Abstract
The Giant Magellan Telescope Multi-object Astronomical and Cosmological Spectrograph (GMACS) is a first light instrument for the Giant Magellan Telescope (GMT). It will provide multi-object spectroscopy in wide wavelength coverage and wide field of view. The scientific objectives include exoplanet atmospheres, star formation and chemical evolution studies, galaxy assembly histories, and intergalactic medium tomography. The optical layouts are optimized to have high throughput in the natural seeing limit. In this presentation, we report the current status of the instrument development.
| Original language | English |
|---|---|
| Title of host publication | Advances in Optical Astronomical Instrumentation 2019 |
| Editors | Simon Ellis, Celine d'Orgeville |
| Publisher | SPIE |
| ISBN (Electronic) | 9781510631465 |
| DOIs | |
| Publication status | Published - 2020 |
| Event | Advances in Optical Astronomical Instrumentation 2019 - Melbourne, Australia Duration: 9 Dec 2019 → 12 Dec 2019 |
Publication series
| Name | Proceedings of SPIE - The International Society for Optical Engineering |
|---|---|
| Volume | 11203 |
| ISSN (Print) | 0277-786X |
| ISSN (Electronic) | 1996-756X |
Conference
| Conference | Advances in Optical Astronomical Instrumentation 2019 |
|---|---|
| Country/Territory | Australia |
| City | Melbourne |
| Period | 9/12/19 → 12/12/19 |
Bibliographical note
Publisher Copyright:© 2020 SPIE.
Keywords
- Extremely large telescopes
- GMACS
- GMT
- Multi-object spectrographs
Fingerprint
Dive into the research topics of 'Giant Magellan Telescope Multi-object Astronomical and Cosmological Spectrograph (GMACS): conceptual design'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver