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FAI Asteroid Observation Log
This table is a preview catalog of asteroid observations carried out by the Fesenkov Astrophysical Institute (FAI) as part of our ongoing contribution to planetary defense and... -
Asteroids rotation periods from Kepler K2
Understanding the rotational periods of asteroids is crucial for gaining insights into their internal structures, compositions, and collisional histories. NASA's Kepler Space... -
(4) Vesta adopted polarimetric light curves
The results of the in situ exploration of the asteroid (4) Vesta by the Dawn spacecraft open new perspectives in the field of interpretation of remote-sensing polarimetric... -
596 Scheila NIR spectra before & after impact
Dust emission was detected on main-belt asteroid 596 Scheila in 2010 December and was attributed to the collision of a few-tens-of-meters projectile on the surface of the... -
LC of the TNO Varuna
From CCD observations carried out with different telescopes, we present short-term photometric measurements of the large trans-Neptunian object Varuna in 10 epochs, spanning... -
Subaru obs. of Vesta in MIR spectral range
Plagioclase feldspars are among the most prevalent minerals in the solar system, and are present in many chondritic and achondritic meteorite families. Nevertheless, spectral... -
Polarimetric survey of Phaethon with PICO
As a function of the solar phase angle, {alpha}, the linear polarization degree (referred to the scattering plane, P_r_) of solar system objects is a good diagnostic for... -
Line list for stellar chemical abundances
The achievable level of precision on photospheric abundances of stars is a major limiting factor on investigations of exoplanet host star characteristics, the chemical histories... -
WISE/NEOWISE Main Belt asteroids: family members
Using albedos from WISE/NEOWISE to separate distinct albedo groups within the Main Belt asteroids, we apply the Hierarchical Clustering Method to these subpopulations and... -
WISE/NEOWISE NEOs preliminary thermal fits
Enhancements to the science data processing pipeline of NASA's Wide-field Infrared Survey Explorer (WISE) mission, collectively known as NEOWISE, resulted in the detection of... -
WISE/NEOWISE observations of main belt asteroids
We present preliminary diameters and albedos for 13511 Main Belt asteroids (MBAs) that were observed during the 3-Band Cryo phase of the Wide-field Infrared Survey Explorer... -
Jovian Trojan asteroids with WISE/NEOWISE: taxonomy
We present updated/new thermal model fits for 478 Jovian Trojan asteroids observed with the Wide-field Infrared Survey Explorer (WISE). Using the fact that the two shortest... -
WISE/NEOWISE observations of Hilda asteroids
We present the preliminary analysis of 1023 known asteroids in the Hilda region of the solar system observed by the NEOWISE component of the Wide-field Infrared Survey Explorer... -
Asteroid cross-referencing : MPC and WSA (UKIRT)
The UKIRT Hemisphere Survey covers the northern sky in the infrared from 0{deg} to 60{deg} decl. Current data releases include both J and K bands, with H-band data forthcoming.... -
Main problem of lunar orbit revisited
A novel algorithm based on the Lindstedt-Poincare method is proposed to construct an analytical solution of the lunar orbit. Based on the analytical solution, a numerical... -
KPIC radial velocity follow up of HR 7672 B
The detection of satellites around extrasolar planets, so called exomoons, remains a largely unexplored territory. In this work, we study the potential of detecting these... -
NIR spectra of 420 near-Earth objects
We report 491 new near-infrared spectroscopic measurements of 420 near-Earth objects (NEOs) collected on the NASA InfraRed Telescope Facility as part of the MIT-Hawaii NEO... -
Yarkovsky drift measurements for NEAs
The Yarkovsky effect is a thermal process acting upon the orbits of small celestial bodies, which can cause these orbits to slowly expand or contract with time. The effect is... -
Near-Earth Object Survey (MANOS) spectroscopy
The Mission Accessible Near-Earth Object Survey (MANOS) aims to observe and characterize small (mean absolute magnitude H~25 mag) Near-Earth Objects (NEOs) that are accessible... -
Spectroscopy of main-belt Ch/Cgh-type asteroids
CM chondrites are the most common type of hydrated meteorites, making up ~1.5% of all falls. Whereas most CM chondrites experienced only low-temperature (~0{deg}C-120{deg}C)...
