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

PER22
PER22
Romania_Pericei_Bathory
1575 AD
F
Romania
-
-

Haplogroups

Not determined
U4c1
AD_1575

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
42.5%
Steppe
30.5%
WHG
9.7%
CHG/Iran N
6.6%
EHG
4.9%
Natufian
2.0%
East Asian
2.0%
Iberomaurusian
0.8%
Native American
0.6%
AASI
0.4%

Publication

Unknown 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

Average Β· Distance: 0.0301

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

Yamnaya_RUS_Samara 44.8%
TUR_Barcin_N 33.5%
WHG 10.7%
TUR_Tepecik_Ciftlik_N 8.8%
MAR_Taforalt 1.1%
Han 1.0%
Nganassan 0.2%

Ancient Population Distances

Closest ancient reference populations
DEU_MA_ACD_Baiuvaric
0.0261
HUN_Sarmatian_Late_Danube-Tisza
0.0290
Bell_Beaker_HUN_EBA
0.0298
HUN_Sarmatian_Late_Transtisza
0.0307
HUN_IA_La_Tene_o
0.0310
HRV_Pop_RomanP
0.0315
UKR_Chernyakhiv_Shyshaky
0.0336
HUN_MA_Szolad
0.0342
Scythian_HUN
0.0353
HUN_MA
0.0355
Iberia_Northeast_c.6CE_PL
0.0356
SVK_IA_Vekerzug
0.0365
Bell_Beaker_Bavaria
0.0377
HUN_Sarmatian_Early_Transtisza
0.0380
ITA_Rome_Renaissance
0.0390

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