Performance of a speckle interferometer

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dc.creatorSaha, S K
dc.creatorJayarajan, A P
dc.creatorSudheendra, G
dc.creatorChandra, A Umesh
dc.date1999-10-28
dc.date.accessioned2026-07-07T02:34:06Z
dc.date.available2026-07-07T02:34:06Z
dc.descriptionAn interferometer system for use at the 2.34 meter Vainu Bappu Telescope (VBT), situated at Vainu Bappu Observatory (VBO), Kavalur, to obtain speckle-grams of astronomical objects in the visible wavelength, has been developed. Laboratory tests of resultant intensity distributions due to a point source, with phase modulation screens, as well as the images obtained using this interferometer at the cassegrain end of the said telescope are discussed.
dc.description10 pages tex files including figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9910507
dc.identifierhttp://arxiv.org/abs/astro-ph/9910507
dc.identifierBull. Astron. Soc. Ind., (1997), 25, 379-387
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15111
dc.subjectAstrophysics
dc.titlePerformance of a speckle interferometer
dc.typetext

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