Astrophysics (Index)About

DESHIMA

(Deep Spectroscopic High-redshift Mapper)
(submillimeter spectrometer)

DESHIMA (for Deep Spectroscopic High-redshift Mapper) is a Japanese/Netherlands submillimeter spectrometer installed on the ASTE submillimeter telescope. (The name DESHIMA was clearly inspired by inspired by the Japanese island, Deshima aka Dejima, which historically served as a Japanese/Netherlands trading port.) The spectrometer's frequency-range at first light (2017) was 335-370 GHz, which allows detection of the ionized carbon fine structure line ([CII]) through a redshift-range of roughly z = 4.2 to 4.6. For sensitivity, the appropriate portions of the instrument are cooled to 0.15 K. The technology is MKID-based filter banks.

DESHIMA 2.0 is an upgrade, installed in Fall of 2023, and as of early 2024, is undergoing commissioning. It covers a broader frequency-range (220-440 GHz), allowing detection of the line through a redshift-range of z = 3.3 to 7.6. The spectrometer is single-pixel, but a future multiple-pixel version is planned.


(instrument,spectrometer,submillimeter)
Further reading:
http://deshima.ewi.tudelft.nl/
https://ui.adsabs.harvard.edu/abs/2020JLTP..199..231T/abstract
https://ui.adsabs.harvard.edu/abs/2012JLTP..167..341E/abstract
https://ui.adsabs.harvard.edu/abs/2022JLTP..209..278T/abstract
https://www.tudelft.nl/en/eemcs/current/science-stories/stories/the-deshima-guide-to-the-galaxy
https://endolab.tudelft.nl/deshima/
https://www.tudelft.nl/en/2019/ewi/dutch-japanese-astronomical-instrument-measures-49-shades-of-far-infrared
http://www2.nao.ac.jp/~eaarc/ALMAUM2021/contents/AkioTaniguchi.pdf
WaveLFreqPhoton
Energy
  
810μm370GHz1.6meVbeginDESHIMA
895μm335GHz1.4meVendDESHIMA

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