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dc.contributor.authorDrory, N.
dc.contributor.authorMacDonald, N.
dc.contributor.authorBershady, M. A.
dc.contributor.authorBundy, K.
dc.contributor.authorGunn, J.
dc.contributor.authorLaw, D. R.
dc.contributor.authorSmith, M.
dc.contributor.authorStoll, R.
dc.contributor.authorTremonti, C. A.
dc.contributor.authorWake, D. A.
dc.contributor.authorYan, R.
dc.contributor.authorWeijmans, A. M.
dc.contributor.authorByler, N.
dc.contributor.authorCherinka, B.
dc.contributor.authorCope, F.
dc.contributor.authorEigenbrot, A.
dc.contributor.authorHarding, P.
dc.contributor.authorHolder, D.
dc.contributor.authorHuehnerhoff, J.
dc.contributor.authorJaehnig, K.
dc.contributor.authorJansen, T. C.
dc.contributor.authorKlaene, M.
dc.contributor.authorPaat, A. M.
dc.contributor.authorPercival, J.
dc.contributor.authorSayres, C.
dc.date.accessioned2015-02-10T13:01:03Z
dc.date.available2015-02-10T13:01:03Z
dc.date.issued2015-02
dc.identifier.citationDrory , N , MacDonald , N , Bershady , M A , Bundy , K , Gunn , J , Law , D R , Smith , M , Stoll , R , Tremonti , C A , Wake , D A , Yan , R , Weijmans , A M , Byler , N , Cherinka , B , Cope , F , Eigenbrot , A , Harding , P , Holder , D , Huehnerhoff , J , Jaehnig , K , Jansen , T C , Klaene , M , Paat , A M , Percival , J & Sayres , C 2015 , ' The MaNGA integral field unit fiber feed system for the Sloan 2.5 m telescope ' , Astronomical Journal , vol. 149 , no. 2 , 77 . https://doi.org/10.1088/0004-6256/149/2/77en
dc.identifier.issn0004-6256
dc.identifier.otherPURE: 159212268
dc.identifier.otherPURE UUID: 27b372c0-9d24-438d-ab68-d591ebd7cef0
dc.identifier.otherBibCode: 2014arXiv1412.1535D
dc.identifier.otherScopus: 84922469449
dc.identifier.otherWOS: 000349360200042
dc.identifier.otherORCID: /0000-0002-5908-6852/work/40233500
dc.identifier.urihttps://hdl.handle.net/10023/6082
dc.descriptionN.D. acknowledges support through CONACyT grants 167332 and 180125. K.B. was supported by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. M.A.B. acknowledges support from the Leverhulme Foundation.en
dc.description.abstractWe describe the design, manufacture, and performance of bare-fiber integral field units (IFUs) for the SDSS-IV survey Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) on the the Sloan 2.5 m telescope at Apache Point Observatory. MaNGA is a luminosity-selected integral-field spectroscopic survey of 104 local galaxies covering 360–1030 nm at R~2200. The IFUs have hexagonal dense packing of fibers with packing regularity of 3 μm (rms), and throughput of 96 ± 0.5% from 350 nm to 1 μm in the lab. Their sizes range from 19 to 127 fibers (3–7 hexagonal layers) using Polymicro FBP 120:132:150 μm core:clad:buffer fibers to reach a fill fraction of 56%. High throughput (and low focal-ratio degradation (FRD)) is achieved by maintaining the fiber cladding and buffer intact, ensuring excellent surface polish, and applying a multi-layer anti-reflection (AR) coating of the input and output surfaces. In operations on-sky, the IFUs show only an additional 2.3% FRD-related variability in throughput despite repeated mechanical stressing during plate plugging (however other losses are present). The IFUs achieve on-sky throughput 5% above the single-fiber feeds used in SDSS-III/BOSS, attributable to equivalent performance compared to single fibers and additional gains from the AR coating. The manufacturing process is geared toward mass-production of high-multiplex systems. The low-stress process involves a precision ferrule with a hexagonal inner shape designed to lead inserted fibers to settle in a dense hexagonal pattern. The ferrule ID is tapered at progressively shallower angles toward its tip and the final 2 mm are straight and only a few microns larger than necessary to hold the desired number of fibers. Our IFU manufacturing process scales easily to accommodate other fiber sizes and can produce IFUs with substantially larger fiber counts. To assure quality, automated testing in a simple and inexpensive system enables complete characterization of throughput and fiber metrology. Future applications include larger IFUs, higher fill factors with stripped buffer, de-cladding, and lenslet coupling.
dc.language.isoeng
dc.relation.ispartofAstronomical Journalen
dc.rights© 2015. The American Astronomical Society. All rights reserved. Originally published by The Astronomical Journal, http://dx.doi.org/10.1088/0004-6256/149/2/77.en
dc.subjectAstrophysicsen
dc.subjectInstrumentation and Methods for Astrophysicsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe MaNGA integral field unit fiber feed system for the Sloan 2.5 m telescopeen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/0004-6256/149/2/77
dc.description.statusPeer revieweden


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