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Development of a near-infrared wide-field integral field unit by ultra-precision diamond cutting
- Source :
- Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 10, Issue 1, 015004 (March 2024)
- Publication Year :
- 2024
-
Abstract
- Integral Field Spectroscopy (IFS) is an observational method to obtain spatially resolved spectra over a specific field of view (FoV) in a single exposure. In recent years, near-infrared IFS has gained importance in observing objects with strong dust attenuation or at high redshift. One limitation of existing near-infrared IFS instruments is their relatively small FoV, less than 100 arcsec$^2$, compared to optical instruments. Therefore, we have developed a near-infrared (0.9-2.5 $\mathrm{\mu}$m) image-slicer type integral field unit (IFU) with a larger FoV of 13.5 $\times$ 10.4 arcsec$^2$ by matching a slice width to a typical seeing size of 0.4 arcsec. The IFU has a compact optical design utilizing off-axis ellipsoidal mirrors to reduce aberrations. Complex optical elements were fabricated using an ultra-precision cutting machine to achieve RMS surface roughness of less than 10 nm and a P-V shape error of less than 300 nm. The ultra-precision machining can also simplify alignment procedures. The on-sky performance evaluation confirmed that the image quality and the throughput of the IFU were as designed. In conclusion, we have successfully developed a compact IFU utilizing an ultra-precision cutting technique, almost fulfilling the requirements.<br />Comment: 24 pages, 18 figures, 7 tables. Accepted for publication in JATIS
- Subjects :
- Astrophysics - Instrumentation and Methods for Astrophysics
Subjects
Details
- Database :
- arXiv
- Journal :
- Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 10, Issue 1, 015004 (March 2024)
- Publication Type :
- Report
- Accession number :
- edsarx.2403.01668
- Document Type :
- Working Paper
- Full Text :
- https://doi.org/10.1117/1.JATIS.10.1.015004