read.spe.xml

filename

- whether the result should be a pretty-printed XML object. Requires
package <code>XML</code>.

as.xml.object

- determines behavior when file does not
contain XML footer. By default throws error message

stop.if.old.fmt

The new SPE file format, introduced in 2012, was designed to be backwards compatible with the
previous format 2.5. The most prominent change is the new plain text XML footer holding vast
experimental metadata that gets attached at the end of the file. Thus, the file contains 3
blocks: a 4100-bytes long binary header, a chunk with spectral data, and the XML footer.
This function retrieves the XML footer, if it is available, and by default throws error otherwise.

Comfortable ways to work with hyperspectral data sets.
I.e. spatially or time-resolved spectra, or spectra with any other kind
of information associated with each of the spectra. The spectra can be data
as obtained in XRF, UV/VIS, Fluorescence, AES, NIR, IR, Raman, NMR, MS,
etc. More generally, any data that is recorded over a discretized variable,
e.g. absorbance = f (wavelength), stored as a vector of absorbance values
for discrete wavelengths is suitable.

Claudia Beleites

hyperSpec

Work with Hyperspectral Data, i.e. Spectra + Meta Information
(Spatial, Time, Concentration, ...)

Valter Sergo

Alois Bonifacio

Marcel Dahms

Bj<c3><b6>rn Egert

Simon Fuller

Vilmantas Gegzna

Rustam Guliev

Bryan Hanson

Michael Hermes

Martin Kammer

Roman Kiselev

Sebastian Mellor

read.spe.xml function

Read XML footer from SPE file format version 3.0 — read.spe.xml

Read XML footer from SPE file format version 3.0

read.spe.xml: Read XML footer from SPE file format version 3.0

Description

Usage

Arguments

Value