... | ... |
@@ -52,7 +52,7 @@ CNE(assembly1Fn=character(1), assembly2Fn=character(1), |
52 | 52 |
\item{CNE12}{Object of class \code{"GRangePairs"}: |
53 | 53 |
The preliminary CNEs from axt file with assembly1 as reference.} |
54 | 54 |
\item{CNE21}{Object of class \code{"GRangePairs"}: |
55 |
- The preliminart CNEs from axt file with assembly2 as reference.} |
|
55 |
+ The preliminary CNEs from axt file with assembly2 as reference.} |
|
56 | 56 |
\item{CNEMerged}{Object of class \code{"GRangePairs"}: |
57 | 57 |
The CNEs after merging CNE1 and CNE2.} |
58 | 58 |
\item{CNEFinal}{Object of class \code{"GRangePairs"}: |
... | ... |
@@ -33,20 +33,20 @@ |
33 | 33 |
} |
34 | 34 |
\item{background}{ |
35 | 35 |
\code{character}(1): |
36 |
- can be "chromosome" or "genome". When slice the CNE density, |
|
36 |
+ can be "chromosome" or "genome". When using \code{slice} for the CNE density, |
|
37 | 37 |
the background is calculated on a per-chromosome or whole-genome basis. |
38 | 38 |
} |
39 | 39 |
\item{minCNEs}{ |
40 |
- \code{integer}(1): the minimal number of CNEs that a GRB need to have. |
|
40 |
+ \code{integer}(1): the minimal number of CNEs that a GRB needs to have. |
|
41 | 41 |
} |
42 | 42 |
} |
43 | 43 |
\details{ |
44 |
- First we calculated the CNE densities from the CNEs. |
|
44 |
+ First we calculate the CNE densities from the CNEs. |
|
45 | 45 |
Then we segment the regions according to the values of CNE densities. |
46 | 46 |
The regions with CNE densities above the expected CNE densities * ratio are |
47 | 47 |
considered as putative GRBs. |
48 |
- Of course, the putative GRBs that do not encompass any gene are filtered out. |
|
49 |
- Finanlly, the GRBs that have fewered than \code{minCNEs} number of CNEs will |
|
48 |
+ Putative GRBs that do not encompass any gene are filtered out. |
|
49 |
+ Finally, the GRBs that have fewer than \code{minCNEs} number of CNEs will |
|
50 | 50 |
be filtered out. |
51 | 51 |
} |
52 | 52 |
\value{ |
... | ... |
@@ -6,8 +6,8 @@ |
6 | 6 |
} |
7 | 7 |
\description{ |
8 | 8 |
CNE widths can follow heavy tailed distribution that are associated with power-laws. |
9 |
- This function plot the reverse cumulative density distribution of CNE widths, |
|
10 |
- and fit a discrete power-law distribution. |
|
9 |
+ This function plots the reverse cumulative density distribution of CNE widths, |
|
10 |
+ and fits a discrete power-law distribution. |
|
11 | 11 |
Goodness of fit can also be evaluated. |
12 | 12 |
} |
13 | 13 |
\usage{ |
... | ... |
@@ -1,10 +1,10 @@ |
1 | 1 |
\name{read.rmskFasta} |
2 | 2 |
\alias{read.rmskFasta} |
3 | 3 |
\title{ |
4 |
- Read a soft reoeat masked fasta |
|
4 |
+ Read a soft repeat masked fasta |
|
5 | 5 |
} |
6 | 6 |
\description{ |
7 |
- Read a soft repeat masked fasta file into a \code{GRanges}. |
|
7 |
+ Read a soft repeat masked fasta file into a \code{GRanges} object. |
|
8 | 8 |
} |
9 | 9 |
\usage{ |
10 | 10 |
read.rmskFasta(fn) |
... | ... |
@@ -5,7 +5,7 @@ |
5 | 5 |
Read the cne file from Ancora format. |
6 | 6 |
} |
7 | 7 |
\description{ |
8 |
- Read the Ancora CNE file into a \code{GRanges} or \code{GRangePairs}. |
|
8 |
+ Read the Ancora CNE file into a \code{GRanges} or \code{GRangePairs} object. |
|
9 | 9 |
} |
10 | 10 |
\usage{ |
11 | 11 |
readAncora(fn, assembly=NULL, tAssemblyFn=NULL, qAssemblyFn=NULL) |
... | ... |
@@ -6,7 +6,7 @@ |
6 | 6 |
} |
7 | 7 |
\description{ |
8 | 8 |
Query the SQLite database based on chromosome, |
9 |
-coordinates and some other criterias. |
|
9 |
+coordinates and some other criteria. |
|
10 | 10 |
Primarily not intended to be used directly. |
11 | 11 |
For the CNE density plot, \code{fetchCNEDensity} function should be used. |
12 | 12 |
} |
... | ... |
@@ -15,7 +15,7 @@ |
15 | 15 |
\item{distance}{ |
16 | 16 |
It can be "far", "medium" or "close". It defines the scoring matrix used in |
17 | 17 |
\emph{lastz} aligner. |
18 |
- Generally, if two species are close to each other at human and chimp level, |
|
18 |
+ Generally, if two species are close to each other, for example human and chimp, |
|
19 | 19 |
"close" should be used. |
20 | 20 |
If two species have a divergence time of 100 MYA, "far" should be used. |
21 | 21 |
In other cases, "medium" should be used. |