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
[11]   VIRUS: an ultracheap 1000-object IFU spectrograph [J].
Hill, GJ ;
MacQueen, PJ .
SURVEY AND OTHER TELESCOPE TECHNOLOGIES AND DISCOVERIES, 2002, 4836 :306-312
[12]   Volume phase holographic (VPH) grisms for optical and infrared spectrographs [J].
Hill, GJ ;
Wolf, MJ ;
Tufts, JR ;
Smith, EC .
SPECIALIZED OPTICAL DEVELOPMENTS IN ASTRONOMY, 2003, 4842 :1-9
[13]  
HILL GJ, 2004, P SPIE, V5492
[14]  
KELZ A, 2004, P SPIE, V5492
[15]   The VIMOS and NIRMOS multi-object spectrographs for the ESO-VLT [J].
Le Fèvre, O ;
Saisse, M ;
Mancini, D ;
Vettolani, G ;
Maccagni, D ;
Picat, JP ;
Mellier, Y ;
Mazure, A ;
Cuby, JG ;
Delabre, B ;
Garilli, B ;
Hill, L ;
Prieto, E ;
Voet, C ;
Arnold, L ;
Bau-Nogué, S ;
Cascone, E ;
Conconi, P ;
Finger, G ;
Huster, G ;
Laloge, A ;
Lucuix, C ;
Mattaini, E ;
Schipani, P ;
Waultier, G ;
Zerbi, F ;
Avila, G ;
Beletic, J ;
d'Odorico, S ;
Moorwood, A ;
Monnet, G ;
Reyes, J .
OPTICAL AND IR TELESCOPE INSTRUMENTATION AND DETECTORS, PTS 1 AND 2, 2000, 4008 :546-557
[16]   The Anglo-Australian Observatory 2dF facility [J].
Lewis, IJ ;
Cannon, RD ;
Taylor, K ;
Glazebrook, K ;
Bailey, JA ;
Baldry, IK ;
Barton, JR ;
Bridges, TJ ;
Dalton, GB ;
Farrell, TJ ;
Gray, PM ;
Lankshear, A ;
McCowage, C ;
Parry, IR ;
Sharples, RM ;
Shortridge, K ;
Smith, GA ;
Stevenson, J ;
Straede, JO ;
Waller, LG ;
Whittard, JD ;
Wilcox, JK ;
Willis, KC .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 333 (02) :279-298
[17]   Weak lensing from space. II. Dark matter mapping [J].
Massey, R ;
Rhodes, J ;
Refregier, A ;
Albert, J ;
Bacon, D ;
Bernstein, G ;
Ellis, R ;
Jain, B ;
McKay, T ;
Perlmutter, S ;
Taylor, A .
ASTRONOMICAL JOURNAL, 2004, 127 (06) :3089-3101
[18]   Measurements of Ω and Λ from 42 high-redshift supernovae [J].
Perlmutter, S ;
Aldering, G ;
Goldhaber, G ;
Knop, RA ;
Nugent, P ;
Castro, PG ;
Deustua, S ;
Fabbro, S ;
Goobar, A ;
Groom, DE ;
Hook, IM ;
Kim, AG ;
Kim, MY ;
Lee, JC ;
Nunes, NJ ;
Pain, R ;
Pennypacker, CR ;
Quimby, R ;
Lidman, C ;
Ellis, RS ;
Irwin, M ;
McMahon, RG ;
Ruiz-Lapuente, P ;
Walton, N ;
Schaefer, B ;
Boyle, BJ ;
Filippenko, AV ;
Matheson, T ;
Fruchter, AS ;
Panagia, N ;
Newberg, HJM ;
Couch, WJ .
ASTROPHYSICAL JOURNAL, 1999, 517 (02) :565-586
[19]   Very wide integral field unit of VIRMOS for the VLT:: Design and performances [J].
Prieto, E ;
Le Fèvre, O ;
Saisse, M ;
Voet, C ;
Bonneville, C .
OPTICAL AND IR TELESCOPE INSTRUMENTATION AND DETECTORS, PTS 1 AND 2, 2000, 4008 :510-521
[20]   Observational evidence from supernovae for an accelerating universe and a cosmological constant [J].
Riess, AG ;
Filippenko, AV ;
Challis, P ;
Clocchiatti, A ;
Diercks, A ;
Garnavich, PM ;
Gilliland, RL ;
Hogan, CJ ;
Jha, S ;
Kirshner, RP ;
Leibundgut, B ;
Phillips, MM ;
Reiss, D ;
Schmidt, BP ;
Schommer, RA ;
Smith, RC ;
Spyromilio, J ;
Stubbs, C ;
Suntzeff, NB ;
Tonry, J .
ASTRONOMICAL JOURNAL, 1998, 116 (03) :1009-1038