Call for Proposals

To: Observers on the Automated Planet Finder (APF) 2.4 m telescope
From: Claire Max, UCO Director
Date: March 10th, 2021
Semester 2021B
(August 1st, 2021 through January 31st, 2022)

Deadline: Tuesday, April 20th, 2021 at 5:00 pm PST

The APF is now by default a queue scheduled telescope. Because of this policy:

  • Requested nights should be “clear” nights with no correction for weather, only science observation time and overheads will be charged to a program.
  • The TAC will be allocating time based on the expected 800 hours of clear time for UC proposals.
  • Queue priorities will be set based on TAC grades.
  • We welcome all proposals for high resolution, R > 80,000, spectroscopy of stars as well as proposals for precision radial velocities of GKM stars.
  • We encourage proposals to request additional time for your program on the cover sheet, in case other programs cannot be executed or the APF is undersubscribed.


Proposal Information

Information about the APF telescope can be found at:
https://apf.ucolick.org

For the 2021B semester, 800 hours will be available in the APF queue for UC proposals.

The time will be scheduled in two different modes at the request of the observers. The observer can (1) ask for their targets to be inserted into the queue operated by the University of California Observatories (Cadence), or (2) ask for specific nights and conduct observations as they wish (Classical). Classical requests need to be justified.

All time requests should be in hours. The cover sheet should list the request in nights, assuming 10 hours per night, with fractional nights as appropriate. The TAC will allocate grades to the proposals and those grades (A, B, C) will determine the relative priority on any given night, with guaranteed or purchased time being granted A time.

The queue will be run on all nights, except for the whole or half nights allocated to specific classical programs. The queue software is capable of handling multiple programs per night. The target list and the data files for a given observer will be private to the PI unless otherwise requested. A given program can be executed on any given night the queue is running, with the balance of observing time monitored over the course of the semester to match the allocated amount. Simple cadence requirements, ranging from multiple times a night, to once a month can be met and the total observations can easily be supported.

 

Sincerely,

Claire Max, UCO Director
Director's Office
UCO/Lick Observatory
Interdisciplinary Sciences Building
University of California
1156 High Street
Santa Cruz, CA 95064