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]
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]
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.
