Presentation + Paper
29 August 2022 The Magellan infrared multi-object spectrograph project: 2022 update
Nicholas P. Konidaris II, Gwen C. Rudie, Andrew B. Newman, Alica E. Lanz, Jason E. Williams, Tyson S. Hare, Robert Barkhouser, Julia Brady, Jeffrey D. Crane, Daniel D. Kelson, Gerrad Killion, Vince Kowal, Solange Ramirez, Stephen A. Smee, Johanna K. Teske, Stephanie Wachter
Author Affiliations +
Abstract
The Magellan Infrared Multi-object Spectrograph (MIRMOS) is a near-infrared (NIR) spectrograph with both multi-object (MOS) and integral field unit (IFU) capabilities designed for the Magellan 6.5-meter telescopes. MIRMOS’s design is optimized for both faint-object spectroscopy, and with the insertion of a diffuser, for ultra-high-signal-to-noise transmission spectroscopy of exoplanet atmospheres. To maximize MIRMOS’s scientific returns, it has an instantaneous wavelength range from 0.89-2.4 µm with a spectral resolution >3, 400 in the Y, J, H, and K bands. The front end switches between a mechanical slit mask robot capable of deploying 92 slits over a 13′ × 3 ′ field, and an image slicer IFU with a wide field of 26′′ × 20′′. In this proceeding, we will describe the current state of the instrument, with a focus on its optical design.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Nicholas P. Konidaris II, Gwen C. Rudie, Andrew B. Newman, Alica E. Lanz, Jason E. Williams, Tyson S. Hare, Robert Barkhouser, Julia Brady, Jeffrey D. Crane, Daniel D. Kelson, Gerrad Killion, Vince Kowal, Solange Ramirez, Stephen A. Smee, Johanna K. Teske, and Stephanie Wachter "The Magellan infrared multi-object spectrograph project: 2022 update", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 1218415 (29 August 2022); https://doi.org/10.1117/12.2626995
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KEYWORDS
Cameras

Spectrographs

Aspheric lenses

Collimators

Telescopes

Image quality

Imaging systems

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