GMACS











The Giant Magellan Telescope Multi-object Astronomical and Cosmological Spectrograph (GMACS) is a wide field, multi-object, moderate-resolution, optical spectrograph being designed for the Giant Magellan Telescope (GMT). Our goal is to create an instrument capable of spectroscopically observing the faintest possible targets, which are currently known only from imaging observations. High throughput, simultaneous wide wavelength coverage, accurate and precise sky subtraction, moderate resolution, relatively wide field, and substantial multiplexing are crucial design drivers for the instrument.

GMACS

Figure 1: The current GMACS concept. The VPH gratings and camera assemblies can rotate independently of each other (90° range of motion). Masks are exchanged using a cassette system at the top of the instrument.

History

GMACS has a long history of design studies and active collaboration with GMT partner institutions, in the form of instrument software development by Korean collaborators (S. Pak), mechanical design planning from partners in Brazil (K. Taylor), optical design studies by Carnegie (S. Shectman and R. Bernstein), and project management provided by C. Froning at UT-Austin.

A GMACS community workshop during 2014 March 18-19 at Texas A&M University helped to define the scientific requirements for the instrument. The workshop included 51 participants, representing all of the GMT partners and including representatives from national and international non-partners. The participants provided expertise in a wide range of astrophysical areas through contributed talks and breakout groups focused on (1) stars, star-formation, and planets; (2) resolved Galaxies (including Dwarf Galaxies) and near-field cosmology; and (3) distant galaxies (including reionization and first light science). Past design studies, requirements from GMTO and input from the scientific community have been condensed into key design requirements and formal instrument development has begun. An advantage of the instrument history is that most technical risks to the project are well known and most have well-considered mitigation strategies (i.e. appropriate detectors, optics blanks, lens fabrication vendors, etc. are identified or commercially available).

Click to read the Conceptual Design Report for the previous iteration of GMACS.

Design

The current concept for GMACS includes ≥20 interchangeable multi-object slit masks which are placed at the focal plane of the GMT. After passing through a field lens and collimator lens group, a dichroic splits the beam into “blue” (reflected) and “red” (transmitted) channels split at around 600nm. Exchangeable VPH gratings disperse the light which is then focused onto each red or blue optimized CCD array (8k x 12k pixels) via camera lens groups, again optimized for each wavelength range. The position of the camera optical assembly is controlled with an active flexure control system. As the telescope tracks an object, this system responds to the changing gravity vector, removing flexure induced image motion. GMACS will also contain an internal wavelength calibration system and cameras for target acquisition and mask alignment.

Key design parameters are summarized in the table below.

Parameter Requirement / Goal Comments
Field of View 30 arcmin sq. / 50 arcmin sq.
Wavelength coverage 350-950nm / 320-1000nm
Spectral Resolution Blue: 1000-6000 Red: 1000-6000 0.7” slit width, full coverage at lower resolutions, wavelength coverage at higher resolutions is sacrificed
Image Quality 0.30 / 0.15 arcsec 80% EE
Spectral Stability 0.3 / 0.1 spectral resolution elements/hour
Grating Exchange 1 / ≥2 gratings Multiple wavelength regions
Slit Mask Exchange 12 / ≥20 Cassette style mask changer

Click to use the GMACS exposure time calculator

GMACS trade studies

How GMACS fits into the GMT

GMACS will be mounted in the Gregorian Instrument Rotator as shown in the figure below. The instrument design will also include handling and test carts to facilitate assembly, integration and verification of the instrument, as well as instrument exchange at the telescope.

gmacs in telescope

Figure 2: GMACS will be mounted in the Gregorian Instrument Rotator.

For more information on GMACS and the GMT, please visit our Publications page.

 
Astronomy Group
4242 TAMU
College Station, TX 77843-4242
Ph: (979) 845 7717
Texas A&M University - College of Science