Slit device for FOCCoS - PFS - Subaru

被引:1
|
作者
de Oliveira, Antonio Cesar [1 ]
Gunn, James E. [2 ]
de Oliveira, Ligia Souza [3 ]
de Arruda, Marcio Vital [1 ]
Marrara, Lucas Souza [3 ]
dos Santos, Leandro Henrique [1 ]
Ferreira, Decio [1 ]
dos Santos, Jesulino Bispo [1 ]
Rosa, Josimar Aparecido [1 ]
Ribeiro, Flavio Felipe [1 ]
Vilaca, Rodrigo de Paiva [1 ]
Verducci Junior, Orlando [1 ]
Sodre Junior, Laerte [4 ]
de Oliveira, Claudia Mendes [4 ]
机构
[1] MCT LNA, Lab Nacl Astrofis, Itajuba, MG, Brazil
[2] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[3] OIO Oliveira Instrumentacao Opt LTDA, Sao Paulo, SP, Brazil
[4] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, IAG USP, Sao Paulo, SP, Brazil
关键词
Spectrograph; Optical Fibers; Slit device;
D O I
10.1117/12.2056400
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 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.
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页数:13
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