Fabry–Perot-based Fourier-transform hyperspectral imaging allows multi-labeled fluorescence analysis

2014 ◽  
Vol 53 (14) ◽  
pp. 2983 ◽  
Author(s):  
Marco Pisani ◽  
Massimo Zucco
1980 ◽  
Vol 87 ◽  
pp. 631-632
Author(s):  
Donald N. B. Hall

During the past week we have heard a considerable number of papers dealing with spectroscopic observations in the 1-5μm region of the infrared. I predict that as instruments and detectors continue to improve, such observations will play a major role in the study of interstellar molecules in both molecular clouds and circumstellar clouds around evolved stars. Fourier Transform spectrometers and Fabry Perot interferometers have already yielded spectra of such sources with spectral resolution and radial velocity precision fully comparable to millimeter wave observations. The critical need is to improve the limiting magnitude of such observations by 3-5 stellar magnitudes so that one can study large numbers of sources rather than the few brightest in each class.


2008 ◽  
Vol 16 (4) ◽  
pp. 371-380 ◽  
Author(s):  
Nathalie Gorretta ◽  
Gilles Rabatel ◽  
Jean-Michel Roger ◽  
Christophe Fiorio ◽  
Camille Lelong ◽  
...  

2020 ◽  
Vol 35 (1) ◽  
pp. 117-125 ◽  
Author(s):  
Songyue Shi ◽  
Kevin Finch ◽  
Yue She ◽  
Gerardo Gamez

The optimization of a Fourier transform-based Abel's inversion algorithm allows the reconstruction of high-fidelity radially resolved OES images from SPS-PbHSI acquisition for plasma diagnostics for the first time.


1984 ◽  
Vol 79 ◽  
pp. 515-517
Author(s):  
Paul Atherton

Imaging Spectroscopy is a technique in which a spectrum is obtained for each spatial resolution element across a wide field. The data is essentially 3-D, and may be viewed as a series of monochromatic images, or as a two dimensional array of spectra. A device generating such data may be called an imaging spectrometer. In a previous paper (Atherton, 1983 SPIE 445, 535) three different imaging spectrometers - based on grating, Fabry-Perot and Fourier Transform devices - were compared in terms of their ability to obtain spectral and spatial information over a wide field and broad band, to the same spectral resolution and S/N ratio, using the same detector array. From such a study it is clear that interferometer based devices are significantly faster than conventional grating spectrographs.


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