The surface of (136108) Haumea (2003 EL61), the largest carbon-depleted object in the trans-Neptunian belt

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Table 2:

Normalized reflectivity gradient $S_{\rm ir}'$ and depth of the 1.52 and 2.02 $\mu$ m bands D, as defined in the text, for all the considered infrared spectra.
Name	$^{a}S_{\rm ir}'$	D_1.52	$^{b}\varepsilon_{1.52}$	D_2.02	$^{b}\varepsilon_{2.02}$
Aug. 2005	1.07	31.13	7.2	49.7	13.5
sp 2006all	-1.40	34.0	4.8	53.8	6.6
2006 phase1	1.61	33.9	6.7	55.8	10.0
2006 phase2	-1.77	33.3	5.6	51.3	10.2
2006 phase3	-2.12	38.3	7.0	54.6	10.6
2006 phase4	-2.32	32.4	9.2	49.5	13
2006 phase5	-1.97	33.1	7.8	59.8	10.6

^a Uncertainties of 2%/1000 Å in the slope are typical due to systematic errors (see text for details); $^{b}~\varepsilon$ are the errors associated with D.

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