|Application Submission Deadline
|06:00:00 UTC 29 September 2023
|Expected Time Allocation Announcement
|mid December 2023
|Observing Period 2024-S1
|8 January 2024 – 30 September 2024
This Announcement of Opportunity is an invitation to the user-communities of the LMT partners to submit scientific proposals requesting observing time on the 50-meter diameter LMT. The deadline to receive proposals is 06:00 UTC on 29 September 2023. The schedule for the next observing season (2024-S1) is 8 January 2024 – 30 September 2024.
The LMT was able to reopen for scientific observations in January 2023, after experiencing downtime in the fall of 2022 due to a need to adjust the telescope’s balance. The scientific program during the 2023-S1 semester has been significantly impacted and delayed by a forest fire in February 2023 which damaged electrical power and fiber-optic cables. This was followed by a series of electrical storms in June 2023 which resulted in further damage to the electrical-grid power lines and also to the site´s electrical substation. Repairs to the electrical substation are not expected to be completed until October 2023. Given the uncertainty in the precise schedule, and considering the engineering activities that must be completed once electrical power at the site is restored, we are forced to delay the start of the next observing season until early January 2024.
Given the lost telescope-time during the 2023-S1 observing season and the large number of excellent scientific proposals, the highest-priority A-grade projects that cannot be completed or attempted before the end of this year will automatically be carried over to the 2024-S1 observing season. We anticipate that approximately 630 hours will be committed to night-time observations of new approved projects from the 2024-S1 review process, and of order 125 hours will be devoted to those carry-over projects from the previous season.
This estimate of available observing time for new scientific projects in the 2024-S1 season takes into account the continued engineering work at the telescope, the nominal loss of time due to weather, the standard observing overheads and the normal calibration observations that are made each night, as well as time expected to be committed to the TolTEC Legacy public surveys. Please note that the time calculators in use for the proposal process also account for observing overheads within an observation, such as motions to reference positions, in their estimation of total required observing time. Finally, we note that observers may anticipate that the on-set of the “rainy season” during the summer will increasingly impact the scheduling of the highest-frequency instruments towards the end of the 2024-S1 observing period (LMT-site Weather Conditions).
Given the anticipated significant demand for telescope time, the LMT user-community is encouraged to submit shorter, high-impact scientific projects that will lead to published research papers that demonstrate the unique capabilities of the telescope facility. Opportunities to submit longer-term large projects will be offered in future Calls for Proposals.
Further information about this proposal opportunity is presented on the LMT website and will be summarized in a series of webinars to be announced shortly.
Principal Investigators that are affiliated with national institutions and universities within the eligible LMT user-communities (Mexico, USA and Spain) will be able to submit proposals and share LMT observing time during the 2024-S1 observing season in the following proportions:
The telescope time associated with each scheduled project will be allocated (charged) to a particular observing queue of the LMT user-communities according to the affiliation of the Principal Investigator. The affiliation of co-investigators, including those external to the eligible LMT user-communities, does not impact the time allocated (charged) to each user-community. For further information on time allocation, please refer to the “Observing Procedures” information page.
The LMT has developed new policies concerning non-standard proposals that may be submitted to the proposal review. We summarize each below:
Unanticipated mechanical problems and natural disasters (forest fires and damage to power infrastructure from severe storms) have greatly impacted the 2023-S1 observing season, both in terms of available observing time and the commissioning of TolTEC. Therefore all remaining A-ranked 2023-S1 projects (including TolTEC projects) that cannot be completed or attempted before the end of the year will automatically be carried over to 2024-S1 season. All PIs of those 2023-S1 proposals with lower ranks are encouraged to update and resubmit their proposals, taking note of referee´s comments, if they are not attempted during the 2023-S1 season.
In the observing period 2024-S1 the LMT will offer the opportunity to conduct observations with the following instruments: TolTEC, SEQUOIA, Redshift Search Receiver (RSR), B4R and MSIP1mm. Summaries of instrument capabilities, observing modes, and time calculators can be found on the “Instrumentation” webpage. Please refer to the LMT “Telescope Description” page for details on the telescope design and function.
The TolTEC, SEQUOIA, RSR and MSIP1mm instruments and data reduction software are fully supported by the LMT and hence no collaboration with members of their instrument teams is required. All observations with these instruments are carried out by a trained observatory staff using a flexible scheduling queue and are processed by a dedicated data reduction pipeline. Each proposing team should read the instrument descriptions carefully and propose only the supported observing modes for each instrument. Proposals requiring a non-standard mode should first contact the LMT Helpdesk at least one week before the proposal deadline to establish its technical feasibility prior to submitting the proposal.
In contrast, the 2mm B4R instrument has been developed and funded independently with no participation from the LMT partners. The B4R team in Japan will provide the technical support and assistance during the preparation of proposals, scientific observations and the data-analysis for all scheduled projects. Therefore the use of the B4R instrument requires a scientific collaboration with the B4R team. Principal Investigators requesting to use the B4R instrument should contact the LMT Helpdesk in order to be put in contact with the B4R instrument team.
TolTEC will continue to operate as a “shared risk” instrument for the 2024-S1 semester. At this time, the commissioning of TolTEC has not allowed an accurate estimation of the instrument mapping speed under the best weather conditions. As a consequence, our estimates of this quantity for the coming semester are uncertain. Therefore, in order to allow TolTEC proposals to be submitted, we have estimated the mapping speed based on commissioning data and reasonable assumptions about the atmosphere and the telescope surface accuracy. Users requesting TolTEC time should make use of the observing time calculator provided with this call for proposals. It is important to consider the uncertainty in the mapping speed of TolTEC when planning projects for this proposal review.
Given the uncertainty in the required observing time to reach a specific sensitivity and our interest in offering opportunities for TolTEC observations to as many members of the LMT user-communities as possible in this initial season, TolTEC proposals should be limited to a maximum of 5 hours as determined by the sensitivity calculator.
The proposal submission process is identical for all members of the eligible scientific communities. LMT observing proposals will be made through a simple web-based form (lmtobservatory.org). Proposals will be required to include a list of participating researchers, a description of the scientific goals and technical feasibility using the requested instruments, and a justification of any special scheduling or weather requirements. Please note that this year the scientific and technical justification documents are required to be in pdf format.
Further details, instructions, and resources on how to prepare and submit a scientific proposal to the LMT can be found on the “Proposal Guidance” information page.
The LMT proposal review will be carried out as a “dual anonymous” review, and all proposals must be submitted in a format that preserves the anonymity of the proposal team. Please see the information page describing the dual anonymous format and procedures for preparation of dual anonymous proposals.
All proposals will be subject to a technical assessment prior to a scientific review conducted by a Time Allocation Committee constituted by members of the eligible user-communities, and supported by independent external expert evaluations. Each user-community will provide a unified prioritized list of proposals covering all scientific areas, based primarily on their anticipated scientific impact, that will be merged into the LMT observing schedule.
The full and proportionate allocation of observing time for the prioritized scientific projects from each user-community will be flexibly scheduled during the observing season to maximize the efficiency of the overall scientific program and the telescope operation. Further information regarding the proposal review process and Time Allocation Committee can be found on the Proposal Review webpage.
We anticipate the scientific and technical reviews to be completed by mid December 2023.
Principal Investigators of the highest-priority projects will be contacted regarding the creation of observing scripts prior to the flexible scheduling of the observations For more information regarding science observing, see the Observing Procedures webpage.
For additional general information on the Call for Proposals, or for assistance with the proposal submission process, please contact the LMT Help Desk.