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Khoe-San associated haplogroups L0d and L0k – Further analysis

Y- chromosome and mtDNA comparative studies

3. MITOCHONDRIAL-DNA STUDIES

3.3 Haplogroup assignment and structure

3.3.2 Khoe-San associated haplogroups L0d and L0k – Further analysis

The sub-haplogroups of the Khoe-San associated haplogroups L0d/k were differentially distributed in the different sample groups included in this study (Figure 3.7 and 3.8)

Just by observing the distribution over the different sampling groups in the form of bar-charts (Figure 3.8) one could immediately see the differences. It was especially clear between the southern-San/Coloured/Khoe groups (KAR, COL, CAC, KHO, CNC, NAM) and the San groups located north of them (GUG, JOH, XUN). To further investigate these differential distributions, analysis of sub-haplogroup distribution was done.

Sample groups were arranged in a southeast to northwest direction and coloured with increasing shade from the southeast to the northwest; the resultant distribution of L0d/k subgroups is represented in Figure 3.10. A clear clinal pattern for all of the haplogroups was observed. L0d2a and L0d3 seemed to have a more southeastern distribution (lighter shades), while L0d2b, L0d2c, L0d1a has and intermediate central pattern. L0d1c, L0k1 as well as the few sequences belonging to L0dx and L0d2d, however, was much darker and seem to predominate in the northern groups.

To further investigate this apparent clinal distributions contour plots of the haplogroups were constructed with the Surfer v.8.06.39 program and is shown in Figure 3.11.

Figure 3.10 Bar-graph indicating the clinal distribution of the L0d/k subgroups. Darker shades are north-western groups and lighter shades are southern groups

0%

L0d1a L0d1b L0d1c L0d2a L0d2b L0d2c L0d2d L0d3 L0dx L0k1

KWE

The contour plots reflected the distributions of the L0d/k subgroups as discussed in section 3.1.3.2. Certain haplogroups (L0d3 and L0d2a) had higher frequencies in the southeast than the northwest; others had a more gradual and central distribution (L0d1a, L0d1b, L0d2c and L0d2b), while some had higher frequencies in the north (L0k1 and to a certain extent L0d1c).

In the contour plots of Figure 3.11, all the haplogroups except L0d2b and L0d1c seemed to have a unimodal distribution with a single point of highest frequency and then decreasing frequencies from there in a clinal fashion. L0d2b showed two peaks represented by the

Figure 3.11 Contour plots indicating the frequency distributions of L0d/k subgroups

have any significance. L0d1c also showed a bimodal distribution pattern. To analyse this further the L0d1c group was split up into two groups. The first group was the L0d1c1 sequences as defined by Behar et al., (Behar et al., 2008), and are represented by the star-like expansion pattern within L0d1c in the network (Figure 3.6). The second group L0d1c- was the remaining L0d1c sequences after the L0d1c1 sequences were removed.

Contour plots of these groups are presented in Figure 3.12.

From Figure 3.12 it can be seen that L0d1c originally had a unimodal clinal distribution but a subsequent expansion in the L0d1c1 subgroup occurred that caused elevated

L0d1c1 L0d1c-

L0d1c

A

B C

Figure 3.12 Contour plots of L0d1c split into two subgroups, L0d1c1 and the remaining L0d1c sequences (L0d1c-).

frequencies in the XUN. L0d1c1 did not occur in the KWE and were at low frequencies in the JOH. This led to the overall bimodal distribution of L0d1c.

To further analyse the individual haplogroup histories, to test if they had notable expansions and to date these expansions, mismatch distributions of the sub-haplogroup sequences were constructed (Figure 3.13 and Table 3.3)

Table 3.3 Mismatch distribution statistics (haplogroups)

* T – Time before present that expansion took place (calculation explained in section 2.2.2.3)

# expansion hypothesis rejected - 95% CI overlap + excluded – too few sequences

HG – Haplogroup, SSD - Sum of Squared deviation

Mismatch distribution statistics and the results for a spatial expansion test are shown in Table 3.3 (the p-value indicate the probability that the simulated SSD (simulated under an expansion scenario) is not significantly different from the observed SSD). All L0d subgroups except L0d2b, L0d2c and L0dx tested positive for expansions. The haplogroups that indicated expansions with the highest significance was L0d1a and L0d2a. Their mismatch distributions showed smooth unimodal distributions with low raggedness values.

Their

τ

(Tau) values, however, differed with the

τ

value of L0d2a indicating a much more recent expansion.

τ

values of the L0d1 haplogroups were similar (indicating expansions of around 27 000 years BP) while L0d3 had a smaller

τ

value and L0d2a and L0k1 the smallest (indicating expansions around 6 000 years BP). Both M and R haplogroups experienced expansions ~ 40 000 to 50 000 years BP.

Figure 3.13 Mismatch distributions of L0d/k sub-haplogroups and comparative groups. # expansion hypothesis rejected - 95% CI

#

#

#

Caveats associated with the coalescence analysis employed in mismatch distributions are the assumption of a single exponentially growing population and the large degrees of statistical uncertainty. Also, by applying these methods earlier population expansions can be obscured by recent population bottlenecks (Excoffier and Schneider, 1999). Mismatch distributions have been reported previously to have less ability to predict population expansions than neutrality test summary statistics such as Tajima’s D (Tajima, 1989), Fu’s Fs (Fu, 1997) and the R2 statistic (Ramos-Onsins and Rozas, 2002). Diversity estimates together with the neutrality tests for the L0d sub-haplogroups are shown in Table 3.4. Also included as comparative samples are other sub-haplogroups in the study group that had more than 10 representative sequences.

Table 3.4 Diversity statistics and neutrality tests of L0d/k subgroups and comparative haplogroups

Group N section 2.2.3. The two non-African macro-haplogroups had very big effective population sizes while the African haplogroup Ne was smaller. In the L0d subgroups the largest Ne was detected in L0d1a, L0d1b and L0d2a while L0d3 and L0k1 had the smallest Ne.

Under neutral expectations with random mating, constant population sizes and no selection π and θ should be equal (Jobling et al., 2004c). Neutrality tests were done to detect deviations from the assumptions of neutrality and constant population size. Significantly

growth and/or positive selection. The Fs and R2 statistic have been reported to detect population expansions very successfully (Ramos-Onsins and Rozas, 2002; Pilkington et al., 2008). Fs is based on the probability of drawing a number of haplotypes that is greater or equal to the observed number of samples drawn from a population of constant size. R2 is based on the difference between the average number of nucleotide differences and the number of singleton mutations. The R2 statistic is especially powerful when sample sizes are small (~10) and Fs have a greater ability to detect population expansions when sample sizes are large (~50) (Ramos-Onsins and Rozas, 2002; Pilkington et al., 2008).

In the comparative groups the non-African haplogroups M and R tested positive for population expansion in all three neutrality tests with highly significant P-values. The L0d group as a whole had significant D and Fs values but not for R2. R2, however, does not perform reliably at large sample sizes (Ramos-Onsins and Rozas, 2002). Of the L0d subgroups L0d2a had the highest significance in all three neutrality tests. L0d1b also attained significance in all three tests while L0d1a had a very significant Fs value but did not reach significance in the Tajima’s D and R2 tests.

While neutrality tests are widely employed to test hypotheses of population expansion events, recent improvements in coalescence inference methods led to increased accuracy, without the need to assume a single exponential growth curve (Shapiro et al., 2004;

Atkinson et al., 2008). One of these methods, Bayesian Skyline Plots (BSPs) (Drummond et al., 2005), were employed to further visually represent the changes in Ne through time, were constructed for each haplogroup (Figure 3.14).

The BSPs of all the L0d sub-haplogroups, except L0d1a, indicated a recent increase in Ne

(Figure 3.14). L0d1a had an increase that started around 25 000 – 30 000 years BP and a recent decrease that started around 5 000 years BP. L0d1c had a constant population size over a extended period and then similar to L0d1a, started to decrease around 5 000 years BP. Around a 1 000 years BP, however, it increased rapidly. L0d1b had an increase that started around 14 000 years BP and a further increase recently. Despite a shallow coalescence time, L0d2a showed a dramatic increase from 8 000 years BP onwards and a further recent increase. The L0d3 BSP profile that included east African and the Kuwait

haplotypes (L0d3+) showed a slow decline over an extended period followed by a recent increase in Ne. The L0d3 profile that only included the southern African L0d3 haplotypes (L0d3-) showed a more intense decline and an increase that started later than in the L0d3+

profile.

Figure 3.14 Bayesian Skyline plots of haplogroups showing changes in Ne through time. A log scale of Ne is represented on the Y-axis, while years before present is represented on the X-axis, with the present indicated by 0. L0d3+ is L0d3 including the east African and Kuwait sequences. L0d3- includes only L0d3 sequences from the present study. The black bold vertical lines indicate the coalescence date and the lighter vertical lines the 95% confidence intervals for the coalescence. The blue lines indicate the 95% confidence intervals for the plot-lines

L0d3- L0d3+

L0d2a L0d1b

L0d1c L0d1a

3.3.3 Discussion of analyses of Khoe-San associated haplogroups L0d and