VIRUS: a massively-replicated IFU spectrograph for HET

被引:15
作者
Hill, GJ [1 ]
MacQueen, PJ [1 ]
Tejada, C [1 ]
Cobos, FJ [1 ]
Palunas, P [1 ]
Gebhardt, K [1 ]
Drory, N [1 ]
机构
[1] Univ Texas, McDonald Observ, Austin, TX 78712 USA
来源
GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3 | 2004年 / 5492卷
关键词
astronomical instrumentation : spectrographs; integral field; VIRUS; IFU;
D O I
10.1117/12.552474
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We investigate the role of industrial replication in the construction of the next generation of spectrographs for large telescopes. In this paradigm, a simple base spectrograph unit is replicated to provide multiplex advantage, while the engineering costs are amortized over many copies. We argue that this is a cost-effective approach when compared to traditional spectrograph design, where each instrument is essentially a one-off prototype with heavy expenditure on engineering effort. As an example of massive replication, we present the design of, and the science drivers for, the Visible IFU Replicable Ultra-cheap Spectrograph (VIRUS). This instrument is made up of 132 individually small and simple spectrographs, each fed by a fiber integral field unit. The total VIRUS-132 instrument covers similar to29 sq. arcminutes per observation, providing integral field spectroscopy from 340 to 570 nm, simultaneously, of 32,604 spatial elements, each 1 sq. arcsecond on the sky. VIRUS-132 will be mounted on the 9.2 m Hobby-Eberly Telescope and fed by a new wide-field corrector with a science field in excess of 16.5 arcminutes diameter. VIRUS represents a new approach to spectrograph design, offering the science multiplex advantage of huge sky coverage for an integral field spectrograph, coupled with the engineering multiplex advantage of >10(2) spectrographs making up a whole.
引用
收藏
页码:251 / 261
页数:11
相关论文
共 27 条
[1]  
ALDERING, 2004, UNPUB PASP
[2]   Integral field spectroscopy with the gemini multiobject spectrograph. I. Design, construction, and testing [J].
Allington-Smith, J ;
Murray, G ;
Content, R ;
Dodsworth, G ;
Davies, R ;
Miller, BW ;
Jorgensen, I ;
Hook, I ;
Crampton, D ;
Murowinski, R .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2002, 114 (798) :892-912
[3]  
BACON R, 2004, P SPIE, V5492
[4]  
BARDEN S, 2004, P SPIE, V5492
[5]   Volume-phase holographic gratings and their potential for astronomical applications [J].
Barden, SC ;
Arns, JA ;
Colburn, WS .
OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2, 1998, 3355 :866-876
[6]  
BARDEN SC, 1988, P C TUCS AZ APR 11 1, P113
[7]   SparsePak: A formatted fiber field unit for the WIYN Telescope Bench Spectrograph. I. Design, construction, and calibration [J].
Bershady, MA ;
Andersen, DR ;
Harker, J ;
Ramsey, LW ;
Verheijen, MAW .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2004, 116 (820) :565-590
[8]   Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler [J].
Blake, C ;
Glazebrook, K .
ASTROPHYSICAL JOURNAL, 2003, 594 (02) :665-673
[9]  
CLAVER CF, 2004, P SPIE, V5489
[10]   The DEIMOS spectrograph for the Keck II telescope: integration and testing [J].
Faber, SM ;
Phillips, AC ;
Kibrick, RI ;
Alcott, B ;
Allen, SL ;
Burrous, J ;
Cantrall, T ;
Clarke, DA ;
Coil, AL ;
Cowley, DJ ;
Davis, M ;
Deich, WTS ;
Dietsch, K ;
Gilmore, DK ;
Harper, CA ;
Hilyard, DF ;
Lewis, JP ;
McVeigh, MM ;
Newman, J ;
Osborne, J ;
Schiavon, RP ;
Stover, RJ ;
Tucker, D ;
Wallace, V ;
Wei, MZ ;
Wirth, GD ;
Wright, CA .
INSTRUMENT DESIGN AND PERFORMANCE FOR OPTICAL/INFRARED GROUND-BASED TELESCOPES, PTS 1-3, 2003, 4841 :1657-1669