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

MGS178
MGS178
Austria_ViennaBasin_Modling_Avar
775 AD
F
Austria
-
Mödling-An der Goldenen Stiege (Lower Austria, Mödling District); Mödling

Haplogroups

Not determined
H3h6
650-800 CE

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
55.5%
Steppe
33.5%
WHG
4.7%
EHG
2.6%
CHG/Iran N
1.3%
Natufian
1.2%
East Asian
1.2%

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: 0.0352

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

TUR_Barcin_N 45.9%
Yamnaya_RUS_Samara 38.0%
TUR_Tepecik_Ciftlik_N 10.1%
WHG 5.3%
Han 0.7%

Ancient Population Distances

Closest ancient reference populations
HRV_LIA_La_Tene
0.0302
HUN_Sarmatian_Late_Transtisza
0.0305
HUN_La_Tene
0.0310
HRV_EIA
0.0324
GRC_Logkas_MBA
0.0329
HUN_Avar_Late_Visonta
0.0330
HRV_MBA
0.0353
SVK_IA_Vekerzug
0.0355
DEU_MA_Alemannic_o1
0.0362
HUN_IA_Syrmian_SremGroup
0.0369
HRV_MBA_LBA
0.0369
HUN_Sarmatian_Early_Transtisza
0.0375
ITA_Proto-Villanovan
0.0379
HUN_LBA_EIA
0.0380
AUT_IA_La_Tene
0.0388

Modern Population Genetic Proximity

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

Archaeological Site Location

48.0790, 16.2796

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