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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 NEWFIRM Observing software: From Design To Implementation

The NEWFIRM Observing Software: From Design To Implementatio...

引用

2nd conference on advanced software and control for Astronomy

作者： Daly, P. N. Buchholz, N. C. Fitzpatrick, M. J. Mills, D. Valdes, F. G. Zarate, N. Swaters, R. Probs, R. G. Dickinson, M. Natl Opt Astron Observ 950 N Cherry Ave Tucson AZ 85719 USA Univ Maryland Dept Astron College Pk MD 20742 USA

ISBN: (纸本)9780819472298

NEWFIRM is the wide-field infra-red mosaic camera just delivered and commissioned on the Mayall 4-m telescope on Kitt Peak. As with other major instrumentation projects, the software was part of a, design, development, implementation and delivery strategy. In this paper, we describe the final implementation of the NEWFIRM software from acquisition within a MONSOON controller environment, directed by the observation control system, to the quick-look functionality at the telescope and final delivery of standardized data products via the pipeline. NEWFIRM is, therefore, the culmination of several years of design and development effort on several fronts.

关键词： software control Systems Data Products Pipeline Reduction Guiding

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A Framework for the Subaru telescope Observation control System Based on the Command Design Pattern

A Framework for the Subaru Telescope Observation Control Sys...

引用

2nd conference on advanced software and control for Astronomy

作者： Jeschke, Eric Bon, Bruce Inagaki, Takeshi Streeper, Sam Natl Inst Nat Sci Natl Astron Observ Japan Subaru Telescope Hilo HI 96720 USA

ISBN: (纸本)9780819472298

Subaru telescope is developing a second-generation Observation control System (OCS) that specifically addresses some of the deficiencies of the current Subaru OCS. One area of concern is better extensibility: the current system uses a custom language for implementing commands with a complex macro processing subsystem written in C. It is laborious to improve the language and awkward for scientists to extend and use standard programming techniques. Our Generation 2 OCS provides a lightweight, object-oriented task framework based on the Command design pattern. The framework provides a base task class that abstracts services for processing status and other common infrastructure activities. Upon this are built and provided a set of "atomic" tasks for telescope and instrument commands. A set of "container" tasks based on common sequential and concurrent command processing paradigms is also included. Since all tasks share the same exact interface, it is straightforward to build up compound tasks by plugging simple tasks into container tasks and container tasks into other containers, and so forth. In this way various advanced astronomical workflows can be readily created, with well controlled behaviors. In addition, since tasks are written in Python, it is easy for astronomers to subclass and extend the standard observatory tasks with their own custom extensions and behaviors, in a high-level, full-featured programming language. In this talk we will provide an overview of the task framework design and present preliminary results on the use of the framework during two separate engineering runs.

关键词： Design Pattern Command Processing Tasks Python Framework

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A Lightweight, Fault-Tolerant Middleware for a Subaru telescope Second Generation Observation control System

A Lightweight, Fault-Tolerant Middleware for a Subaru Telesc...

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2nd conference on advanced software and control for Astronomy

作者： Jeschke, Eric Bon, Bruce Inagaki, Takeshi Streeper, Sam Natl Inst Nat Sci Natl Astron Observ Japan Subaru Telescope Hilo HI 96720 USA

ISBN: (纸本)9780819472298

Subaru telescope is developing a second-generation Observation control System that specifically addresses some of the shortcomings of the current Subaru OCS. Two areas of concern are complexity and failure handling. The current system has over 1000 dedicated OCS processes spread across a dozen hosts and provides nothing in the way of automated failover. Furthermore, manual failover is so fraught with difficulty that it is rarely attempted. Our Generation 2 OCS is written almost entirely in Python and builds upon a Subaru-developed middleware based on the XML-RPC protocol. This framework offers the following benefits: has very few dependencies outside of standard Python provides a nearly seamless remote proxy object-oriented interface provides optional user/password authentication and/or SSL encryption is extremely simple to use from client applications is connectionless, and assists transparent failover of communications and distributed services on a set of hosts has reasonable performance for a wide range of needs allows multiple language bindings for dynamic languages, requires no interface stub files The "back end" (service side) of the OCS is nearing completion, and has already been used successfully during two separate OCS engineering runs. It is comprised of only a couple dozen processes, and provides automated failover capabilities on a rack of commodity x86 Linux servers. We provide an overview of the middleware use, its design and its failover capabilities. Some data on the performance of communications using the middleware protocol is included.

关键词： Middleware XML-RPC Python Framework Failover

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An Amateur telescope control System: Towards a Generic telescope control Model

An Amateur Telescope Control System: Towards a Generic Teles...

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2nd conference on advanced software and control for Astronomy

作者： Tobar, Rodrigo J. von Brand, Horst H. Araya, Mauricio A. Lopez, Joao S. Univ Tecn Federico Santa Maria Dept Informat Valparaiso 1680 Chile

ISBN: (纸本)9780819472298

control System for an Amateur telescope (CSAT) is a distributed telescope control system model for amateur telescopes with transparent interchangeable components, built using the ALMA Common software (ACS) framework. The CSAT project has been thought as the first step towards a generic telescope control model, which will consist on a generic control framework for any telescope mount. With the ACS Container/Component model, a completely different hardware can be supported by just re-implementing the low-level components for the new setup. This way, CSAT becomes a very good example of all the features that ACS provides for building a generic telescope control framework.

关键词： CORBA ACS TCS Amateur telescope Distributed systems

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software for the EVLA, Current Status

Software for the EVLA, Current Status

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2nd conference on advanced software and control for Astronomy

作者： Butler, Bryan J. Harland, David Truitt, Brian Rochford, James Witz, Stephan Natl Radio Astron Observ Socorro NM 87801 USA

ISBN: (纸本)9780819472298

The Expanded Very Large Array (EVLA) project is the next generation instrument for high resolution long-millimeter to short-meter wavelength radio astronomy. It is currently funded by NSF, with completion scheduled for 2012. The EVLA will upgrade the VLA with new feeds, receivers, data transmission hardware, correlator, and a new software system to enable the instrument to achieve its full potential. This software includes both that required for controlling and monitoring the instrument and that involved with the scientific dataflow. This manuscript presents an update on the overall design, and details for the pre-observing portions of the software, including: user authentication;proposal preparation, submission, and handling;and observation preparation. It will focus particularly on the observation preparation software, describing an implementation of a web-based interface for creation of a detailed observation description, and plans to achieve common observation preparation software with the ALMA telescope.

关键词： NRAO EVLA software

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Installation and first light of the BOOTES-IR near-IR camera

Installation and first light of the BOOTES-IR near-IR camera

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2nd conference on advanced software and control for Astronomy

作者： Cunniffe, R. Castro-Tirado, A. J. Kubanek, P. Jelinek, M. Vitek, S. Gorosabel, J. Postigo, A. de Ugarte Riva, A. Zerbi, F. Claret, A. Sanchez-Fernandez, C. CSIC Inst Astrofis Andalucia Granada 18008 Spain Osservetorio Astronom Brera I-23807 Merate Lc Italy ESAC Madrid Spain

ISBN: (纸本)9780819472298

BIRCAM is a near-infrared (0.8-2.5um) cryogenic camera based on a 1Kx1K HgCdTe array. It was designed for - and is now mounted at - one of the Nasmyth foci of the fast-slewing 0.6 m BOOTES-IR telescope at the Sierra Nevada Observatory (OSN) in Spain. The primary science mission is prompt Gamma Ray-Burst afterglow research, with an implied demand for extremely time-efficient operation. We describe the challenges of installing a heavy camera on a small high-speed telescope, of integrating the dithering mechanism, the filterwheel, and the array itself into a high-efficiency instrument, the design of the software to meet the requirements.

关键词： Robotic telescopes telescope software near-IR instrumentation cryogenics

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advanced Technology Solar telescope M1 Thermal control System Design, Modeling and Prototype Testing

Advanced Technology Solar Telescope M1 Thermal Control Syste...

引用

conference on Ground-Based and Airborne instrumentation for Astronomy II

作者： Hansen, Eric Bulau, Scott Phelps, LeEllen AURA National Solar Observatory (United States)

ISBN: (纸本)9780819472229

The advanced Technology Solar telescope (ATST) project plans to implement thermal control of the primary mirror using jet impingement of temperature controlled air on the backside of the meniscus mirror. This technique will be used to minimize temperature rise of the optical surface due to coating absorption, minimizing mirror seeing effects. The performance of this system has been evaluated using numerical modeling techniques and weather data recorded at the proposed observatory site. To aid in the design of the M I thermal control system for the ATST, a prototype test bed was designed, fabricated and tested. This paper reviews the progress and results of this development program

关键词： solar telescope thermal control mirror seeing

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LBTI software Architecture

LBTI Software Architecture

引用

2nd conference on advanced software and control for Astronomy

作者： Vaitheeswaran, Vidhya Hinz, Phil Kraus, Joseph Breuninger, Andrew Univ Arizona Steward Observ 933 N Cherry Ave Tucson AZ 85721 USA South African Large Telescope Karoo South Africa

ISBN: (纸本)9780819472298

LBTI is a thermal imager and a nulling interferometer to be installed on the Large Binocular telescope (LBT). Here, we present the distributed component architecture model and its simple yet powerful software structure designed to complement the LBTI hardware model that comprises pyramid wave front sensors with its control electronic universal beam combiner, phase sensor, science imager, and all housekeeping duties to run the cryogenics, compressors, vibration monitors and the interface to the telescope control systems.

关键词： Interferometer software

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advanced Technology Solar telescope lower enclosure thermal system

Advanced Technology Solar Telescope lower enclosure thermal ...

引用

conference on Modeling, Systems Engineering and Project Management for Astronomy III

作者： Phelps, L. Warner, M. Natl Solar Observ Tucson AZ 85719 USA

ISBN: (纸本)9780819472274

The exterior of the advanced Technology Solar telescope enclosure requires cooling to eliminate so-called external dome seeing caused by solar loading during the observing day. This is achieved by way of coolant circulation through external plate coil panels, thereby maintaining the exterior surfaces of the enclosure at or just below ambient air temperature. As the distance from the optical path increases (e.g., on the surface of the lower enclosure), the stringency of the temperature requirement is diminished, thereby allowing a greater difference between the surface temperature and the ambient air temperature. This paper presents a comparison of the modeled performance of an active thermal control strategy on the lower enclosure to a passive strategy that employs concrete panels. A life-cycle cost analysis of each option is also presented.

关键词： ATST telescope enclosure thermal performance modeling CFD thermal control dome seeing

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Mechanical alignment of tertiary mirror and positioner on the LMT telescope - art. no. 70183M

Mechanical alignment of tertiary mirror and positioner on th...

引用

International conference on advanced Optical and Mechanical Technologies in telescopes and instrumentation

作者： Gale, David M. Inst Nacl Astrofis Opt & Electr Puebla 72840 Mexico

ISBN: (纸本)9780819472281

The Large Millimeter telescope (LMT) at Cerro La Negra in Central Mexico is Currently being fitted Out with optical, mechanical and control systems. The tertiary mirror is a 1.1 x 1.7m ellipse, mounted oil a positioner which provides tracking in elevation and 180 degrees image direction switching between detectors. Installation and alignment of mirror and positioner must be achieved with high accuracy in a construction-site environment, at an altitude of 4600m. Alignment equipment should be intuitive to use, easy to install, and have minimum interference with other site tasks. Alignment will be achieved with small diameter, well-collimated laser beams, pre-aligned to the telescope elevation and primary reflector (optic) axes. Although a total station and laser tracker are available, the laser beam method has theoretically higher accuracy, gives faster, more intuitive results and requires no time-sharing with the former instruments. This paper describes the alignment concept, equipment to be used, pre-installation testing, and alignment procedures to be carried out at the telescope.

关键词： LMT laser alignment Bessel beams Gaussian collimation LDM crosshair target

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