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Polarimetry of Main-Belt Asteroids
We present the results of a polarimetric survey of main-belt asteroids at Complejo Astronomico El Leoncito (CASLEO), San Juan, Argentina. The aims of this survey are to increase... -
Gaia-FUN-SSO network. Apophis campaign
Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gaia-FUN-SSO) play a key role in ensuring that moving objects first detected by ESA's... -
Photometry of 16 Flora family asteroids
It is known that the Yarkovsky effect moves small asteroids to larger/smaller semimajor axes depending on their prograde/retrograde spins. The YORP effect influences asteroid... -
Lightcurves of Near-Earth Asteroid 162173 (1999 JU3)
Near-Earth asteroid (hereafter NEA) 162173 (1999 JU3) is a potential target of two asteroid sample return missions not only because of its accessibility but also because of the... -
Asteroid brightness and geometry
We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We... -
Colors of Minor Bodies in the Outer Solar System
We present a compilation of all available colors for 104 Minor Bodies in the Outer Solar System (MBOSSes); for each object, the original references are listed. The measurements... -
Orbital Elements of Minor Planets 1998
The catalogue contains osculating elements of all permanently numbered minor planets as of November 25, 1996. The elements are given with respect to the ecliptic plane and... -
Orbital Elements of Minor Planets 1997
The catalogue contains osculating elements of all permanently numbered minor planets as of November 7, 1995. The elements are given with respect to the ecliptic plane and... -
EPN-TAP table for MPC Asteroid Orbital Data
The EPN-TAP 2.0 version of the complete asteroid data from the Minor Planet Center (MPC), updated once per month. The MPC operates at the Smithsonian Astrophysical Observatory... -
Asteroids II Machine-Readable Data Base
This data set was assembled by E. F. Tedesco, Jet Propulsion Laboratory, in March 1988 from files provided by the contributors to the above reference. Included are asteroid... -
IRAS Asteroid and Comet Survey
The main purpose of the Infrared Astronomical Satellite (IRAS) was to survey the sky in four infrared wavelength bands centered at 12, 25, 60 and 100 um. Data for 25 comets,... -
Asteroid phase curve coefficients from ATLAS observations
Asteroid phase curves are used to derive fundamental physical properties through the determination of the absolute magnitude H. The upcoming visible Legacy Survey of Space and... -
Occultations of stars by large TNO 2004-2014
Occultations of stars brighter than 15m by largest trans-Neptunian objects (TNOs) are predicted. Search was performed using the following catalogues: Hipparcos (Cat. ; Tycho2... -
AKARI Near Infrared Asteroid Spectral Catalog V1
Knowledge of water in the solar system is important for the understanding of a wide range of evolutionary processes and the thermal history of the solar system. To explore the... -
AKARI IRC slow-scan asteroid catalog, AcuA-ISS
We present an asteroidal catalog from the mid-infrared wavelength region using the slow-scan observation mode obtained by the Infrared Camera (IRC) on-board the Japanese... -
Asteroid catalog using AKARI (AcuA). V1.
The AKARI Infrared Astronomical Satellite observed the whole sky in the far infrared (50-180{mu}m) and the mid-infrared (9 and 18{mu}m) between May 2006 and August 2007... -
CCD photometry of 23 minor planets
We present CCD photometric observations of 23 main-belt asteroids, of which 8 have never been observed before thus the data of these objects are the first in the literature. The... -
CCD photometry of 23 minor planets
We present CCD photometric observations of 23 main-belt asteroids, of which 8 have never been observed before thus the data of these objects are the first in the literature. The... -
2007-2016 Pulkovo Uranian satellites obs.
We present the results of the observations of the Uranian satellites made with the 26-inch refractor at the Pulkovo Observatory in 2007-2016. During this time we got 17 normal... -
1847 WISE-observed asteroids thermal properties
We present new thermophysical model (TPM) fits of 1847 asteroids, deriving thermal inertia, diameter, and Bond and visible geometric albedo. We use thermal flux measurements...
