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Lehner, M. J.; Wang, S-Y.; Reyes-Ruiz, M.; Zhang, Z-W.; Figueroa, L.; Huang, C-K.; Yen, W-L.; Alcock, C.; Alvarez Santana, F.; Castro-Chacón, J.; Chen, W-P.; Chu, Y-H.; Cook, K. H.; Geary, J. C.; Hernández, B.; Karr, J.; Kavelaars, J. J.; Norton, T.; Szentgyorgyi, A.
Proceedings of the International Astronomical Union, 11/2017, Letnik: 14, Številka: S339Journal Article
TAOS II is a next-generation occultation survey with the goal of measuring the size distribution of the small end of the Kuiper Belt (objects with diameters 0.5–30 km). Such objects have magnitudes r > 30, and are thus undetectable by direct imaging. The project will operate three telescopes at San Pedro Mártir Observatory in Baja California, México. Each telescope will be equipped with a custom-built camera comprised of a focal-plane array of CMOS imagers. The cameras will be capable of reading out image data from 10,000 stars at a cadence of 20 Hz. The telescopes will monitor the same set of stars simultaneously to search for coincident occultation detections, thus minimising the false-positive rate. This talk described the project, and reported on the progress of the development of the survey infrastructure.
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Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
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Vir: Osebne bibliografije
in: SICRIS
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