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

CSK073
CSK073
Austria_ViennaBasin_Csokorgasse_Avar
750 AD
F
Austria
-
Csokorgasse (Vienna); Vienna

Haplogroups

Not determined
H3h6
600-800 CE

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
45.4%
Steppe
37.0%
WHG
7.2%
Natufian
4.0%
EHG
4.0%
East Asian
1.6%
CHG/Iran N
0.8%

Publication

Moedling2024; WangHofmanováNature2025

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: 0.0429

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

Yamnaya_RUS_Samara 42.3%
TUR_Barcin_N 33.0%
TUR_Tepecik_Ciftlik_N 15.0%
WHG 8.8%
Nganassan 0.9%

Ancient Population Distances

Closest ancient reference populations
HUN_Sarmatian_Late_Transtisza
0.0284
SVK_IA_Vekerzug
0.0311
HRV_MBA_LBA
0.0333
DEU_MA_ACD_Baiuvaric
0.0338
HUN_EIA_Prescythian_Mezocsat
0.0354
HUN_Sarmatian_Early_Transtisza
0.0360
HUN_MA_Szolad
0.0374
HUN_Sarmatian_Late_Danube-Tisza
0.0378
ITA_Collegno_MA
0.0380
ITA_Rome_Renaissance
0.0394
DEU_Singen_EIA
0.0407
ITA_Etruscan_Campiglia_CEU_o
0.0408
Iberia_Northeast_c.6CE_PL
0.0414
Scythian_HUN
0.0417
HUN_Avar_Late_Visonta
0.0418

Modern Population Genetic Proximity

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

Archaeological Site Location

48.1521, 16.4666

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