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 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, ...)
X
Y
X
and Y
OR
an object of class ArAr
, ReOs
, RbSr
or
SmNd
TRUE
to show grain numbers)TRUE
, plots \(^{36}\)Ar/\(^{40}\)Ar
vs. \(^{39}\)Ar/\(^{40}\)Ar. If FALSE
, plots
\(^{40}\)Ar/\(^{36}\)Ar vs. \(^{39}\)Ar/\(^{36}\)Ar.FALSE
, suppresses the graphical outputplot=FALSE
, returns a list with the following items:
a
or, if x
has class
ArAr
, the atmospheric \(^{40}\)Ar/\(^{36}\)Ar ratio and
its standard errordata(examples)
isochron(examples$ArAr)
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