Binospec: A Wide-field Imaging Spectrograph for the MMT
Binospec: A Wide-field Imaging Spectrograph for the MMT
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DOI:
10.1088/1538-3873/ab1d78
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发表时间:
2019-05
影响因子:
3.5
通讯作者:
D. Fabricant;R. Fata;H. Epps;T. Gauron;Mark Mueller;Joseph M. Zajac;S. Amato;J. Barberis;H. Bergner;P. Brennan;Warren L. Brown;I. Chilingarian;J. Geary;V. Kradinov;B. McLeod;Matthew J. Smith;D. Woods
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文献类型:
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作者:
D. Fabricant;R. Fata;H. Epps;T. Gauron;Mark Mueller;Joseph M. Zajac;S. Amato;J. Barberis;H. Bergner;P. Brennan;Warren L. Brown;I. Chilingarian;J. Geary;V. Kradinov;B. McLeod;Matthew J. Smith;D. Woods
Binospec is a high-throughput, 370 to 1000 nm, imaging spectrograph that addresses two adjacent 8′ by 15′ fields of view. Binospec was commissioned in late 2017 at the f/5 focus of the 6.5 m MMT and is now available to all MMT observers. Aperture masks cut from stainless steel with a laser cutter are used to define the entrance apertures that range from 15′ long slits to hundreds of 2″ slitlets. System throughputs, including the MMT’s mirrors and the f/5 wide-field corrector peak at ∼30%. Three reflection gratings, duplicated for the two beams, provide resolutions (λ/Δλ) between 1300 and >5000 with a 1″ wide slit. Two through-the-mask guiders are used for target acquisition, mask alignment, guiding, and precision offsets. A full-time Shack-Hartmann wavefront sensor allows continuous adjustment of primary mirror support forces, telescope collimation and focus. Active flexure control maintains spectrograph alignment and focus under varying gravity and thermal conditions.