Comparison of positions and magnitudes of asteroids observed in the sloan digital sky survey with those predicted for known asteroids

Mario Jurić, Željko Ivezić, Robert H. Lupton, Tom Quinn, Serge Tabachnik, Xiaohui Fan, James E. Gunn, Gregory S. Hennessy, Gillian R. Knapp, Jeffrey A. Munn, Jeffrey R. Pier, Constance M. Rockosi, Donald P. Schneider, Jonathan Brinkmann, István Csabai, Masataka Fukugita

Research output: Contribution to journalArticle

69 Citations (Scopus)

Abstract

We positionally correlate known asteroids with a sample of ∼18,000 asteroids detected by the Sloan Digital Sky Survey (SDSS). We find 2641 unique matches, which represent the largest sample of asteroids with both accurate multicolor photometry and known orbital parameters. The matched objects are predominantly bright and demonstrate that the SDSS photometric pipeline recovers ∼90% of the known asteroids in the observed region. For the recovered asteroids, we find a large offset (∼0.4 mag) between Johnson V magnitudes derived from SDSS photometry and the predicted magnitudes. This offset varies with the asteroid color, from 0.34 mag for blue asteroids to 0.44 mag for red asteroids, and is probably caused by the use of unfiltered CCD observations in the majority of recent asteroid surveys. This systematic photometric error leads to an overestimate of the number of asteroids brighter than a given absolute magnitude limit by a factor of ∼1.7. The distribution of the matched asteroids in orbital parameter space indicates strong color segregation. We confirm that some families are dominated by a single asteroid type (e.g., the Koronis family by red asteroids and the Themis family by blue asteroids), while others appear to be a mixture of blue and red objects (e.g., the Nysa-Polana family). Asteroids with the bluest i*-z* colors, which can be associated with the Vesta family, show particularly striking localization in orbital parameter space.

Original languageEnglish (US)
Pages (from-to)1776-1787
Number of pages12
JournalAstronomical Journal
Volume124
Issue number3 1761
DOIs
StatePublished - Sep 2002
Externally publishedYes

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asteroids
asteroid
comparison
color
orbitals
photometry
systematic errors
charge coupled devices

Keywords

  • Minor planets, asteroids
  • Solar system: general

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Comparison of positions and magnitudes of asteroids observed in the sloan digital sky survey with those predicted for known asteroids. / Jurić, Mario; Ivezić, Željko; Lupton, Robert H.; Quinn, Tom; Tabachnik, Serge; Fan, Xiaohui; Gunn, James E.; Hennessy, Gregory S.; Knapp, Gillian R.; Munn, Jeffrey A.; Pier, Jeffrey R.; Rockosi, Constance M.; Schneider, Donald P.; Brinkmann, Jonathan; Csabai, István; Fukugita, Masataka.

In: Astronomical Journal, Vol. 124, No. 3 1761, 09.2002, p. 1776-1787.

Research output: Contribution to journalArticle

Jurić, M, Ivezić, Ž, Lupton, RH, Quinn, T, Tabachnik, S, Fan, X, Gunn, JE, Hennessy, GS, Knapp, GR, Munn, JA, Pier, JR, Rockosi, CM, Schneider, DP, Brinkmann, J, Csabai, I & Fukugita, M 2002, 'Comparison of positions and magnitudes of asteroids observed in the sloan digital sky survey with those predicted for known asteroids', Astronomical Journal, vol. 124, no. 3 1761, pp. 1776-1787. https://doi.org/10.1086/341950
Jurić, Mario ; Ivezić, Željko ; Lupton, Robert H. ; Quinn, Tom ; Tabachnik, Serge ; Fan, Xiaohui ; Gunn, James E. ; Hennessy, Gregory S. ; Knapp, Gillian R. ; Munn, Jeffrey A. ; Pier, Jeffrey R. ; Rockosi, Constance M. ; Schneider, Donald P. ; Brinkmann, Jonathan ; Csabai, István ; Fukugita, Masataka. / Comparison of positions and magnitudes of asteroids observed in the sloan digital sky survey with those predicted for known asteroids. In: Astronomical Journal. 2002 ; Vol. 124, No. 3 1761. pp. 1776-1787.
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AU - Jurić, Mario

AU - Ivezić, Željko

AU - Lupton, Robert H.

AU - Quinn, Tom

AU - Tabachnik, Serge

AU - Fan, Xiaohui

AU - Gunn, James E.

AU - Hennessy, Gregory S.

AU - Knapp, Gillian R.

AU - Munn, Jeffrey A.

AU - Pier, Jeffrey R.

AU - Rockosi, Constance M.

AU - Schneider, Donald P.

AU - Brinkmann, Jonathan

AU - Csabai, István

AU - Fukugita, Masataka

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N2 - We positionally correlate known asteroids with a sample of ∼18,000 asteroids detected by the Sloan Digital Sky Survey (SDSS). We find 2641 unique matches, which represent the largest sample of asteroids with both accurate multicolor photometry and known orbital parameters. The matched objects are predominantly bright and demonstrate that the SDSS photometric pipeline recovers ∼90% of the known asteroids in the observed region. For the recovered asteroids, we find a large offset (∼0.4 mag) between Johnson V magnitudes derived from SDSS photometry and the predicted magnitudes. This offset varies with the asteroid color, from 0.34 mag for blue asteroids to 0.44 mag for red asteroids, and is probably caused by the use of unfiltered CCD observations in the majority of recent asteroid surveys. This systematic photometric error leads to an overestimate of the number of asteroids brighter than a given absolute magnitude limit by a factor of ∼1.7. The distribution of the matched asteroids in orbital parameter space indicates strong color segregation. We confirm that some families are dominated by a single asteroid type (e.g., the Koronis family by red asteroids and the Themis family by blue asteroids), while others appear to be a mixture of blue and red objects (e.g., the Nysa-Polana family). Asteroids with the bluest i*-z* colors, which can be associated with the Vesta family, show particularly striking localization in orbital parameter space.

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