LCDB Data

Download LCDB README.TXT for explanations of field names and data

LCDB References table with BibCode links to ADS

To shorten some field names, 'SOURCE' is reduced to 'S' and 'FLAG' is reduced to 'F'.
For example, 'HSOURCE' is 'HS'.

BibCode links open a new window

Summary

NumberNameDesigFamilyCSClassDiamSDiamFDiamHSHHBandGSGAlbSAlbFAlbedoPFPeriodPerDescAmpFAmpMinAmpMaxUNotesPoleBINSurveyIsPrivateNotesEx
1902082006 AQ2006 AQNEAASC 0.713M18.1 M0.15A 0.20 182   0.253-  ? 0 

Details

ReferenceBibCodeWorked asDateObs    PABLPABBPhaseFamilyClassDiamMethDiamFDiamDiamErrHSHHErrHBandGSGGErrAlbSAlbFAlbedoAlbErrPFPeriodPerErrPerDescAmpFAmpMinAmpMaxAmpErrUNotesPoleBINSurveyIsPrivateNotesEx
Veres 20152015Icar..261...34V2006 AQ           18.340.45  0.2120.117             N   0 
Warner 2015g2015MPBu...42...79W2006 AQ2014-11-115.99.956.1                  182.2.   0.250.023-  ? 0See footnotes
Pajuelo 2018b2018MNRAS.477.5590P2006 AQ     K, Cg                        S   0 
Binzel 20192019Icar..324...41B2006 AQ2014-12-0222.911.865.7 S                        N   0See footnotes

Details Notes
Warner 2015g
No events seen and not likely so because of the long second period. The long period is attributed to
the primary body while the short period is presumed to be due to the rotation of the fully
asynchronous satellite.

Binzel 2019
MITHNEOS Method: NIR


Binary

ReferenceBibCodeBTypePer1Per1ErrAmp1Amp1ErrPer2Per2ErrAmp2Amp2ErrPOrbPOrbErrEventMinEventMaxDsDpFDsDpDsDpErrADpADpErr
Warner 2015g2015MPBu...42...79WA182.2.0.250.022.6210.0010.080.01