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Proposals & Updates for Time on Optical/IR Telescopes
Time on all Optical/IR UAO telescopes is allocated in two semesters: February-July (A) and August-January (B). Proposal deadlines are now October 1 and April 1, or a nearby date (Apr 3, 2023 for 2023B) if the time falls on a weekend: See the call for proposals email. Late proposals will not be considered.
GTO proposals are due Apr 24, 2023.
All proposers (general and GTO partners) should submit electronically the completed latex form and the processed pdf version to a site to be announced later. Passwords will have been provided in the respective Call for Proposals from the TAC Chair. Unless you receive special permission from the TAC Chair, the proposals must be submitted by the deadline.
Make sure to download the current proposal template file soprop.tex and class file soprop.cls, which are required to produce the pdf file that is uploaded by the electronic submission form. Your proposal will not be processed by the automated account if you use an outdated version of the template files. They are attached (unchanged, actually) to the cal lfor proposals.
The new submission site is https://mtnops-tac.as.arizona.
We update these notes whenever we're given new news. It's always safest to contact the PI of an instrument.
LBT: Proposers need to also submit Phase I Tool (PIT) form by noon on April 3 as well. The PIT form is available at https://sites.google.com/a/
MMTCam: MMTCam should only be used for ToO imaging projects, and projects that require shallow u band imaging. Note that there is no guiding with MMTCam. Non-ToO imaging projects, particularly those needing deep exposures, should use Binospec, where guiding is possible and the noise is much lower. ToO projects can of course use Binospec, and indeed current ToO projects have time assigned on both instruments.
MMT Red Channel: Red Channel is NOT available because of serious CCD issues. Contact Joannah Hinz for details. (Sept 8, 2021).
MagAO : MagAO will NOT be available in 2023B. Contact Laird Close (lclose@as.arizona.edu) for information. (Sept 9, 2022)
MagAO-X: Will not be offered in 2023B. Talk to Jared Males for information about 2024A.
Michigan/Magellan IFUM- Mario Mateo is the PI of a set of three IFU systems for Magellan/Clay. Contact him (mmateo@umich.edu) for more information and to propose. Here is some information: Three fiber-fed IFUs: Low Surface Brightness (LSB) at 1.90 arcsec/spaxel and 18x20 spaxels, Standard-seeing (STD at 1.09 pixels per spaxel with 23x24 spaxels, High Resolution (HR) with 0.54 arcssec per spaxel and 27x32 spaxels. Resolutions range from 1000 to 38000. All three modes support three different resolutions; IFUs user-deployable but only one can be used at a time; Optical Layout: Hexagonal lenslet array defines field. Barlow lenses modify field scale to make lenslets, fiber mounts more manageable; Occultors (focal plane masks) available to block bright sources in field; User-selected slit mechanism to choose spectral resolution (at cost of light loss); IFU-M fibers feed MSpec (the spectrograph for M2FS) and can use all MSpec features (order isolation, spectral resolutions, CCD configs, etc.); contact Mario or the TAC Chairman for a table of IFU parameters and other information.
MAESTRO: The MMT Advanced Echelle Spectrograph will not be supported this semester.
The Arizona Radio Observatory (ARO) at regular intervals solicits proposals for the 10-meter Submillimeter Telescope (SMT) located on Mount Graham, Arizona, and the new ALMA Prototype 12-meter Telescope (12m) located on Kitt Peak, Arizona. There will be an email call for proosals. The new ARO website is HERE.
(Mar 14, 2023)

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