تقرير
DOTIFS: a new multi-IFU optical spectrograph for the 3.6-m Devasthal optical telescope
| العنوان: | DOTIFS: a new multi-IFU optical spectrograph for the 3.6-m Devasthal optical telescope |
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| المؤلفون: | Chung, Haeun, Ramaprakash, A. N., Omar, Amitesh, Ravindranath, Swara, Chattopadhyay, Sabyasachi, Rajarshi, Chaitanya V., Khodade, Pravin |
| المصدر: | Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91470V (18 July 2014) |
| سنة النشر: | 2018 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Instrumentation and Methods for Astrophysics |
| الوصف: | Devasthal Optical Telescope Integral Field Spectrograph (DOTIFS) is a new multi-object Integral Field Spectrograph (IFS) being designed and fabricated by the Inter-University Center for Astronomy and Astrophysics (IUCAA), Pune, India, for the Cassegrain side port of the 3.6m Devasthal Optical Telescope, (DOT) being constructed by the Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital. It is mainly designed to study the physics and kinematics of the ionized gas, star formation and H II regions in the nearby galaxies. It is a novel instrument in terms of multi-IFU, built in deployment system, and high throughput. It consists of one magnifier, 16 integral field units (IFUs), and 8 spectrographs. Each IFU is comprised of a microlens array and optical fibers and has 7.4'' x 8.7'' field of view with 144 spaxel elements, each sampling 0.8'' hexagonal aperture. The IFUs can be distributed on the telescope side port over an 8' diameter focal plane by the deployment system. Optical fibers deliver light from the IFUs to the spectrographs. Eight identical, all refractive, dedicated spectrographs will produce 2,304 R~1800 spectra over 370-740nm wavelength range with a single exposure. Volume Phase Holographic gratings are chosen to make smaller optics and get high throughput. The total throughput of the instrument including the telescope is predicted as 27.5% on average. Observing techniques, data simulator and reduction software are also under development. Currently, conceptual and baseline design review has been done. Some of the components have already been procured. The instrument is expected to see its first light in 2016. Comment: 8 pages, 6 figures, Conference Presentation at SPIE Astronomical Telescopes + Instrumentation, 2014, Montr\'eal, Quebec, Canada |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.1117/12.2053051 |
| URL الوصول: | http://arxiv.org/abs/1810.03614 |
| رقم الأكسشن: | edsarx.1810.03614 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.1117/12.2053051 |
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