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

I10372
I10372
Italy_Sicily_LBA
1248 BC
F
Italy
-
Marcita (Sicily, Trapani, Castelvetrano)

Haplogroups

Not determined
K1a3a
1377-1130 calBCE (3005±20 BP, PSUAMS-5891)

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
81.8%
Steppe
6.5%
WHG
5.2%
CHG/Iran N
4.9%
Natufian
1.1%
EHG
0.5%

Publication

FernandesNatureEcologyEvolution2020; FernandesNatEcolEvol2020; FernandesReichNatEcolEvol2020

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: 0.0430

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

TUR_Barcin_N 62.8%
TUR_Tepecik_Ciftlik_N 24.5%
Yamnaya_RUS_Samara 7.9%
WHG 4.8%

Ancient Population Distances

Closest ancient reference populations
ITA_Sicily_LBA
0.0244
BGR_Middle_C
0.0346
BGR_C
0.0381
ITA_Sicily_MBA
0.0400
SRB_Starcevo_N
0.0416
HUN_ALPc_Szatmar_MN
0.0421
BGR_Varna_C
0.0447
FRA_MN_Lingolsheim
0.0447
ROU_C
0.0455
HUN_Protoboleraz_LCA
0.0456
HUN_LN_EarlyC_Lengyel
0.0457
BGR_Late_C
0.0458
ITA_Olmo_di_Nogara_MBA
0.0462
HUN_ALPc_Tiszadob_MN
0.0464
HUN_Tisza_LN
0.0465

Modern Population Genetic Proximity

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

Archaeological Site Location

37.6800, 12.7890

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