1 See Harris et al. 2005. Icarus, 179, 95-108.                               
 2 The measured thermal infrared fluxes were lightcurve-corrected to the mean 
 - optical lightcurve magnitude on the assumption that the optical and        
 - thermal-infrared lightcurves are identical.                                
 3 Lightcurve amplitude is small (0.11 mag.) and no correction is applied to  
 - the measured thermal infrared fluxes.  Lightcurve amplitude from Harris et 
 - al. (2006).  (This data set may be found on the web at                     
 - http://www.psi.edu/pds/resource/lc.html.)                                  
 4 See Mueller et al. 2003. American Astronomical Society, DPS meeting #35,   
 - #22.04                                                                     
 5 Filter photometry                                                          
 6 N-band spectroscopy                                                        
 7 Lightcurve amplitude is small (0.04-0.20 mag.) and no correction is        
 - applied to the measured thermal infrared fluxes.  Lightcurve amplitude from
 - Harris et al. (2006). (This data set may be found on the web at            
 - http://www.psi.edu/pds/resource/lc.html.)                                  
 8 Lightcurve amplitude is small (0.11-0.20 mag.) and no correction is        
 - applied to the measured thermal infrared fluxes.  Lightcurve amplitude from
 - Harris et al. (2006). (This data set may be found on the web at            
 - http://www.psi.edu/pds/resource/lc.html.)                                  
 9 Lightcurve amplitude is small (0.15 mag.) and no correction is applied to  
 - the measured thermal infrared fluxes.  Lightcurve amplitude from Harris et 
 - al. (2006).  (This data set may be found on the web at                     
 - http://www.psi.edu/pds/resource/lc.html.)                                  
10 The absolute magnitude H used to derive albeos was derived from optical    
 - observations obtained at ESO, La Silla on 2002-11-28.                      
11 Thermal models were applied only to the measurments obtained with N-band   
 - filters.                                                                   
12 The whole data set (N-band and Q-band) was used.                           
13 Lightcurve amplitude is rather small (0.30 mag.) and asteroid rotation     
 - period long (23.76 hours). No correction was thus applied to the measured  
 - thermal infrared fluxes.  Lightcurve amplitude from Harris et al. (2006).  
 - (This data set may be found on the web at                                  
 - http://www.psi.edu/pds/resource/lc.html.)                                  
14 Data reduction by Michael Mueller and in part by Marco Delbo. Results      
 - presented at the DPS 2003: Mueller, et al. AAS, DPS meeting #35, #22.04;   
 - Bulletin of the American Astronomical Society, Vol. 35, p.955.             
15 See Delbo et al. 2003. Icarus, 166, 116.