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

I15337
I15337
USA_MD_Catoctin_AfricanAmerican
1812 AD
F
USA
-
Cemetery for Enslaved at Catoctin Furnace (Maryland)

Haplogroups

Not determined
L3e2
1775-1850 CE

Ancestry Components

Estimated ancestral proportions from ancient reference populations
Sub-Saharan
94.6%
Iberomaurusian
2.0%
CHG/Iran N
1.6%
ANE
1.2%
Native American
0.4%
AASI
0.2%

Publication

HarneyBioRxiv2022,HarneyScience2023; HarneyReichBioRxiv2022; HarneyReichScience2023

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

Good Β· Distance: 0.0238

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

Yoruba 48.8%
Gambian 41.2%
ETH_4500BP 6.0%
Yamnaya_RUS_Samara 2.4%
Kura-Araxes_ARM_Kaps 0.9%
BRA_LapaDoSanto 0.7%

Ancient Population Distances

Closest ancient reference populations
COG_Kindoki_230BP
0.0616
TZA_Pemba_600BP
0.0714
COG_NgongoMbata_220BP
0.0715
UGA_Munsa_500BP
0.0926
ZAF_400BP
0.0929
BWA_Taukome_1100BP
0.1065
KEN_Kakapel_300BP
0.1081
KEN_IA_Deloraine
0.1284
BWA_Xaro_1400BP
0.1389
KEN_Kakapel_900BP
0.2210
CMR_Shum_Laka
0.2260
KEN_LSA
0.2321
KEN_Nyarindi_3500BP
0.2340
ETH_Mota
0.2374
TZA_Gishimangeda
0.2382

Modern Population Genetic Proximity

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

Archaeological Site Location

39.5810, -77.4340

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