πŸ†• Advanced Report, now with Y-DNA, mtDNA & ROH analysis Discover your paternal & maternal haplogroups, shown only when AI prediction confidence is high enough to be reliable. Plus ROH endogamy insights, ancient sample matches, all interpreted by Claude AI. Raw DNA file required for these new analyses (not available with G25 coordinates).
Discover Now
🍽️ DNA-Based Nutrition Report: Discover Which Foods Fuel Your Body Upload your 23andMe, AncestryDNA or MyHeritage file and discover exactly which foods fuel your body, based on your personal genetic blueprint.
Try our Free Test

Sample Information

I17913
I17913
Serbia_BA_Maros
1950 BC
F
Serbia
-
Ostojicevo (North Banat District, Čoka Municipality, Ostojicevo)

Haplogroups

Not determined
H4a1a
Maros culture – early Thracian
2100-1800 BCE

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
58.1%
Steppe
23.8%
WHG
8.2%
CHG/Iran N
7.1%
EHG
2.7%
Natufian
0.1%

Publication

LazaridisAlpaslanRoodenbergScience2022; LazaridisReichScience2022

G25 Coordinates

Download the G25 scaled coordinates for this sample to use in calculators like GEDmatch, Vahaduo, or our own calculators.

Download G25 (.txt)

G25 Ancestry Model Cached

Poor Β· Distance: 0.0408

Model based on Davidski's G25 standard reference populations (nMonte-style optimization).

TUR_Barcin_N 46.1%
Yamnaya_RUS_Samara 31.1%
TUR_Tepecik_Ciftlik_N 14.0%
WHG 8.8%

Ancient Population Distances

Closest ancient reference populations
HUN_La_Tene
0.0296
HRV_EIA
0.0305
SRB_Mokrin_EBA_Maros_oAegean
0.0305
CZE_LBA_Knoviz_o3
0.0306
HUN_LBA_EIA
0.0320
AUT_IA_La_Tene
0.0331
ITA_Etruscan
0.0332
ITA_Proto-Villanovan
0.0347
HRV_MBA
0.0354
HUN_IA_Syrmian_SremGroup
0.0356
HRV_IA
0.0359
GRC_Logkas_MBA
0.0364
HUN_EIA
0.0366
HRV_LIA_La_Tene
0.0373
DEU_MA_Alemannic_o1
0.0373

Modern Population Genetic Proximity

Heatmap based on G25 Euclidean distance to 3,000+ modern populations

Archaeological Site Location

45.8881, 20.1667

We use cookies to enhance your experience. By continuing to visit this site you agree to our use of cookies. Learn more