hunter-gatherers in Europe throughout the Neolithic[11-16]. For example, ancient DNA has shown that farmers traversed large portions of Europe with limited initial admixture from hunter-gatherers[3,5,7,8], and furthermore that farmers and hunter-gatherers lived in close proximity in some locations long after the arrival of agriculture[15,16]. However, genetic data have yet to be used systematically to model the population interactions and transformations during the course of the Neolithic period. Key open questions include whether migrating farmers mixed with hunter-gatherers at each stage of the expansion (and if so how soon after arriving) and whether the previously observed increase in hunter-gatherer ancestry among farmers in several parts of Europe by the Middle Neolithic[5-9] represented a continuous versus discrete process and a continent-wide phenomenon versus a collection of parallel, local events.We compiled a high-resolution data set of 180 Neolithic and Chalcolithic European genomes (pre-dating the arrival of steppe ancestry in the third millennium BCE [ref 5]) from what are now Hungary, Germany, and Spain, of which 130 individuals are newly reported here, 45 with new direct radiocarbon dates (Table 1; Fig. 1A, B; Extended Data Tables 1, 2; Supplementary Tables 1, 2; Supplementary Information sections 1–3). We enriched for DNA fragments covering a set of ~1.23 million single nucleotide polymorphism (SNP) targets[7] and called one allele at random per site, obtaining largely high-quality data, with at least 100,000 SNPs hit at least once (average coverage ~0.1 or higher) for 90 of the 130 samples (Methods). The majority (90) of our new samples comprise an approximately 3000-year transect of the prehistory of the Carpathian Basin (Supplementary Information section 1), from both the eastern (Great Hungarian Plain, or Alföld) and western (Transdanubia) portions of present-day Hungary. For our primary analyses, we retained 104 samples from 15 population groupings (Methods; Table 1), which we merged with 50 Neolithic individuals from the literature[4,5,7,17,18]. We co-analyzed these samples with 25 Neolithic individuals (~6500–6000 BCE) from northwestern Anatolia[7] to represent the ancestors of the first European farmers (FEF; Supplementary Information section 4) and four primary European hunter-gatherer individuals[4,7,17,19,20] (“WHG,” western hunter-gatherers; Table 1).
Table 1
Neolithic population groups and western hunter-gatherer individuals in the study
Population
Country
Samples*
Appx. dates (BCE)
Körös EN
HungaryE
6/5/3†
6000–5500
Starčevo EN
HungaryW
5/4/4
6000–5500
ALPc MN
HungaryE
25/20/22
5500–5000
LBKT MN
HungaryW
8/7/7
5500–5000
Vinča MN
HungaryW
6/6/0
5500–5000
Tisza LN
HungaryE
6/6/5
5000–4500
TDLN
HungaryW
15/14/14
5000–4500
Tiszapolgár CA
HungaryE
5/5/0
4500–4000
Lasinja CA
HungaryW
7/7/6
4300–3900
Protoboleráz CA
HungaryE
4/4/4
3800–3600
Baden CA
Hungary
13/12/10
3600–2850
LBK EN
Germany
30/15/29
5500–4850
Germany MN
Germany
8/4/7
4600–3000
Blätterhöhle MN
Germany
4/4/4†
4100–3000
Iberia EN
Spain
7/2/7
5500–4500
Iberia MN
Spain
4/0/4
3900–3600
Iberia CA
Spain
27/15/27
3000–2200
KO1 HG
HungaryE
1/0/1
5700
LB1 HG
Spain
1/0/1
5900
LOS HG
Luxembourg
1/0/1
6100
VIL HG
ItalyE
1/0/1
12,000
Total number/new in this study/used in final analyses
Includes one hunter-gatherer individual treated separately
Eastern
Western
EN/MN/LN, Early/Middle/Late Neolithic; CA, Chalcolithic; HG, hunter-gatherer (LB1, La Braña 1; LOS, Loschbour; VIL, Villabruna)
Figure 1
Spatial and temporal contexts of European Neolithic samples
a, b, Locations of samples used for analyses, with close-up of Hungary (orange shading for Alföld and light blue for Transdanubia). c, Sample dates arranged by longitude. d, Hunter-gatherer genetic cline (derived from MDS analysis; Supplementary Information section 5) as a function of longitude. The four primary WHG individuals are shown together with “BIC” (Bichon, ~11,700 BCE from Switzerland[21]), “EHG” (eastern hunter-gatherers, ~7000–5000 BCE from Russia[5,7]), and “ElM” (El Mirón, ~17,000 BCE from Spain[20]). Random jitter is added to separate overlapping positions in a–c. GerMN, Germany MN; Blatt., Blätterhöhle; Protob., Protoboleráz.
Extended Data Table 1
Information for Neolithic individuals from Hungary.
ID
Population
Site
Lat.
Long.
Date
Sex
Mt Hap
γ Hap
Cov.
HG%
ALD
Ref.
GEN68
Körös
Törökszentmiklós road 4 site 3
47.2
20.4
5706–5541
F
k1a
‥
6.16
−2.16±1.5
0±0.0
HUNG276, KO2
Körös
Berettyóújfalu-Morotva-liget
47.3
21.5
5713–5566
F
K1a
‥
0.91
−1.49±1.6
0±0.0
[7, 17]
TIDO2a
Körös
Tiszaszőlős-Domaháza
47.6
20.7
5736–5547
M
K1
I2a2
0.45
79.3±2.1
16±3.8
BAM17b
Starčevo
Alsónyék-Bátaszék, Mérnöki telep
46.2
18.7
5832–5667
M
T1a2
H2
1.47
7.76±1.7
4.5±1.9
BAM25
Starčevo
Alsónyék-Bátaszék, Mérnöki telep
46.2
18.7
5702–5536
M
N1a1a1
H2
0.22
1.62±1.9
0±0.0
[5, 7]
BAM4a
Starčevo
Alsónyék-Bátaszék, Mérnöki telep
46.2
18.7
5641–5547
M
K1a4
G2a2a1
0.20
3.39±2.0
0±0.0
LGCS1a
Starčevo
Lánycsók
46.0
18.6
5800–5500
M
W5
G2a2b2b1a
0.77
−0.63±1.6
0±0.0
BAL25b
LBKT
Bátaszék-Lajvér
46.2
18.7
5208–4948
M
K1b1a
G2a2a1
2.77
0.06±1.5
0±0.0
BOVO1b
LBKT
Bölcske-Gyűrűsvölgy
46.7
19.0
5300–4900
F
H
‥
0.01
10.9±6.3
0±0.0
BUD4a
LBKT
Budakeszi-Szőlőskert
47.5
18.9
5300–4900
M
T1a
G2a2b2a
0.17
6.72±2.3
36±6.1
BUD9a
LBKT
Budakeszi-Szőlőskert
47.5
18.9
5300–4900
F
U2
‥
1.10
1.87±1.6
13±5.3
GEN18
LBKT
Alsónyék, site 11
46.2
18.7
5309–5074
M
T2c1
G2a2b2b1
1.48
2.66±1.5
35±12
KON3
LBKT
Enese elkerülő, Kóny, Proletár-dülö, M85, site 2
47.6
17.4
5300–4900
F
T2b
‥
0.03
2.79±4.0
0±0.0
SZEH4
LBKT
Szemely-Hegyes
46.4
18.7
5207–4944
F
N1a1a1a3
‥
0.07
1.88±3.0
0±0.0
[5, 7]
CEG07B
ALPc
Cegléd, site 4/1
47.2
19.9
5300–4900
M
J2b1
G2a2b2a
0.30
11.4±1.9
0±0.0
CEG08b
ALPc
Cegléd, site 4/1
47.2
19.9
5300–4900
F
J1c1
‥
0.19
11.0±2.2
23±3.0
EBSA2a
ALPc
Ebes-Sajtgyár
47.5
21.5
5300–4900
F
K1a
‥
0.05
16.2±3.1
0±0.0
EBVO5a
ALPc
Ebes-Zsongvölgy
47.5
21.5
5300–4900
M
V1a
CT
0.04
9.25±3.3
0±0.0
HAJE10a
ALPc
Hajdúnánás-Eszlári út
47.9
21.4
5221–5000
M
J2b1
I
0.29
10.8±1.8
0±0.0
HAJE7a
ALPc
Hajdúnánás-Eszlári út
47.9
21.4
5302–5057
M
K1a
I2
1.57
9.15±1.7
6.2±5.7
HELI11a
ALPc
Hejőkürt-Lidl
47.9
21.0
5209–4912
M
N1a1a1
I2a2a1b
0.99
6.01±1.8
14±2.0
HELI2a
ALPc
Hejőkürt-Lidl
47.9
21.0
5300–4900
M
U8b1b
I
0.09
7.39±2.6
4.4±1.7
HUNG302, NE2
ALPc
Debrecen Tocopart Erdoalja
47.5
21.6
5291–5056
F
H
‥
4.88
11.0±1.7
0±0.0
[7, 17]
HUNG372, NE5
ALPc
Kompolt-Kígyósér
47.2
20.8
5295–4950
M
J1c1
C1a2
4.25
7.48±1.6
0±0.0
[7, 17]
HUNG86, NE3
ALPc
Garadna-Elkerülő út site 2
48.5
21.2
5281–5026
F
X2b-T226C
‥
3.32
12.1±1.7
18±3.2
[7, 17]
MEMO24b
ALPc
Mezőkövesd-Mocsolyás
47.8
20.6
5500–5300
M
U8b1b
CT
0.04
11.7±3.3
26±12
MEMO2b
ALPc
Mezőkövesd-Mocsolyás
47.8
20.6
5500–5300
F
K1a1
‥
2.28
8.99±1.7
24±5.2
MEMO7a
ALPc
Mezőkövesd-Mocsolyás
47.8
20.6
5481–5361
F
HV
‥
0.26
1.64±1.9
13±6.1
PF325, NE1
ALPc
Polgár-Ferenci-hát
47.9
21.2
5306–5071
F
U5b2c
‥
1.52
8.12±1.8
11±3.9
[7, 17]
PF839/1198, NE4
ALPc
Polgár-Ferenci-hát
47.9
21.2
5211–5011
F
J1c5
‥
3.49
9.95±1.7
25±10
[7, 17]
POPI5a
ALPc
Polgár-Piócás
47.9
21.1
5300–4900
M
K1a1
I2a2a
0.31
9.75±2.0
11±3.7
PULE1.18a
ALPc
Pusztataskony-Ledence
47.5
20.5
5300–4900
F
T2c1d1
‥
0.29
10.6±1.8
0±0.0
PULE1.23a
ALPc
Pusztataskony-Ledence
47.5
20.5
5300–4900
F
H1e
‥
0.17
9.52±2.2
11±3.4
TISO13a
ALPc
Tiszadob-Ókenéz
48.0
21.2
5208–4942
M
J1c2
I2a2a
1.21
12.9±1.7
22±7.6
TISO1b
ALPc
Tiszadob-Ókenéz
48.0
21.2
5300–4900
M
H7
I2a2a1b1
0.11
7.24±2.4
0±0.0
TISO3a
ALPc
Tiszadob-Ókenéz
48.0
21.2
5300–4900
F
U5b2b1a
‥
0.27
12.1±2.1
8.4±5.2
SEKU10a
Vinča
Szederkény-Kukorica-dülö
45.6
18.3
5320–5080
M
K2a
G2a2b2a1a
0.24
2.28±1.9
0±0.0
SEKU6a
Vinča
Szederkény-Kukorica-dülö
45.6
18.3
5321–5081
F
H26
‥
1.15
9.16±1.7
9.0±9.4
VEGI17a
Vinča
Versend-Gilencsa
45.6
18.3
5400–5000
F
U2
‥
0.01
−6.14±5.6
0±0.0
VEGI3a
Vinča
Versend-Gilencsa
45.6
18.3
5400–5000
M
T2b
H2
0.41
0.53±1.8
0±0.0
Gorzsa18
Tisza
Hódmezővásárhely-Gorzsa
46.4
20.4
5000–4500
M
U5b2c
I2a1
6.87
7.77±1.6
13±4.3
Gorzsa4
Tisza
Hódmezővásárhely-Gorzsa
46.4
20.4
5000–4500
F
T1a
‥
0.06
11.3±3.0
22±11
KOKE3a
Tisza
Hódmezővásárhely-Kökénydomb Vörös tanya
46.4
20.2
5000–4500
M
K1b1
I
0.06
13.7±3.2
0±0.0
PULE1.24
Tisza
Pusztataskony-Ledence
47.5
20.5
5000–4500
F
K1a4
‥
0.40
10.4±1.9
18±7.2
VSM3a
Tisza
Vésztő-Mágor
46.9
21.2
5000–4500
M
H26
G2a
0.09
6.92±2.6
0±0.0
ALE14a
TDLN
Alsónyék-Elkerülő site 2
46.2
18.7
5030–4848
M
U8b1b
G2a
0.05
−1.11±3.2
0±0.0
ALE4a
TDLN
Alsónyék-Elkerülő site 2
46.2
18.7
5016–4838
M
T2c1
F
0.03
10.6±3.6
0±0.0
BAL3a
TDLN
Bátaszék-Lajvér
46.2
18.7
4800–4500
M
T2f
H1b1
0.91
6.89±1.7
22±9.0
CSAT19a
TDLN
Csabdi-Télizöldes
47.5
18.6
4800–4500
M
H
H
0.52
5.82±1.8
34±9.6
CSAT25a
TDLN
Csabdi-Télizöldes
47.5
18.6
4826–4602
M
T2b
I2
0.43
13.5±1.9
26±8.1
FAGA1a
TDLN
Fajsz-Garadomb
46.4
18.9
5100–4750
M
HVOa
I
0.09
5.08±2.4
0±0.0
FAGA2a
TDLN
Fajsz-Garadomb
46.4
18.9
5195–4842
F
H
‥
0.49
11.9±1.8
14±4.1
FEB3a
TDLN
Felsőörs-Bárókert
47.0
18.0
4800–4500
M
H44
J2a
0.16
6.31±2.1
0±0.0
HUNG347, NE7
TDLN
Apc-Berekalja
47.2
19.8
4491–4357
M
N1a1a1a
I
4.85
10.6±1.6
19±3.1
[7, 17]
SZEH5a
TDLN
Szemely-Hegyes
46.0
18.3
4904–4709
M
K1b1a
G
0.01
10.8±6.5
0±0.0
SZEH7b
TDLN
Szemely-Hegyes
46.0
18.3
4930–4715
F
K1a
‥
0.52
3.44±1.7
0±0.0
VEJ12a
TDLN
Veszprém Jutasi út
47.1
17.9
4800–4500
M
U8b1a2b
H
0.10
6.17±2.3
0±0.0
VEJ2a
TDLN
Veszprém Jutasi út
47.1
17.9
4800–4500
M
T2b
C
0.34
5.63±1.8
0±0.0
VEJ5a
TDLN
Veszprém Jutasi út
47.1
17.9
4936–4742
M
J1c2
G2a2a1
0.62
7.78±1.8
15±2.9
GEN67
Tiszapolgár
Törökszentmiklós road 4 site 3
47.2
20.4
4444–4257
M
H1
I2a2a1b
2.28
13.0±1.7
50±15
PULE1.10a
Tiszapolgár
Pusztataskony-Ledence
47.5
20.5
4500–4000
M
T2c1
I2a
0.28
9.03±2.0
0±0.0
PULE1.13a
Tiszapolgár
Pusztataskony-Ledence
47.5
20.5
4500–4000
M
T2c1
G2a2b2a1a1c1a
0.38
10.3±1.9
0±0.0
PULE1.9a
Tiszapolgár
Pusztataskony-Ledence
47.5
20.5
4500–4000
M
H26
G2a2b
0.11
11.6±2.4
0±0.0
GEN100
Lasinja
Alsónyék, site 11
46.2
18.7
4300–3900
F
T2b
‥
1.81
9.51±1.6
45±11
GEN49
Lasinja
Nemesnádudvar-Papföld
46.3
19.1
4228–3963
M
T2b23
CT
0.97
12.8±1.8
27±6.8
KEFP2a
Lasinja
Keszthely-Fenékpuszta
46.7
17.2
4300–3900
F
J2b1a
‥
0.74
9.12±1.7
21±5.4
KON2a
Lasinja
Enese elkerülő, Kóny, Proletár-dülö, M85, site 2
47.6
17.4
4333–4072
F
K2a
‥
2.13
10.3±1.7
21±6.4
M6-116.12a
Lasinja
Lánycsók, Csata-alja
46.0
18.6
4232–4046
F
T2f8a
‥
0.64
9.68±1.7
29±11
VEJ9a
Lasinja
Veszprém Jutasi út
47.1
17.9
4339–4237
M
H40
CT
0.05
8.83±3.2
0±0.0
GEN60
Protoboleráz
Abony, Turjányos-dűlő
47.2
20.0
3909–3651
M
H
G2a2b2a
1.88
14.0±1.6
37±8.8
GEN61
Protoboleráz
Abony, Turjányos-dűlő
47.2
20.0
3800–3600
M
J1c
I2c
0.76
10.8±1.7
65±13
GEN62
Protoboleráz
Abony, Turjányos-dűlő
47.2
20.0
3762–3636
F
N1a1a1a3
‥
4.81
8.00±1.6
37±9.6
GEN63
Protoboleráz
Abony, Turjányos-dűlő
47.2
20.0
3658–3384
M
U5a1c1
I2c
1.92
11.9±1.7
34±8.1
GEN12a
Baden
Budakalász-Luppa csárda
47.6
19.0
3340–2945
M
H26a
G2a2b2a1a1b1
1.98
13.8±1.6
34±7.2
GEN13a
Baden
Budakalász-Luppa csárda
47.6
19.0
3332–2929
M
HV
G2a2b2a1a
2.65
11.3±1.6
27±6.6
GEN15a
Baden
Budakalász-Luppa csárda
47.6
19.0
3367–3103
M
J2a1a1
G2a2b2a1a1c1a
1.66
10.8±1.7
22±9.3
GEN16a
Baden
Alsónémedi
47.3
19.2
3346–2945
F
T2b
‥
4.30
12.9±1.6
38±16
GEN17a
Baden
Alsónémedi
47.3
19.2
3359–3098
M
U5b3f
G2a2a
0.82
10.7±1.7
21±6.4
GEN21
Baden
Balatonlelle-Felső-Gamász
46.8
17.7
3600–2850
M
K1a
I2a1
0.67
12.3±1.7
0±0.0
GEN22
Baden
Balatonlelle-Felső-Gamász
46.8
17.7
3332–2929
M
U5a1
I2a1a1
2.31
14.5±1.7
25±6.6
GEN55
Baden
Vámosgyörk
47.7
19.9
3600–2850
F
T2c1d1
‥
0.81
13.1±1.7
22±6.6
HUNG353, CO1
Baden
Apc-Berekalja
47.2
19.8
3315–2923
F
H
‥
4.56
15.1±1.7
0±0.0
[7, 17]
Vors1
Baden
Vörs
46.7
17.3
3300–2850
F
T2f
‥
0.03
4.47±4.2
0±0.0
Cov: average coverage per SNP. HG%: inferred percentage of hunter-gatherer ancestry (mean ± standard error). ALD inferred date of admixture (generations in the past; mean ± standard error; zero implies no date obtained). Ref: reference for published data; if blank, newly published sample in this study (asterisk denotes a published individual with new sequencing data added). Radiocarbon dates are in normal text, while dates estimated from archaeological context are in italics. Further information can be found in Supplementary Table 1.
Extended Data Table 2
Information for Neolithic individuals from Germany and Spain.
ID
Population
Site
Lat.
Long.
Date
Sex
Mt Hap
Y Hap
Cov.
HG%
ALD
Ref.
HAL03a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5295–5057
F
T2b
‥
0.01
−5.13±6.8
0±0.0
HAL07a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5212–4992
F
N1a1a1
‥
0.05
1.72±3.2
0±0.0
HAL15a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5199–4857
M
N1a1a1a3
G2
0.02
5.26±5.0
0±0.0
HAL17b
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
V1
‥
0.02
9.21±4.2
0±0.0
HAL18a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
K2a
‥
0.02
0.27±4.6
0±0.0
HAL19
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
K1a2
‥
0.86
7.10±1.7
16±7.6
[7]*
HAL2
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5211–4963
M
N1a1a1a2
G2a2a1
0.76
1.91±1.7
11±2.4
[5, 7]*
HAL20b
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
M
K1a2
G2a2a
0.06
2.53±3.1
0±0.0
HAL21a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
M
T2b
G2a2a
0.01
−4.41±5.8
0±0.0
HAL22b
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
T2b
‥
0.02
−7.71±4.7
0±0.0
HAL24
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5201–4850
M
X2d1
G2a2a1
0.42
6.39±1.8
0±0.0
[5, 7]*
HAL25
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5210–5002
M
K1a
G2a2a1
0.49
2.58±1.7
18±6.6
[5, 7]*
HAL27a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
M
N1a1a3
G2a2a
0.05
3.84±3.0
0±0.0
HAL31a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5295–5057
F
K1
‥
0.12
4.54±2.3
11±3.1
HAL32b
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
H26
‥
0.23
3.34±2.0
23±4.4
HAL34
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5219–5021
F
N1a1a1
‥
0.25
5.63±2.0
9.2±5.0
[5, 7]*
HAL35b
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
J1c
‥
0.10
3.93±2.4
0±0.0
HAL38a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
V1
‥
0.29
1.10±1.9
0±0.0
HAL39b
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5210–5002
M
H1e
G2a2a1
0.08
3.96±2.6
0±0.0
HAL4
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5202–4852
F
N1a1a1a
‥
6.92
6.55±1.6
18±5.9
[5, 7]*
HAL40a
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5500–4850
F
T2b
‥
0.17
2.50±2.1
0±0.0
HAL5
LBK
Halberstadt-Sonntagsfeld
51.9
11.0
5211–4991
F
T2c1
‥
2.23
2.98±1.6
15±5.4
[5, 7]*
KAR16A
LBK
Karsdorf
51.3
11.7
5500–4850
M
H46b
T1a
0.09
0.28±2.6
13±5.1
[7]
KAR6
LBK
Karsdorf
51.3
11.7
5217–5041
M
H1/H1au1b
CT
0.10
5.78±2.5
0±0.0
[5, 7]
LBK1976
LBK
Viesenhäuser Hof
48.8
9.2
5500–4850
F
T2e
‥
0.44
3.46±1.7
18±4.4
[5, 7]
LBK1992
LBK
Viesenhäuser Hof
48.8
9.2
5500–4850
F
T2b
‥
2.66
5.68±1.6
12±4.3
[5, 7]
LBK2155
LBK
Viesenhäuser Hof
48.8
9.2
5500–4850
F
T2b
‥
3.63
4.84±1.5
13±4.4
[5, 7]
Stuttgart
LBK
Viesenhäuser Hof
48.8
9.2
5310–5076
F
T2c1d1
‥
9.65
3.00±1.6
22±8.1
[4]*
UWS4
LBK
Unterwiederstedt
51.7
11.5
5223–5021
F
J1c17
‥
18.6
5.70±1.6
13±14
[5, 7]
ESP30
GermanyMN
Esperstedt
51.4
11.7
3970–3710
M
H1e1a
I
0.09
22.0±2.7
0±0.0
[5, 7]
HAL13a
GermanyMN
Halberstadt-Sonntagsfeld
51.9
11.0
4600–4300
F
V1a
‥
0.11
9.04±2.4
13±4.3
QLB15D
GermanyMN
Quedlinburg
51.8
11.1
3654–3527
M
HV
R
0.16
20.9±2.2
36±8.7
[5, 7]
QLB18A
GermanyMN
Quedlinburg
51.8
11.1
3640–3376
F
T2e1
‥
0.41
19.6±1.8
23±4.9
[5, 7]
SALZ3B
GermanyMN
Salzmünde-Schiebzig
51.5
11.8
3400–3025
M
U3a1
G2a2a1
0.09
14.9±2.7
0±0.0
[7]
SALZ57A
GermanyMN
Salzmünde-Schiebzig
51.5
11.8
3345–3097
F
H3
‥
0.02
25.0±4.4
0±0.0
SALZ77A
GermanyMN
Salzmünde-Schiebzig
51.5
11.8
3400–3025
M
H3
IJK (x J)
0.02
21.3±5.0
0±0.0
Bla16
Blätterhöhle
Blätterhöhle Cave
51.4
7.6
3958–3344
M
U5b2a2
R1b1
0.80
39.5±1.9
15±5.8
Bla28
Blätterhöhle
Blätterhöhle Cave
51.4
7.6
3337–3024
M
J1c1b1
R1
0.10
51.9±2.7
11±4.5
Bla5
Blätterhöhle
Blätterhöhle Cave
51.4
7.6
3704–3117
F
H5
‥
5.07
41.2±1.9
24±4.7
Bla8
Blätterhöhle
Blätterhöhle Cave
51.4
7.6
4038–3532
M
U5b2b2
I2a1
4.58
72.6±2.0
12±2.9
CB13
Iberia EN
Cova Bonica
41.4
1.9
5469–5327
F
K1a2a
‥
0.98
9.97±1.7
17±3.5
[18]
E-06-Ind1
Iberia EN
EI Prado de Pancorbo
42.6
−3.1
4827–4692
F
K1a4a1
‥
0.47
8.72±1.8
17±2.3
E-14-Ind2
Iberia EN
EI Prado de Pancorbo
42.6
−3.1
5216–5031
F
H1
‥
0.38
7.52±1.8
19±2.8
Troc1
Iberia EN
Els Trocs
42.5
0.5
5311–5218
F
J1c3
‥
0.69
7.15±1.7
12±9.1
[5, 7]
Troc3
Iberia EN
Els Trocs
42.5
0.5
5294–5066
M
T2c1d/T2c1d2
R1b1a
1.31
9.91±1.8
49±22
[5, 7]
Troc5
Iberia EN
Els Trocs
42.5
0.5
5310–5078
M
N1a1a1
I2a1b1
13.8
6.83±1.6
6.8±2.8
[5, 7]
Troc7
Iberia EN
Els Trocs
42.5
0.5
5303–5075
F
V
‥
1.57
11.0±1.7
18±4.8
[5, 7]
Mina18
Iberia MN
La Mina
41.3
−2.3
3893–3661
F
U5b1
‥
13.6
22.8±1.7
42±18
[5, 7]
Mina3
Iberia MN
La Mina
41.3
−2.3
3900–3600
M
K1a1b1
H2
0.38
19.5±1.9
80±20
[5, 7]
Mina4
Iberia MN
La Mina
41.3
−2.3
3900–3600
M
H1
I2a2a1b2
3.95
22.6±1.9
25±6.2
[5, 7]
Mina6
Iberia MN
La Mina
41.3
−2.3
3900–3600
F
K1b1a1
‥
1.36
18.9±1.7
46±8.2
[5, 7]
1.-K11
Iberia CA
La Chabola de la Hechicera
42.6
−2.6
3263–2903
M
X2b
I2a2
0.18
27.8±2.1
68±28
3.-K11
Iberia CA
La Chabola de la Hechicera
42.6
−2.6
3627–3363
F
J2a1a1
‥
0.12
24.4±2.4
27±11
5.-K18
Iberia CA
La Chabola de la Hechicera
42.6
−2.6
3090–2894
M
J1c1
I2a2
0.10
18.5±2.5
43±11
ES.1/4
Iberia CA
EI Sotillo
42.6
−2.6
2571–2347
M
H3
I
0.07
25.4±2.8
0±0.0
ES-6G-110
Iberia CA
EI Sotillo
42.6
−2.6
2916–2714
M
H3
I2a2a
0.05
25.4±3.2
0±0.0
Inventario0/4
Iberia CA
EI Sotillo
42.6
−2.6
2481–2212
M
X2b
I2a2a
0.12
29.6±2.5
56±23
LHUE11J.5
Iberia CA
Alto de la Huesera
42.6
−2.6
3092–2877
F
U5b1
‥
1.19
26.7±1.9
40±9.7
LHUE2010.10
Iberia CA
Alto de la Huesera
42.6
−2.6
3014–2891
F
J1c1
‥
0.11
25.2±2.5
64±13
LHUE2010.11
Iberia CA
Alto de la Huesera
42.6
−2.6
3092–2918
M
V
G2a2a
5.36
28.9±1.8
38±12
LHUE2014.11J
Iberia CA
Alto de la Huesera
42.6
−2.6
3100–2850
F
U5b2b
‥
0.06
26.3±3.0
0±0.0
LY.II.A.10.15066
Iberia CA
Las Yurdinas II
42.6
−2.7
3350–2750
M
U5b2b3a
I2a2a
1.93
30.0±1.8
0±0.0
LY.II.A.10.15067
Iberia CA
Las Yurdinas II
42.6
−2.7
3350–2750
F
J2a1a1
‥
0.30
23.8±2.0
0±0.0
LY.II.A.10.15068
Iberia CA
Las Yurdinas II
42.6
−2.7
3350–2750
F
K1a4a1
‥
0.39
29.2±1.9
26±10
LY.II.A.10.15069
Iberia CA
Las Yurdinas II
42.6
−2.7
3354–2943
F
J1c3
‥
4.24
25.1±1.7
28±15
MIR1
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
F
K1a
‥
0.24
24.2±2.1
0±0.0
[7]
MIR13
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
F
H3c3
‥
0.10
27.8±2.4
0±0.0
[7]
MIR14
Iberia CA
EI Mirador Cave
42.3
−3.5
2568–2346
M
H3
I2a2a
0.94
23.3±1.8
57±15
[7]
MIR17
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
F
J1c1
‥
0.22
23.6±2.2
0±0.0
[7]
MIR18
Iberia CA
EI Mirador Cave
42.3
−3.5
2865–2575
F
H1t
‥
1.58
20.0±1.6
0±0.0
[7]
MIR19
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
M
H3
I
0.06
21.8±3.1
0±0.0
[7]
MIR2
Iberia CA
EI Mirador Cave
42.3
−3.5
2857–2496
F
K1b1a1
‥
0.98
22.6±1.7
56±8.9
[7]
MIR202-037-n105
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
M
K1a
I2a2a
5.73
19.9±1.7
0±0.0
MIR21
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
M
H3
I
0.11
24.7±2.4
55±17
[7]
MIR22
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
F
K1a2a
‥
2.79
22.6±1.7
62±10
[7]
MIR24
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
M
J2b1a3
G2a2b2b
0.06
20.0±3.0
0±0.0
[7]
MIR25
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2346
M
U3a1
I2a1a1
0.73
25.3±1.7
34±15
[7]
MIR5, MIR6
Iberia CA
EI Mirador Cave
42.3
−3.5
2900–2679
M
X2b
I2a2a2a
10.4
20.7±1.7
0±0.0
[7]
Cov: average coverage per SNP. HG%: inferred percentage of hunter-gatherer ancestry (mean ± standard error). ALD: inferred date of admixture (generations in the past; mean ± standard error; zero implies no date obtained). Ref: reference for published data; if blank, newly published sample in this study (asterisk denotes a published individual with new sequencing data added). Radiocarbon dates are in normal text, while dates estimated from archaeological context are in italics. Further information can be found in Supplementary Table 1.
A principal component analysis (PCA) of our samples shows that, as expected, all of the Neolithic individuals fall along a cline of admixture between FEF and WHG (Extended Data Fig. 1). Y-chromosome diversity also indicates contributions from ancestral Anatolian farmer and local hunter-gatherer populations, dominated by haplogroups G and I (the latter especially common in Iberia; Supplementary Information section 3). The European populations are consistent with a common origin in Anatolia (Supplementary Information section 4), reflected in the low differentiation among EN groups in the PCA. Over the course of the Neolithic, we observe a trend of increasing hunter-gatherer ancestry in each region, although at a slower rate in Hungary than in Germany and Spain, and with limited intra-population heterogeneity (Fig. 2A; Supplementary Information section 6). We also find that this hunter-gatherer ancestry is more similar to the eastern WHG individuals (KO1 and VIL) farther east and more similar to the western WHG individuals (LB1 and LOS) farther west (Fig. 2B). While this pattern does not demonstrate directly where mixture between hunter-gatherers and farmers took place, it suggests, given that European hunter-gatherers display a strong correlation between genetic and geographic structure (Fig. 1D), that hunter-gatherer ancestry in farmers was to a substantial extent derived from populations in relatively close proximity.
Extended Data Figure 1
First two principal components from PCA
We computed PCs for a set of 782 present-day western Eurasian individuals genotyped on the Affymetrix Human Origins array (background gray points) and then projected ancient individuals onto these axes. Shown is a closeup omitting the present-day Bedouin population.
Figure 2
Admixture parameters for test individuals and populations
a, Estimated individual hunter-gatherer ancestry versus sample date, with best-fitting regression lines for each region (excluding Blätterhöhle). Standard errors are around 2% for hunter-gatherer ancestry and 100 years for dates (Methods; Extended Data Tables 1, 2). b, Relative affinity of hunter-gatherer ancestry in Neolithic individuals, measured as f4(LB1+LOS, KO1+VIL; Anatolia, X) (positive, more similar to eastern WHG; negative, more similar to western WHG; standard errors ~5×10−4), with best-fitting regression line (|Z| > 3 for aggregate differences among the three regions). c, Population-level average sample ages and dates of admixture, plus or minus two standard errors. Colored fill indicates the inferred primary hunter-gatherer ancestry component, with darker shades corresponding to higher confidence (all admixed populations except LBK and Tisza significant at p < 0.05; see Extended Data Table 3 and Supplementary Information section 6). Dashed lines denote the approximate date of arrival of farming in each region.
To analyze admixed hunter-gatherer ancestry more formally, we modeled Neolithic farmers in an admixture graph framework. We started with a “scaffold” model (Extended Data Fig. 2) consisting of Neolithic Anatolians, the four reference WHG individuals, and two outgroups (Mbuti and Kostenki 14 [refs 20, 22]), with significant signals of admixture in LB1 and KO1 (Supplementary Information sections 5–6). We then added each Neolithic population to this model in turn, fitting them as a mixture of FEF and either one or two hunter-gatherer ancestry components. To check for robustness, we repeated our analyses using transversions or outgroup-ascertained SNPs only, with in-solution capture data for LOS, and with additional or alternative hunter-gatherers in the model (Extended Data Table 3; Supplementary Information section 6), and in all cases the results were qualitatively consistent. We find that almost all ancient groups from Hungary have ancestry significantly closest to one of the more eastern WHG individuals (KO1 or VIL); the samples from present-day Germany have the greatest affinity to LOS; and all three Iberian groups contain LB1-related ancestry (Fig. 2C; Extended Data Table 3). This pattern implies that admixture into European farmers occurred multiple times from local hunter-gatherer populations. Moreover, combining the proportions and sources of hunter-gatherer ancestry, populations from the three regions are distinguishable at all stages of the Neolithic. Thus, any further long-range migrations that may have occurred after the initial spread of agriculture in the studied regions (and before large incursions from the steppe) were not substantial enough to homogenize the ancestry of farming populations.
Extended Data Figure 2
Scaffold admixture graph used for modeling European Neolithic populations
Dotted lines denote admixture events. Neolithic Anatolians, LB1, and KO1 are modeled as admixed, with Basal Eurasian ancestry, deeper European hunter-gatherer ancestry, and FEF ancestry, respectively. European test populations are fit as a mixture of FEF and ancestry related to one or two of the four WHG individuals (here VIL-related as an example). See Supplementary Information section 6 for full details.
Extended Data Table 3
Admixture graph results for Neolithic populations
Main scaffold
Alternative scaffold
Population
HG ancestry
WHG affinity
HG ancestry
WHG affinity
Körös EN
0.0 ± 1.2%
0.0 ± 1.2%
Starčevo EN
2.3 ± 1.0%
KO1/VIL*
2.3 ± 1.0%
VIL
ALPc MN
8.8 ± 0.6%
KO1* + VIL
9.5 ± 0.6%
KO1* + VIL
LBKT MN
0.8 ± 0.9%
VIL*
0.5 ± 0.9%
VIL
Tisza LN
8.4 ± 1.3%
KO1/VIL
9.8 ± 1.3%
KO1/VIL + EHG
TDLN
8.2 ± 0.7%
KO1/VIL*
8.4 ± 0.7%
KO1*
Lasinja CA
10.7 ± 0.9%
KO1/VIL*
10.6 ± 0.9%
KO1/VIL*
Protoboleráz CA
12.7 ± 0.9%
KO1/VIL*
12.5 ± 0.9%
KO1/VIL
Baden CA
13.0 ± 0.7%
KO1/VIL*
13.4 ± 0.7%
KO1*
LBK EN
4.2 ± 0.6%
KO1 + LOS
5.0 ± 0.6%
KO1*
Germany MN
17.0 ± 1.1%
LOS*
18.3 ± 1.1%
LOS + KO1
Blätterhöhle MN
40.6 ± 1.5%
KO1/VI L* + LOS
42.6 ± 1.5%
KO1* + LOS
Iberia EN
10.0 ± 0.8%
LB1*
10.4 ± 0.8%
LB1*
Iberia MN
23.3 ± 1.1%
LB1* + LOS
24.8 ± 1.1%
LB1* + LOS
Iberia CA
26.5 ± 0.7%
LB1* + LOS/KO1/VIL*
27.5 ± 0.7%
LB1* + VIL*
Hunter-gatherer ancestry in Neolithic populations as inferred from admixture graph analyses. Shown are the inferred ancestry proportions for the best-fitting FEF+WHG model, along with the WHG individual(s) inferred to be related to the hunter-gatherer sources, with * denoting statistical significance (Methods). The two sets of results are for the primary scaffold model (Extended Data Fig. 2) and an alternative admixture graph scaffold including EHG (Supplementary Information section 6). Plus signs indicate two components, while slashes indicate single components with one of two or three possibilities.
Additional insights about population interactions can be gained by studying the dates of admixture events. We used ALDER (ref. 23) to estimate dates of admixture for Neolithic individuals based on the recombination-induced breakdown of contiguous blocks of FEF and WHG ancestry over time (Extended Data Tables 1, 2, 4; Extended Data Fig. 3). The ALDER algorithm is not able to accommodate large amounts of missing data, so we developed a strategy for running it with the relatively low coverage of ancient DNA (Supplementary Information section 7). The dates we obtain (Fig. 2D) are based on a model of a single wave of admixture, which means that if the true history for a population includes multiples waves or continuous admixture, we will obtain an intermediate value. In particular, for later populations, this history could include mixture with previously admixed groups (either farmers with substantially different hunter-gatherer ancestry proportions or hunter-gatherers with farmer ancestry).
Extended Data Table 4
Average dates of admixture for Neolithic populations
Population
Individual-based
Group-based
Average sample date (BCE)
Körös EN
5631 ± 31
Starčevo EN
4.5 ± 1.9
1.9 ± 0.9
5738 ± 35
ALPc MN
17.8 ± 2.0
16.4 ± 2.6
5180 ± 31
LBKT MN
30.3 ± 5.8
31.5 ± 10.9
5142 ± 93
Tisza LN
18.2 ± 6.6
12.6 ± 3.1
4750 ± 145
TDLN
20.9 ± 2.7
19.1 ± 3.8
4681 ± 32
Lasinja CA
29.3 ± 5.2
23.0 ± 4.1
4123 ± 59
Protoboleráz CA
44.3 ± 6.4
19.8 ± 5.4
3674 ± 35
Baden CA
27.6 ± 3.8
26.2 ± 6.9
3176 ± 49
LBK EN
14.9 ± 2.4
15.4 ± 3.6
5128 ± 38
Germany MN
26.2 ± 4.4
55.0 ± 41.2
3724 ± 46
Blätterhöhle MN
18.5 ± 4.6
23.1 ± 6.2
3414 ± 84
Iberia EN
19.4 ± 2.3
17.5 ± 5.9
5107 ± 20
Iberia MN
49.9 ± 7.7
40.0 ± 6.9
3749 ± 74
Iberia CA
49.6 ± 5.2
56.5 ± 7.9
2808 ± 27
Dates of admixture (in generations in the past) as inferred from ALDER through two different methods. On the left are the average individual-level dates used in our main analyses, and on the right are direct estimates for population groups. By default, for group-level estimates, we used all individuals that yielded a date in our standard ALDER procedure, but because of missing data, for some populations we used a subset of individuals (typically those with highest coverage): Starčevo (BAM17b, BAM4a, and LGCS1a; we note that in this case only BAM17b had an ALDER signal individually), ALPc (HAJE7a, HELI11a, MEMO2b, NE1, NE3, NE4, and TISO13a), Tisza (Gorzsa18 and PULE1.24), Baden (GEN12a, GEN13a, GEN15a, GEN17a, GEN22, and GEN55), LBK (HAL19, HAL2, HAL4, HAL5, LBK1992, and Stuttgart), and Iberia CA (LHUE11J.5, LHUE2010.11, LY.II.A.10.15066, LY.II.A.10.15069, MIR14, MIR2, and MIR22). For the group-level estimate for Iberia MN, we use a fitting start point of 0.8 cM instead of the program-inferred minimum of 0.6 because of a noticeably lower standard error. For our main analyses, we omit the outlier Protoboleráz individual GEN61, yielding an average date of 36.0 ± 5.2 generations, to help capture uncertainty due to the disagreement between the individual-level and group-level estimates shown here. Average sample dates (except for Körös) are based on the same weighting as the individual-level average dates of admixture for compatibility (Supplementary Information section 7).
Extended Data Figure 3
Examples of ALDER weighted LD decay curves
Weighted LD is shown as a function of genetic distance d, using Neolithic Anatolians and WHG as references, for four individuals: BAM17b (Starčevo EN), CB13 (Iberia EN), Bla8 (Blätterhöhle hunter-gatherer), and KO1. The results shown here use helper individuals M11–363 (Neolithic Anatolian), L11–322 (Neolithic Anatolian), BIC, and LB1, respectively, and have fitted dates (blue curves) of 3.8±1.2, 18.3±6.0, 13.1±2.7, and 21.6±8.8 generations (compared to final individual-level dates of 4.5±1.9, 17.5±3.5, 12.1±2.9, and 21.0±7.0 generations; see Supplementary Information section 7). Note different x-axis scales for the four individuals.
For our most complete time series, from Hungary, we infer admixture dates throughout the Neolithic that are on average mostly 18–30 generations old (500–840 years), indicating ongoing population transformation and admixture (Fig. 2D; Extended Data Table 4). This pattern is accompanied by a gradual increase in hunter-gatherer ancestry over time, although never reaching the levels observed in MN Germany or Iberia (Fig. 2A). While the majority of the EN samples from Hungary do not have significantly more hunter-gatherer ancestry than Neolithic Anatolians (Fig. 2A; Extended Data Tables 1, 2), one Starčevo individual, BAM17b, is inferred to have 7.8 ± 1.7% hunter-gatherer ancestry and a very recent ALDER date of 4.5 ± 1.9 generations (5865 ± 65 BCE; 1.9 ± 0.9 generations using a group-level estimate; Extended Data Table 4), consistent with having one or two hunter-gatherer ancestors in the past few generations. Additionally, one newly sampled Körös individual, TIDO2a, is similar to KO1 in having ~80% WHG and ~20% FEF ancestry and an ALDER date of 16.1 ± 3.8 generations, reinforcing the distinctive heterogeneity of the Tiszaszőlős site, the source for both TIDO2a and KO1. We also infer an average admixture date of 5675 ± 55 BCE for the ALPc MN, again suggesting that in Hungary, interaction between Anatolian migrants and local hunter-gatherers began in the Early Neolithic (cf. refs 14, 24–26). The greatest differences between Alföld and Transdanubia are observed in the MN, with substantially more hunter-gatherer ancestry in ALPc than LBKT (Fig. 2; Extended Data Table 3), and overall, we observe slight trends toward more hunter-gatherer ancestry to the north and east (Extended Data Fig. 4), as expected based on the greater archaeological evidence of hunter-gatherer settlement and interactions[24]. By the LN and CA, however, and especially in the Baden period (when the region became culturally unified[27]), our results are broadly similar over the two halves of present-day Hungary.
Extended Data Figure 4
Hunter-gatherer ancestry as a function of latitude and longitude for Neolithic individuals
a, b, EN/MN Hungary. c, d, LN/CA Hungary. e, f, Iberia. Protob., Protoboleráz.
From Germany, we analyzed a large sample of the EN LBK culture and 11 individuals from the MN period, four of them from the Blätterhöhle site, which has been shown to have featured a combination of farmer and hunter-gatherer occupation to a relatively late date[15]. The average date of admixture for LBK (5545 ± 65 BCE) is more recent than the dates for EN/MN populations from Hungary, and the total hunter-gatherer ancestry proportion in LBK (~4–5%) is intermediate between LBKT and ALPc. This ancestry is most closely related to a combination of KO1 and LOS, although the assignment of the hunter-gatherer source(s) is not statistically significant (Fig. 2B; Extended Data Table 3). These results are consistent with genetic and archaeological evidence for LBK origins from the early LBKT (ref. 26), followed by additional, Central European WHG admixture after about 5500 BCE. Our “Germany MN” grouping shows increased hunter-gatherer ancestry (~17%, most closely related to LOS) and a more recent average date of admixture, reflecting gene flow from hunter-gatherers after the LBK period. We successfully sequenced a total of 17 Blätterhöhle MN samples, many of them with distinct individual labels from ref. 15, although surprisingly, the genome-wide data indicated that these corresponded to only four unique individuals (Supplementary Information section 8), for which we merged libraries to increase coverage. In accordance with previous results[15], we find that the three farmer individuals (classified based on stable isotopes) harbored 40–50% hunter-gatherer ancestry, while Bla8, who showed signatures associated with a hunter-gatherer-fisher lifestyle, was closer genetically to hunter-gatherers but was also admixed, with ~27% ancestry from farmers. Our results thus provide evidence of asymmetric gene flow between farmers and hunter-gatherers at Blätterhöhle centered around the relatively late date of ~4000 BCE (ALDER dates of 10–25 generations).In Iberia, we again see widespread evidence of local hunter-gatherer admixture, with confidently inferred LB1-related ancestry in all three population groups (EN, MN, and CA). For Iberia EN, we infer an average admixture date of 5650 ± 65 BCE, which rises to 5860 ± 110 BCE when considering only the five oldest samples (of which the earliest, CB13 [ref. 18] has an individual estimate of 5890 ± 105 BCE). Given that farming is thought to have begun in Spain around 5500 BCE (ref. 28), these dates suggest the presence of at least a small proportion of hunter-gatherer ancestry in earlier Cardial Neolithic populations acquired along their migration route (although our admixture graph analysis only confidently detected an LB1-related component). The later Iberians have large proportions of hunter-gatherer ancestry, approximately 23% for MN (from the site of La Mina, in north-central Iberia) and 27% for CA, and also relatively old ALDER dates (approximately 50 generations, or 1400 years), indicating that most of the admixture occurred well before their respective sample dates. Both populations have evidence of ancestry related to a different WHG individual in addition to LB1 (Fig. 2C; Extended Data Table 3), suggesting a non-local source for at least some of the hunter-gatherer ancestry gained between the EN and MN.Synthesizing our time series data, we compared the observed ALDER dates and hunter-gatherer ancestry proportions of Neolithic populations to those estimated for simulated data under different temporal admixture scenarios (Fig. 3; Extended Data Fig. 5; Supplementary Information section 9). We assumed dates of 5900 BCE (Hungary) or 5500 BCE (Germany and Spain) for the onset of mixture. While none of the scenarios match the data perfectly, a good fit for Hungary is provided by a model (bottom solid green curve in both panels of Fig. 3) of an initial admixture pulse (approximately 1/4 of the total hunter-gatherer ancestry observed by the end of the time series) followed by continuous gene flow. By contrast, scenarios such as a single admixture pulse or continuous mixture decreasing by 5% or more per generation provide too much hunter-gatherer ancestry at early dates. Alföld and Transdanubia should be considered as separate series, but their parameters follow mostly similar trajectories, with the exception of the MN, where LBKT has a relatively old admixture date (albeit with large uncertainty) and ALPc a relatively high hunter-gatherer ancestry proportion (possibly influenced by the bias of sampling in favor of the middle and northern parts of the Alföld). Considering the other regions, even after normalizing for the different total hunter-gatherer ancestry proportions, we observe a high degree of local distinctiveness, for example in the older ALDER dates for Iberia MN/CA and the markedly higher hunter-gatherer ancestry in Blätterhöhle (Extended Data Fig. 5). We note that while the simulated data are generated under a model of gene flow from an unadmixed hunter-gatherer source population into a series of farmer populations in a single line of descent, observed admixture could also be influenced by flow in the other direction (from farmers to hunter-gatherers) or could reflect immigration of new farmer populations (either via their own previous hunter-gatherer admixture or new admixture between farming populations with different proportions of hunter-gatherer ancestry). Based on archaeological evidence, such a scenario is possible, for example, for the introduction of hunter-gatherer ancestry into TDLN from Southeastern European farmers via the dispersal of the northern Balkan Vinča or Sopot cultures to Transdanubia[14,29,30].
Figure 3
Hungary time series and simulated data
a, Dates of admixture. b, Hunter-gatherer ancestry proportions, normalized by the total in the most recent (rightmost) population. Symbols are as in Figs 1 and 2, here showing population-level averages plus or minus two standard errors. Yellow dashed lines represent continuous admixture simulations: from top to bottom, diminishing 5% per generation, diminishing 3%, diminishing 1%, and uniform. Green solid lines represent pulse-plus-continuous admixture simulations: from top to bottom, all hunter-gatherer ancestry in a pulse at time zero; 3/4 of final hunter-gatherer ancestry in an initial pulse, followed by uniform continuous gene flow; half in initial pulse and half continuous; and 1/4 in initial pulse.
Extended Data Figure 5
Germany and Iberia time series and simulated data
a, Dates of admixture. b, Hunter-gatherer ancestry proportions, normalized by the total in the most recent (rightmost) population. Symbols are as in Figs 1 and 2, here showing population-level averages plus or minus two standard errors. Yellow dashed lines represent continuous admixture simulations: from top to bottom, diminishing 5% per generation, diminishing 3%, diminishing 1%, and uniform. Green solid lines represent pulse-plus-continuous admixture simulations: from top to bottom, all hunter-gatherer ancestry in a pulse at time zero; 3/4 of final hunter-gatherer ancestry in an initial pulse, followed by uniform continuous gene flow; half in initial pulse and half continuous; and 1/4 in initial pulse.
Our results provide greatly increased detail in understanding population interactions and admixture during the European Neolithic. In each of our three study regions, the arrival of farmers prompted admixture with local hunter-gatherers, which unfolded over many centuries: almost all sampled populations have more hunter-gatherer ancestry and more recent dates of admixture than their local predecessors, suggesting recurrent changes in genetic composition and significant hunter-gatherer gene flow beyond initial contact. These transformations left distinct signatures in each region, implying that they resulted from a complex web of local interactions rather than a uniform demographic phenomenon. Our transect of Hungary, in particular, with representative samples from many archaeological cultures across the region and throughout the Neolithic and Chalcolithic, illustrates the power of dense ancient DNA time series. Future work with continually improving data sets and statistical models promises to yield many more insights about historical population transformations in space and time.
Methods
Experimental procedures
Prehistoric teeth and petrous bone samples from Hungary were taken under sterile conditions in the Hungarian Museums and anthropological collections. Samples other than Gorzsa were documented, cleaned, and ground into powder either in the Anthropological Department of the Johannes Gutenberg University of Mainz, during the course of the German Research Foundation project AL 287-10-1, or in Budapest, in the Laboratory of Archaeogenetics of the Institute of Archaeology, Research Centre for the Humanities, Hungarian Academy of Sciences, following published protocols[26]. DNA was extracted in Budapest using 0.08–0.11g powder via published methods[31], using High Pure Viral NA Large Volume Kit columns (Roche)[32,33]. DNA extractions were tested by PCR, amplifying the 16117–16233 bp fragment of the mitochondrial genome, and visualized on a 2% agarose gel. DNA libraries were prepared from clean and successful extraction batches using UDG-half and no-UDG treated methods[5,34]. We included milling (hydroxylapatite blanks to control for cleanness) and extraction negative controls in every batch. Bar-code adapter ligated libraries were amplified with TwistAmp Basic (Twist DX Ltd), purified with Agencourt AMPure XP (Beckman Coulter), and checked on 3% agarose gel[5]. Library concentration was measured on a Qubit 2.0 fluorometer. Promising libraries after initial quality control analysis were shipped to Harvard Medical School, where further processing took place. All other samples were prepared similarly in dedicated clean rooms at Harvard Medical School and the University of Adelaide in accordance with published methods[5,7,33]. For samples LHUE2010.11 (one library) and MIR202-037-n105, we used magnetic bead cleanups instead of MinElute column cleanups between enzymatic reactions with magnetic bead cleanups and SPRI bead cleanup instead of the final PCR cleanup[35,36].We initially screened the libraries via in-solution hybridization to a set of probes targeting mitochondrial DNA (mtDNA)[37] plus roughly 3000 nuclear SNP targets, using a protocol described previously[5,33] with amplified baits synthesized by CustomArray, Inc. Libraries with good screening results—limited evidence of contamination, reasonable damage profiles, and substantial coverage on targeted segments—were enriched for a genome-wide set of ~1.2 million SNPs[7,33] and sequenced to greater depth. Raw sequencing data were processed by trimming bar-codes and adapters, merging read pairs with at least 15 base pairs of overlapping sequence, and mapping to the human reference genome (version hg19). Reads were filtered for mapping and base quality, duplicate molecules were removed, and two terminal bases were clipped to eliminate damage (five for UDG-minus libraries)[5]. All libraries had a rate of at least 4.8% C-to-T substitutions in the final base of screening sequencing reads (Supplementary Table 1), consistent with damage patterns expected for authentic ancient DNA (refs 34, 38). Pseudo-haploid genotypes at each SNP were called by choosing one allele at random from among mapped reads. Sex determinations for each individual were made by manually examining the factions of reads mapping to the X and Y chromosomes and imposing thresholds for males and females (with any indeterminate samples labeled as unknown).Mitochondrial DNA sequences were reassembled in Geneious R10 to rCRS (ref. 39) and RSRS (ref. 40), and SNPs with at least 3× coverage and a minimum variant frequency of 0.7 were called. The assembly and the resulting list of SNPs were double-checked against phylotree.org (mtDNA tree Build 17; 18 Feb 2016). Haplotype calls are given in Extended Data Tables 1 and 2 and Supplementary Table 2. On the Y chromosome, 15,100 SNPs were targeted and sequenced, and the detected derived and ancestral alleles were compared to the ISOGG Y-tree (www.isogg.org) version 12.34, updated on 5th February 2017. Haplogroup definitions are detailed in Supplementary Information section 3.We merged libraries from the same individual (for those with more than one) and then combined our new samples with genome-wide data from the literature (ancient individuals as described and as listed in Extended Data Tables 1 and 2 and present-day individuals from the SGDP [ref. 41]) using all autosomal SNPs (~1.15 million) from our target set. For two replications of our admixture graph analyses, we restricted either to the subset of transversions (~280K SNPs) or to the subset from panels 4 and 5 of the Affymetrix Human Origins array (ascertained as heterozygous in a San or Yoruba individual; ~260K SNPs). For PCA (Extended Data Fig. 1), we merged with a large set of present-day samples[33] and used all autosomal Human Origins SNPs (~593K).To test for possible contamination, we used contamMix (ref. 42) and ANGSD (ref. 43) to estimate rates of apparent heterozygosity in haploid genome regions (mtDNA and the X chromosome in males, respectively). Any samples with > 5% mtDNA mismatching or > 2% X contamination were excluded from further analyses, with the exception of Bla5 (Supplementary Information section 8). We also removed samples identified as clear outliers in PCA or with significant population genetic differences between all sequencing data and genotypes called only from sequences displaying ancient DNA damage signatures. A total of 19 samples were excluded based on one of these criteria. For individual-level f-statistic analyses (Fig. 2A–B), we restricted to samples with a maximum level of uncertainty, defined as a standard error of at most 7×10−4 for the statistic f4(Mbuti, WHG; Anatolia, X). This threshold (corresponding to an average coverage of approximately 0.05, or ~60K SNPs hit at least once) was met by 89 of the 112 samples passing QC (and 49 of the 50 samples from the literature). We did not impose such a threshold for ALDER analyses, but because low coverage results in a weaker signal, only one of the 23 high-uncertainty individuals in our primary data set provided an ALDER date (as compared to 89 of the 130 low-uncertainty individuals).
Population assignments
In most cases, population groupings were used that correspond to archaeological culture assignments based on chronology, geography, and material culture traits. Occasionally, we merged populations that appeared similar genetically in order to increase power: we pooled samples from all phases and groups of the eastern Hungarian MN into a single ALPc population; merged six Sopot with eight Lengyel individuals for the western Hungarian TDLN; combined one Hunyadihalom (Middle CA from the Danube-Tisza interfluve in central Hungary) with Lasinja; pooled four LBK samples from Stuttgart with the majority from farther to the northeast (primarily Halberstadt); and merged several cultures of the German MN into a single group. Other populations vary in their degrees of date and site heterogeneity, with Iberia MN the most homogeneous and Iberia EN and CA among the least (Extended Data Tables 1, 2; Supplementary Table 1). For our main analyses, we excluded the Vinča and Tiszapolgár population groups because they lacked sufficient high-quality data.We note that the designations EN, MN, LN, and CA have different meanings in different areas. For our study regions, each term generally refers to an earlier period in Hungary than in Germany and Spain (for example, ALPc and LBKT MN in Hungary are roughly contemporaneous with LBK and Iberia EN). In order to maintain agreement with the archaeological literature, we use the established definitions, with the appropriate word of caution that they should be treated separately in each region.
Sample dates
We report 52 newly obtained accelerator mass spectrometry (AMS) radiocarbon dates for Neolithic individuals (45 direct, 7 indirect), focusing on representative high-quality samples from each site and any samples with chronological uncertainty. These are combined with 58 radiocarbon dates from the literature[4,5,7,17,18,26,29,30,44,45]. We report the 95.4% calibrated confidence intervals (CI) from OxCal (ref. 46) version 4.2 with the IntCal13 calibration curve[47] in Extended Data Tables 1 and 2. For use in ALDER analyses (Supplementary Information section 7), we use the mean and standard deviation of the calibrated date distributions; while the distributions are non-normal, we find that on average the mean plus or minus two standard deviations contains more than 95.4% of the probability density. For samples without direct radiocarbon dates but with dates from other samples or materials at the same site, we form a conservative 95.4% CI by taking the minimum and maximum bounds of any of the calibrated CIs from the site. Finally, for the remaining samples, we use plausible date ranges based on archaeological context; we assume independence across individuals but as a result take a conservative approach and treat the assigned range as ± one standard error (e.g., an estimated range of 4800–4500 BCE becomes 4650 ± 150 BCE).
Population genetic analyses
We performed PCA by computing components for present-day populations and then projecting ancient individuals using the “lsqproject” and “shrinkmode” options in smartpca (ref. 48). Admixture graphs and f-statistics were implemented through ADMIXTOOLS (ref. 49). To obtain calendar dates of admixture, we combine the ALDER results (in generations in the past) with the ages of the Neolithic individuals, assuming an average generation time of 28 years[50,51]. All analytical procedures are described in full detail in Supplementary Information sections 4–9.
Data availability
The aligned sequences are available through the European Nucleotide Archive under accession number PRJEB22629. Genotype datasets used in analysis are available at https://reich.hms.harvard.edu/datasets.
First two principal components from PCA
We computed PCs for a set of 782 present-day western Eurasian individuals genotyped on the Affymetrix Human Origins array (background gray points) and then projected ancient individuals onto these axes. Shown is a closeup omitting the present-day Bedouin population.
Scaffold admixture graph used for modeling European Neolithic populations
Dotted lines denote admixture events. Neolithic Anatolians, LB1, and KO1 are modeled as admixed, with Basal Eurasian ancestry, deeper European hunter-gatherer ancestry, and FEF ancestry, respectively. European test populations are fit as a mixture of FEF and ancestry related to one or two of the four WHG individuals (here VIL-related as an example). See Supplementary Information section 6 for full details.
Examples of ALDER weighted LD decay curves
Weighted LD is shown as a function of genetic distance d, using Neolithic Anatolians and WHG as references, for four individuals: BAM17b (Starčevo EN), CB13 (Iberia EN), Bla8 (Blätterhöhle hunter-gatherer), and KO1. The results shown here use helper individuals M11–363 (Neolithic Anatolian), L11–322 (Neolithic Anatolian), BIC, and LB1, respectively, and have fitted dates (blue curves) of 3.8±1.2, 18.3±6.0, 13.1±2.7, and 21.6±8.8 generations (compared to final individual-level dates of 4.5±1.9, 17.5±3.5, 12.1±2.9, and 21.0±7.0 generations; see Supplementary Information section 7). Note different x-axis scales for the four individuals.
Hunter-gatherer ancestry as a function of latitude and longitude for Neolithic individuals
a, b, EN/MN Hungary. c, d, LN/CA Hungary. e, f, Iberia. Protob., Protoboleráz.
Germany and Iberia time series and simulated data
a, Dates of admixture. b, Hunter-gatherer ancestry proportions, normalized by the total in the most recent (rightmost) population. Symbols are as in Figs 1 and 2, here showing population-level averages plus or minus two standard errors. Yellow dashed lines represent continuous admixture simulations: from top to bottom, diminishing 5% per generation, diminishing 3%, diminishing 1%, and uniform. Green solid lines represent pulse-plus-continuous admixture simulations: from top to bottom, all hunter-gatherer ancestry in a pulse at time zero; 3/4 of final hunter-gatherer ancestry in an initial pulse, followed by uniform continuous gene flow; half in initial pulse and half continuous; and 1/4 in initial pulse.Information for Neolithic individuals from Hungary.Cov: average coverage per SNP. HG%: inferred percentage of hunter-gatherer ancestry (mean ± standard error). ALD inferred date of admixture (generations in the past; mean ± standard error; zero implies no date obtained). Ref: reference for published data; if blank, newly published sample in this study (asterisk denotes a published individual with new sequencing data added). Radiocarbon dates are in normal text, while dates estimated from archaeological context are in italics. Further information can be found in Supplementary Table 1.Information for Neolithic individuals from Germany and Spain.Cov: average coverage per SNP. HG%: inferred percentage of hunter-gatherer ancestry (mean ± standard error). ALD: inferred date of admixture (generations in the past; mean ± standard error; zero implies no date obtained). Ref: reference for published data; if blank, newly published sample in this study (asterisk denotes a published individual with new sequencing data added). Radiocarbon dates are in normal text, while dates estimated from archaeological context are in italics. Further information can be found in Supplementary Table 1.Admixture graph results for Neolithic populationsHunter-gatherer ancestry in Neolithic populations as inferred from admixture graph analyses. Shown are the inferred ancestry proportions for the best-fitting FEF+WHG model, along with the WHG individual(s) inferred to be related to the hunter-gatherer sources, with * denoting statistical significance (Methods). The two sets of results are for the primary scaffold model (Extended Data Fig. 2) and an alternative admixture graph scaffold including EHG (Supplementary Information section 6). Plus signs indicate two components, while slashes indicate single components with one of two or three possibilities.Average dates of admixture for Neolithic populationsDates of admixture (in generations in the past) as inferred from ALDER through two different methods. On the left are the average individual-level dates used in our main analyses, and on the right are direct estimates for population groups. By default, for group-level estimates, we used all individuals that yielded a date in our standard ALDER procedure, but because of missing data, for some populations we used a subset of individuals (typically those with highest coverage): Starčevo (BAM17b, BAM4a, and LGCS1a; we note that in this case only BAM17b had an ALDER signal individually), ALPc (HAJE7a, HELI11a, MEMO2b, NE1, NE3, NE4, and TISO13a), Tisza (Gorzsa18 and PULE1.24), Baden (GEN12a, GEN13a, GEN15a, GEN17a, GEN22, and GEN55), LBK (HAL19, HAL2, HAL4, HAL5, LBK1992, and Stuttgart), and Iberia CA (LHUE11J.5, LHUE2010.11, LY.II.A.10.15066, LY.II.A.10.15069, MIR14, MIR2, and MIR22). For the group-level estimate for Iberia MN, we use a fitting start point of 0.8 cM instead of the program-inferred minimum of 0.6 because of a noticeably lower standard error. For our main analyses, we omit the outlier Protoboleráz individual GEN61, yielding an average date of 36.0 ± 5.2 generations, to help capture uncertainty due to the disagreement between the individual-level and group-level estimates shown here. Average sample dates (except for Körös) are based on the same weighting as the individual-level average dates of admixture for compatibility (Supplementary Information section 7).
Authors: Doron M Behar; Mannis van Oven; Saharon Rosset; Mait Metspalu; Eva-Liis Loogväli; Nuno M Silva; Toomas Kivisild; Antonio Torroni; Richard Villems Journal: Am J Hum Genet Date: 2012-04-06 Impact factor: 11.025
Authors: Guido Brandt; Wolfgang Haak; Christina J Adler; Christina Roth; Anna Szécsényi-Nagy; Sarah Karimnia; Sabine Möller-Rieker; Harald Meller; Robert Ganslmeier; Susanne Friederich; Veit Dresely; Nicole Nicklisch; Joseph K Pickrell; Frank Sirocko; David Reich; Alan Cooper; Kurt W Alt Journal: Science Date: 2013-10-11 Impact factor: 47.728
Authors: Zuzana Hofmanová; Susanne Kreutzer; Garrett Hellenthal; Christian Sell; Yoan Diekmann; David Díez-Del-Molino; Lucy van Dorp; Saioa López; Athanasios Kousathanas; Vivian Link; Karola Kirsanow; Lara M Cassidy; Rui Martiniano; Melanie Strobel; Amelie Scheu; Kostas Kotsakis; Paul Halstead; Sevi Triantaphyllou; Nina Kyparissi-Apostolika; Dushka Urem-Kotsou; Christina Ziota; Fotini Adaktylou; Shyamalika Gopalan; Dean M Bobo; Laura Winkelbach; Jens Blöcher; Martina Unterländer; Christoph Leuenberger; Çiler Çilingiroğlu; Barbara Horejs; Fokke Gerritsen; Stephen J Shennan; Daniel G Bradley; Mathias Currat; Krishna R Veeramah; Daniel Wegmann; Mark G Thomas; Christina Papageorgopoulou; Joachim Burger Journal: Proc Natl Acad Sci U S A Date: 2016-06-06 Impact factor: 11.205
Authors: Wolfgang Haak; Oleg Balanovsky; Juan J Sanchez; Sergey Koshel; Valery Zaporozhchenko; Christina J Adler; Clio S I Der Sarkissian; Guido Brandt; Carolin Schwarz; Nicole Nicklisch; Veit Dresely; Barbara Fritsch; Elena Balanovska; Richard Villems; Harald Meller; Kurt W Alt; Alan Cooper Journal: PLoS Biol Date: 2010-11-09 Impact factor: 8.029
Authors: Iosif Lazaridis; Nick Patterson; Alissa Mittnik; Gabriel Renaud; Swapan Mallick; Karola Kirsanow; Peter H Sudmant; Joshua G Schraiber; Sergi Castellano; Mark Lipson; Bonnie Berger; Christos Economou; Ruth Bollongino; Qiaomei Fu; Kirsten I Bos; Susanne Nordenfelt; Heng Li; Cesare de Filippo; Kay Prüfer; Susanna Sawyer; Cosimo Posth; Wolfgang Haak; Fredrik Hallgren; Elin Fornander; Nadin Rohland; Dominique Delsate; Michael Francken; Jean-Michel Guinet; Joachim Wahl; George Ayodo; Hamza A Babiker; Graciela Bailliet; Elena Balanovska; Oleg Balanovsky; Ramiro Barrantes; Gabriel Bedoya; Haim Ben-Ami; Judit Bene; Fouad Berrada; Claudio M Bravi; Francesca Brisighelli; George B J Busby; Francesco Cali; Mikhail Churnosov; David E C Cole; Daniel Corach; Larissa Damba; George van Driem; Stanislav Dryomov; Jean-Michel Dugoujon; Sardana A Fedorova; Irene Gallego Romero; Marina Gubina; Michael Hammer; Brenna M Henn; Tor Hervig; Ugur Hodoglugil; Aashish R Jha; Sena Karachanak-Yankova; Rita Khusainova; Elza Khusnutdinova; Rick Kittles; Toomas Kivisild; William Klitz; Vaidutis Kučinskas; Alena Kushniarevich; Leila Laredj; Sergey Litvinov; Theologos Loukidis; Robert W Mahley; Béla Melegh; Ene Metspalu; Julio Molina; Joanna Mountain; Klemetti Näkkäläjärvi; Desislava Nesheva; Thomas Nyambo; Ludmila Osipova; Jüri Parik; Fedor Platonov; Olga Posukh; Valentino Romano; Francisco Rothhammer; Igor Rudan; Ruslan Ruizbakiev; Hovhannes Sahakyan; Antti Sajantila; Antonio Salas; Elena B Starikovskaya; Ayele Tarekegn; Draga Toncheva; Shahlo Turdikulova; Ingrida Uktveryte; Olga Utevska; René Vasquez; Mercedes Villena; Mikhail Voevoda; Cheryl A Winkler; Levon Yepiskoposyan; Pierre Zalloua; Tatijana Zemunik; Alan Cooper; Cristian Capelli; Mark G Thomas; Andres Ruiz-Linares; Sarah A Tishkoff; Lalji Singh; Kumarasamy Thangaraj; Richard Villems; David Comas; Rem Sukernik; Mait Metspalu; Matthias Meyer; Evan E Eichler; Joachim Burger; Montgomery Slatkin; Svante Pääbo; Janet Kelso; David Reich; Johannes Krause Journal: Nature Date: 2014-09-18 Impact factor: 49.962
Authors: Iain Mathieson; Iosif Lazaridis; Nadin Rohland; Swapan Mallick; Nick Patterson; Songül Alpaslan Roodenberg; Eadaoin Harney; Kristin Stewardson; Daniel Fernandes; Mario Novak; Kendra Sirak; Cristina Gamba; Eppie R Jones; Bastien Llamas; Stanislav Dryomov; Joseph Pickrell; Juan Luís Arsuaga; José María Bermúdez de Castro; Eudald Carbonell; Fokke Gerritsen; Aleksandr Khokhlov; Pavel Kuznetsov; Marina Lozano; Harald Meller; Oleg Mochalov; Vyacheslav Moiseyev; Manuel A Rojo Guerra; Jacob Roodenberg; Josep Maria Vergès; Johannes Krause; Alan Cooper; Kurt W Alt; Dorcas Brown; David Anthony; Carles Lalueza-Fox; Wolfgang Haak; Ron Pinhasi; David Reich Journal: Nature Date: 2015-11-23 Impact factor: 49.962
Authors: Lia Betti; Robert M Beyer; Eppie R Jones; Anders Eriksson; Francesca Tassi; Veronika Siska; Michela Leonardi; Pierpaolo Maisano Delser; Lily K Bentley; Philip R Nigst; Jay T Stock; Ron Pinhasi; Andrea Manica Journal: Nat Hum Behav Date: 2020-07-06
Authors: Mary E Prendergast; Mark Lipson; Elizabeth A Sawchuk; Iñigo Olalde; Christine A Ogola; Nadin Rohland; Kendra A Sirak; Nicole Adamski; Rebecca Bernardos; Nasreen Broomandkhoshbacht; Kimberly Callan; Brendan J Culleton; Laurie Eccles; Thomas K Harper; Ann Marie Lawson; Matthew Mah; Jonas Oppenheimer; Kristin Stewardson; Fatma Zalzala; Stanley H Ambrose; George Ayodo; Henry Louis Gates; Agness O Gidna; Maggie Katongo; Amandus Kwekason; Audax Z P Mabulla; George S Mudenda; Emmanuel K Ndiema; Charles Nelson; Peter Robertshaw; Douglas J Kennett; Fredrick K Manthi; David Reich Journal: Science Date: 2019-05-30 Impact factor: 47.728
Authors: Vagheesh M Narasimhan; Nick Patterson; Priya Moorjani; Nadin Rohland; Rebecca Bernardos; Swapan Mallick; Iosif Lazaridis; Nathan Nakatsuka; Iñigo Olalde; Mark Lipson; Alexander M Kim; Luca M Olivieri; Alfredo Coppa; Massimo Vidale; James Mallory; Vyacheslav Moiseyev; Egor Kitov; Janet Monge; Nicole Adamski; Neel Alex; Nasreen Broomandkhoshbacht; Francesca Candilio; Kimberly Callan; Olivia Cheronet; Brendan J Culleton; Matthew Ferry; Daniel Fernandes; Suzanne Freilich; Beatriz Gamarra; Daniel Gaudio; Mateja Hajdinjak; Éadaoin Harney; Thomas K Harper; Denise Keating; Ann Marie Lawson; Matthew Mah; Kirsten Mandl; Megan Michel; Mario Novak; Jonas Oppenheimer; Niraj Rai; Kendra Sirak; Viviane Slon; Kristin Stewardson; Fatma Zalzala; Zhao Zhang; Gaziz Akhatov; Anatoly N Bagashev; Alessandra Bagnera; Bauryzhan Baitanayev; Julio Bendezu-Sarmiento; Arman A Bissembaev; Gian Luca Bonora; Temirlan T Chargynov; Tatiana Chikisheva; Petr K Dashkovskiy; Anatoly Derevianko; Miroslav Dobeš; Katerina Douka; Nadezhda Dubova; Meiram N Duisengali; Dmitry Enshin; Andrey Epimakhov; Alexey V Fribus; Dorian Fuller; Alexander Goryachev; Andrey Gromov; Sergey P Grushin; Bryan Hanks; Margaret Judd; Erlan Kazizov; Aleksander Khokhlov; Aleksander P Krygin; Elena Kupriyanova; Pavel Kuznetsov; Donata Luiselli; Farhod Maksudov; Aslan M Mamedov; Talgat B Mamirov; Christopher Meiklejohn; Deborah C Merrett; Roberto Micheli; Oleg Mochalov; Samariddin Mustafokulov; Ayushi Nayak; Davide Pettener; Richard Potts; Dmitry Razhev; Marina Rykun; Stefania Sarno; Tatyana M Savenkova; Kulyan Sikhymbaeva; Sergey M Slepchenko; Oroz A Soltobaev; Nadezhda Stepanova; Svetlana Svyatko; Kubatbek Tabaldiev; Maria Teschler-Nicola; Alexey A Tishkin; Vitaly V Tkachev; Sergey Vasilyev; Petr Velemínský; Dmitriy Voyakin; Antonina Yermolayeva; Muhammad Zahir; Valery S Zubkov; Alisa Zubova; Vasant S Shinde; Carles Lalueza-Fox; Matthias Meyer; David Anthony; Nicole Boivin; Kumarasamy Thangaraj; Douglas J Kennett; Michael Frachetti; Ron Pinhasi; David Reich Journal: Science Date: 2019-09-06 Impact factor: 47.728
Authors: Mark Lipson; Pontus Skoglund; Matthew Spriggs; Frederique Valentin; Stuart Bedford; Richard Shing; Hallie Buckley; Iarawai Phillip; Graeme K Ward; Swapan Mallick; Nadin Rohland; Nasreen Broomandkhoshbacht; Olivia Cheronet; Matthew Ferry; Thomas K Harper; Megan Michel; Jonas Oppenheimer; Kendra Sirak; Kristin Stewardson; Kathryn Auckland; Adrian V S Hill; Kathryn Maitland; Stephen J Oppenheimer; Tom Parks; Kathryn Robson; Thomas N Williams; Douglas J Kennett; Alexander J Mentzer; Ron Pinhasi; David Reich Journal: Curr Biol Date: 2018-02-28 Impact factor: 10.834