2021
DOI: 10.1088/1538-3873/abd4bc
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The TAOS II Survey: Real-time Detection and Characterization of Occultation Events

Abstract: The Transneptunian Automated Occultation Survey (TAOS II) is a blind occultation survey with the aim of measuring the size distribution of Trans-Neptunian Objects with diameters in the range of 0.3 ≲ D ≲ 30 km. TAOS II will observe as many as 10,000 stars at a cadence of 20 Hz with all three telescopes simultaneously. This will produce up to ∼20 billion photometric measurements per night, and as many as ∼6 trillion measurements per year, corresponding to over 70 million individual light curves. A very fast ana… Show more

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Cited by 10 publications
(8 citation statements)
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“…One of the best next steps is to send orbiters to the Uranus (Cartwright et al 2021;Leonard et al 2021) and Neptune systems 6 to complete crater measurements to much smaller diameters and deepen understanding of the satellites' geologies. It is also important to perform occultation surveys of KBOs, including bodies with diameters <1 km (Huang et al 2021), as escaped KBOs are the expected main source of the heliocentric population of satellite impactors. However, even this may not completely resolve what has impacted outer solar system satellites, as this will only provide a snapshot of the current (0 to ∼3 Ga) heliocentric impactor population and not show what this or the other possible populations may have looked like in the very early solar system (see Morbidelli & Nesvorný 2020, for a review of dynamical and collisional evolution of the Kuiper Belt).…”
Section: Implications For Outer Solar System Impactormentioning
confidence: 99%
“…One of the best next steps is to send orbiters to the Uranus (Cartwright et al 2021;Leonard et al 2021) and Neptune systems 6 to complete crater measurements to much smaller diameters and deepen understanding of the satellites' geologies. It is also important to perform occultation surveys of KBOs, including bodies with diameters <1 km (Huang et al 2021), as escaped KBOs are the expected main source of the heliocentric population of satellite impactors. However, even this may not completely resolve what has impacted outer solar system satellites, as this will only provide a snapshot of the current (0 to ∼3 Ga) heliocentric impactor population and not show what this or the other possible populations may have looked like in the very early solar system (see Morbidelli & Nesvorný 2020, for a review of dynamical and collisional evolution of the Kuiper Belt).…”
Section: Implications For Outer Solar System Impactormentioning
confidence: 99%
“…Nevertheless, the last decade has seen increased availability of QE-boosting technologies such as backside illumination (BSI) in CIS, improvements in the performance and arrangement of column-parallel ADCs allowing larger area and threesided buttable sensors. Specific applications are already making use of the advantages of CIS, such as the ability to address subsets of individual pixels as in the TAOS-II project (Huang et al 2021), which uses the Teledyne CIS113 (Wang et al 2020) with deported ADCs. Another useful characteristic of CIS is the achievement of high frame rates coupled with low readout noise ( 1 e − ) thanks to highly parallel readout.…”
Section: Introductionmentioning
confidence: 99%
“…Nevertheless, the last decade has seen increased availability of QE-boosting technologies such as backside illumination (BSI) in CIS, improvements in the performance and arrangement of column-parallel ADCs allowing larger area and 3-side buttable sensors. Specific applications are already making use of the advantages of CIS such as the ability to address subsets of individual pixels as in the TAOS-II project (Huang et al 2021), which uses the Teledyne CIS113 (Wang et al 2020) with deported ADCs. Another useful characteristic of CIS is the achievement of high frame rates coupled with low readout noise ( 1 e − ), thanks to highly parallel readout.…”
Section: Introductionmentioning
confidence: 99%