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dc.contributor.authorde Oliveira, Antonio Cesar-
dc.contributor.authorGunn, James E-
dc.contributor.authorde Oliveira, Ligia Souza-
dc.contributor.authorde Arruda, Marcio Vital-
dc.contributor.authorMarrara, Lucas Souza-
dc.contributor.authordos Santos, Leandro Henrique-
dc.contributor.authorFerreira, Decio-
dc.contributor.authordos Santos, Jesulino Bispo-
dc.contributor.authorRosa, Josimar Aparecido-
dc.contributor.authorRibeiro, Flavio Felipe-
dc.contributor.authorVilaca, Rodrigo de Paiva-
dc.contributor.authorVerducci Junior, Orlando-
dc.contributor.authorSodre Junior, Laerte-
dc.contributor.authorde Oliveira, Claudia Mendes-
dc.date.accessioned2022-01-25T15:00:50Z-
dc.date.available2022-01-25T15:00:50Z-
dc.date.issued2014en_US
dc.identifier.citationde Oliveira, Antonio Cesar, Gunn, James E, de Oliveira, Ligia Souza, de Arruda, Marcio Vital, Marrara, Lucas Souza, dos Santos, Leandro Henrique, Ferreira, Decio, dos Santos, Jesulino Bispo, Rosa, Josimar Aparecido, Ribeiro, Flavio Felipe, Vilaca, Rodrigo de Paiva, Verducci Junior, Orlando, Sodre Junior, Laerte, de Oliveira, Claudia Mendes. (2014). Slit device for FOCCoS - PFS - Subaru. ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION, 9151 (10.1117/12.2056400en_US
dc.identifier.issn0277-786X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1tt4fs6s-
dc.description.abstractThe Fiber Optical Cable and Connector System, “FOCCoS”, subsystem of the Prime Focus Spectrograph, “PFS”, for Subaru telescope, is responsible to feed four spectrographs with a set of optical fibers cables. The light injection for each spectrograph is assured by a convex curved slit with a linear array of 616 optical fibers. In this paper we present a design of a slit that ensures the right direction of the fibers by using masks of micro holes. This kind of mask is made by a technique called electroforming, which is able to produce a nickel plate with holes in a linear sequence. The precision error is around 1-mu m in the diameter and 1-mu m in the positions of the holes. This nickel plate may be produced with a thickness between 50 and 200 microns, so it may be very flexible. This flexibility allows the mask to be bent into the shape necessary for a curved slit. The concept requires two masks, which we call Front Mask, and Rear Mask, separated by a gap that defines the thickness of the slit. The pitch and the diameter of the holes define the linear geometry of the slit; the curvature of each mask defines the angular geometry of the slit. Obviously, this assembly must be mounted inside a structure rigid and strong enough to be supported inside the spectrograph. This structure must have a CTE optimized to avoid displacement of the fibers or increased FRD of the fibers when the device is submitted to temperatures around 3 degrees Celsius, the temperature of operation of the spectrograph. We have produced two models. Both are mounted inside a very compact Invar case, and both have their front surfaces covered by a dark composite, to reduce stray light. Furthermore, we have conducted experiments with two different internal structures to minimize effects caused by temperature gradients. This concept has several advantages relative to a design based on Vgrooves, which is the classical option. It is much easier and quicker to assemble, much cheaper, more accurate, easier to adjust; and it also offers the possibility of making a device much more strong, robust and completely miniaturized.en_US
dc.language.isoen_USen_US
dc.relation.ispartofADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATIONen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleSlit device for FOCCoS - PFS - Subaruen_US
dc.typeConference Articleen_US
dc.identifier.doidoi:10.1117/12.2056400-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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