MMIRS resides permanently at the MMT, and the observing is run in queue mode only. Astronomers do not need to be present at the MMT for their observations. If you have questions about queue observing, please contact Joannah Hinz.
Instrument description for observers
- About Queue Scheduling
- General Target Submission Information
- Imaging Targets
- Long Slit Targets
- Multi-Object Slit Mask Targets
- MMIRSMask – Interactive Mask Design Software
Raw data for all observations and reduced data for spectra only can be obtained by clicking the personalized link for your program or by emailing the SAO Telescope Data Center helpdesk. The data reduction pipeline was written by I. Chilingarian.