2P/Encke, the Taurid complex NEOs and the Maribo and Sutter’s Mill meteorites

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Volume 584 (December 2015)

A&A, 584 (2015) A97

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Table 3

Photometry results.

Object name	H_a^a (mag)	H_a^b (mag)	R_eff (km)

2P/Encke	14.17 ±0.03	14.34 ±0.03	3.7 ^c, 3.4^d

1998 QS₅₂	14.03 ±0.03	14.09 ±0.03	3.9^c, 3.8^d
1999 RK₄₅	18.77 ±0.05	18.83 ±0.05	0.4^c, 0.4^d
2003 QC₁₀	17.61 ±0.03	17.24 ±0.03	0.8^c, 0.9^d
2003 UL₃	17.46 ±0.08	17.63 ±0.08	0.8^c, 0.7^d

1999 VT₂₅	20.98 ±0.05	20.28 ±0.05	0.2^c, 0.2^d
2001 VH₇₅	18.08 ±0.04	17.86 ±0.04	0.6^c, 0.7^d
1984 KB	15.87 ±0.04	16.00 ±0.04	1.7^c, 1.6^d
1998 SS₄₉	15.46 ±0.04	15.49 ±0.04	2.0 ^c, 2.0^d
2004 WS₂	17.74 ±0.03	17.36 ±0.03	0.7^c, 0.8^d
2002 SY₅₀	17.01 ±0.04	16.64 ±0.04	1.0^c, 1.2^d

2000 CT₃₃	14.26 ±0.03	14.42 ±0.03	3.5^c, 3.3^d
2004 RP₁₉₁	16.45 ±0.04	16.58 ±0.04	1.3^c, 1.2^d

Notes.

^(a)

Average absolute magnitude of the object and associated error obtained using the IAU-adopted phase law as phase function approximation.

^(b)

Average absolute magnitude of the object and associated error obtained using the linear phase function approximation.

^(c)

Effective radius corresponding to the absolute magnitude in Col. a.

^(d)

Effective radius corresponding to the absolute magnitude in Col. b.

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