First Results from the rapid-response spectrophotometric characterization of Near-Earth Objects
arXiv:1903.08320 · doi:10.3847/1538-3881/ab1138
Abstract
As part of our multi-observatory, multi-filter campaign, we present \rmi color observations of 82 Near-Earth Objects (NEOs) obtained with the RATIR instrument on the 1.5m robotic telescope at the San Pedro Martir's National Observatory in Mexico. Our project is particularly focused on rapid response observations of small ( m) NEOs. The rapid response and the use of spectrophotometry allows us to constrain the taxonomic classification of NEOs with high efficiency. Here we present the methodology of our observations and our result, suggesting that the ratio of C-type to S-type asteroids in a size range of 30-850m is 1.1, which is in accordance with our previous results. We also find that 10 of all NEOs in our sample are neither C- nor S-type asteroids
arXiv comment31 pages, 4 tables, 10 figures
References in corpus (14)
- Solar System Objects Observed in the SDSS Commissioning Data
- Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS
- Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry
- A spectroscopic survey of the small near-Earth asteroid population: peculiar taxonomic distribution and phase reddening
- Physical Characterization of Warm Spitzer-observed Near-Earth Objects
- Multi-filter transit observations of WASP-39b and WASP-43b with three San Pedro Mártir telescopes
- A detailed study of the optical attenuation of gamma-ray bursts in the Swift era
- Characterization of Near-Earth Asteroids using KMTNet-SAAO
- First Results from the Rapid-Response Spectrophotometric Characterization of Near-Earth Objects using UKIRT
- The Need for Speed in Near-Earth Asteroid Characterization
- Photometric Observations of Supernova 2013cq Associated with GRB 130427A
- Photometric survey of 67 near-Earth objects
- Olivine-rich asteroids in the near-Earth space
- A spectroscopic and photometric study of the planetary nebulae Kn 61 and Pa 5