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control system of the FOCAS instrument for the SUBARU telescope

Control system of the FOCAS instrument for the SUBARU telesc...

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telescope control Systems ii conference

作者： Sasaki, T Yoshida, M Shimizu, Y Kosugi, G Kashikawa, N Yadoumaru, Y Takata, T Iye, M National Astronomical Observatory (Japan)

ISBN: (纸本)0819425346

control software of FOCAS ( Faint Object Camera And Spectrograph) is being developed as a prototype of control software for SUBARU observing instruments. The software system consists of several processes;a network interface process, a user interface process, a central control engine process, a command dispatcher process, local control units, and a data acquisition system. Each process is communicated to other processes and controlled by passing messages of commands and its status. A control flow and generalized command messages are defined following the software guideline for the SUBARU instruments. Functionality of each process is presented. Related off-line software for making multi-slit plates and for data analysis is briefly described.

关键词： Subaru telescope astronomical instrument spectrograph control software FOCAS

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Integration tests of the VLT telescope control System

Integration tests of the VLT Telescope Control System

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telescope control Systems ii conference

作者： Chiozzi, G Wirenstrand, K Ravensbergen, M Gilli, B European Southern Observatory (Germany)

ISBN: (纸本)0819425346

The installation of the complete VLT telescope control system on the observatory is a complex task. It is important that the various components of the system have been carefully tested and integrated before. This paper presents the ESO strategy to pre-installation testing. In particular, results and experiences from pre-erection tests of the telescope structure are presented. In these tests, the complete telescope structure, including both axes with encoders and drives, has been built up at the premises of the European manufacturer (in Milan, Italy). These tests provide valuable input for the erection on Paranal. To this system, ESO added control electronics and software, which was tested with the telescope. The complete positioning of both main axes is under test, including slewing and tracking performance tests, as far as this is possible without using the sky. The VLT control software and most parts of the VLT control electronics have also been tested on the NTT on La Silla. Since the NTT upgrade software is practically a subset of the VLT software, the NTT tests have provided invaluable feedback for the VLT, The NTT tests are described in a separate paper presented at this conference[7]. The paper also briefly discusses subsystem tests, and presents results from some of the subsystem tests performed in Europe.

关键词： control system real time control testing telescope integration

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control software and scheduling of the Liverpool Robotic telescope

Control software and scheduling of the Liverpool Robotic Tel...

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telescope control Systems ii conference

作者： Steele, IA Carter, D Liverpool John Moores Univ. (United Kingdom)

ISBN: (纸本)0819425346

The Liverpool telescope will be a fully robotic 2m telescope situated in La Palma and managed from Liverpool John Moores University. The data flows between the robotic components of the telescope are discussed and the functionality of those components described. We pay particular attention to the design of the telescope scheduler. Using simulations we show that a relatively simple dispatch scheduler may be tuned to produce a schedule that has acceptable trade-offs between conflicting scheduling criteria.

关键词： telescopes robotic telescopes telescope control systems telescope scheduling

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The Portable telescope control System project

The Portable Telescope Control System project

引用

telescope control Systems ii conference

作者： Bailey, J Prestage, R Anglo-Australian Observatory Epping NSW 2121 PO Box 296 Australia Joint Astronomy Centre Hilo HI 96720 660 N A'ohoku Place United States

ISBN: (纸本)0819425346

The Portable telescope control System (PTCS) project is a collaboration between the Anglo-Australian Observatory and the Joint Astronomy Centre, Hawaii. The project aims to develop telescope control software in a form which is portable between a wide range of computer systems, and which can easily be adapted to different telescopes. PTCS uses the DRAMA software environment which provides a high degree of operating system independence. The PTCS design is based on tested algorithms used in existing successful telescope control systems. The initial version of PTCS is now being interfaced to an EPICS based drive servo system for use with the James Clerk Maxwell sub-millimetre telescope on Mauna Kea.

关键词： telescope control Systems DRAMA EPICS

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NTT project: a field test of the VLT software and hardware

NTT project: a field test of the VLT software and hardware

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telescope control Systems ii conference

作者： Wallander, A Spyromilio, J European Southern Observatory (Germany)

ISBN: (纸本)0819425346

The NTT project had the principal aim of field testing the VLT control system prior to installation on UT1 on Paranal. In July 96 we began installing the control electronics and software. The telescope was stripped down to the field electronics and completely rewired. First light was achieved 2 months later and the integration of the system was completed 4 months after that. The VLT control system has been proven to be functional and fundamentally sound. Over 80% of the VLT control system is mirrored on the NTT with deviations only allowed where the hardware made it impossible to reuse the code prepared for Paranal. The NTT will operate with the complete control system executing service observations following the shake down period in early 1997.

关键词： prototyping control systems software engineering pointing tracking

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User interface and control software for the HIRES image rotator on Keck-1

User interface and control software for the HIRES image rota...

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telescope control Systems ii conference

作者： Kibrick, R Conrad, A Gathright, J Tucker, D University of California/Santa Cruz Lick Observatory (United States) California Association for Research in Astronomy and W. M. Keck Observatory (United States)

ISBN: (纸本)0819425346

We describe the control and user interface software for the image rotator on the High Resolution Echelle Spectrometer (HIRES), located at the Nasmyth focus of the Keck-l 10-meter telescope. This image rotator counteracts the field rotation induced by the alt-az telescope mount and aligns the image delivered to the spectrometer slit and the slit-viewing TV camera. The rotator can align the image so that either a specified position angle on the sky or the atmospheric dispersion vector is held fixed relative to the slit. The rotator is physically an integral part of the spectrometer;but, since it affects telescope pointing and auto-guiding, it can also be considered part of the telescope. Accordingly, it interacts with the control systems for both the telescope and spectrometer. The apportionment of rotator control functions between these two systems poses interesting operational challenges. Since the telescope operator and the observer each need to operate the rotator at various times, their respective user interfaces must provide consistent rotator control and status functions.

关键词： image rotator user interface

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Galileo high-resolution encoder system

Galileo high-resolution encoder system

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telescope control Systems ii conference

作者： Mancini, D Cascone, E Schipani, P Astronomical Observatory of Capodimonte (Italy)

ISBN: (纸本)0819425346

The Galileo National telescope (TNG) is a 3.6 meter Alt-Az telescope installed at the Astronomical Observatory of the Rogue de Los Muchachos in La Palma, Canary Islands (Spain). The TNG motion control system, designed and realized by the Technology Working Group (TWG), is completely digital because of the versatility of this system typology. In a digital control system using an encoder as transducer means to have a digital feedback signal, therefore directly comparable with the reference without any conversion that is essential with other kinds of transducers. In the following the Galileo telescope (TNG) encoder system with its control electronics and the management software will be described. It has been realized by a collaboration between the Heidenhain Company and the TWG. The TNG encoder system, at the state of the art, has one of the highest performance in the telescopes field, in terms of resolution, accuracy, readout time, reliability.

关键词： encoder telescope position transducer control system

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Preparation for VLT software commissioning at Paranal.

Preparation for VLT software commissioning at Paranal.

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telescope control Systems ii conference

作者： Allaert, E Raffi, G European Southern Observatory (Germany)

ISBN: (纸本)0819425346

The Very Large telescope (VLT) software commissioning has started since a while, earlier than any VLT subsystems were ready for integration. This was possible thanks to the New Technology telescope (NTT) upgrade (reported in a separate paper, Ref. 3), which shares most of the software with the VLT. The integration tests with the main VLT structure do also represent another fundamental milestone in the software commissioning process (see also separate paper, Ref. 4). The whole control software is based on a very distributed computer architecture. The final layout of the computers (workstations and microprocessors), networking devices and underlying concepts have been tested both at the NTT and on the so called VLT computer control model, a relevant off-line subset of the computer equipment to be used in the VLT control room and telescope area for one unit telescope. The VLT common software, including a real-time database, is the stable core of the whole VLT control software. This comprises also high level applications, like the Real-Time Display (RTD), the Panel Editor and the CCD software to be used for technical CCDs. It is distributed with a policy of regular releases, subject to automatic regression tests and is used by VLT Consortia and Contractors too. New modules have been added to insert the VLT control software in the Data Flow context, interfacing it in particular to Scheduler and Archive. The VLT software support team will soon start regular operation at the VLT Paranal site, providing continuity between the integration activities of the various subsystems. They will be the front-end of the commissioning effort, based also on background support provided over links from the European headquarters.

关键词： control software commissioning network computer architecture software management progress report

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Subaru observation control system

Subaru observation control system

引用

telescope control Systems ii conference

作者： Kosugi, G Sasaki, T Aoki, T Kawai, J Koura, N Kusumoto, T National Astronomical Observatory (Japan) Kiso Observatory/Univ. of Tokyo (Japan) Fujitsu Ltd. (Japan) Fuji FACOM System Corp. (Japan)

ISBN: (纸本)0819425346

An observation with Subaru telescope is designed to be executed by the central scheduler process. control commands are abstracted common to all observation instruments so that the observers are free from the consciousness of the difference between many instruments as much as possible. An abstraction command which is described in an observation procedure is expanded to a device dependent command script, and the script is dispatched to the telescope and instruments by referring to the instrument table. Device dependent commands are processed synchronously or asynchronously by checking the status against interlocks. The structure of the scheduler and the instrument table, the flow of commands such as an abstraction command, a device dependent command script and a device dependent command, their examples and syntax are described.

关键词： Subaru telescope observation control scheduling software

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Chopping secondary mirror control systems for the W. M. Keck telescopes

Chopping secondary mirror control systems for the W. M. Keck...

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telescope control Systems ii conference

作者： Lupton, W W. M. Keck Observatory (United States)

ISBN: (纸本)0819425346

The Keck 1 chopping secondary was built by the Pale Alto Research Laboratories of the Lockheed (now Lockheed Martin) Missiles and Space Company. The only software component of the delivered system is a proprietary error correction algorithm;Keck wrote software to generate acceleration-limited Azimuth and Elevation demands, to rotate these demands as a function of telescope position, to interact with the error correction system, and to manage hardware start-up and shutdown. The Keck 2 chopping secondary, also built by Lockheed, was originally conceived as an infrared fast steering mechanism (IFSM) and is simpler than the Keck 1 system, with lower power and acceleration limits and, therefore, lower chop amplitude and frequency specifications. As far as possible, it provides the same external interfaces as the Keck 1 system. A new EPICS-based telescope control system has been written for Keck 2 and was retrofitted on Keck 1 in March 1997. The Keck 1 chopper control software has been converted to the EPICS environment and, at the same time, altered so that the same software supports both choppers. This conversion has retained as much as possible of the complex real-time code of the old system while at the same time fully utilizing EPICS facilities. The paper presents more details of both the old and the new systems and illustrates how the new system is simpler than the old as well as being much better integrated into the overall telescope control system. Operational experience will be presented.

关键词： chopper control EPICS infrared Keck telescope Lockheed Tcl/Tk VME VxWorks

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