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

MGS334
MGS334
Austria_ViennaBasin_Modling_Avar
775 AD
-
Austria
-
Mödling

Haplogroups

R1a1a1b
X2+225+@16223
R β€Ί M207 β€Ί M173 β€Ί M420 β€Ί M459 β€Ί CTS5437 β€Ί M515 β€Ί M198 β€Ί M417 β€Ί PF6162
cca

Ancestry Components

Estimated ancestral proportions from ancient reference populations
ANF
51.1%
Steppe
32.9%
WHG
6.5%
Natufian
5.1%
EHG
2.8%
CHG/Iran N
1.6%

Publication

Moedling2024

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: 0.0290

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

Yamnaya_RUS_Samara 36.1%
TUR_Barcin_N 30.7%
TUR_Tepecik_Ciftlik_N 24.7%
WHG 8.5%

Ancient Population Distances

Closest ancient reference populations
HUN_Sarmatian_Late_Transtisza
0.0333
SVK_IA_Vekerzug
0.0336
HRV_LIA_La_Tene
0.0336
HUN_La_Tene
0.0338
AUT_IA_La_Tene
0.0349
HUN_Sarmatian_Early_Transtisza
0.0352
HRV_EIA
0.0356
HUN_Avar_Late_Visonta
0.0367
CZE_LBA_Knoviz_o3
0.0378
HUN_IA_La_Tene
0.0379
HUN_EIA_Prescythian_Mezocsat
0.0381
HRV_MBA
0.0381
SRB_BA_Maros
0.0383
DEU_MA_Alemannic_o1
0.0384
SRB_Mokrin_EBA_Maros
0.0387

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