Corpus ID: 227119135

A Deep Search for Emission From "Rock Comet" (3200) Phaethon At 1 AU

@article{Ye2020ADS,
  title={A Deep Search for Emission From "Rock Comet" (3200) Phaethon At 1 AU},
  author={Q. Ye and M. Knight and M. Kelley and N. Moskovitz and Annika Gustafsson and D. Schleicher},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2020}
}
We present a deep imaging and spectroscopic search for emission from (3200) Phaethon, a large near-Earth asteroid that appears to be the parent of the strong Geminid meteoroid stream, using the 4.3 m Lowell Discovery Telescope. Observations were conducted on 2017 December 14-18 when Phaethon passed only 0.07 au from the Earth. We determine the $3\sigma$ upper level of dust and CN production rates to be 0.007-0.2 $\mathrm{kg~s^{-1}}$ and $2.3\times10^{22}~\mathrm{molecule~s^{-1}}$ through… Expand

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References

SHOWING 1-10 OF 13 REFERENCES
The Pan-STARRS1 Surveys
  • 768
  • PDF
First-generation instrumentation for the Discovery Channel Telescope
  • 17
  • Highly Influential
Using Cometary Activity to Trace the Physical and Chemical Evolution of Cometary Nuclei
  • 93
  • PDF
Pan-STARRS Photometric and Astrometric Calibration
  • 101
  • Highly Influential
  • PDF
Physical and Chemical Properties of Meteoroids, ed
  • 2019
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
  • 909
  • Highly Influential
Contributions of the Astronomical Observatory
  • Skalnate Pleso,
  • 2019
Photutils: Photometry tools
  • 12
The Active Asteroids, 221–241, doi: 10.2458/azu uapress 9780816532131-ch012
  • 2015
...
1
2
...