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

HRR1513623
HRR1513623
China_Xinjiang_Hami_Lafuqueke_TangDynasty_Gaochang_Uyghur
750 AD
-
China
-
-

Haplogroups

Not determined
Not determined
cca

Ancestry Components

Estimated ancestral proportions from ancient reference populations
East Asian
92.0%
ANF
1.8%
Steppe
1.8%
WHG
1.4%
CHG/Iran N
1.2%
Iberomaurusian
1.2%
EHG
0.5%

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

Very Poor Β· Distance: 0.0981

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

Nganassan 46.9%
Han 42.9%
Kura-Araxes_ARM_Kaps 2.9%
BRA_LapaDoSanto 2.6%
MAR_Taforalt 2.4%
WHG 1.2%
IRN_Ganj_Dareh_N 0.9%
Dinka 0.1%

Ancient Population Distances

Closest ancient reference populations
KAZ_Nomad_HP
0.0287
KAZ_Tasmola_IA_o2
0.0304
KAZ_Kayalyk_MA
0.0333
MNG_Xianbei_IA
0.0358
KAZ_Pazyryk_IA_o
0.0358
HUN_Avar_Early_Danube-Tisza
0.0364
MNG_EIA_3
0.0399
KAZ_Hun-Sarmatian
0.0401
KAZ_Korgantas_IA_o2
0.0418
HUN_Avar_Middle_Danube-Tisza
0.0441
RUS_Late_Xiongnu
0.0447
CHN_Tuwaxingcun_IA
0.0453
KAZ_Golden_Horde_Asian
0.0464
RUS_Shamanka_N
0.0475
RUS_Lokomotiv_N
0.0482

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