Plots cogenetic Ar-Ar, Rb-Sr, Sm-Nd, Re-Os or Lu-Hf data as X-Y
scatterplots, fits an isochron curve through them using the
yorkfit
function, and computes the corresponding isochron
age, including decay constant uncertainties.
isochron(x, ...)# S3 method for default
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
line.col = "red", lwd = 2, title = TRUE, ...)
# S3 method for ArAr
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
inverse = TRUE, line.col = "red", lwd = 2, plot = TRUE,
exterr = TRUE, ...)
# S3 method for PbPb
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
inverse = TRUE, line.col = "red", lwd = 2, plot = TRUE,
exterr = TRUE, ...)
# S3 method for RbSr
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
line.col = "red", lwd = 2, plot = TRUE, exterr = TRUE, ...)
# S3 method for ReOs
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
line.col = "red", lwd = 2, plot = TRUE, exterr = TRUE, ...)
# S3 method for SmNd
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
line.col = "red", lwd = 2, plot = TRUE, exterr = TRUE, ...)
# S3 method for LuHf
isochron(x, xlim = NA, ylim = NA, alpha = 0.05,
sigdig = 2, show.numbers = FALSE, ellipse.col = rgb(0, 1, 0, 0.5),
line.col = "red", lwd = 2, plot = TRUE, exterr = TRUE, ...)
EITHER a matrix with the following five columns:
the x-variable
the standard error of X
the y-variable
the standard error of Y
the correlation coefficient of X
and Y
OR
an object of class ArAr
, ReOs
, RbSr
,
SmNd
or LuHf
.
optional arguments
2-element vector with the plot limits of the x-axis
2-element vector with the plot limits of the y-axis
confidence cutoff for the error ellipses
the number of significant digits of the numerical values reported in the title of the graphical output
logical flag (TRUE
to show grain numbers)
background colour of the error ellipses
colour of the isochron line
line width
add a title to the plot?
if TRUE
, plots \(^{36}\)Ar/\(^{40}\)Ar
vs. \(^{39}\)Ar/\(^{40}\)Ar. If FALSE
, plots
\(^{40}\)Ar/\(^{36}\)Ar vs. \(^{39}\)Ar/\(^{36}\)Ar.
if FALSE
, suppresses the graphical output
propagate external sources of uncertainty (J, decay constant)?
if plot=FALSE
, returns a list with the following items:
the intercept of the straight line fit and its standard error
the slope of the fit and its standard error
this either equals a
or, if x
has class
ArAr
, the atmospheric \(^{40}\)Ar/\(^{36}\)Ar ratio and
its standard error
the \(^{40}\)Ar/\(^{39}\)Ar, Re-Os, Rb-Sr or Sm-Nd age and its standard error
# NOT RUN {
data(examples)
isochron(examples$ArAr)
# }
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