Focal ratio degradation and transmission in VIRUS-P optical fibers

We have conducted extensive tests of both transmission and focal ratio degradation (FRD) on two integral field units currently in use on the VIRUS-P integral field spectrograph. VIRUS-P is a prototype for the VIRUS instrument proposed for the Hobby-Eberly Telescope at McDonald Observatory. All tests have been conducted at an input f-ratio of F/3.65 and with an 18% central obscuration in order to simulate optical conditions on the HET. Transmission measurements were conducted with narrow-band interference filters (FWHM: 10 nm) at 10 discrete wavelengths (337 to 600 nm), while FRD tests were made at 365 nm, 400 nm and 600 nm. The influence of wavelength, end immersion, fiber type and length on both FRD and transmission is explored. Most notably, we find no wavelength dependence on FRD down to 365 nm. All fibers tested are within the VIRUS instrument specifications for both FRD and transmission. We present the details of our differential FRD testing method and explain a simple and robust technique of aligning the test bench and optical fiber axes to within ±0.1 degrees.

[1]  Andreas Kelz a,et al.  Prototype development of the Integral-Field unit for VIRUS , 2006 .

[2]  Roger Haynes,et al.  Multiple‐Object and Integral Field Near‐Infrared Spectroscopy Using Fibers , 1999 .

[3]  Ian R. Parry,et al.  A method for determining the focal ratio degradation of optical fibres for astronomy , 1994 .

[4]  Ian Robert Parry Optical fibres for integral field spectroscopy , 2006 .

[5]  Andreas Kelz,et al.  Design, construction, and performance of VIRUS-P: the prototype of a highly replicated integral-field spectrograph for HET , 2008, Astronomical Telescopes + Instrumentation.

[6]  William W. Craig,et al.  Measurement of fibers to be used in fiber fed spectroscopy , 1988 .

[7]  J. Schmoll,et al.  Statistical Test of Optical Fibers for Use in PMAS, the Potsdam Multi‐Aperture Spectrophotometer , 2003, astro-ph/0304288.

[8]  G. Ávila Tests of optical fibres for astronomical instrumentation at ESO. , 1988 .

[9]  M. Bershady,et al.  SparsePak: A Formatted Fiber Field Unit for the WIYN Telescope Bench Spectrograph. I. Design, Construction, and Calibration , 2004, astro-ph/0403456.

[10]  Samuel Charles Barden Review of fiber optic properties for astronomical spectroscopy , 1995, Defense, Security, and Sensing.

[11]  Eli Atad-Ettedgui,et al.  Optomechanical Technologies for Astronomy , 2006 .

[12]  Martin M. Roth The Aip Photometric Testbench , 1998 .

[13]  Lawrence W. Ramsey,et al.  Focal ratio degradation in optical fibers of astronomical interest , 1988 .

[14]  D. O. Astronomy,et al.  The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX): Description and Early Pilot Survey Results , 2008, 0806.0183.

[15]  Matthew A. Bershady,et al.  SparsePak: A Formatted Fiber Field Unit for The WIYN Telescope Bench Spectrograph. II. On-Sky Performance , 2005 .

[16]  Joss Bland-Hawthorn,et al.  New age fibers: the children of the photonic revolution , 2004, SPIE Astronomical Telescopes + Instrumentation.

[17]  Frank Grupp,et al.  Measuring the properties of optical fibers: First results from the AIP fiber testbench for fiber bundle IFUs , 2006 .

[18]  C. A. Clayton The implications of image scrambling and focal ratio degradation in fibre optics on the design of astronomical instrumentation , 1989 .