The DESI Fiber View Camera System. (7th May 2019)
- Record Type:
- Journal Article
- Title:
- The DESI Fiber View Camera System. (7th May 2019)
- Main Title:
- The DESI Fiber View Camera System
- Authors:
- Baltay, C.
Rabinowitz, D.
Besuner, R.
Casetti, D.
Emmet, W.
Fagrelius, P.
Girard, T.
Heetderks, H.
Lampton, M.
Lathem, A.
Levi, M.
Padmanabhan, N.
Silber, J. - Abstract:
- Abstract: The Dark Energy Spectroscopic Instrument (DESI) is a 5000 fiber multi-object spectrometer now being installed at the prime focus of the 4 m Mayall telescope at Kitt Peak. Using DESI to measure ∼35 million galaxy redshifts and using the Baryon Acoustic Oscillation (BAO) technique to measure distances, the results will probe the nature of the recently discovered mysterious component of our universe called dark energy. Computer controlled robotic positioners move the 120 μ m diameter fibers to positions of galaxies whose location on the sky have been obtained in a previous target selection imaging survey. To achieve good throughput the fibers should be centered on the target position to within 3 μ m. The robotic positioners however are only capable of a 50 μ m precision on their first move. To achieve the desired precision, the Fiber View Camera (FVC) system has been implemented. The FVC, located near the hole in the primary mirror of the Mayall telescope, has been designed to take an exposure of the focal plane, located at the prime focus some 12 m above the FVC, after the robotic positioners have completed their first move. The FVC is intended to measure the fiber locations with a precision of 3 μ m and issue a set of fiber coordinate corrections for the second move correcting the fiber positions by the robotic positioners. Tests show that after two iterations better than 99% of the fibers will be in their intended location to within the desired precision. ThisAbstract: The Dark Energy Spectroscopic Instrument (DESI) is a 5000 fiber multi-object spectrometer now being installed at the prime focus of the 4 m Mayall telescope at Kitt Peak. Using DESI to measure ∼35 million galaxy redshifts and using the Baryon Acoustic Oscillation (BAO) technique to measure distances, the results will probe the nature of the recently discovered mysterious component of our universe called dark energy. Computer controlled robotic positioners move the 120 μ m diameter fibers to positions of galaxies whose location on the sky have been obtained in a previous target selection imaging survey. To achieve good throughput the fibers should be centered on the target position to within 3 μ m. The robotic positioners however are only capable of a 50 μ m precision on their first move. To achieve the desired precision, the Fiber View Camera (FVC) system has been implemented. The FVC, located near the hole in the primary mirror of the Mayall telescope, has been designed to take an exposure of the focal plane, located at the prime focus some 12 m above the FVC, after the robotic positioners have completed their first move. The FVC is intended to measure the fiber locations with a precision of 3 μ m and issue a set of fiber coordinate corrections for the second move correcting the fiber positions by the robotic positioners. Tests show that after two iterations better than 99% of the fibers will be in their intended location to within the desired precision. This paper describes the design of the FVC system, the R&D program preceding the final design, and the tests that have been carried out to demonstrate that the FVC can achieve the required precision. … (more)
- Is Part Of:
- Publications of the Astronomical Society of the Pacific. Volume 131:Number 1000(2019)
- Journal:
- Publications of the Astronomical Society of the Pacific
- Issue:
- Volume 131:Number 1000(2019)
- Issue Display:
- Volume 131, Issue 1000 (2019)
- Year:
- 2019
- Volume:
- 131
- Issue:
- 1000
- Issue Sort Value:
- 2019-0131-1000-0000
- Page Start:
- Page End:
- Publication Date:
- 2019-05-07
- Subjects:
- instrumentation: detectors -- galaxies: statistics -- (cosmology:) dark energy
Astronomy -- Periodicals
Astronomy
Periodicals
Periodicals
520.5 - Journal URLs:
- http://ejournals.ebsco.com/direct.asp?JournalID=101605 ↗
http://iopscience.iop.org/journal/1538-3873 ↗
http://www.journals.uchicago.edu/PASP/journal/ ↗
http://www.jstor.org/journals/00046280.html ↗
http://www.iop.org/ ↗ - DOI:
- 10.1088/1538-3873/ab15c2 ↗
- Languages:
- English
- ISSNs:
- 0004-6280
- Deposit Type:
- Legaldeposit
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