Table 3: Best fit of asteroids and meteorite spectra. The five first ranked meteorite analogs have been tabulated. When the meteorite is presented several times in the table for the same asteroid, this represents the differences in preparation of the analyzed sample. Metallic meteorites are the best fit for eight of our asteroids (the exception is the asteroid 766 Moguntia). The table also ranks a heated sample of meteorite Murchinson (marked by *), two samples of fresh cut Tagish Lake meteorite (one of them is presented for several asteroids), one Abee sample, one CM2 meteorite from Antarctica (LEW85311) and one lodranite (MAC88177). The last column show the slope of each asteroid NIR spectrum. We add the IRAS albedo (labeled A) when available.

Spectrum		 Meteorite Type $\chi^2$ $(\times 10^6)$ S ($\mu $m-1)
325 Heidelberga DRP78007 Iron 244  
  Butler Iron 270  
A = 0.1068 DRP78007 Iron 287 0.27
  DRP78007 Iron 378  
  DRP78007 Iron 415  
497 Iva Odessa Iron IA 264  
  Cassey Iron IAB 613  
  Tagish Lake CI/CM 698 0.32
  Butler Iron 993  
  DRP78007 Iron 1280  
558 Carmen Chulafinnee Iron IIIAB 86  
  DRP78007 Iron 152  
A = 0.1161 DRP78007 Iron 159 0.256
  DRP78007 Iron 273  
  Feni Iron 322  
687 Tinette Chulafinnee Iron IIIAB 319  
  Feni Iron 335  
  Feni Iron 341 0.25
  Tagish Lake CI/CM 372  
  Tagish Lake CI/CM 394  
766 Moguntia Ozona H6 92  
  ALH84028 CV3 115  
  Murchison* CM2 147 0.065
  Allende CV3 189  
  Murchison CM2 333  
860 Ursina Murchinson* CM2 418  
  Abee E4 471  
  Feni Iron 507 0.21
A = 0.1618 Feni Iron 519  
  Odessa Iron 629  
909 Ulla Mundrabilla Iron 218  
  MAC88177 Lodranite 218  
A = 0.0343 Mundrabilla Iron 262 0.15
  Mundrabilla Iron 325  
  Murchinson* CM2 343  
1280 Baillauda DRP78007 Iron 271  
  Tagish Lake CI/CM 407  
A = 0.0505 DRP78007 Iron 408 0.27
  DRP78007 Iron 507  
  DRP78007 Iron 508  
1564 Srbija Odessa Iron IA 176  
  Odessa Iron IA 182  
  LEW85311 CM2 408 0.24
  Tagish Lake CI/CM 416  
  Feni Iron 421  


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