Abstract
We describe the design and construction of a formatted fiber field unit,
SparsePak, and characterize its optical and astrometric performance.
This array is optimized for spectroscopy of low surface brightness
extended sources in the visible and near-infrared. SparsePak contains
82, 4.7" fibers subtending an area of
72''×71'' in the telescope focal plane and
feeds the WIYN Bench Spectrograph. Together, these instruments are
capable of achieving spectral resolutions of
λ/Δλ~20,000 and an area-solid angle product of ~140
arcsec2 m2 per fiber. Laboratory measurements of
SparsePak lead to several important conclusions on the design of fiber
termination and cable curvature to minimize focal ratio degradation.
SparsePak itself has throughput above 80% redward of 5200 Å and
90%-92% in the red. Fed at f/6.3, the cable delivers an output of 90%
encircled energy at nearly f/5.2. This has implications for performance
gains if the WIYN Bench Spectrograph were to have a faster collimator.
Our approach to integral-field spectroscopy yields an instrument that is
simple and inexpensive to build, yet yields the highest area-solid angle
product per spectrum of any system in existence. An Appendix details the
fabrication process in sufficient detail for others to repeat. SparsePak
was funded by the National Science Foundation and the University of
Wisconsin-Madison Graduate School, and is now publicly available on the
WIYN Telescope through the National Optical Astronomical Observatories.
Original language | English |
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Title of host publication | Publications of the Astronomical Society of the Pacific |
Publisher | The University of Chicago Press |
Pages | 565-590 |
Volume | 116 |
DOIs | |
Publication status | Published - 1-Jun-2004 |
Keywords
- Galaxies: Kinematics and Dynamics
- Instrumentation: Spectrographs
- methods: laboratory