Properties of the Trans-Neptunian Belt: Statistics from the Canada-France-Hawaii Telescope Survey

@article{Trujillo2001PropertiesOT,
  title={Properties of the Trans-Neptunian Belt: Statistics from the Canada-France-Hawaii Telescope Survey},
  author={Chadwick A. Trujillo and David C. Jewitt and Jane X. Luu},
  journal={The Astronomical Journal},
  year={2001},
  volume={122},
  pages={457 - 473}
}
We present the results of a wide-field survey designed to measure the size, inclination, and radial distributions of Kuiper Belt objects (KBOs). The survey found 86 KBOs in 73 deg2 observed to limiting red magnitude of 23.7 using the Canada-France-Hawaii Telescope and the 12K × 8K CCD mosaic camera. For the first time, both ecliptic and off-ecliptic fields were examined to more accurately constrain the inclination distribution of the KBOs. The survey data were processed using an automatic… 

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References

SHOWING 1-10 OF 45 REFERENCES

Pencil-Beam Surveys for Faint Trans-Neptunian Objects

Motivated by a desire to understand the size distribution of objects in the Edgeworth-Kuiper belt, an observing program has been conducted at the Palomar 5 m and Canada-France-Hawaii 3.6 m

Population of the Scattered Kuiper Belt

The discovery of three new scattered Kuiper Belt objects (SKBOs) from a wide-field survey of the ecliptic are presented, demonstrating that the SKBOs are similar in number and mass to the KuiPer Belt inside 50 AU.

Large Kuiper Belt Objects: The Mauna Kea 8K CCD Survey

We describe a large-area ecliptic survey designed to assess the sky-plane surface density of bright Kuiper Belt objects. We used an 8192 × 8192 pixel CCD mosaic to image 51.5 deg2 to a 50% detection

The Solar System Beyond Neptune

The aim of this research is to study the objects in the Kuiper Belt, in order to understand the nature of its origin and the evolutionary processes which have affected the Kuiper Belt. Particular

Keck Pencil-Beam Survey for Faint Kuiper Belt Objects

We present the results of a pencil-beam survey of the Kuiper Belt using the Keck 10 m telescope. A single 0.01 deg2 field is imaged 29 times for a total integration time of 4.8 hr. Combining

The Inclination Distribution of the Kuiper Belt

We develop a general method for determining the unbiased inclination distribution of the Kuiper belt using only the inclination and latitude of discovery of known Kuiper belt objects (KBOs). These

A Wide-Field CCD Survey for Centaurs and Kuiper Belt Objects

A modified Baker-Nunn camera was used to conduct a wide-field survey of 1428 deg2 of sky near the ecliptic in search of bright Kuiper Belt objects and Centaurs. This area is an order of magnitude

The Discovery of Halley-sized Kuiper Belt Objects Using the Hubble Space Telescope

We report the statistical detection (at the >99% confidence level) of a population of 28th magnitude objects exhibiting proper motions of ~1 arcsecond per hour at quadrature in deep HST/WFPC2 images.

A Semiautomated Sky Survey for Slow-moving Objects Suitable for a Pluto Express Mission Encounter

We have developed a robust computer program that quickly and efficiently searches for moving objects in large-format CCD images. We describe the initial application of this program to a survey for

The Edge of the Solar System

We have surveyed for Kuiper Belt objects (KBOs) in six fields of the ecliptic (total sky area 1.5 deg2) to limiting magnitudes between R = 24.9 and R = 25.9. This is deep enough to detect KBOs of