Optical Design of a Versatile FIRST High-resolution near-IR Spectrograph

被引:0
作者
Zhao, Bo [1 ]
Ge, Jian [1 ]
机构
[1] Univ Florida, Dept Astron, Bryant Space Sci Ctr 211, Gainesville, FL 32611 USA
来源
GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY IV | 2012年 / 8446卷
关键词
Silicon immersion grating; Echelle; high resolution; white pupil; cross-dispersion; VPH gratings; Doppler & fibers;
D O I
10.1117/12.926135
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We report the update optical design of a versatile FIRST high resolution near IR spectrograph, which is called Florida IR Silicon immersion grating spectromeTer (FIRST). This spectrograph uses cross-dispersed echelle design with white pupils and also takes advantage of the image slicing to increase the spectra resolution, while maintaining the instrument throughput. It is an extremely high dispersion R1.4 (blazed angle of 54.74 degrees) silicon immersion grating with a 49 mm diameter pupil is used as the main disperser at 1.4 mu m-1.8 mu m to produce R=72,000 while an R4 echelle with the same pupil diameter produces R=60,000 at 0.8 mu m-1.35 mu m. Two cryogenic Volume Phase Holographic (VPH) gratings are used as cross-dispersers to allow simultaneous wavelength coverage of 0.8 mu m-1.8 mu m. The butterfly mirrors and dichroic beamsplitters make a compact folding system to record these two wavelength bands with a 2kx2k H2RG array in a single exposure. By inserting a mirror before the grating disperser (the SIG and the echelle), this spectrograph becomes a very efficient integral field 3-D imaging spectrograph with R=2,000-4,000 at 0.8 mu m-1.8 mu m by coupling a 10x10 telescope fiber bundle with the spectrograph. Details about the optical design and performance are reported.
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页数:6
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共 11 条
  • [1] ELODIE: A spectrograph for accurate radial velocity measurements
    Baranne, A
    Queloz, D
    Mayor, M
    Adrianzyk, G
    Knispel, G
    Kohler, D
    Lacroix, D
    Meunier, JP
    Rimbaud, G
    Vin, A
    [J]. ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1996, 119 (02): : 373 - 390
  • [2] Attaining Doppler precision of 3 m s(-1)
    Butler, RP
    Marcy, GW
    Williams, E
    McCarthy, C
    Dosanjh, P
    Vogt, SS
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1996, 108 (724) : 500 - 509
  • [3] Non-cooled near infrared spectroscopy
    Dallier, R
    Cuby, JG
    [J]. INFRARED ASTRONOMICAL INSTRUMENTATION, PTS 1-2, 1998, 3354 : 833 - 844
  • [4] Ge, 2006, SPIE, V6273
  • [5] Ge, 2012, SPIE
  • [6] Jones, 2009, ASTROPHYSICS SPACE S, P415
  • [7] Pepe F., 2002, The Messenger, V110, P9
  • [8] High-resolution fiber-coupled spectrograph of the Hobby-Eberly Telescope
    Tull, RG
    [J]. OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2, 1998, 3355 : 387 - 398
  • [9] VOGT S, 1994, P SOC PHOTO-OPT INS, V2198, P362, DOI 10.1117/12.176725
  • [10] Yamamuro, 2006, OPTICAL ENG, V45, P41