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Furthermore, phase gaps were detected in all InSAR pairs that include this area (Additional file 1).
Most of these large gaps are located on chromosomes 14 and X, where 36 (SSC14) and 27 (SSCX) large gaps were detected However, there were also chromosomes with no large gaps between the SNPs (chromosomes 2, 3, 6, 10, 12, 16 and 18).
Moreover, four small gaps were detected and in particular, close to the porcine position 64.6 Mb.
The largest gaps were detected in C03, with 30.6 cM between BodCAPS22 and CB10267.
These gaps were detected in all LGs except LG 2, suggesting that such gaps are not restricted to a particular region of the chromosomes.
A total of 785 gaps were detected by GapCloser that cover 1.5 Mb residues of which 197 gaps were completely filled up, leaving only 1.47% (0.73 Mb) gaps inside the 94 scaffolds.
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In addition to the scarcity of observatories, observatory data are not complete, and some important gaps are detected from time to time, so those better selections would have precluded obtaining representative results for the whole seasonal and solar cycle spans.
In the proposed approach, instead of working hard to arrive at a complete description initially, an iterative methodology permits incremental improvements of PKB until only non-relevant gaps are detected.
More recently, a superconducting gap was detected in Li-decorated monolayer graphene using ARPES measurements22 and the data used to suggest a Tc ~ 6 K.
A small, but clear, gap is detected.
When a significant gap is detected compared to this predicted exponential profile, the model order, i.e., the smallest signal eigenvalue, is found.
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