OSIRIS tunable imager and spectrograph-for the GTC. instrument status.

被引：83

作者：

Cepa, J ^{[1
]}

Aguiar, M ^{[1
]}

Bland-Hawthorn, J ^{[1
]}

Castañeda, H ^{[1
]}

Cobos, F ^{[1
]}

Correa, S ^{[1
]}

Espejo, C ^{[1
]}

Fragoso, AB ^{[1
]}

Fuentes, J ^{[1
]}

Gigante, JV ^{[1
]}

González, J ^{[1
]}

González-Escalera, V ^{[1
]}

González-Serrano, JI ^{[1
]}

Joven, E ^{[1
]}

López, JC ^{[1
]}

Militello, C ^{[1
]}

Peraza, L ^{[1
]}

Pérez, A ^{[1
]}

Pérez, J ^{[1
]}

Rasilla, JL ^{[1
]}

Sánchez, B ^{[1
]}

Tejada, C ^{[1
]}

机构：

[1] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Tenerife, Spain

来源：

INSTRUMENT DESIGN AND PERFORMANCE FOR OPTICAL/INFRARED GROUND-BASED TELESCOPES, PTS 1-3 | 2003年 / 4841卷

关键词：

tunable imaging; fast spectrophotometry; Fabry-Perot interferometers; multiple object spectroscopy; GTC;

D O I：

10.1117/12.460913

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the optical Day One instrument for the 10.4m Spanish telescope GTC to be installed in the Observatorio del Roque de Los Muchachos (La Palma, Spain). This instrument, operational in mid-2004, covers from 360 up to 1000 mn. OSIRIS observing modes include direct imaging with tunable and conventional filters, long slit and multiple object spectroscopy and fast spectrophotometry. The OSIRIS wide field of view, high efficiency and the new observing modes (tunable imaging and fast spectrophotometry) for 8-10m class telescopes will provide GTC with a powerful tool for their scientific exploitation. The present paper provides an updated overview of the instrument development, of some of the scientific projects that will be tackled with OSIRIS and of the general requirements driving the optical and mechanical design.

引用

页码：1739 / 1749

页数：11

共 8 条

[1] TTF: A flexible approach to narrowband imaging [J].

Bland-Hawthorn, J ;

Jones, DH .

OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2, 1998, 3355 :855-865

[2]

COBOS FJ, 2002, SPIE

[3]

FUENTES J, 2002, SPIE

[4] Microslit nod-shuffle spectroscopy: A technique for achieving very high densities of spectra [J].

Glazebrook, K ;

Bland-Hawthorn, J .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2001, 113 (780) :197-214

[5]

GONZALEZ J, 2002, SPIE

[6]

JOVEN E, 2002, IN PRESS OPTICAL DEC, V2

[7]

PERAZA L, 2002, SPIE

[8]

RASILLA JL, 2002, SPIE

← 1 →