ANDES, the high-resolution spectrograph for the ELT: RIZ & UBV spectrographs' preliminary design, analysis, and integration of the vacuum vessel and thermal enclosure

Bibcode
2024SPIE13096E..4KS
DOI
10.1117/12.3020150
Santos Diaz, P.; Kern, J.; Genolet, L.; Chazelas, B.; Hughes, I.; Lanotte, A. A.; Weber, M.; Füßlein, C.; Lovis, C.; Dionies, F.; Vega-Moreno, A.; Peñate Castro, J.; Calvo Ortega, Rocio; Varas Gonzalez, Roberto; Simoes, Roberto; Tenegi, F.; Ivanisenko, Y.; Brynnel, J.; Weingrill, J.; Sigwarth, M.; Sordet, M.; Bellido, O.; Järvinen, A.; Aliverti, M.; Cabona, L.; Coretti, I.; Di Marcantonio, P.; Marconi, A.; Oliva, E.; Pariani, G.; Redaelli, E. M. A.; Riva, M.; Zanutta, A.
Bibliographical reference

Ground-based and Airborne Instrumentation for Astronomy X

Advertised on:
7
2024
Number of authors
33
IAC number of authors
3
Citations
0
Refereed citations
0
Description
The RIZ & UBV visible spectrographs of the ANDES instrument, which are foreseen to be installed at the Extremely Large Telescope, require to be under a very stable high vacuum and at an extremely stable temperature of 1mK to reach the radial velocity goal of 10cm/s RMS over a 10-year period. The baseline design, integration and first analyses of the 5.5t aluminum vacuum tank, vacuum system, and the thermal enclosure of the two-room temperature spectrographs are presented in this paper. A very analogous configuration is proposed for both instruments in view of their similarities. In addition, this article addresses the finite rigidity of the Nasmyth platform and its consequences on the instrument design together with a potential collaborative multi-CAD Product Design Management platform description.
Type
Non-refereed

It may interest you

  • Non-refereed
    The Multi Frequency Instrument 2 (MFI2): mechanical design, manufacture, integration, and commissioning of the MFI2 for the QUIJOTE facility in Tenerife (Canary Islands)
    The QUIJOTE (Q-U-I JOint TEnerife) experiment combines the operation of two radio-telescopes and three instruments working in the microwave bands from 10 to 47 GHz at the Teide Observatory, Tenerife, which has already been presented in previous SPIE meetings. The new Multi Frequency Instrument (MFI2) led by the Instituto de Astrofísica de Canarias
    Lorenzo-Hernández, Haroldo et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..33L
    Citations
    0
  • Non-refereed
    First light of the upgraded Gregor Infrared Spectrograph
    For more than ten years, the Gregor Infrared Spectrograph (GRIS) has been the infrared spectropolarimeter on the Gregor telescope since its inauguration in 2012. The instrument mainly performs polarimetric observations of the wavelength regions at 1083 and 1565nm, which have high scientific potential. There, observers can find spectral lines that
    Quintero Noda, C. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..42Q
    Citations
    0
  • Non-refereed
    Performance of the image persistence model for Euclid infrared detectors
    Large-format infrared detectors are at the heart of major ground and space-based astronomical instruments, and the HgCdTe HxRG is the most widely used. The Near Infrared Spectrometer and Photometer (NISP) of the ESA's Euclid mission launched in July 2023 hosts 16 H2RG detectors in the focal plane. Their performance relies heavily on the effect of
    Kubik, B. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13103E..15K
    Citations
    0