Statistical Test of Optical Fibers for Use in PMAS, the Potsdam Multi‐Aperture Spectrophotometer

Focal ratio degradation measurements of optical fibers for the Potsdam Multi-Aperture Spectrophotometer integral field instrument have been performed using the Photometric Testbench of the Potsdam Astrophysical Institute. An effort has been made to obtain sufficiently large statistical samples of individual fiber measurements. The optimization of the measurement process has made it possible to study quantitatively the effects of different coupling methods (air-glass vs. immersion) and of imperfections such as defocus, lateral displacement, and angular misalignment. Furthermore, the effects of mechanical stress on focal ratio degradation have been investigated, confirming the presumed cause of modal noise that is known to limit the maximum signal-to-noise ratio one can achieve with fiber-coupled echelle spectrographs.

[1]  Roger Haynes,et al.  TEIFU: a thousand element integral field unit for the WHT fed by the ELECTRA AO system , 1998, Astronomical Telescopes and Instrumentation.

[2]  Uwe Laux,et al.  PMAS fiber spectrograph: design, manufacture, and performance , 2000, Astronomical Telescopes and Instrumentation.

[3]  Juergen Schmoll,et al.  PMAS -- the Potsdam multiaperture spectrophotometer: a progress report , 1998, Astronomical Telescopes and Instrumentation.

[4]  David L. Crawford,et al.  Instrumentation in Astronomy VI , 1986 .

[5]  B. Krauskopf,et al.  Proc of SPIE , 2003 .

[6]  Gordon A. H. Walker,et al.  Modal Noise in High‐Resolution, Fiber‐fed Spectra: A Study and Simple Cure , 2001 .

[7]  Christoph U. Keller,et al.  PEPSI spectro-polarimeter for the LBT , 2003, SPIE Astronomical Telescopes + Instrumentation.

[8]  Svend-Marian Bauer,et al.  Design study for the Potsdam Multiaperture Spectrophotometer (PMAS) , 1997, Other Conferences.

[9]  W. V. Breugel,et al.  Imaging the Universe in Three Dimensions , 2000 .

[10]  Ian R. Parry,et al.  CIRPASS: a NIR integral field and multi-object spectrograph , 2000, Astronomical Telescopes and Instrumentation.

[11]  Oliver LeFevre,et al.  Very wide integral field unit of VIRMOS for the VLT: design and performances , 2000, Astronomical Telescopes and Instrumentation.

[12]  家 正則,et al.  Optical and IR telescope instrumentation and detectors : 27-31 March 2000, Munich, Germany , 2000 .

[13]  Luca Pasquini,et al.  FLAMES: a multi-object fiber facility for the VLT , 2000, Astronomical Telescopes and Instrumentation.