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3-D Spectroscopy with a Fourier Transform Spectrometer

Published online by Cambridge University Press:  12 April 2016

J.P. Maillard
J.P. Maillard*
Affiliation:
Institut d’Astrophysique de Paris- CNRS, Paris, France

Abstract

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With the advent of bidimensional array detectors the throughput advantage of a Fourier Transform Spectrometer (FTS) can be used to create a new type of 3-D spectrometer. The classical multiplex property in the spectral domain of a FTS is multiplied by the number of pixel of the array. The points of the entrance field are all observed in parallel. After discussing the properties of this instrument, the coupling of the FTS of the CFH Telescope to a camera equipped with a NICMOS 3 array is described. With this combination, spectro-imaging in any bandpass between 1 and 2.5 µm is possible within a circular 24” field of view, with a scale of 0.33”/pixel, at seeing-limited spatial resolution. Any spectral resolution is choosable up to 30,000. Illustrations are given by a study of the dark side of Venus at 1.27 µm and of planetary nebulae at 2 µm. Many other objects can benefit from this observing mode in the near infrared. Further developments of this 3-D technique are discussed.

Type
4. Fourier Transform Spectroscopy
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 316 - 327
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Bacon, R., Adam, G., Baranne, A., Courtes, G., Dubet, D., Dubois, J.P., Georgelin, Y., Monnet, G., Pecontal, E., and Urios, J., 1988, in Very Large Telescope and their Instrumentation, ESO Conference No. 30, vol. II, p. 1185 Google Scholar
Bézard, B., de Bergh, C., Crisp, D., and Maillard, J- P, 1990, Nature, 345, 508 Google Scholar
Clark, C.C., Simons, D.A., and Massey, S., 1994, in Infrared Astronomy with Arrays: the next generation, Ian McLean, (ed), Kluwer, vol. 190, 283 Google Scholar
Courtes, G., 1960, Ann. d’Astrophysique, 23, 96 Google Scholar
Cox, P., Maillard, J.P., Forveille, T., Simons, D., Guilloteau, S., Huggins, P.J., Omont, A., and Bachiller, R., 1994, this conferenceGoogle Scholar
Maillard, J.P., 1988, in Very Large Telescope and their Instrumentation, ESO Conference No. 30, vol. II, p. 1243 Google Scholar
Maillard, J.P. and Michel, G., 1982, in Instrumentation for Astronomy with Large Optical Telescopes, IAU Colloquium No. 67, Humphries, C.M. (ed), D. Reidel (Pub), vol. 92, 213 Google Scholar
Maillard, J.P. and Simons, D., 1992, in Solar Physics and Astrophysics at Interferometric Resolution, ESA Workshop, Damé, L. and Guyenne, T.D (ed), ESA SP-344, 205 Google Scholar
Maillard, J.P., Bézard, B., Domisse, L., Crisp, D. and Simons, D., 1993, B.A.A.S, 25, 1095 Google Scholar
Smith, H.A., Larson, H.P., and Fink, U., 1981, Ap. J., 244, 835 CrossRefGoogle Scholar