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Simultaneous Bidimensional Spectroscopy of Extened Objects Using Optical Fibers: Application to Seyfert Galaxies

Published online by Cambridge University Press:  12 April 2016

S. Arribas ,
E. Mediavilla ,
A. García Marín ,
B. García Lorenzo  and
J. L. Rasilla
S. Arribas
Affiliation:
Institute de Astrofísica de Canarias, 38200-La Laguna (Tenerife)SPAIN
E. Mediavilla
Affiliation:
Institute de Astrofísica de Canarias, 38200-La Laguna (Tenerife)SPAIN
A. García Marín
Affiliation:
Institute de Astrofísica de Canarias, 38200-La Laguna (Tenerife)SPAIN
B. García Lorenzo
Affiliation:
Institute de Astrofísica de Canarias, 38200-La Laguna (Tenerife)SPAIN
J. L. Rasilla
Affiliation:
Institute de Astrofísica de Canarias, 38200-La Laguna (Tenerife)SPAIN

Abstract

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In this communication we summarize the main characteristics of three optical fiber systems, namely HEXAFLEX, HEXAFLEX-II, and 2D-FIS, developed for performing simultaneous bidimensional spectroscopy of extended objects. They have been used at the 4.2m William Herschel (WHT) and the 2.5m Nordic Optical Telescope (NOT), which are sited at the Observatorio del Roque de los Muchachos. These systems have been used to observe the circumnuclear regions of several Seyfert galaxies. They show clear advantages over other instruments based on more classical techniques, at least for these complex objects of small angular size on the sky. Some examples will be given to illustrate this.

Type
3. Integral Field Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 235 - 238
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Arribas, S., Mediavilla, E. & Rasilla, J.L., 1991, ApJ, 369; p. 260.Google Scholar
Arribas, S. & Mediavilla, E., 1993, ApJ, 410; p. 552.Google Scholar
Arribas, S., Mediavilla, E. & Rasilla, J.L., 1993, in Fiber Optics in Astronomy II (ASP Conf. Ser. 37), ed. Gray, P.M., p. 322.Google Scholar
Barden, S.C. & Wade, R.C., 1988, in Fiber Optics in Astronomy I (ASP Conf. Ser. 3), ed. Barden, S.C., p. 113.Google Scholar
Carter, D., Benn, C.R., Rutten, R.G.M., Breare, J.M., Rudd, P.J., King, D.L., Clegg, R.E.S., Dhillon, V.S., Arribas, S., Rasilla, J.L., Garca, A., Jenkins, C.R. & Charles, P.A., 1993, WHT - ISIS Users’ Manual, Isaac Newton Group, La Palma.Google Scholar
García Marín, A., Rasilla, J.L., Arribas, S. & Mediavilla, E. 1994, to appear in “Instrumentation in Astronomy”, SPIE vol. 2198.Google Scholar
Gray, P.M., Phillips, M.M., Turtle, A.J. & Ellis, R., 1982, Proc. ASA 4 (4), p. 477.Google Scholar
Mediavilla, E., Arribas, S. & Rasilla, J.L., 1992, ApJ, 396; p. 517.Google Scholar
Mediavilla, E. & Arribas, S., 1993a, Nature, vol. 365, p. 420.Google Scholar
Mediavilla, E. & Arribas, S., 1993b, Fiber Optics in Astronomy II (ASP Conf. Ser. 37), ed. Gray, P.M., p. 331.Google Scholar
Vanderriest, C. & Lemonnier, J.-P., 1988, Instrumentation for Ground-Based Optical Astronomy, ed. Robinson, L.B., p. 304.Google Scholar