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Basic principle of multi-object spectroscopy
Basic principle of multi-object spectroscopy

A multi-object spectrometer is a type of optical spectrometer capable of simultaneously acquiring the spectra of multiple separate objects in its field of view.[1] It is used in astronomical spectroscopy and is related to long-slit spectroscopy.[2] This technique became available in the 1980s.[3]

Description

The term multi-object spectrograph is commonly used for spectrographs using a bundle of fibers to image part of the field. The entrance of the fibers is at the focal plane of the imaging instrument. The bundle is then reshaped; the individual fibers are aligned at the entrance slit of a spectrometer, dispersing the light on a detector.[1]

This technique is closely related to integral field spectrography (IFS), more specifically to fiber-IFS. It is a form of snapshot hyperspectral imaging, itself a part of imaging spectroscopy.

Apertures

External image
image icon Photographs of the Configurable Slit Unit on MOSFIRE Left: full picture, in a configuration for imaging. Right: close-up on the knife-edge slits.[4][5]

Typically, the apertures of multi-object spectrographs can be modified to fit the needs of the given observation.[6]

For example, the MOSFIRE (Multi-Object Spectrometer for Infra-Red Exploration )[7] instrument on the W. M. Keck Observatory contains the Configurable Slit Unit (CSU)[8] allowing arbitrary positioning of up to forty-six 18 cm slits by moving opposable bars.[5]

Some fiber-fed spectroscopes, such as the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) can move the fibers to desired position. The LAMOST moves its 4000 fibers separately within designated areas for the requirements of a measurement, and can correct positioning errors in real time.[9]

The James Webb Space Telescope uses a fixed Micro-Shutter Assembly (MSA), an array of nearly 250000 5.1 mm by 11.7 mm shutters that can independently be opened or closed to change the location of the open slits on the device.[10]

Uses in telescopes

Ground-based instruments

Instruments with multi-object spectrometry capabilities are available on most 8-10 meter-class ground-based observatories.[6] For example, the Large Binocular Telescope,[11] W. M. Keck Observatory,[12] Gran Telescopio Canarias,[13] Gemini Observatory,[14] New Technology Telescope,[15] William Herschel Telescope,[16] UK Schmidt Telescope[17] and LAMOST[3] include such system.

Four instruments in the Very Large Telescope, including the KMOS (K-band multi-object spectrograph)[18] and the VIMOS (Visible Multi Object Spectrograph)[19] instruments, have multi-object spectroscopic capabilities.

Space-based instruments

The Hubble Space Telescope has been operating the NICMOS (Near Infrared Camera and Multi-Object Spectrometer)[20] from 1997 to 1999 and from 2002 to 2008.

The James Webb Space Telescope's NIRSpec (Near-Infrared Spectrograph) instrument is a multi-object spectrometer.[21]

References

  1. ^ a b "multi-object spectrograph". astro.vaporia.com. Retrieved 2023-08-07.
  2. ^ "Multi Object Spectroscopy (decommissioned)". eso.org. European Southern Observatory. Retrieved 2023-08-07.
  3. ^ a b Chu, Yaoquan. The Large Sky Area Multi-Object Fibre Spectroscopy Telescope ( LAMOST) Project. Conference of the Working Group of IAU Commission 9 on “Wide-Field Imaging” held in Athens, Greece, May 20–25, 1996. Springer Dordrecht. doi:10.1007/978-94-011-5722-3_9.
  4. ^ Goodrich, Bob; Adkins, Sean (2011). "The Imminent Arrival of MOSFIRE, Keck's New Infrared, Multi-Object, Imaging Spectrograph". Keck Observers' Newsletter (10).
  5. ^ a b McLean, Ian S.; Steidel, Charles C.; Harland, Epps; Matthews, Keith; Adkins, Sean; Konidaris, Nicholas; Weber, Bob; Aliado, Ted; Brims, George; Canfield, John; Cromer, John; Fucik, Jason; Kulas, Kristin; Mace, Greg; Magnone, Ken; Rodriguez, Hector; Wang, Eric; Weiss, Jason (2010-07-20). McLean, Ian S.; Ramsay, Suzanne K.; Takami, Hideki (eds.). "Design and development of MOSFIRE: the multi-object spectrometer for infrared exploration at the Keck Observatory" (PDF). SPIE Conference Proceedings. Ground-based and Airborne Instrumentation for Astronomy III. 7735. SPIE: 77351E. Bibcode:2010SPIE.7735E..1EM. doi:10.1117/12.856715. S2CID 122823326.{{cite journal}}: CS1 maint: date and year (link)
  6. ^ a b "JWST Multi-Object Spectroscopy". JWST User Documentation. 2022-10-17. Retrieved 2023-08-07.
  7. ^ "MOSFIRE Home Page". www2.keck.hawaii.edu. 2020-10-07. Retrieved 2023-08-07.
  8. ^ "Multi-Object Spectrometer for Infra-Red Exploration First Light Obtained: April 4, 2012". irlab.astro.ucla.edu. Retrieved 2023-08-07.
  9. ^ "Fiber positioning". lamost.org. 2012-08-14. Retrieved 2023-08-07.
  10. ^ "NIRSpec Micro-Shutter Assembly". jwst-docs.stsci.edu. 2023-04-24. Retrieved 2023-08-07.
  11. ^ "Instruments - an overview". Large Binocular Telescope Observatory. Retrieved 2023-08-07.
  12. ^ "Keck I And Keck II Telescopes". W. M. Keck Observatory. Retrieved 2023-08-07.
  13. ^ "MEGARA". Gran Telescopio CANARIAS. 2023-05-08. Retrieved 2023-08-07.
  14. ^ "The GMOS (Gemini Multi-Object Spectrograph) project at the ATC". 2003-09-12. Retrieved 2023-08-07.
  15. ^ "EFOSC Overview". eso.org. European Southern Observatory. Retrieved 2023-08-07.
  16. ^ "WEAVE - instrumental overview". ing.iac.es. 2023-07-05. Retrieved 2023-08-07.
  17. ^ "The UK Schmidt Telescope". aat.anu.edu.au. 21 May 2014. Retrieved 2023-08-07.
  18. ^ "KMOS - K-band Multi Object Spectrograph". eso.org. European Southern Observatory. Retrieved 2023-08-07.
  19. ^ "VIMOS - VIsible MultiObject Spectrograph". eso.org. European Southern Observatory. Retrieved 2023-08-07.
  20. ^ "Hubble's Instruments: NICMOS - Near Infrared Camera and Multi-Object Spectrometer". esahubble.org. Retrieved 2023-08-07.
  21. ^ "NIRSpec Multi-Object Spectroscopy". JWST User Documentation. 2023-04-24. Retrieved 2023-08-07.
source: http://en.wikipedia.org/wiki/Multi-Object_Spectrometer