Introduction
Dogs have coexisted with humans for thousands of years and have been used as guard animals to herd livestock, hunt, and protect homes, as well as companion animals (
Wayne and Von 2012;
Larson et al., 2012;
Pedersen et al., 2015). Canis lupus, the wolf, is estimated to have given rise to dogs roughly 100,000 years ago. Since prehistoric times, the dog species has evolved through stringent selection (for desirable traits) which has ultimately led to the evolution of more than 350 distinct breeds of dogs worldwide. Scientific breeding of dogs is now a popular practice to entice dog owners and buyers by stamping on desirable traits of purebred dogs. This although increases the price, also necessitates molecular testing of parentage to verify the claim of parentage of the animals.
Molecular markers can identify the degree of genetic relatedness between animals, making parentage and individual identification easier. Microsatellites are tracts composed of short tandem repeats (STRs) or simple sequence repeats (SSRs) of DNA patterns ranging between one to six nucleotides, with repeats of 5 to 50 times (
Vieira et al., 2016). Repeat sequences are distributed ubiquitously in the genome, highly variable, and have been demonstrated to be effective tools in genome mapping (
Oudet et al., 1991). Microsatellites have been effectively used to determine the molecular signatures or DNA fingerprints of individuals (humans and animals), to determine parentage, to build pedigree, to select animals through marker-assisted selection for genetic improvement through selective breeding, etc. The use of microsatellites as molecular markers for animal identification and parentage verification generated highly accurate and effective results (
Linacre et al., 2011).
Identification of breed-specific molecular signatures benefits dog owners and breeders, and helps characterize the dog germplasm maintained in India (both foreign and indigenous). Parentage determination using microsatellite and SNP marker panels (
Kalbfleisch et al., 2014; Heaton et al., 2014;
Yu et al., 2015;
Flanagan et al., 2019) have been reported for different species. Relevant literature reports the associated prospects and challenges with parentage determination in humans and animals (
Stark et al., 2014;
Chan et al., 2014;
Goswami, 2015). Very limited works have reported on applications of SSR markers for parentage determination in dogs (
Hollinshead et al., 2020), especially in India. The present research has been designed to investigate the informative microsatellite markers for parentage testing in canines. A Ph.D. thesis has been submitted from our lab on parentage determination in cattle and buffalo using microsatellites as well as SNP markers (
Singh 2021) and relevant literature was published and presented (
Singh et al 2022;
Mukhopadhyay and Singh 2021). The goal of this work is to create and standardize a set of SSR primers to validate and verify parentages in dogs using the most popular dog breeds maintained in India.
Materials and Methods
Experimental Animal Selection and DNA Extraction
The experimental animals were selected based on trio and duo relationship to assess the informativeness of the markers for parentage determination, belonging to ten divergent germplasm, namely, (Labrador (Abbreviated as Lab), German Shepherd (GS), Pug, Mudhol Hound (MH), Tibetan Mastiff (TMS), Beagle, Belgian Malinois (BM), Pointer, and Cane Corso (CC)) breeds and Gaddi dogs. The animals were available from dog owners, and breeders belonging to four Indian states: Punjab, Himachal Pradesh, Haryana, and Maharastra (
Table 1). Two ml of peripheral blood was collected aseptically with an anticoagulant (0.5 M EDTA). Genomic DNA was extracted using the commercially available kit and Phenol:Chloroform: Isoamyl alcohol method (PCI) method (with modification of
Sambrook et al., 2001). Samples collected from distant places were stored at -20° and transported to the lab maintaining a cold chain. The quality and quantity of the extracted DNA were then measured with a NanoDrop (Thermo Scientific, Waltham, MA, USA), and agarose gel electrophoresis, respectively.
SSR-Marker Selection:
Initially, 15 microsatellite markers (5' fluorescent labeled with FAM, HEX, or TAMRA) (
Table 2) were selected based on the higher polymorphism information content (PIC) and observed heterozygosity (He) from various literature (Mellersh et al 1997, Neff et al 1998, Sargan 2007, Coutt 2009, David Parra et al 2009, Whiteside 2011). The primers were custom synthesized and the SSR-length polymorphism was done from Biologia Research India Pvt. Ltd, Karnal, India.
Analysis of SSR-Length Polymorphism Results:
The genotypic data were first manually checked for inconsistencies using Microsoft Office Excel 2007. The Peak Scanner™ Software v1.0 and GeneMapper® Software were used to perform the analysis of *.fsa files. The Windows OS-based stand-alone Peak Scanner™ Software (v1.0) (
https://peak-scanner-software.software.informer.com/1.0/) was used to accurately identify the correct peaks and fragment sizes vis-s-via functional annotation (viz. labeling, merging, and splitting) of peaks and further the peak data was feed in Microsoft Excel for the genetic analysis parameters. The descriptive statistics based on genotyping data were obtained using the Genetic Analysis in Excel (GenAlEx) tool v. 6.5 (
Peakall and Smouse, 2012). The number of alleles per locus (Na), the effective number of alleles (Ne), and the fixation index (F) expected homozygosity and heterozygosity (
Levene 1949) and expected heterozygosity (
Nei 1973).
The Hardy-Weinberg equilibrium test was carried out with the help of the POPGENE computer program (
Raymond and Rousset, 1995), which was used to estimate F-statistics (the global mean inbreeding coefficient [FIT], the average inbreeding coefficient of an individual concerning the local subpopulation [FIS], and the average inbreeding coefficient of subpopulations relative to the total population [FST]) for each locus, the pairwise FST Allelic occurrence, Genic Variation Statistics for All Locations Molecular Evolutionary Genetics, Summary of Heterozygosity Statistics (Nei, 1987). The exclusion probability (Jamieson and Taylor 1997) and the polymorphism information content(
Botstein et al., 1980) were calculated by using PARFEX v1.0 EXCEL™ tool and Cervus 3.0.7 software (
https://cervus.software.informer.com/download/). The probability of exclusion or power of exclusion (PE) is a priori statistic that determines the likelihood for a sample to be representative of a population (
Zhou et al., 2017).
The genetic parameters were obtained using the following formula:
Polymorphism Informative Content (PIC) for co-dominant markers |
PICi =1−ΣP2i − (ΣP2i) 2 + ΣP4i Where, n: number of alleles; pi & pj = allele frequencies in population i and j, respectively (Botstein et al., 1980) |
Heterozygosity (He) |
H = 1− Σ h= Σ2pq Where, h: Homozygosity; p & q: frequencies of two alleles of a locus |
Homozygosity (Ho), |
h = Σi (pi)2 Where, pi: frequency of ith allele of a locus |
Probability of exclusion (PE) |
PE = h2 (1−2hH2) Where, h: frequency of heterozygotes, H: frequency of homozygotes |
Likelihood ratio for parentage assignment |
L(H1,H2)|=P(D|H1)/P(D|H2) where. H1: The first hypothesis stating the agreement that the candidate parental pair is the true parental pair H2: hypothesis stating that the alternative candidate parental pair is the true parental pair and D: data in the form of offspring and parental genotypes |
Results and Discussions
Genetic Diversity of Microsatellites
Out of 15 SSR markers used 12 markers were amplified for the samples under study. The results obtained have been presented based on the output of these 12 markers.
Table 3 shows the sample size, observed number of alleles, effective number of alleles, and microsatellite loci of the experimental samples. The number of alleles per SSR locus (Na) ranged from 5 (NPPM10) to 29 (PEZ12), with a mean of 15.4167 (± 8.2402 s.e.). The number of effective alleles per locus (Ne) varied from 3.6140 (NPPM10) to 15.2178 (PEZ16), with a mean value of 7.9664 (±4.2066 s.e.). The mean value of Shannon's Information index (I) was 2.1804 (± 0.5581 s.e.)
Measures of Heterozygosity Statistics
The average expected heterozygosity (Ave_Exp_Het) across all loci was 0.85 (
Table 4). The observed heterozygosity (Obs_Het) average was 0.80. The expected heterozygosity was found to be relatively high for all the markers as all the markers have heterozygosity of more than 0.5. All 12 markers were found to be highly polymorphic and can be used for the genetic studies of the dogs.
Therefore, the Mean (± SEM) observed heterozygosity, averaged over loci, was 0.8020 ± 0.1345, which was lower than the expected heterozygosity
The population inbreeding coefficient (FIS) ranged from −0.1400 (NPPM10) to 0.2274 (NPPM930). The Fis value was positive in a few markers, indicating the in-breeding of the population. The FST values of all the loci was 0.0000 which indicated there was no genetic subdivision. The genetic variation existed within dogs (
Table 5).
Hardy–Weinberg Test
The results of HWE tests of the 12 microsatellite loci indicated UOR4107 shows significant differences (
P > 0.05) and NPPM30, NPPM769, NPPM905, NPPM930, PEZ16, NPPM244 are statistically significant (
P > 0.001) (
Table 6). The deviation from the hardy Weinberg can be due to the non-random mating or due to some evolutionary processes.
The observed F for the markers lies between the upper and the lower limit of 95% which depicted that markers were not under any selection pressure or associated with any of the quantitative traits. Thus these markers can be used for the parentage identification I dogs
Table 7.
Ewens-Watterson Test for Neutrality for the markets.
Table 7.
Ewens-Watterson Test for Neutrality for the markets.
Locus |
n |
k |
Obs.F |
Min F |
Max F |
Mean* |
SE* |
L95* |
U95* |
NPPM30 |
114 |
9 |
0.178 |
0.111 |
0.870 |
0.310 |
0.013 |
0.169 |
0.617 |
NPPM769 |
114 |
20 |
0.074 |
0.050 |
0.722 |
0.131 |
0.002 |
0.082 |
0.237 |
PEZ11 |
114 |
25 |
0.073 |
0.040 |
0.668 |
0.100 |
0.001 |
0.066 |
0.168 |
NPPM905 |
114 |
10 |
0.236 |
0.100 |
0.855 |
0.279 |
0.010 |
0.156 |
0.541 |
NPPM930 |
114 |
13 |
0.137 |
0.077 |
0.812 |
0.215 |
0.006 |
0.127 |
0.422 |
NPPM10 |
114 |
5 |
0.277 |
0.200 |
0.932 |
0.507 |
0.028 |
0.265 |
0.866 |
PEZ12 |
114 |
29 |
0.097 |
0.035 |
0.629 |
0.082 |
0.001 |
0.056 |
0.140 |
PEZ17 |
114 |
10 |
0.181 |
0.100 |
0.855 |
0.277 |
0.009 |
0.161 |
0.519 |
PEZ16 |
114 |
28 |
0.066 |
0.036 |
0.639 |
0.086 |
0.001 |
0.058 |
0.145 |
UOR4107 |
104 |
11 |
0.235 |
0.091 |
0.826 |
0.251 |
0.007 |
0.143 |
0.471 |
NPPM244 |
114 |
17 |
0.129 |
0.059 |
0.759 |
0.157 |
0.003 |
0.097 |
0.291 |
NPPM858 |
114 |
8 |
0.227 |
0.125 |
0.885 |
0.346 |
0.014 |
0.188 |
0.648 |
Polymorphism Information Content and Probability Of Exclusion
Polymorphism Information Content (PIC) and the probability of Exclusion are indeed important measures in genetic research of microsatellites. PIC and probability of exclusion were used to assess the informativeness of a genetic marker. High PIC values suggest that a marker is highly informative and can discriminate well between alleles, making it useful for various applications such as genetic diversity studies and parentage studies (
Serrote et al., 2020). The use of quantitative genotypes for statistical assignment of parentage has been discussed by
Hamilton (2021). Parentage assignment using genotyping by sequencing data has been recently reported by
Whalen et al. (2019) All the markers in the study were highly polymorphic, as all had a PIC value of more than 0.673. Probability of exclusion represents the marker's average capability to eliminate one parent when the genotype of that parent is unknown, to confirm the parent's contribution to the offspring's genotype when the offspring's genotype is either known or unknown, or to exclude both potential parent pairs when determining offspring parentage. The exclusion probability for all the markers values greater than 0.658 which depicts that all the markers were highly informative which can help to achieve the 99.9% success rate for the parentage studies as the combined exclusion probability (CPE) values of (2.82E-12) 0.99999995.
Table 8.
PIC and PE of the markers.
Table 8.
PIC and PE of the markers.
SN |
Marker |
Polymorphism information Content |
Exclusion Probability |
1 |
PEZ16 |
0.932 |
0.972 |
2 |
NPPM769 |
0.926 |
0.966 |
3 |
PEZ11 |
0.916 |
0.959 |
4 |
PEZ12 |
0.893 |
0.944 |
5 |
NPPM930 |
0.854 |
0.895 |
6 |
NPPM244 |
0.831 |
0.872 |
7 |
PEZ17 |
0.811 |
0.841 |
8 |
NPPM30 |
0.797 |
0.824 |
9 |
NPPM858 |
0.765 |
0.794 |
10 |
UOR4107 |
0.754 |
0.777 |
11 |
NPPM905 |
0.753 |
0.782 |
12 |
NPPM10 |
0.673 |
0.658 |
A total of 12 microsatellite loci were found and analyzed after being combined into four multiplex PCR reaction systems and genotyped in two multiplex loading systems. Because of the high variability of these microsatellite loci, very precise genotyping panels could be utilized for individual genotyping, parentage verification, and individual identification. The total diversity structure was found to be quite strong, and it corresponded with the use of the varieties and the breeding program's tactics based on parental group pairings. All of these findings highlight the significance and necessity of maintaining these genotypes in germplasm repositories.
In conclusion, the results of analyzing the dog populations in India using 12 new microsatellite markers revealed their average anticipated heterozygosity and observation heterozygosity. As a result, these microsatellite markers are highly applicable to the populations studied. These findings suggest that the microsatellite markers have acceptable resolution when used to detect variations between dog breeds. Furthermore, power exclusion will be employed as a strong tool for paternity testing.
Future Prospectives
In the future, the microsatellites identified in this work could be used to assess dog population structure, history, and diversity, hence assisting in the genetic improvement of Indian dog breeds. To overcome outstanding identifying issues, more phenotypic and passport data checks are required.
Author Contributions
YS: Did the lab work and sample collection; BPK: manuscript writing; MPK: Data analysis; YHM: Sample collection from Karnataka; CSM: Designed the project and was the Principal Investigator, proofreading. All authors contributed to the manuscript revision, and read, and approved the present version.
Acknowledgments
The authors thankfully acknowledge the funding provided by the Department of Biotechnology, Government of India, through the collaborative research project “Parentage Determination and Cytogenetic Profiling in DoGerman Shepherd (GS) (DBT-19I)”. A special note of thanks to Mr. Anil Jamwal, integrated farmer and T. Mastiff breeder, Palampur, Mr. Newton Sidhu, Director, PHG-CTBI, Mohali, and different pet owners for providing samples of dogs.
Competing Interests
The authors declare no competing interests.
Ethics Approval and Consent to Participate
Permission from the Institutional Animal Ethics Committee (IAEC) was obtained (IAEC/2020/200-219, 14.12.2020)
Consent for Publication
Obtained from the Office of the Director of Research, Guru Angad Dev Veterinary and Animal Sciences University, Ludhiana
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Table 1.
Family orientation (Sire/Dam/Offspring) and breed detail of the experimental animals.
Table 1.
Family orientation (Sire/Dam/Offspring) and breed detail of the experimental animals.
SN |
Sire |
Dam |
Offspring |
Trio-Id |
Duo-Id |
Breed |
1 |
1 |
2 |
3 |
T1 |
-- |
Labrador |
2 |
7 |
8 |
9 |
T2 |
-- |
Labrador |
3 |
16 |
17 |
18 |
T3 |
-- |
German Shepherd |
4 |
25 |
26 |
27 |
T4 |
-- |
German Shepherd |
5 |
40 |
41 |
42 |
T5 |
-- |
Pug |
6 |
47 |
48 |
46 |
T6 |
-- |
Mudhol Hound |
7 |
50 |
51 |
49 |
T7 |
-- |
Mudhol Hound |
8 |
54 |
53 |
52 |
T8 |
-- |
Mudhol Hound |
9 |
57 |
56 |
55 |
T9 |
-- |
Mudhol Hound |
10 |
60 |
59 |
58 |
T10 |
-- |
Mudhol Hound |
11 |
64 |
65 |
66 |
T11 |
-- |
Tibetan Mastiff |
12 |
67 |
68 |
69 |
T12 |
-- |
Gaddi |
13 |
67 |
68 |
70 |
T13 |
-- |
Gaddi |
14 |
67 |
68 |
71 |
T14 |
-- |
Gaddi |
15 |
82 |
83 |
84 |
T15 |
-- |
Belgian Malinois |
16 |
93 |
94 |
95 |
T16 |
-- |
Cane Corso |
17 |
13 |
NA |
15 |
-- |
D1 |
Pug |
18 |
22 |
NA |
24 |
-- |
D2 |
German Shepherd |
19 |
31 |
NA |
33 |
-- |
D3 |
Pug |
20 |
NA |
85 |
86 |
-- |
D5 |
Beagle |
21 |
NA |
87 |
88 |
-- |
D6 |
Pointer |
22 |
NA |
87 |
89 |
-- |
D7 |
Pointer |
23 |
61 |
62 |
NA |
-- |
D4 |
Gaddi* |
Table 2.
Detail of the 5' labeled simple sequence repeat primers.
Table 2.
Detail of the 5' labeled simple sequence repeat primers.
SN |
Loci |
Forward_Primer (5’ to 3’) sequence (and length) |
FReverese_Primer (5’ to 3’) sequence (and length) |
Allele_S ize |
TM |
Dye |
|
NPPM10 |
GTGGACCATGTGACTCTTGA (20) |
TTTGTGTGATGCCACTACAGTAAG (24) |
176-182 |
58 |
6-FAM |
|
NPPM244 |
GTCACTTAATAGGATGATTTCTTGG (25) |
CTAAAACCTGGATTGTCTAATTTGT (25) |
315-338 |
58 |
6-FAM |
|
NPPM30 |
AGGACTATTTCACGCCTTGTTG (22) |
ATTCCCACCTCAGTGATTACAG (22) |
276-286 |
58 |
HEX |
|
NPPM769 |
TGGTAGCCACAGAAGCATTG (20) |
TTGGATTAAGTGTGTAGTCCTGAGC (25) |
218-238 |
58 |
TAMRA |
|
NPPM855* |
TGAGTTTTTGGTCCCCTCCA (20) |
CTCTGGTCCAGCAGTTGAAAC (21) |
226-238 |
58 |
TAMRA |
|
NPPM858 |
CAGTTTGCTACCTTTTGTGTAATCA (25) |
CTCACCCATTGTAGTCTCTGTCTTC (25) |
187-204 |
58 |
HEX |
|
NPPM905 |
TCCAGAGTCACAACTTCAGAAAC (23) |
GCTAGATTGCTGCCCTTTACTC (22) |
201-221 |
58 |
HEX |
|
NPPM930 |
TCTTTACCCTTCTGGAAAATGAG (23) |
GTGATTGAACACGCAAGGGAT (21) |
247-262 |
58 |
TAMRA |
|
NPPM981* |
GAACATCTTCCTTCTTCCACTG (22) |
TCCTAGAGACC TGGGATGAAGT (22) |
318-328 |
58 |
HEX |
|
PEZ11 |
ATTCTCTGCCTCTCCCTTTG (20) |
TGTGGATAATCTCTTCTGTC (20) |
121-173 |
55 |
6-FAM |
|
PEZ12 |
GTAGATTAGATCTCAGGCAG (20) |
TAGGTCCTGGTAGGGTGTGG (20) |
266-313 |
58 |
TAMRA |
|
PEZ16 |
GCTCTTTGTAAAATGACCTG (20) |
GTGGGAATCGTCCTAAAACCC (21) |
281-317 |
58 |
6-FAM |
|
PEZ17 |
CTAAGGGACTGAACTTCTCC (20) |
GTGGAACCTGCTTAAGATTC (20) |
199-227 |
58 |
HEX |
|
PEZ22* |
TGGGGAGATCTACAGACCAC (20) |
CTAATGTGTCTCTCAAGCCG (20) |
171-189 |
55 |
6-FAM |
|
UOR4107 |
TGACCCTTCTACAACTCGGG (20) |
TGTGACCAGTCACTGCTTCC (20) |
220-232 |
58 |
TARMA |
Table 3.
Genetic parameters of the 12 microsatellite loci obtained from dog populations.
Table 3.
Genetic parameters of the 12 microsatellite loci obtained from dog populations.
Locus |
Sample Size |
na* |
ne* |
I* |
NPPM30 |
114 |
9 |
5.61 |
1.86 |
NPPM769 |
114 |
20 |
13.59 |
2.76 |
PEZll |
114 |
25 |
13.74 |
2.85 |
NPPM905 |
114 |
10 |
4.25 |
1.69 |
NPPM930 |
114 |
13 |
7.29 |
2.16 |
NPPM10 |
114 |
5 |
3.61 |
1.36 |
PEZ12 |
114 |
29 |
10.36 |
2.80 |
PEZ17 |
114 |
10 |
5.51 |
1.88 |
PEZ16 |
114 |
28 |
15.22 |
3.02 |
UOR4107 |
104 |
11 |
4.26 |
1.73 |
NPPM244 |
114 |
17 |
7.75 |
2.34 |
NPPM858 |
114 |
8 |
4.40 |
1.71 |
Mean |
113 |
15.42 |
7.97 |
2.18 |
St . Dev |
|
8.24 |
4.21 |
0.56 |
Table 4.
Measures of genetic variation (Heterozygosity Statistics for All Loci) in dog population.
Table 4.
Measures of genetic variation (Heterozygosity Statistics for All Loci) in dog population.
Locus |
Sample Size |
Obs_Hom |
Obs_Het |
Exp_Hom* |
Exp_Het* |
Nei** |
Avg_Het |
NPPM30 |
114 |
0.12 |
0.88 |
0.17 |
0.83 |
0.82 |
0.82 |
NPPM769 |
114 |
0.04 |
0.96 |
0.07 |
0.93 |
0.93 |
0.93 |
PEZll |
114 |
0.00 |
1.00 |
0.06 |
0.94 |
0.93 |
0.93 |
NPPM905 |
114 |
0.26 |
0.74 |
0.23 |
0.77 |
0.76 |
0.76 |
NPPM930 |
114 |
0.33 |
0.67 |
0.13 |
0.87 |
0.86 |
0.86 |
NPPM10 |
114 |
0.18 |
0.82 |
0.27 |
0.73 |
0.72 |
0.72 |
PEZ12 |
114 |
0.04 |
0.96 |
0.09 |
0.91 |
0.90 |
0.90 |
PEZ17 |
114 |
0.23 |
0.77 |
0.17 |
0.83 |
0.82 |
0.82 |
PEZ16 |
114 |
0.25 |
0.75 |
0.06 |
0.94 |
0.93 |
0.93 |
UOR4107 |
104 |
0.29 |
0.71 |
0.23 |
0.77 |
0.77 |
0.77 |
NPPM244 |
114 |
0.46 |
0.54 |
0.12 |
0.88 |
0.87 |
0.87 |
NPPM858 |
114 |
0.19 |
0.81 |
0.22 |
0.78 |
0.77 |
0.77 |
Mean |
113 |
0.20 |
0.80 |
0.15 |
0.85 |
0.84 |
0.84 |
St . Dev |
|
0.13 |
0.13 |
0.07 |
0.07 |
0.07 |
0.07 |
Table 5.
Summary of the F-Statistics and gene flow among dog populations.
Table 5.
Summary of the F-Statistics and gene flow among dog populations.
Locus |
Sample Size |
Fis |
Fit |
Fst |
Nm* |
|
NPPM769 |
114 |
-0.042 |
-0.042 |
0.000 |
**** |
|
PEZll |
114 |
-0.079 |
-0.079 |
0.000 |
**** |
|
NPPM905 |
114 |
0.036 |
0.036 |
0.000 |
**** |
|
NPPM930 |
114 |
0.227 |
0.227 |
0.000 |
**** |
|
NPPMlO |
114 |
-0.140 |
-0.140 |
0.000 |
**** |
|
PEZ12 |
114 |
-0.068 |
-0.068 |
0.000 |
**** |
|
PEZ17 |
114 |
0.057 |
0.057 |
0.000 |
**** |
|
PEZ16 |
114 |
0.193 |
0.193 |
0.000 |
**** |
|
UOR4107 |
104 |
0.070 |
0.070 |
0.000 |
**** |
|
NPPM244 |
114 |
0.376 |
0.376 |
0.000 |
**** |
|
NPPM858 |
114 |
-0.044 |
-0.044 |
0.000 |
**** |
|
Mean |
113 |
0.046 |
0.050 |
0.000 |
1000 |
|
Table 6.
Summary of the chi-square and Hardy Weinberg test.
Table 6.
Summary of the chi-square and Hardy Weinberg test.
Locus |
DF |
ChiSq |
Probability |
Significance |
NPPM30 |
36 |
142.027 |
0.000 |
*** |
NPPM769 |
190 |
324.874 |
0.000 |
*** |
PEZ11 |
300 |
368.802 |
0.004 |
*** |
NPPM905 |
45 |
162.047 |
0.000 |
*** |
NPPM930 |
78 |
165.012 |
0.000 |
*** |
NPPM10 |
10 |
29.441 |
0.001 |
*** |
PEZ12 |
406 |
399.108 |
0.587 |
ns |
PEZ17 |
45 |
60.104 |
0.065 |
ns |
PEZ16 |
378 |
565.516 |
0.000 |
*** |
UOR4107 |
55 |
80.343 |
0.015 |
* |
NPPM244 |
136 |
274.682 |
0.000 |
*** |
NPPM858 |
28 |
34.536 |
0.184 |
ns |
|
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