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dc.date.accessioned 2020-06-25T12:21:32Z
dc.date.available 2020-06-25T12:21:32Z
dc.date.issued 1973
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/99079
dc.description.abstract Of the different ways to introduce the Schmidt correction of the camera in a spectrograph, the case was studies in which it is effected in the collimator. Equations which describe the form of the wavefront at one side of the grating as function of the form at the other side were found. The sixth order terms in the correction to compensate for the deformation of the wave front in the path from the collimator to the grating and to the mirror were also found. The aberrations for a correction which is symmetrical around* the collimator axis were calculated. The limit of camera aperture for which this aberrations are tolerable is between F/D = 4 and F/D = 3 according to the size and number of lines of the grating. Este trabajo será publicado en Óptica Acta. en
dc.language es es
dc.subject Galaxias es
dc.title Aberrations of spectrographs with the correction of the Schmidt camera effected in the collimator en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person de Novarini, L.R. es
sedici.creator.person Platzeck, R. es
sedici.creator.person Simón, J.M. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 17 es


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