| Literature DB >> 20211033 |
Junwu Ma1, Nathalie Iannuccelli, Yanyu Duan, Weibing Huang, Beili Guo, Juliette Riquet, Lusheng Huang, Denis Milan.
Abstract
BACKGROUND: Variations in recombination fraction (theta) among chromosomal regions, individuals and families have been observed and have an important impact on quantitative trait loci (QTL) mapping studies. Such variations on porcine chromosome X (SSC-X) and on other mammalian chromosome X are rarely explored. The emerging assembly of pig sequence provides exact physical location of many markers, facilitating the study of a fine-scale recombination landscape of the pig genome by comparing a clone-based physical map to a genetic map. Using large offspring of F1 females from two large-scale resource populations (Large White male symbol x Chinese Meishan female symbol, and White Duroc male symbol x Chinese Erhualian female symbol), we were able to evaluate the heterogeneity in theta for a specific interval among individual F1 females.Entities:
Mesh:
Year: 2010 PMID: 20211033 PMCID: PMC2850356 DOI: 10.1186/1471-2164-11-159
Source DB: PubMed Journal: BMC Genomics ISSN: 1471-2164 Impact factor: 3.969
Locations of all markers on the different porcine maps and comparison with those on the human physical map
| Ord.1 | Marker name2 | SSC-X cyto-genetic map | Blast matched clones on pig genome3 | IMpRH map_Carthagene (cR)4 | IMpRH map_INRA2005 (cR)5 | SSC-X clone map (Mb)6 | HSA-X physical map (Mb)7 | INRA genetic map (Kosabi; cM) | JXAU genetic map (Kosabi; cM)8 | USDA-MARC genetic map at NCBI (cM)9 |
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | SW949 | Xp24/Yp | CH242-231E5 | 58 | 2126 | 0 | 0 | 0 | ||
| 2 | Xp24-23 | CH242-336E9 | 285 | 1861 | 7.65 | 11.38 | 0 | 16 | 11.9 | |
| 3 | Xp21 | CH242-273O11 | 523 | 1588 | 21.28 | 25.47 | 23.7 | 46.6 | 33 | |
| 4 | Xp12 | CH242-31B7 | 864 | 1345 | 38.46 | 42.14 | 46 | 65.5 | 55.4 | |
| 5 | Xp11.2 | CH242-69I19 | 976 | 1253 | 42.25 | 47.22 | 56.5 | 76.1 | ||
| 6 | SW2476 | Xp11.2 | CH242-24N13 | 985 | 1250 | 42.70 | 48.32 | |||
| 7 | 992 | 1211 | 59.5 | 78.7 | 65.7 | |||||
| 8 | UMNP448 | CH242-147G7 | 1027 | 1200 | 43.78 | 50.42 | ||||
| 9 | BE102J23.0003R1 | CH242-102J23 | 44.30 | 50.94 | ||||||
| 10 | Near centro-mere | CH242-225C1 | 1293 | 1045 | 54.21 | 63.35 | 62.7 | 79.9 | ||
| 11 | MCSE3F14 | CH242-3F14 | 1301 | 1093 | 55.27 | 65.30 | ||||
| 12 | BE145J20.0597R1 | Xq12 | CH242-145J20 | 58.94 | 69.06 | |||||
| 13 | MCST2J13 | Xq13 | PigE-2J13 | 1480 | 63.85 | 74.74 | ||||
| 14 | Xq13 | CH242-123K13 | 1547 | 1007 | 67.72 | 79.92 | 62.8 | 80.1 | ||
| 15 | MCSE58H4 | Xq13 | CH242-58H4 | 1596 | 983 | 70.38 | 83.46 | |||
| 16 | BE8B11.0679Y1 | Xq21 | CH242-8B11 | 77.85 | 97.31 | |||||
| 17 | MCSE65L7 | Xq21 | CH242-65L7 | 1768 | 932 | 82.80 | 91.66 | |||
| 18 | Xq21 | CH242-203F13 | 1797 | 905 | 93.18 | 62.8 | 80.2 | |||
| 19 | UMNP374 | Xq21 | CH242-74J23 | 1840 | 840 | 97.00 | ||||
| 20 | Xq21 | CH242-166I17 | 1884 | 800 | 99.84 | 62.8 | 80.4 | |||
| 21 | BE497I6FB48R | Xq22 | CH242-497I6 | 88.52 | 103.76 | |||||
| 22 | BE218F2FB67K | Xq22 | CH242-218F2 | 89.33 | 104.46 | 63.2 | ||||
| 23 | Xq22 | CH242-427M6 | 89.90 | 105.02 | 80.9 | |||||
| 24 | BE151D17.0014Y1 | Xq22 | CH242-151D17 | 90.42 | 105.88 | |||||
| 25 | Xq22 | CH242-264N4 | 1991 | 710 | 91.73 | 107.08 | 65.7 | 83.5 | ||
| 26 | BE32D24.0584R1 | Xq22 | CH242-32D24 | 91.73 | 107.03 | |||||
| 27 | BE276J1FB107R | Xq22 | CH242-276J1 | 700 | 91.87 | 107.20 | ||||
| 28 | BE206D8.0949R1 | Xq22 | CH242-206D8 | 92.18 | 107.47 | |||||
| 29 | BE386O15.1136R1 | Xq22 | CH242-386O15 | 92.27 | 107.86 | |||||
| 30 | Xq22 | CH242-477D6 | 93.33 | 107.86 | 85.9 | |||||
| 31 | MCSE313H19.0244 | Xq22 | CH242-313H19 | 93.72 | 108.38 | 67.5 | ||||
| 32 | Xq22 | CH242-17O13 | 687 | 93.87 | 108.58 | |||||
| 33 | Xq22 | CH242-17O13 | 687 | 108.58 | 67.9 | 87 | ||||
| 34 | Xq22 | CH242-231M24 | 682 | 109.41 | 69.8 | 88.1 | ||||
| 35 | MCSE12P4.1041 | Xq22 | CH242-12P4 | 109.65 | 70.1 | |||||
| 36 | MCSE12P4.0112 | Xq22 | CH242-12P4 | 71.2 | ||||||
| 37 | Xq22 | PigE-96O22 | 658 | 110.22 | 72.8 | 90.5 | ||||
| 38 | 2050 | 656 | 73.4 | 90.9 | ||||||
| 39 | BE95P6.0900R1 | Xq22 | CH242-95P6 | 94.38 | 110.48 | |||||
| 40 | Xq22 | CH242-347J6 | 646 | 94.52 | 110.63 | 74.5 | 92.3 | |||
| 41 | BE412O5B120R | Xq22 | CH242-412O5 | 95.59 | 111.90 | |||||
| 42 | BE80C18FB136W | Xq22 | CH242-80C18 | 95.76 | 77 | |||||
| 43 | BE504J7.0664Y1 | Xq22 | CH242-504J7 | 97.03 | ||||||
| 44 | Xq22 | CH242-408J11 | 2168 | 595 | 97.35 | 113.73 | 77.5 | 95.2 | ||
| 45 | Xq22 | CH242-135K13 | 97.56 | 113.90 | 95 | |||||
| 46 | BE371L5.0001Y1 | Xq22 | CH242-371L5 | 97.88 | 114.30 | |||||
| 47 | BE185O8FB63S | Xq22 | CH242-185O8 | 98.02 | 114.48 | 78.3 | ||||
| 48 | BE219E21.0003M1 | Xq22 | CH242-219E21 | 98.16 | 114.79 | |||||
| 49 | 2214 | 540 | 79.1 | 96.5 | ||||||
| 50 | BE28B16.0529Y1 | Xq23 | CH242-28B16 | 99.34 | ||||||
| 51 | UMNP870 | Xq23 | CH242-141A6 | 2246 | 522 | 102.50 | 117.67 | |||
| 52 | 2261 | 506 | 118.15 | 81.6 | 98.8 | |||||
| 53 | Xq23 | CH242-78C24 | 102.00 | 118.36 | 82.5 | 99.5 | ||||
| 54 | UMNP1008 | Xq23 | CH242-458G8 | 2300 | 475 | 101.68 | 118.75 | |||
| 55 | Xq24 | CH242-105E5 | 2454 | 440 | 107.17 | 126.14 | 85 | 101.5 | 87.4 | |
| 56 | Xq24 | CH242-238J16 | 2650 | 304 | 112.30 | 132.31 | 98.4 | 114.1 | 101.9 | |
| 57 | SW707 | 2672 | 286 | 120.8 | 107.9 | |||||
| 58 | SW2137 | 2694 | 273 | 108.1 | ||||||
| 59 | S0218 | Xq25 | CH242-1I19 | 2765 | 211 | 117.02 | 111.4 | 114.4 | ||
| 60 | SW2588 | Xq26 | CH242-394H2 | 3117 | 0 | 125.93 | 150.01 | 159.7 | 128.4 |
1The most likely marker order was determined as the common order shared by most of maps.
2Markers placed on both INRA and JXAU genetic maps are indicated in bold letter, while gene-based markers are shown in italics.
3Pig clones were picked if their available sequences matched marker sequences through blast analysis at Sanger Center's website http://www.sanger.ac.uk.
4IMpRH1 (7000-rad) map was constructed by using Cathagene software.
5Positions of markers were determined by using the reference map of INRA2006 http://rhdev.toulouse.inra.fr/Do=Maps. This map was not oriented, and 0 cR corresponds the the last marker at the end of Xq arm.
6Locations of pig clones have been provided by UCSC Genome Browser http://pre.ensembl.org/Sus_scrofa_map/Location/Genome
7Placement information about homologous human sequences for porcine BAC end sequences is available at Sanger Center's website.
8Bold numbers indicate that the marker orders in two segments (UMNP71-UMNP1218 and ACSL4I3B359M-MCST96O22) on SSC-X clone map are inconsistent with those on the RH map, genetic maps and HSA-X physical map.
9Bold numbers indicate that the markers (SW2476, SW259, SW1994, SW1426 and SW1522) were in reverse order on the USDA-MARC map versus the current genetic maps or other maps.
Figure 1The overall recombinational landscape of porcine X chromosome and intervals with individual heterogeneity of recombination. The top part of this figure represents the genetic position of makers placed on both genetic maps of INRA and JXAU populations compare to the physical position of pig clone map. Markers with a star were used in the initial genotyping experiment. SW259 is located near the centromere. The slope of the curves provides an estimate of the local recombination rate. The patterns for the two populations are similar over the whole chromosome, except for the region from SW980 to SW1903 (gray lines). A (SW2456-UMNP1174), C (SW1426-MCSE347J6) and D (SW1608-S0218-SW2588) delimit three regions of high recombination rates; B (SW259-SW1994-UMNP71) is a recombination coldspot. Heterogeneity of recombination fraction among F1 females was observed for four intervals, including LH-C (UMNP71-SW1943), LH-1 (SW1903-SW2456), LH-2 (SW1608-S0218) and LH-3 (SW1943-SW1608). LH-1 and LH-2 were observed only in the INRA population, and LH-3 was specific to JXAU population, while LH-C was detected in both populations. The lower part presents a more detailed analysis of the recombination patterns in the LH-C interval among 4 F1 full-sisters from INRA population. Females 910002, 910009, 910010 who inherited the same maternal haplotype showed higher recombination rates compared with 910013, who inherited the other maternal haplotype, or compared with the average of the whole population. Number of meioses analysed for each female is presented between parentheses. LH-C could be further narrowed down to a sub-interval UMNP891-UMNP93, flanked by two vertical dash lines.
Variability of recombination fraction (θ) in SSC-X regions of >10 cM among INRA F1 sows.
| No. of sub-family1 | F1 sows | Number of offspring | Marker intervals2 | |||||
|---|---|---|---|---|---|---|---|---|
| θ | θ | θ | θ | θ | θ | |||
| 1 | 910002 | 76 | NA3 | NA | 0.184 | 0.105 | 0.158 | |
| 910009 | 72 | NA | NA | 0.127 | 0.085 | 0.086 | ||
| 910010 | 96 | NA | NA | 0.106 | 0.137 | 0.108 | ||
| 910013 | 55 | NA | NA | 0.109 | 0.164 | 0.127 | ||
| 2 | 910014 | 83 | 0.228 | 0.316 | 0.241 | 0.253 | 0.146 | 0.064 |
| 910016 | 38 | 0.184 | 0.342 | 0.132 | 0.211 | 0.132 | 0.184 | |
| 910020 | 69 | 0.206 | 0.232 | 0.159 | 0.159 | 0.159 | 0.059 | |
| 3 | 910018 | 45 | 0.231 | 0.154 | 0.077 | 0.222 | 0.133 | 0.308 |
| 4 | 910069 | 62 | 0.213 | 0.295 | 0.161 | 0.145 | 0.097 | 0.210 |
| 910071 | 68 | 0.246 | 0.123 | 0.154 | 0.206 | 0.132 | 0.091 | |
| 910072 | 63 | 0.206 | 0.111 | 0.175 | 0.206 | 0.143 | 0.143 | |
| 910074 | 83 | 0.241 | 0.190 | 0.177 | 0.120 | 0.181 | 0.157 | |
| 5 | 910084 | 50 | 0.190 | 0.190 | 0.190 | 0.280 | NA | NA |
| 910086 | 27 | 0.222 | 0.231 | 0.269 | 0.148 | NA | NA | |
| 6 | 910095 | 62 | 0.177 | 0.113 | 0.210 | 0.242 | 0.081 | 0.161 |
| 910096 | 42 | 0.171 | 0.250 | 0.175 | 0.262 | 0.024 | 0.073 | |
| 910097 | 37 | 0.243 | 0.081 | 0.027 | 0.189 | 0.189 | 0.054 | |
| Kosambi distance (cM) | 22,86 | 21,63 | 16.58 | 24.20 | 13.17 | 12.80 | ||
| Morton test | 2,46 | 28.43 | 20.11 | 37.10 | 14.17 | 24.66 | ||
| df | 12 | 12 | 16 | 16 | 14 | 14 | ||
| 0.998 | 0.005 | 0.216 | 0.002 | 0.437 | 0.038 | |||
1Each sub-family consists of F1 full-sisters.
2The recombination coldspot SW259-UMNP71 was not considered.
3Not applicable because animal is not a double-heterozygote for both flanking markers.
4The θ of the F1 full-sisters within the first subfamily for the interval UMNP71-SW1943 are highlighted in bold because they showed the largest difference in θ (P = 0.0004).
5Probability for inter-individual variability of θ.
Variability of recombination fraction (θ) for the UMNP891-UMNP93 interval among INRA F1 female individuals, and among groups of females grouped according to their maternal and paternal haplotypes1.
| No. of sub-family2 | F1 sows | Paternal haplo-type | Maternal haplo-type | N | θ | F1 maternal haplo-type | N | θ | F1 paternal haplo-type | N | θ |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 910002 | 2413 | 1122 | 76 | 1122 | 243 | 0.103 | 2413 | 574 | 0,059 | |
| 910009 | 2413 | 1122 | 72 | 1222 | 526 | 0.055 | 5113 | 235 | 0,055 | ||
| 910010 | 2413 | 1122 | 95 | 3221 | 38 | 0.105 | 5413 | 141 | 0,043 | ||
| 910013 | 2413 | 4311 | 55 | 4311 | 138 | 0.007 | 6323 | 78 | 0,090 | ||
| 2 | 910014 | 5113 | 1222 | 83 | 0.096 | 5221 | 83 | 0.012 | |||
| 910016 | 5113 | 3221 | 38 | 0.105 | |||||||
| 910020 | 5113 | 1222 | 68 | 0.015 | |||||||
| 3 | 910018 | 5113 | 4311 | 46 | 0 | ||||||
| 4 | 910069 | 2413 | 1222 | 62 | 0.032 | ||||||
| 910071 | 2413 | 1222 | 68 | 0.044 | |||||||
| 910072 | 2413 | 1222 | 63 | 0.048 | |||||||
| 910074 | 2413 | 5221 | 83 | 0.012 | |||||||
| 5 | 910084 | 6323 | 1222 | 51 | 0.118 | ||||||
| 910086 | 6323 | 1222 | 27 | 0.037 | |||||||
| 6 | 910095 | 5413 | 1222 | 62 | 0.048 | ||||||
| 910096 | 5413 | 1222 | 42 | 0.048 | |||||||
| 910097 | 5413 | 4311 | 37 | 0.027 | |||||||
| Kosambi distance (cM) | 5.86 | 5.86 | 5.86 | ||||||||
| Morton test | 39.24 | 23.61 | 1.96 | ||||||||
| Df | 16 | 4 | 3 | ||||||||
| 0.0010 | 0.0001 | 0.5800 | |||||||||
1In the region UMNP891-UMNP93, 4 microsatellite markers (UMNP891, MCSE347J6, SW1522, UMNP93) and 7 SNPs were genotyped. For simplicity, we indicated the haplotypes with only microsatellites alleles because they reveal all individual haplotypes formed by all markers analysed on these animals.
2Each sub-family consists of F1 full-sisters.
3The θ of the F1 full-sisters within the first subfamily are highlighted in bold because they showed the largest difference in θ (P = 0.0026).
Variability of recombination fraction (θ) for the MCST96O22-MCSI0244D12 interval among JXAU F1 females grouped by their paternal and maternal haplotypes1.
| JXAU paternal half-sib families (F0 ♂ haplotype = F1 paternal haplotype)2 | N | θ | F1 maternal haplotypes within 0F11 family2 | N | θ | F1 maternal haplotypes within 0F21 family2 | N | θ |
|---|---|---|---|---|---|---|---|---|
| 0F11 {6 [5414] 12} | 518 | 0.071 | 95 | 0.042 | 0F21_1 [1116] 17 | 35 | 0.000 | |
| 0F21 {2 [2514] 12} | 775 | 0.084 | 12 | 0.083 | 0F21_1 [1321] 17 | 60 | 0.167 | |
| 64 | 0.047 | 72 | 0.056 | |||||
| 79 | 0.076 | 0F21_7 [5621] 14 | 24 | 0.042 | ||||
| 0F11_5 [1321] 17 | 137 | 0.095 | 0F21_1 [5121] 13 | 23 | 0.000 | |||
| 0F11_5 [1325] 17 | 18 | 0.056 | 156 | 0.051 | ||||
| 0F11_5 [5321] 14 | 56 | 0.107 | 0F21_1 [5225] 11 | 12 | 0.083 | |||
| 0F11_5 [5325] 17 | 20 | 0.150 | 133 | 0.120 | ||||
| 37 | 0.000 | 0F21_1 [5341] 38 | 22 | 0.227 | ||||
| 0F21_5 [1125] 49 | 28 | 0.036 | ||||||
| 153 | 0.065 | |||||||
| 0F21_5 [5121] 14 | 50 | 0.140 | ||||||
| 7 | 0.286 | |||||||
| Kosambi distance (cM) | 7.96 | 7.19 | 8.47 | |||||
| Morton test | 0.67 | 11.12 | 30.59 | |||||
| df | 1 | 8 | 12 | |||||
| 0.414 | 0.195 | 0.002 | ||||||
| 0.090 | 0.006 | |||||||
1The haplotypes are formed by microsatellite markers (MCST96O22, UMNP891, MCSE347J6, SW1522, UMNP93, UMNP870, MCSI0244D12) within the interval of interest.
2Maternal haplotypes in bold are common to F1 females from both 0F11 and 0F21 families. The number between brackets represents the haplotype over the core UMNP891-UMNP93 interval.
3The pr values are determined after removing the haplotypes with <30 meioses.