1.1.5 (#10)

* Drop C++11 requirement
* Drop citEntry
* Drop personList
* Fix README

Author: egarpor

CRAN-SUBMISSION

@@ -1,3 +1,3 @@
-Version: 1.1.4
-Date: 2022-11-07 19:22:17 UTC
-SHA: 08f5e6db576460ccb5249f795e2a8aac669f975b
+Version: 1.1.5
+Date: 2023-08-19 00:23:24 UTC
+SHA: 38368f4f9475e882c076efe63226f1ee0547fbfe

DESCRIPTION

@@ -1,8 +1,8 @@
 Package: rotasym
 Type: Package
 Title: Tests for Rotational Symmetry on the Hypersphere
-Version: 1.1.4
-Date: 2022-11-07
+Version: 1.1.5
+Date: 2023-08-19
 Authors@R: c(
     person(given = "Eduardo", family = "García-Portugués",
            role = c("aut", "cre"), email = "[email protected]",
@@ -28,5 +28,5 @@ LinkingTo: Rcpp, RcppArmadillo
 URL: https://github.com/egarpor/rotasym
 BugReports: https://github.com/egarpor/rotasym
 Encoding: UTF-8
-RoxygenNote: 7.2.0
+RoxygenNote: 7.2.3
 Roxygen: list(old_usage = TRUE)

NEWS.md

@@ -50,3 +50,7 @@
 * Fix warning in r-devel-linux-x86_64-fedora-clang and  r-devel-linux-x86_64-debian-clang.
 * Fix bug in `kde_level_set()` (example).
 
+# rotasym 1.1.5
+
+* Drop C++11 requirement to adhere to new CRAN policies.
+* Drop `personList()` and `citEntry()`.

README.Rmd

@@ -72,7 +72,7 @@ set.seed(123456789)
 data_0 <- r_vMF(n = n, mu = theta, kappa = 1)
 ```
 
-### Specified-$\boldsymbol{\theta}$ case
+### Specified-θ case
 
 ```{r, specified}
 # theta known
@@ -81,7 +81,7 @@ test_rotasym(data = data_0, theta = theta, type = "loc_vMF")
 test_rotasym(data = data_0, theta = theta, type = "hyb_vMF")
 ```
 
-### Unspecified-$\boldsymbol{\theta}$ case
+### Unspecified-θ case
 
 ```{r, unspecified}
 # theta unknown (employs the spherical mean as estimator)
@@ -93,9 +93,9 @@ test_rotasym(data = data_0, type = "hyb_vMF")
 ## Data application: test for the rotational symmetry of sunspots
 
 The data application in García-Portugués, Paindaveine and Verdebout (2020) can
-be reproduced through the script [sunspots-births.R](https://github.com/egarpor/rotasym/blob/master/data-raw/sunspots-births.R) (data gathering and preprocessing) and the code snippet below.
+be replicated through the script [sunspots-births.R](https://github.com/egarpor/rotasym/blob/master/data-raw/sunspots-births.R) (data gathering and preprocessing) and the code snippet below.
 
-```{r, sunspots_births}
+```{r, sunspots_births, fig.show = 'hold'}
 # Load data
 data("sunspots_births")
 sunspots_births$X <-

README.md

@@ -5,8 +5,8 @@ GPLv3](https://img.shields.io/badge/license-GPLv3-blue.svg)](https://www.gnu.org
 [![R build
 status](https://github.com/egarpor/rotasym/workflows/R-CMD-check/badge.svg)](https://github.com/egarpor/rotasym/actions)
 [![](https://www.r-pkg.org/badges/version/rotasym?color=green)](https://cran.r-project.org/package=rotasym)
-[![](http://cranlogs.r-pkg.org/badges/grand-total/rotasym?color=green)](https://cran.r-project.org/package=rotasym)
-[![](http://cranlogs.r-pkg.org/badges/last-month/rotasym?color=green)](https://cran.r-project.org/package=rotasym)
+[![](http://cranlogs.r-pkg.org/badges/grand-total/rotasym)](https://cran.r-project.org/package=rotasym)
+[![](http://cranlogs.r-pkg.org/badges/last-month/rotasym)](https://cran.r-project.org/package=rotasym)
 
 <!-- <img src="" alt="rotasym  hexlogo" align="right" width="200" style="padding: 0 15px; float: right;"/> -->
 
@@ -56,7 +56,7 @@ set.seed(123456789)
 data_0 <- r_vMF(n = n, mu = theta, kappa = 1)
 ```
 
-### Specified-**θ** case
+### Specified-θ case
 
 ``` r
 # theta known
@@ -80,7 +80,7 @@ test_rotasym(data = data_0, theta = theta, type = "hyb_vMF")
 #> Q_hyb_vMF = 46.329, df = 53, p-value = 0.7297
 ```
 
-### Unspecified-**θ** case
+### Unspecified-θ case
 
 ``` r
 # theta unknown (employs the spherical mean as estimator)
@@ -107,7 +107,7 @@ test_rotasym(data = data_0, type = "hyb_vMF")
 ## Data application: test for the rotational symmetry of sunspots
 
 The data application in García-Portugués, Paindaveine and Verdebout
-(2020) can be reproduced through the script
+(2020) can be replicated through the script
 [sunspots-births.R](https://github.com/egarpor/rotasym/blob/master/data-raw/sunspots-births.R)
 (data gathering and preprocessing) and the code snippet below.
 
@@ -183,12 +183,6 @@ example("sunspots_births")
 #> snspt_+               radius = 1, type = "s", col = "lightblue", alpha = 0.25,
 #> snspt_+               lit = FALSE)
 #> snspt_+ }
-#> Error in dyn.load(dynlib <- getDynlib(dir)) : 
-#>   unable to load shared object '/Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so':
-#>   dlopen(/Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so, 6): Symbol not found: _hb_buffer_add_utf8
-#>   Referenced from: /Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so
-#>   Expected in: flat namespace
-#>  in /Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so
 #> 
 #> snspt_> n_cols <- 100
 #> 
@@ -199,12 +193,6 @@ example("sunspots_births")
 #> snspt_> if (requireNamespace("rgl")) {
 #> snspt_+   rgl::points3d(sunspots_23$X, col = viridisLite::viridis(n_cols)[cuts])
 #> snspt_+ }
-#> Error in dyn.load(dynlib <- getDynlib(dir)) : 
-#>   unable to load shared object '/Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so':
-#>   dlopen(/Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so, 6): Symbol not found: _hb_buffer_add_utf8
-#>   Referenced from: /Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so
-#>   Expected in: flat namespace
-#>  in /Library/Frameworks/R.framework/Versions/4.1-arm64/Resources/library/rgl/libs/rgl.so
 #> 
 #> snspt_> # Spörer's law: sunspots at the beginning of the solar cycle (dark blue
 #> snspt_> # color) tend to appear at higher latitutes, gradually decreasing to the
@@ -218,76 +206,75 @@ example("sunspots_births")
 #> snspt_> plot(kde <- density(x = V, bw = h, n = 2^13, from = -1, to = 1), col = 1,
 #> snspt_+      xlim = c(-1, 1), ylim = c(0, 3), axes = FALSE, main = "",
 #> snspt_+      xlab = "Cosines (latitude angles)", lwd = 2)
+#> 
+#> snspt_> at <- seq(-1, 1, by = 0.25)
+#> 
+#> snspt_> axis(2); axis(1, at = at)
+#> 
+#> snspt_> axis(1, at = at, line = 1, tick = FALSE,
+#> snspt_+      labels = paste0("(", 90 - round(acos(at) / pi * 180, 1), "º)"))
+#> 
+#> snspt_> rug(V)
+#> 
+#> snspt_> legend("topright", legend = c("Full cycle", "Initial 25% cycle",
+#> snspt_+                               "Final 25% cycle"),
+#> snspt_+        lwd = 2, col = c(1, viridisLite::viridis(12)[c(3, 8)]))
+#> 
+#> snspt_> # Density for the observations within the initial 25% of the cycle
+#> snspt_> part1 <- sunspots_23$date < quantile(sunspots_23$date, 0.25)
+#> 
+#> snspt_> V1 <- cosines(X = sunspots_23$X[part1, ], theta = c(0, 0, 1))
+#> 
+#> snspt_> h1 <- bw.SJ(x = V1, method = "dpi")
+#> 
+#> snspt_> lines(kde1 <- density(x = V1, bw = h1, n = 2^13, from = -1, to = 1),
+#> snspt_+       col = viridisLite::viridis(12)[3], lwd = 2)
+#> 
+#> snspt_> # Density for the observations within the final 25% of the cycle
+#> snspt_> part2 <- sunspots_23$date > quantile(sunspots_23$date, 0.75)
+#> 
+#> snspt_> V2 <- cosines(X = sunspots_23$X[part2, ], theta = c(0, 0, 1))
+#> 
+#> snspt_> h2 <- bw.SJ(x = V2, method = "dpi")
+#> 
+#> snspt_> lines(kde2 <- density(x = V2, bw = h2, n = 2^13, from = -1, to = 1),
+#> snspt_+       col = viridisLite::viridis(12)[8], lwd = 2)
+#> 
+#> snspt_> # Computation the level set of a kernel density estimator that contains
+#> snspt_> # at least 1 - alpha of the probability (kde stands for an object
+#> snspt_> # containing the output of density(x = data))
+#> snspt_> kde_level_set <- function(kde, data, alpha) {
+#> snspt_+ 
+#> snspt_+   # Estimate c from alpha
+#> snspt_+   c <- quantile(approx(x = kde$x, y = kde$y, xout = data)$y, probs = alpha)
+#> snspt_+ 
+#> snspt_+   # Begin and end index for the potentially many intervals in the level sets
+#> snspt_+   kde_larger_c <- kde$y >= c
+#> snspt_+   run_length_kde <- rle(kde_larger_c)
+#> snspt_+   begin <- which(diff(kde_larger_c) > 0) + 1
+#> snspt_+   end <- begin + run_length_kde$lengths[run_length_kde$values] - 1
+#> snspt_+ 
+#> snspt_+   # Return the [a_i, b_i], i = 1, ..., K in the K rows
+#> snspt_+   return(cbind(kde$x[begin], kde$x[end]))
+#> snspt_+ 
+#> snspt_+ }
+#> 
+#> snspt_> # Level set containing the 90% of the probability, in latitude angles
+#> snspt_> 90 - acos(kde_level_set(kde = kde, data = V, alpha = 0.10)) / pi * 180
+#>            [,1]      [,2]
+#> [1,] -29.448244 -2.455986
+#> [2,]   2.582017 28.123329
+#> 
+#> snspt_> # Modes (in cosines and latitude angles)
+#> snspt_> modes <- c(kde$x[kde$x < 0][which.max(kde$y[kde$x < 0])],
+#> snspt_+            kde$x[kde$x > 0][which.max(kde$y[kde$x > 0])])
+#> 
+#> snspt_> 90 - acos(modes) / pi * 180
+#> [1] -13.69322  16.49001
 ```
 
 <img src="README/README-sunspots_births-1.png" style="display: block; margin: auto;" />
 
-    #> 
-    #> snspt_> at <- seq(-1, 1, by = 0.25)
-    #> 
-    #> snspt_> axis(2); axis(1, at = at)
-    #> 
-    #> snspt_> axis(1, at = at, line = 1, tick = FALSE,
-    #> snspt_+      labels = paste0("(", 90 - round(acos(at) / pi * 180, 1), "º)"))
-    #> 
-    #> snspt_> rug(V)
-    #> 
-    #> snspt_> legend("topright", legend = c("Full cycle", "Initial 25% cycle",
-    #> snspt_+                               "Final 25% cycle"),
-    #> snspt_+        lwd = 2, col = c(1, viridisLite::viridis(12)[c(3, 8)]))
-    #> 
-    #> snspt_> # Density for the observations within the initial 25% of the cycle
-    #> snspt_> part1 <- sunspots_23$date < quantile(sunspots_23$date, 0.25)
-    #> 
-    #> snspt_> V1 <- cosines(X = sunspots_23$X[part1, ], theta = c(0, 0, 1))
-    #> 
-    #> snspt_> h1 <- bw.SJ(x = V1, method = "dpi")
-    #> 
-    #> snspt_> lines(kde1 <- density(x = V1, bw = h1, n = 2^13, from = -1, to = 1),
-    #> snspt_+       col = viridisLite::viridis(12)[3], lwd = 2)
-    #> 
-    #> snspt_> # Density for the observations within the final 25% of the cycle
-    #> snspt_> part2 <- sunspots_23$date > quantile(sunspots_23$date, 0.75)
-    #> 
-    #> snspt_> V2 <- cosines(X = sunspots_23$X[part2, ], theta = c(0, 0, 1))
-    #> 
-    #> snspt_> h2 <- bw.SJ(x = V2, method = "dpi")
-    #> 
-    #> snspt_> lines(kde2 <- density(x = V2, bw = h2, n = 2^13, from = -1, to = 1),
-    #> snspt_+       col = viridisLite::viridis(12)[8], lwd = 2)
-    #> 
-    #> snspt_> # Computation the level set of a kernel density estimator that contains
-    #> snspt_> # at least 1 - alpha of the probability (kde stands for an object
-    #> snspt_> # containing the output of density(x = data))
-    #> snspt_> kde_level_set <- function(kde, data, alpha) {
-    #> snspt_+ 
-    #> snspt_+   # Estimate c from alpha
-    #> snspt_+   c <- quantile(approx(x = kde$x, y = kde$y, xout = data)$y, probs = alpha)
-    #> snspt_+ 
-    #> snspt_+   # Begin and end index for the potentially many intervals in the level sets
-    #> snspt_+   kde_larger_c <- kde$y >= c
-    #> snspt_+   run_length_kde <- rle(kde_larger_c)
-    #> snspt_+   begin <- which(diff(kde_larger_c) > 0)
-    #> snspt_+   end <- begin + run_length_kde$lengths[run_length_kde$values] - 1
-    #> snspt_+ 
-    #> snspt_+   # Return the [a_i, b_i], i = 1, ..., K in the K rows
-    #> snspt_+   return(cbind(kde$x[begin], kde$x[end]))
-    #> snspt_+ 
-    #> snspt_+ }
-    #> 
-    #> snspt_> # Level set containing the 90% of the probability, in latitude angles
-    #> snspt_> 90 - acos(kde_level_set(kde = kde, data = V, alpha = 0.10)) / pi * 180
-    #>            [,1]      [,2]
-    #> [1,] -29.464311 -2.469989
-    #> [2,]   2.568013 28.107467
-    #> 
-    #> snspt_> # Modes (in cosines and latitude angles)
-    #> snspt_> modes <- c(kde$x[kde$x < 0][which.max(kde$y[kde$x < 0])],
-    #> snspt_+            kde$x[kde$x > 0][which.max(kde$y[kde$x > 0])])
-    #> 
-    #> snspt_> 90 - acos(modes) / pi * 180
-    #> [1] -13.69322  16.49001
-
 ## References
 
 García-Portugués, E., Paindaveine, D., and Verdebout, T. (2020). On

README/README-sunspots_births-1.png

@@ -3,25 +3,17 @@ This is a submission to fix the problems shown on https://cran.r-project.org/web
 
 ## Test environments
 
-* local R installation, R 4.1.0
-* ubuntu 16.04 (on travis-ci), R 3.4.0
+* local R installation, R 4.2.2
 * win-builder (release, devel)
-* Windows Server 2008 R2 SP1, R-devel, 32/64 bit (on R-hub)
-* Windows Server 2008 R2 SP1, R-release, 32/64 bit (on R-hub)
-* Windows Server 2008 R2 SP1, R-oldrel, 32/64 bit (on R-hub)
-* Ubuntu Linux 16.04 LTS, R-release, GCC (on R-hub)
-* Fedora Linux, R-devel, clang, gfortran (on R-hub)
-* Debian Linux, R-devel, GCC ASAN/UBSAN (on R-hub)
-* macOS 10.13.6 High Sierra, R-release, brew (on R-hub)
-* macOS 10.13.6 High Sierra, R-release, CRAN's setup (on R-hub)
-* Oracle Solaris 10, x86, 32 bit, R-release (on R-hub)
-* Oracle Solaris 10, x86, 32 bit, R-release, Oracle Developer Studio 12.6 (on R-hub)
-
-On some platforms:
-
-* "Found the following (possibly) invalid URLs" -- double-checked and correctly spelled
+* Windows Server 2022, R-release, 32/64 bit
+* Windows Server 2022, R-devel, 64 bit
+* Windows Server 2022, R-oldrel, 32/64 bit
+* Windows Server 2022, R-patched, 32/64 bit
+* Ubuntu Linux 20.04.1 LTS, R-release, GCC
+* Ubuntu Linux 20.04.1 LTS, R-devel, GCC
+* Debian Linux, R-release, GCC
+* Debian Linux, R-devel, GCC
 
 ## R CMD check results
 
-0 errors | 0 warnings | 0 notes
-
+0 errors | 0 warnings | 0 notes

cran-comments.md

@@ -4,11 +4,12 @@ note <- paste("R package version", meta$Version)
 
 citHeader("To cite rotasym in publications use:")
 
-citEntry(entry = "Manual",
+bibentry(
+  bibtype      = "Manual",
   title        = "{rotasym}: Tests for Rotational Symmetry on the Hypersphere",
-  author       = personList(as.person("Eduardo Garc\\'ia-Portugu\\'es"),
-                   as.person("Davy Paindaveine"),
-                   as.person("Thomas Verdebout")),
+  author       = c(person(given = "Eduardo", family = "García-Portugués"),
+                   person(given = "Davy", family = "Paindaveine"),
+                   person(given = "Thomas", family = "Verdebout")),
   year         = year,
   note         = note,
   url          = "https://CRAN.R-project.org/package=rotasym",
@@ -18,11 +19,12 @@ citEntry(entry = "Manual",
         paste0(note, "."), "https://CRAN.R-project.org/package=rotasym")
 )
 
-citEntry(entry = "Article",
+bibentry(
+  bibtype      = "Article",
   title        = "On optimal tests for rotational symmetry against new classes of hyperspherical distributions",
-  author       = personList(as.person("Eduardo Garc\\'ia-Portugu\\'es"),
-                   as.person("Davy Paindaveine"),
-                   as.person("Thomas Verdebout")),
+  author       = c(person(given = "Eduardo", family = "García-Portugués"),
+                   person(given = "Davy", family = "Paindaveine"),
+                   person(given = "Thomas", family = "Verdebout")),
   journal      = "Journal of the American Statistical Association",
   year         = "2020",
   volume       = "115",

inst/CITATION

@@ -1,6 +1,2 @@
 ## Set PKG_LIBS
 PKG_LIBS = $(LAPACK_LIBS) $(BLAS_LIBS) $(FLIBS)
-
-## With R 3.1.0 or later, you can uncomment the following line to tell R to
-## enable compilation with C++11 (or even C++14) where available
-CXX_STD = CXX11

src/Makevars

@@ -1,6 +1,2 @@
 ## Set PKG_LIBS
 PKG_LIBS = $(LAPACK_LIBS) $(BLAS_LIBS) $(FLIBS)
-
-## With R 3.1.0 or later, you can uncomment the following line to tell R to
-## enable compilation with C++11 (or even C++14) where available
-CXX_STD = CXX11