peakfit(x, ...)# S3 method for default
peakfit(x, k = "auto", sigdig = 2, log = TRUE, ...)
# S3 method for fissiontracks
peakfit(x, k = 1, exterr = TRUE, sigdig = 2,
log = TRUE, ...)
# S3 method for UPb
peakfit(x, k = 1, type = 4, cutoff.76 = 1100,
cutoff.disc = c(-15, 5), exterr = TRUE, sigdig = 2, log = TRUE, ...)
# S3 method for ArAr
peakfit(x, k = 1, exterr = TRUE, sigdig = 2, log = TRUE,
i2i = FALSE, ...)
# S3 method for ReOs
peakfit(x, k = 1, exterr = TRUE, sigdig = 2, log = TRUE,
i2i = TRUE, ...)
# S3 method for SmNd
peakfit(x, k = 1, exterr = TRUE, sigdig = 2, log = TRUE,
i2i = TRUE, ...)
# S3 method for RbSr
peakfit(x, k = 1, exterr = TRUE, sigdig = 2, log = TRUE,
i2i = TRUE, ...)
# S3 method for UThHe
peakfit(x, k = 1, sigdig = 2, log = TRUE, ...)
[2 x n]
matrix with measurements and their
standard errors, or an object of class fissiontracks
,
UPb
, ArAr
, ReOs
, SmNd
, RbSr
or UThHe
'auto'
automatically
selects the optimal number of components (up to a maximum of 5)
using the Bayes Information Criterion (BIC).type
=1), the
\(^{206}\)Pb/\(^{238}\)U age (type
=2), the
\(^{207}\)Pb/\(^{206}\)Pb age (type
=3), the
\(^{207}\)Pb/\(^{206}\)Pb-\(^{206}\)Pb/\(^{238}\)U age
(type
=4), or the (Wetherill) concordia age (type
=5)type=4
.cutoff.76
) or
between the \(^{206}\)Pb/\(^{238}\)U and
\(^{207}\)Pb/\(^{206}\)Pb age (if
\(^{206}\)Pb/\(^{238}\)U > cutoff.76
). Set
cutoff.disc=NA
if you do not want to use this filter.i2i
to FALSE
uses the default values
stored in settings('iratio',...)
data(examples)
peakfit(examples$FT1,k=2)
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