The phrase "absolute spectrum" is correct and usable in written English.
It can be used in contexts related to physics, optics, or any field discussing a complete range of wavelengths or frequencies.
Example: "The absolute spectrum of the light source was analyzed to determine its color composition."
Alternatives: "complete spectrum" or "full spectrum".
Third, features that model the shape of the power spectrum as a 1/ f-curve as well as the absolute spectrum in the α range are discriminative.
Otherwise, almost no appreciable changes are seen in the spectral shape of H135A compared to that of the wild type except for differences in the amplitude of the bands in the amide I and II regions (1700 1600 and 1600 1500 cm–1, respectively), where strong absorbance by these bands in the absolute spectrum can compromise the linearity in the difference spectrum.
In this paper, methods of obtaining absolute spectra from the non-acoustically treated Markham wind tunnel at the University of Cambridge are discussed.
Finally, a dipole beamforming vector is used to account for the directivity of the landing gear noise, leading to good agreement between absolute spectra from the differently sized arrays.
The analysis of the absolute spectra obtained for NO-covered Pt(111) and Rh(111) electrodes shows a linear variation of the band center frequency of linearly bonded NO with slopes of 65 and 20cm−1 V−1, respectively.
We have obtained the absolute spectra of H and He by analyzing data collected by a series of annual flights of the Balloon borne Experiment with a Superconducting solenoid Spectrometer payload.
It presents spectral theory from a dynamical systems and functional analytic point of view, including essential and absolute spectra, and develops general nonlinear stability results for dissipative and Hamiltonian systems.
Subsequently, absolute spectra were computed via a fast Fourier transform (FFT) for each segment.
Result *.txt files were exported to a data server with absolute spectra intensities and further processed by the BinBase algorithm [32] for removing inconsistent and noisy spectra.
An isosbestic point was observed at 405 nm in the absolute spectra upon conversion from low to high spin.
Fig. 5 shows the results and the inset compares the absolute spectra for P, F & O in the NIR region.
