Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5311
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dc.contributor.authorKameswara Rao, N-
dc.contributor.authorSriram, S-
dc.contributor.authorGabriel, F-
dc.contributor.authorPrasad, B. R-
dc.contributor.authorSamson, J. P. A-
dc.contributor.authorJayakumar, K-
dc.contributor.authorSrinivasan, R-
dc.contributor.authorMahesh, P. K-
dc.contributor.authorGiridhar, S-
dc.date.accessioned2011-01-21T10:06:44Z-
dc.date.available2011-01-21T10:06:44Z-
dc.date.issued2004-12-
dc.identifier.citationAsian Journal of Physics, Vol. 13, No. 3&4, pp. 267-276en
dc.identifier.urihttp://hdl.handle.net/2248/5311-
dc.description.abstractThe optical design and performance of high resolution fiber-fed echelle spectrometer for the 2.34 meter Vainu Bappu Telescope (VBT) is described. An optical fiber of core 100 J-Lm and length 45 meter is used to link the spectrometer with the telescope. The instrument provides a resolving power of 72,000 (4 Km/s) with a 60 J-Lm slit and provides continuous coverage with gaps for ). < 1 J-Lm. The spectrum is recorded on a thinned back-illuminated Marconi 2048 x 4096, 15 J-Lm square pixel, charge coupled device (CCD) detector. The wavelength coverage in a single order varies from roughly 35Aat ,\ = 4050A(range 4030A- 4065A) to 70A(range 8465A- 8535A).The present overall efficiency of the spectrometer at 6000Ais about 10%. The operation of the spectrometer and object acquisition and guiding at the telescope end is described. Some of the observed spectra from VBT are also illustrated.en
dc.language.isoenen
dc.publisherAnita Publicationsen
dc.rights© Anita Publicationsen
dc.titleFiber-fed echelle spectrometer of the 2.34 meter Vainu Bappu Telescopeen
dc.typeArticleen
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