Chincarini 2010 Sooner一个极快速的光学望远镜
主要内容:
准备做这样一个望远镜,可以极其快速的指向所需要观测的方向。另外两个特点是多波段和高时间分辨率。
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Title: | The Sooner: a Large Robotic Telescope | |
Authors: | Chincarini, G.; Zannoni, M.; Covino, S.; Molinari, E.; Benetti, S.; Vitali, F.; Bonoli, C.; Bortoletto, F.; Cascone, E.; Cosentino, R.; D'Alessio, F.; D'Avanzo, P.; De Caprio, V.; Della Valle, M.; Fernandez-Soto, A.; Fugazza, D.; Giro, E.; Gomboc, A.; Guidorzi, C.; Magrin, D.; Malaspina, G.; Mankiewicz, L.; Margutti, R.; Mazzoleni, R.; Nicastro, L.; Riva, A.; Riva, M.; Salvaterra, R.; Spano, P.; Sperandio, M.; Stefanon, M.; Tosti, G.; Testa, V. | |
Publication: | eprint arXiv:1005.1569 | |
Publication Date: | 05/2010 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - Instrumentation and Methods for Astrophysics | |
Comment: | To be published in the proceedings of the conference "The Shocking Universe", San Servolo Venice, September 14-18, 2009. | |
Bibliographic Code: | 2010arXiv1005.1569C |
Abstract
The approach of Observational Astronomy is mainly aimed at the construction of larger aperture telescopes, more sensitive detectors and broader wavelength coverage. Certainly fruitful, this approach turns out to be not completely fulfilling the needs when phenomena related to the formation of black holes (BH), neutron stars (NS) and relativistic stars in general are concerned. Recently, mainly through the Vela, Beppo-SAX and Swift satellites, we reached a reasonable knowledge of the most violent events in the Universe and of some of the processes we believe are leading to the formation of black holes (BH). We plan to open a new window of opportunity to study the variegated physics of very fast astronomical transients, particularly the one related to extreme compact objects. The innovative approach is based on three cornerstones: 1) the design (the conceptual design has been already completed) of a 3m robotic telescope and related focal plane instrumentation characterized by the unique features: "No telescope points faster"; 2) simultaneous multi-wavelengths observations (photometry, spectroscopy o\& polarimetry); 3) high time resolution observations. The conceptual design of the telescope and related instrumentation is optimized to address the following topics: High frequency a-periodic variability, Polarization, High z GRBs, Short GRBs, GRB-Supernovae association, Multi-wavelengths simultaneous photometry and rapid low dispersion spectroscopy. This experiment will turn the "exception" (like the optical observations of GRB 080319B) to "routine".Bibtex entry for this abstract Preferred format for this abstract (see Preferences)
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