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检索条件"任意字段=Conference on Advanced Telescope and Instrumentation Control Software"

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The software for MAGIQ: a new acquisition, guiding and image quality monitoring system at the W. M. Keck Observatory

The Software for MAGIQ: a new acquisition, guiding and image...

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2nd conference on advanced software and control for Astronomy

作者： Kwok, Shui Hung Johnson, Jimmy Adkins, Sean M. McCann, Kevin WM Keck Observ Kamuela HI 96743 USA

ISBN: (纸本)9780819472298

The W. M. Keck Observatory has completed the development and initial deployment of MAGIQ, the Multi-function Acquisition, Guiding and Image Quality monitoring system. MAGIQ is an integrated system for acquisition, guiding and image quality measurement for the Keck telescopes. This system replaces the acquisition and guiding hardware and software for existing instruments at the Observatory and is now the standard for visible wavelength band acquisition cameras for future instrumentation. Innovative features are provided in the MAGIQ software for use by observers and telescope operators including advanced capabilities for acquisition and image quality monitoring. In this paper we report on the design and implementation of the MAGIQ software components, including the process for developing requirements, the implementation choices and strategies, the software features and user interfaces, and the challenges of test and deployment in a working observatory.

关键词： software telescope controls Acquisition Guiding Image Quality

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Automated HST/STIS reference file generation pipeline using OPUS

Automated HST/STIS reference file generation pipeline using ...

引用

2nd conference on advanced software and control for Astronomy

作者： Diaz, Rosa I. Swam, Michel Goudfrooij, Patil Space Telescope Sci Inst Baltimore MD 21218 USA

ISBN: (纸本)9780819472298

Bias and Dark reference, files are part of the basic reduction of the CCD data taken by the Space telescope Imaging Spectrograph (STIS) aboard the Hubble Space telescope (HST). At STScI, the STIS team has been creating these reference files using the Bias and Dark Pipeline. This pipeline system starts with automatic retrieval of bias and dark exposures from the HST archive after they have been ingested. After data retrieval, a number of automatic scripts is executed in a, manner compatible with the OPUS pipeline architecture. We encourage any group looking to streamline a stepwise calibration process to look into this software.

关键词： OPUS HST pipeline STScI STIS PyRAF calibration

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advanced Technology Solar telescope: A progress report

Advanced Technology Solar Telescope: A progress report

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conference on Ground-Based and Airborne instrumentation for Astronomy II

作者： Wagner, J. Rimmele, T. R. Keil, S. Hubbard, R. Hansen, E. Phelps, L. Warner, M. Goodrich, B. Richards, K. Hegwer, S. Kneale, R. Ditsler, J. Natl Solar Observ 950 N Cherry Ave Tucson AZ 85719 USA Natl Solar Observ Sunspot NM 88349 USA

ISBN: (纸本)9780819472229

The four-meter advanced Technology Solar telescope (ATST) will be the most powerful solar telescope and the world's leading resource for studying solar magnetism that controls the solar wind, flares, coronal mass ejections and variability in the Sun's output. Development of a four-meter solar telescope presents many technical challenges (e.g., thermal control of the enclosure, telescope structure and optics). We give a status report of the ATST project (e.g., system design reviews, PDR, Haleakal (a) over bar site environmental impact statement progress) and summarize the design of the major subsystems, including the telescope mount assembly, enclosure, mirror assemblies, wavefront correction, and instrumentation.

关键词： large telescope construction solar astronomy optics wavefront correction telescope enclosure instrumentation high-level software

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Instrument control tool kit for the Subaru telescope laser guide star adaptive optics system

Instrument control tool kit for the Subaru telescope laser g...

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2nd conference on advanced software and control for Astronomy

作者： Dinkins, Matthew Natl Inst Nat Sci Natl Astron Observ Japan Subaru Telescope Hilo HI 96720 USA

ISBN: (纸本)9780819472298

The Subaru Adaptive Optics instrument development requires reliable software that can be quickly modified to facilitate testing and changing demands. A software tool kit was created to allow rapid inclusion of diverse hardware, to isolate specific hardware, to allow expert users to write programs that interface hardware, and to allow multiple access points for control and status. The flexibility of this system allows the software to not only control the Subaru Adaptive Optics Instrument, but also a wide variety of instruments. Also, once a low level interface is written for the hardware, the hardware controls can be combined into any configuration without any programming. This analysis explains the overall software architecture of the system, the methods used to promote hardware testing, the process for adding hardware, and the flexibility inherent in the software's architecture.

关键词： Hardware control Client Server Publish Subscribe Adaptable Tool Kit

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Gathering headers in a distributed environment

Gathering headers in a distributed environment

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2nd conference on advanced software and control for Astronomy

作者： Goodrich, Bret D. Wampler, Steve B. Hubbard, John R. Natl Opt Astron Observ Natl Solar Observ Tucson AZ 85726 USA

ISBN: (纸本)9780819472298

The advanced Technology Solar telescope (ATST) has implemented a novel method for gathering header information on data products. At the time of data collection, the specific state of the telescope and instrumentation needs to be collected and associated with the saved data. The ATST performs this task by issuing a header request event across the ATST event system. All observatory software components that are registered for the event and are participating in the current experiment or observation report status information to a central header repository. Various types of header request events may be selected for start or stop of individual frames, groups of frames, or entire observations. The final data products are created by combining the data files with all or some of stored header information in the database. The resulting data file may be generated in any possible format, including FITS. Much of the implementation of this approach is integrated into the ATST technical framework, simplifying the development process for component writers and ensuring consistent responses to header request events.

关键词： software headers scatter-gather

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The LBT-AdOpt Arbitrator. Coordinating many loosely coupled processes

The LBT-AdOpt Arbitrator. Coordinating many loosely coupled ...

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2nd conference on advanced software and control for Astronomy

作者： Fini, Luca Tosetti, Fabio Busoni, Lorenzo Puglisi, Alfio Xompero, Marco Osserv Astrofis Arcetri INAF I-50125 Florence Italy

ISBN: (纸本)9780819472298

The LBT-AdOpt Supervisor is a collection of software processes which control the operations on the set of devices which make up the Adaptive Optics subsystem. The Arbitrator is the software component which coordinates the operations of the Supervisor in order to support operations at the telescope in reply to requests issued by the Instrument control software. In this paper we describe the architecture of the Arbitrator, based on an extremely modular, extensible and maintainable approach, designed using object-oriented techniques, that include intensive use of classes, exception handling and design patterns, as well as a, clear division of tasks.

关键词： Adaptive Optics control software LBT

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Concise telescope pointing algorithm using IAU 2000 precepts

Concise telescope pointing algorithm using IAU 2000 precepts

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2nd conference on advanced software and control for Astronomy

作者： Wallace, Patrick T. Rutherford Appleton Lab STFC Space Sci & Technol Dept Didcot OX11 0QX Oxon England

ISBN: (纸本)9780819472298

The accuracy requirements for pointing a ground-based telescope or antenna are comparatively modest;the latest Earth orientation models used by specialists have precision goals measured in microareseconds and are excessive for such humble applications. Abridged formulations offer an attractive alternative: easier to get right, and much quicker to compute. Moreover, the revised computational procedures that the IAU introduced in 2000 to assist high-precision studies of Earth rotation lend themselves to approximation. Together with basic models for aberration and refraction, a page of inline C code is enough to predict the observed altazimuth coordinates of a star to an accuracy of 1-2 arcseconds, which is adequate for pointing a small telescope. This can be complemented by a similarly concise formulation of the basic pointing corrections for an equatorial or altazimuth mount.

关键词： pointing precession

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software design for the control system of Small LAMOST

Software design for the control system of Small LAMOST

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2nd conference on advanced software and control for Astronomy

作者： Yang, Shihai Chinese Acad Sci Nanjing Inst Astron Opt & Technol Natl Astron Observ Nanjing 210042 Peoples R China

ISBN: (纸本)9780819472298

The Large Sky Area Multi-Object Fiber Spectroscopic telescope, LAMOST hereafter, will become an astronomical telescope with largest field of view and most efficient observation in 4-m aperture telescopes in the world by its completion in 2008. In June 2007, Small System for LAMOST was completed successfully. Small LAMOST is composed of mirror with aperture of 3 meter (effective aperture of 2 meter), 250 fibers, one spectrograph, two 4k x 4k CCD camera, tracking and controlling system. This paper presents the study in Small LAMOST. It comprises three main parts. First, it introduces the software design for the control system of Small LAMOST, including Mount tracking, Focal Plane tracking, GPS time ticking and time synchronization between computers, auto-guiding, etc. The design has proved correct and feasible. Second, it describes some technical solutions to the requirements of precision, real time and open architecture for Small LAMOST. Lastly, sonic experimental data and curves are given to show the tracking precision of Small LAMOST.

关键词： software servo control real time tracking drive system Small LAMOST

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Wind Evaluation Breadboard electronics and software

Wind Evaluation Breadboard electronics and software

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2nd conference on advanced software and control for Astronomy

作者： Nunez, Miguel Reyes, Marcos Viera, Teodora Zuluaga, Pablo Inst Astrofis Canarias Tenerife Spain

ISBN: (纸本)9780819472298

WEB, the Wind Evaluation Breadboard, is an Extremely Large telescope Primary Mirror simulator, developed with the aim of quantifying the ability of a segmented primary mirror to cope with wind disturbances. This instrument supported by the European Community (Framework Programme 6, ELT Design Study), is developed by ESO, IAC, MEDIA-ALTRAN, JUPASA and FOGALE. The WEB is a bench of about 27 tons and 7 meter diameter emulating a segmented primary mirror and its cell, with 7 hexagonal segments simulators, including electromechanical support systems. In this paper we present the WEB central control electronics and the software development which has to interface with: position actuators, auxiliary slave actuators, edge sensors, azimuth ring, elevation actuator, meteorological station and air balloons enclosure. The set of subsystems to control is a reduced version of a real telescope segmented primary mirror control system with high real time performance but emphasizing on development time efficiency and flexibility, because WEB is a test bench. The paper includes a detailed description of hardware and software, paying special attention to real time performance. The Hardware is composed of three computers and the software architecture has been divided in three intercommunicated applications and they have been implemented using Labview over Windows XP and Pharlap ETS real time operating system. The edge sensors and position actuators close loop has a sampling and commanding frequency of 1 KHz.

关键词： ELT ESO IAC WEB segmented primary mirror wind soft-ware Labview

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software structure for Vega/Chara instrument

Software structure for Vega/Chara instrument

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2nd conference on advanced software and control for Astronomy

作者： Clausse, J-M CNRS UNS OCA UMR6525 Lab AH Fizeau F-06130 Grasse France

ISBN: (纸本)9780819472298

VEGA (Visible spEctroGraph and polArimeter) is one of the focal instruments of the CHARA array at Mount Wilson near Los Angeles. Its control system is based on techniques developed on the GI2T interferometer (Grand Interferometre a 2 telescopes) and on the SIRIUS fibered hyper telescope testbed at OCA (Observatoire de la Cote d'Azur). This article describes the software and electronics architecture of the instrument. It is based on local network architecture and uses also Virtual Private Network connections. The server part is based on Windows XP (VC++). The control software is on Linux (C, GTK). For the control of the science detector and the fringe tracking systems, distributed API use real-time techniques. The control software gathers all the necessary informations of the instrument. It allows an automatic management of the instrument by using an original task scheduler. This architecture intends to drive the instrument from remote sites, such as our institute in South of France.

关键词： Interferometer Real time software scheduler intensified detector instrument control

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