OSIRIS software: An overview

José C. López-Ruiz; Marta Aguiar; Enrique Joven; Alberto Herrera; José V. Gigante; Antonio Cruz-López; Ignacio González-Serrano

doi:10.1117/12.461617

OSIRIS software: An overview

José C. López-Ruiz^*
, Marta Aguiar
, Enrique Joven
, Alberto Herrera
, José V. Gigante
, Antonio Cruz-López
, Ignacio González-Serrano

^*Corresponding author for this work

Research output: Contribution to journal › Conference article › peer-review

4 Citations (Scopus)

Abstract

OSIRIS (Optical System for Imaging and low/intermediate-Resolution Integrated Spectroscopy) is an instrument designed to obtain images and low resolution spectra of astronomical objects in the optical domain (from 365 through 1000nm). It will be installed on Day One (middle of 2004) in the Nasmyth focus of the 10-meter Spanish GTC Telescope. This paper shows an overview of the OSIRIS instrument software. Its architecture is distributed with real time features, having in mind to build a reusable, maintainable and inexpensive system. In this paper, we outline the main performances of the current design and some examples already implemented are given.

Original language	English
Pages (from-to)	545-552
Number of pages	8
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	4848
DOIs	https://doi.org/10.1117/12.461617
Publication status	Published - 2002
Externally published	Yes
Event	Advanced Telescope and Instrumentation Control Software II - Waikoloa, HI, United States Duration: 27 Aug 2002 → 28 Aug 2002

Keywords

Component model
Object oriented design
RTOS
Software architecture
Use cases

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10.1117/12.461617

Cite this

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title = "OSIRIS software: An overview",

abstract = "OSIRIS (Optical System for Imaging and low/intermediate-Resolution Integrated Spectroscopy) is an instrument designed to obtain images and low resolution spectra of astronomical objects in the optical domain (from 365 through 1000nm). It will be installed on Day One (middle of 2004) in the Nasmyth focus of the 10-meter Spanish GTC Telescope. This paper shows an overview of the OSIRIS instrument software. Its architecture is distributed with real time features, having in mind to build a reusable, maintainable and inexpensive system. In this paper, we outline the main performances of the current design and some examples already implemented are given.",

keywords = "Component model, Object oriented design, RTOS, Software architecture, Use cases",

author = "L{\'o}pez-Ruiz, \{Jos{\'e} C.\} and Marta Aguiar and Enrique Joven and Alberto Herrera and Gigante, \{Jos{\'e} V.\} and Antonio Cruz-L{\'o}pez and Ignacio Gonz{\'a}lez-Serrano",

year = "2002",

doi = "10.1117/12.461617",

language = "English",

volume = "4848",

pages = "545--552",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "SPIE",

note = "Advanced Telescope and Instrumentation Control Software II ; Conference date: 27-08-2002 Through 28-08-2002",

}

TY - JOUR

T1 - OSIRIS software

T2 - Advanced Telescope and Instrumentation Control Software II

AU - López-Ruiz, José C.

AU - Aguiar, Marta

AU - Joven, Enrique

AU - Herrera, Alberto

AU - Gigante, José V.

AU - Cruz-López, Antonio

AU - González-Serrano, Ignacio

PY - 2002

Y1 - 2002

N2 - OSIRIS (Optical System for Imaging and low/intermediate-Resolution Integrated Spectroscopy) is an instrument designed to obtain images and low resolution spectra of astronomical objects in the optical domain (from 365 through 1000nm). It will be installed on Day One (middle of 2004) in the Nasmyth focus of the 10-meter Spanish GTC Telescope. This paper shows an overview of the OSIRIS instrument software. Its architecture is distributed with real time features, having in mind to build a reusable, maintainable and inexpensive system. In this paper, we outline the main performances of the current design and some examples already implemented are given.

AB - OSIRIS (Optical System for Imaging and low/intermediate-Resolution Integrated Spectroscopy) is an instrument designed to obtain images and low resolution spectra of astronomical objects in the optical domain (from 365 through 1000nm). It will be installed on Day One (middle of 2004) in the Nasmyth focus of the 10-meter Spanish GTC Telescope. This paper shows an overview of the OSIRIS instrument software. Its architecture is distributed with real time features, having in mind to build a reusable, maintainable and inexpensive system. In this paper, we outline the main performances of the current design and some examples already implemented are given.

KW - Component model

KW - Object oriented design

KW - RTOS

KW - Software architecture

KW - Use cases

UR - https://www.scopus.com/pages/publications/0036988897

U2 - 10.1117/12.461617

DO - 10.1117/12.461617

M3 - Conference article

AN - SCOPUS:0036988897

SN - 0277-786X

VL - 4848

SP - 545

EP - 552

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

Y2 - 27 August 2002 through 28 August 2002

ER -

OSIRIS software: An overview

Abstract

Keywords

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