Table 3: NEATM fits to the available thermal-infrared data: the MIRSI data as given in Table 2, and the five IRAS sightings (Tedesco 1992). No attempt at lightcurve-correction was made.
$\eta$ p_V D (km)

MIRSI 0.93 0.188 103.8

IRAS 1 0.93 0.178 106.6

IRAS 2 0.94 0.226 94.7

IRAS 3 1.06 0.161 112.2

IRAS 4 0.96 0.191 103.0

IRAS 5 0.82 0.231 93.6

**Table 3:** NEATM fits to the available thermal-infrared data: the MIRSI data as given in Table 2, and the five IRAS sightings (Tedesco 1992). No attempt at lightcurve-correction was made.
	$\eta$	p_V	D (km)
MIRSI	0.93	0.188	103.8
IRAS 1	0.93	0.178	106.6
IRAS 2	0.94	0.226	94.7
IRAS 3	1.06	0.161	112.2
IRAS 4	0.96	0.191	103.0
IRAS 5	0.82	0.231	93.6

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