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Title: Phase curves of small bodies from the SLOAN Moving Objects Catalog

Journal Article · · Astronomy and Astrophysics
ORCiD logo [1]; ORCiD logo [2];  [2]; ORCiD logo [3]
  1. Universidad de Alicante (Spain); Instituto de Astrofísica de Andalucía (Spain); Ministry of Science, Technology and Innovation (Brazil). National Observatory
  2. Universidad de Alicante (Spain)
  3. Universidad de Alicante (Spain); University of Barcelona (Spain)

Extensive photometric surveys continue to produce enormous stores of data on small bodies. These data are typically sparsely obtained at arbitrary (or unknown) rotational phases. Therefore, new methods for processing such data need to be developed to make the most of these vast catalogs. We aim to produce a method of recreating the phase curves of small bodies by considering the uncertainties introduced by the nominal errors in the magnitudes and the effect introduced by rotational variations. Here, we use the SLOAN Moving Objects Catalog data as a benchmark to construct phase curves of all small bodies in u', g', r', i', and z' filters. From the phase curves, we obtain the absolute magnitudes and we use them to set up the absolute colors, which are the colors of the asteroids that are not affected by changes in the phase angle. We selected objects with ≥3 observations taken in at least one filter and spanning over a minimum of 5 degrees in the phase angle. We developed a method that combines Monte Carlo simulations and Bayesian inference to estimate the absolute magnitudes using the HG12* photometric system. We obtained almost 15 000 phase curves, with about 12 000 of these including all five filters. The absolute magnitudes and absolute colors are compatible with previously published data that support our method. The method we developed is fully automatic and well suited for a run based on large amounts of data. Moreover, it includes the nominal uncertainties in the magnitudes and the whole distribution of possible rotational states of the objects producing what are possibly less precise values, that is, larger uncertainties, but more accurate, namely, closer to the actual value. To our knowledge, this work is the first to include the effect of rotational variations in such a manner.

Research Organization:
US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Office of Science (SC); Alfred P. Sloan Foundation; National Aeronautics and Space Administration (NASA); National Science Foundation (NSF)
OSTI ID:
1982280
Journal Information:
Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 657; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English

References (40)

Major achievements of the Rosetta mission in connection with the origin of the solar system journal October 2017
Solar System Science with LSST journal May 2009
Selecting candidate V-type asteroids from the analysis of the Sloan Digital Sky Survey colors journal August 2006
Surface composition of Hilda asteroids from the analysis of the Sloan Digital Sky Survey colors journal February 2008
Detecting active comets in the SDSS journal February 2010
Taxonomy of asteroids in the Cybele region from the analysis of the Sloan Digital Sky Survey colors journal April 2010
A three-parameter magnitude phase function for asteroids journal October 2010
Ensemble properties of comets in the Sloan Digital Sky Survey journal March 2012
Asteroid taxonomic signatures from photometric phase curves journal May 2012
The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys journal September 2013
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 – Preliminary results journal November 2015
Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry journal April 2016
Asteroid phase curves from ATLAS dual-band photometry journal January 2021
Online multi-parameter phase-curve fitting and application to a large corpus of asteroid photometric data journal July 2011
H, G1, G2 photometric phase function extended to low-accuracy data journal April 2016
New phase-magnitude curves for some main belt asteroids, fit of different photometric systems and calibration of the albedo - Photometry relation journal May 2019
Solar System evolution from compositional mapping of the asteroid belt journal January 2014
SDSS-based taxonomic classification and orbital distribution of main belt asteroids journal February 2010
SDSS photometry of asteroids in cometary orbits journal December 2012
Characterizing spectral continuity in SDSSugriz′ asteroid photometry journal May 2015
Absolute magnitudes and phase coefficients of trans-Neptunian objects journal February 2016
Near-infrared colors of minor planets recovered from VISTA-VHS survey (MOVIS) journal June 2016
J-PLUS: The Javalambre Photometric Local Universe Survey journal February 2019
Inversion of HIPPARCOS andGaiaphotometric data for asteroids journal October 2019
J-PLUS: A first glimpse at the spectrophotometry of asteroids journal November 2021
Taxonomy of asteroid families among the Jupiter Trojans: comparison between spectroscopic data and the Sloan Digital Sky Survey colors journal April 2008
Surface composition of Hungaria asteroids from the analysis of the Sloan Digital Sky Survey colors journal July 2008
The Sloan Digital Sky Survey: Technical Summary journal September 2000
Solar System Objects Observed in the Sloan Digital Sky Survey Commissioning Data journal November 2001
Comparison of Positions and Magnitudes of Asteroids Observed in the Sloan Digital Sky Survey with Those Predicted for Known Asteroids journal September 2002
The Sloan Digital Sky Survey View of the Palomar-Green Bright Quasar Survey journal September 2005
Sloan Digital sky Survey Observations of Kuiper belt Objects: Colors and Variability journal March 2012
THE UBV ( RI ) C COLORS OF THE SUN journal May 2012
The determination of asteroid H and G phase function parameters using Gaia DR2 journal April 2021
Absolute colours and phase coefficients of trans-Neptunian objects: HV − HR and relative phase coefficients journal August 2018
Absolute colours and phase coefficients of trans-Neptunian objects: correlations and populations journal July 2019
Matplotlib: A 2D Graphics Environment journal January 2007
The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa journal June 2006
Variations in color and reflectance on the surface of asteroid (101955) Bennu journal November 2020
LSST: From Science Drivers to Reference Design and Anticipated Data Products journal March 2019