SparsePak: A Formatted Fiber Field Unit for The WIYN Telescope Bench Spectrograph. I. Design, Construction, and Calibration
arXiv:astro-ph/0403456 · doi:10.1086/421057
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"x71" in the telescope focal plane, and feeds the WIYN Bench spectrograph. Together, these instruments are capable of achieving spectral resolutions of lambda/dlambda ~ 20000 and an area--solid-angle product of ~140 arcsec^2 m^2 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 >80% redwards of 5200 A, and 90-92% in the red. Fed at f/6.3, the cable delivers an output 90% encircled energy at nearly f/5.2. This has implications for performance gains if the WIYN Bench Spectrograph had a faster collimator. Our approach to integral-field spectroscopy yields an instrument which 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.
accepted for publication in PASP; 17 pages text, 16 figures (embedded)
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- The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
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- SDSS J131339.98+515128.3: A new gravitationally lensed quasar selected based on near-infrared excess
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- ZFIRE: Using H equivalent widths to investigate the in situ initial mass function at z~2
- An Improved Test of the Binary Black Hole Hypothesis for Quasars with Double-peaked Broad Balmer Lines
- Testing the Modern Merger Hypothesis via the Assembly of Massive Blue Elliptical Galaxies in the Local Universe
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- Fundamental physics with blazar spectra: a critical appraisal
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- Asteroseismology of luminous red giants with Kepler. II. Dependence of mass loss on pulsations and radiation
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- Hot planets around cool stars -- two short-period mini-Neptunes transiting the late K-dwarf TOI-1260
- The QUaD Galactic Plane Survey 1: Maps And Analysis of Diffuse Emission
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- Carbon and Nitrogen Abundances in Early-type Galaxies
- K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
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- Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
- CII and HI 21-cm line intensity mapping from the EoR: Impact of the light-cone effect on auto and cross-power spectra
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- BANYAN. X. Discovery of a wide, low-gravity L-type companion to a fast-rotating M3 dwarf
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- The first observed stellar occultations by the irregular satellite (Saturn IX) Phoebe and improved rotational period
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- Search for TeV Emission at the Location of Milagro Sky Survey Hot Spot Using the Whipple Gamma-Ray Telescope
- Effective Field Theory analysis of He- scattering data
- Formation of Lunar Swirls
- Towards convergence of turbulent dynamo amplification in cosmological simulations of galaxies
- Direct Wide-Field Radio Imaging in Real-Time at High Time Resolution using Antenna Electric Fields
- The Fornax3D project: Planetary nebulae catalogue and independent distance measurements to Fornax cluster galaxies
- Charge-Injection Device Imaging of Sirius with Contrast Ratios Greater than 1:26 Million
- Direct Imaging of Irregular Satellite Disks in Scattered Light
- Toward the Analysis of JWST Exoplanet Spectra: the effective temperature in the context of direct imaging
- Image Processing in Python With Montage
- Gas flow in barred potentials II. Bar Driven Spiral Arms
- On the influence of the Illuminati in astronomical adaptive optics
- The astronomizings of Dr. Anderson and the curious case of his disappearing nova
- The panchromatic polarization signatures of Active Galactic Nuclei
- IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
- Satellites of the Broucke-Hadjidemetriou-Hénon family of periodic unequal-mass three-body orbits
- Double-humped Super-luminous Supernovae
- Opportunities to Search for Extra-Terrestrial Intelligence with the Five-hundred-meter Aperture Spherical radio Telescope
- The remnant and origin of the historical supernova 1181AD
- Photometric Study on Stellar Magnetic Activity: I. Flare Variability of Red Dwarf Stars in the Open Cluster M37
- Evidence for mixing between ICM and stripped ISM by the analysis of the gas metallicity in the tails of jellyfish galaxies
- Identifications of RR Lyrae stars and Quasars from the simulated data of Mephisto-W Survey
- A kinematically decoupled component in NGC4778
- Pa, H, and Attenuation in NGC 5194 and NGC 6946
- Effect of background magnetic field on the normal modes of conformal dissipative chiral hydro and a novel mechanism for explaining pulsar kicks
- A Convolutional Autoencoder-Based Pipeline for Anomaly Detection and Classification of Periodic Variables
- An Empirical Mass-Radius Relation for Cool Giant Planets
- Phantom Inflated Planets in Occurrence Rate Based Samples
- SparsePak Observations of Diffuse Ionized Gas Halo Kinematics in NGC 891
- Magnetic-oscillation mechanism for understanding periodic or quasi-periodic modulation of the timing residuals from pulsars
- Issues with Core-Collapse Supernova Progenitor Models
- Decomposition of stellar populations in CosmoDC2 galaxies using SCARLET and Deep Learning
- Radio-Frequency Interference at the McGill Arctic Research Station
- The Correlation Calibration of PAPER-64 data
- A roadmap to gamma-ray bursts: new developments and applications to cosmology
- PISCOLA: a data-driven transient light-curve fitter
- Laser guide star return-flux gain from frequency chirping
- Introducing the FLAMINGOS-2 Split-K Medium Band Filters: The Impact on Photometric Selection of High-z Galaxies in the FENIKS-pilot survey
- Influence of database noises to machine learning for spatiotemporal chaos
- Atmospheric density uncertainty effects on the orbital lifetime estimation for CubeSats at LEO
- Uncertainty-Aware Learning for Improvements in Image Quality of the Canada-France-Hawaii Telescope
- Search for Cosmological time dilation from Gamma-Ray Bursts -- A 2021 status update
- Theoretical clues about dust accumulation and galaxy obscuration at high and low redshift
- A new method for the determination of action integrals in the study of galactic dynamics
- Self-Bayesian Aberration Removal via Constraints for Ultracold Atom Microscopy