Importantly, this interpretation has not been tested observationally, as KBOs 4 K × 4 K) EMCCD and CMOS sensors and will thus increase the areal FOV substantially.
The break in the size distribution is generally attributed to collisions that break up small KBOs (radius r ≤ 10 km) and that therefore modifies their size distribution. Observations and theory suggest the existence of a break in the power-law size distribution at smaller KBO radii (Schlichting et al. Determining the abundance, material properties and collisional processes of sub-km-sized Kuiper Belt Objects (KBOs) is important, since these bodies provide the link between the largest KBOs and the dust-producing debris disk observed around other stars. The Kuiper Belt consists of a disc of icy bodies located beyond the orbit of Neptune. Instrumentation: detectors, instrumentation: photometers, methods: observational, techniques: photometric, occultations 1 INTRODUCTION In addition, it also has unique capability in the detection of faint near-Earth asteroids and will be used for the monitoring of short-duration transient and periodic sources, particularly those discovered by the intermediate Palomar Transient Factory (iPTF), and the upcoming Zwicky Transient Facility (ZTF). CHIMERA was primarily developed to enable the characterization of the size distribution of sub-km Kuiper Belt Objects via stellar occultation, a science case that motivates the frame-rate, the simultaneous multi-colour imaging and the wide field of view of the instrument.
CHIMERA SOFTWARE FULL
An electron multiplying CCD (EMCCD) detector is employed for both optical channels, each capable of simultaneously delivering sub-electron effective read noise under multiplication gain and frame rates of up to 26 fps full frame (several 1000 fps windowed), over a fully corrected 5 × 5 arcmin field of view. Additional narrow-band filters will also become available as required. Simultaneous optical imaging in two bands is enabled by a dichroic beam splitter centred at 567 nm, with Sloan u′ and g′ bands available on the blue arm and Sloan r′, i′ and z_s bands available on the red arm. It does not store any personal data.The Caltech HIgh-speed Multi-colour camERA (CHIMERA) is a new instrument that has been developed for use at the prime focus of the Hale 200-inch telescope. The cookie is set by the GDPR Cookie Consent plugin and is used to store whether or not user has consented to the use of cookies. The cookie is used to store the user consent for the cookies in the category "Performance". This cookie is set by GDPR Cookie Consent plugin. The cookie is used to store the user consent for the cookies in the category "Other. The cookies is used to store the user consent for the cookies in the category "Necessary".
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