The system software development for Prime Focus Spectrogrsph on Subaru Telescope
Atsushi Shimono, Naoyuki Tamura, Hajime Sugai, Hiroshi Karoji (Kavli, Institute for the Physics, Mathematics of the Universe, The University of, Tokyo, Japan)

TL;DR
This paper presents the conceptual design of the control and observation preparation software for the Prime Focus Spectrograph on the Subaru Telescope, enabling efficient multi-object astronomical observations.
Contribution
It introduces the integrated system design for software managing fiber positioning, telescope pointing, and data archiving for the PFS instrument.
Findings
Design of software architecture for PFS control system
Efficient fiber allocation algorithms for target observation
Integration of control software with database systems
Abstract
The Prime Focus Spectrograph (PFS) is a wide field multi-fiber spectrograph using the prime focus of the Subaru telescope, which is capable of observing up to 2400 astronomical objects simultaneously. The instrument control software will manage the observation procedure communicateing with subsystems such as the fiber positioner "COBRA", the metrology camera system, and the spectrograph and camera systems. Before an exposure starts, the instrument control system needs to access to a database where target lists provided by observers are stored in advance, and accurately position fibers onto astronomical targets as requested therein. This fiber positioning will be carried out interacting with the metrology system which measures the fiber positions. In parallel, the control system can issue a command to point the telescope to the target position and to rotate the instrument rotator.…
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