Multi-Object Spectrometer

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.

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

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

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

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.

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.