Niall I. Gaffney
Hobby-Eberly Telescope
Mark E. Cornell
McDonald Observatory
We present the initial design of the planning and scheduling software
for the 9.2 meter Hobby-Eberly Telescope (HET) currently being
commissioned in West Texas. The HET is operated by McDonald
Observatory on behalf of the University of Texas at Austin, the
Pennsylvania State University, Stanford University,
Ludwig-Maximilians Universitat München, and Georg-August
Universitat Göttingen. Once completely operational, 85 nights
are expected to be used in a queued mode where the night is
dynamically scheduled as observing conditions change. In this mode,
data are acquired by resident astronomers on behalf of potentially
many different PIs for many different observational projects each night.
In order to reduce construction costs, the HET is fixed in altitude at
, and tracks an object with an Arecibo-style
tracker.
Consequently, the HET can access only a limited portion of the sky at
any time and can only track an object for roughly an hour at a time.
Because of these motion constraints, efficient use of the telescope
relies strongly on software. Software tools are required to know when
and how an object can be observed and how best to sequence
observations over the course of a night. Our system contains both
planning and scheduling tools. Planning tools are used to determine
the feasibility of observations to be made with the HET. Scheduling
tools are used to schedule observations during a night and over the
course of an observing semester. Initially, command line driven tools
were developed which make conceptually separate numerical calculations
for HET operations. Next, TCL/TK GUIs were layered on top of the
command line driven programs. This scheme has two benefits: pipeline
processing of object lists will be possible without using the GUIs and
several simple tools can be combined to create one, more complex,
tool. We will present examples of our planning and scheduling
software, their functionality, and their expected use.