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

ADELE034
ADELE034
Greece_Crete_WWII_ExecutedCitizen
1941 AD
-
Greece
-
-

Haplogroups

Not determined
Not determined

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
51.3%
Steppe
18.8%
CHG/Iran N
15.9%
Natufian
10.4%
Sub-Saharan
1.2%
WHG
1.1%
EHG
0.9%
ANE
0.2%
East Asian
0.2%

Publication

https://www.fsigenetics.com/article/S1872-4973(24)00054-1/abstract

View Study

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

Good Β· Distance: 0.0189

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

TUR_Tepecik_Ciftlik_N 23.8%
Yamnaya_RUS_Samara 22.4%
TUR_Barcin_N 21.3%
Levant_PPNB 16.7%
Kura-Araxes_ARM_Kaps 10.0%
IRN_Ganj_Dareh_N 5.0%
Yoruba 0.8%

Ancient Population Distances

Closest ancient reference populations
IND_Roopkund_B
0.0218
ITA_Rome_Imperial
0.0247
ITA_Venosa_EMA
0.0249
ITA_Collegno_MA_o1
0.0274
DEU_MA_Erfurt1
0.0285
DEU_MA_Erfurt3
0.0297
ITA_Ordona_MA
0.0358
ITA_Tivoli_Renaissance
0.0374
VK2020_ITA_Foggia_MA
0.0378
ITA_Marsiliana_Imperial
0.0390
ITA_Prenestini_tribe_IA_o
0.0421
ITA_Rome_Late_Antiquity
0.0427
Levant_LBN_MA_o4
0.0437
ITA_Tarquinia_EMA
0.0437
ITA_Chiusi_EMA
0.0440

Modern Population Genetic Proximity

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

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