Table 1
Nightly averaged photometric and polarimetric parameters of 252P/LINEAR taken by IRSF/SIRPOL.
UT 2016+ | Filter | P(a) | ![]() |
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MAR 04 | J | 19.46 | 0.85 | −0.68 | 1.01 | 18.12 | 1.41 | 10.69 | 13.28 ± 0.19 |
(ϕ(i) = 78.7°) | H | 19.57 | 0.79 | −0.46 | 0.47 | 18.17 | 0.92 | 10.91 | 12.60 ± 0.18 |
MAR 09 | J | 26.04 | 0.99 | −0.34 | 0.29 | 25.19 | 0.99 | 7.33 | 12.49 ± 0.17 |
H | 24.00 | 0.91 | −0.38 | 0.18 | 23.23 | 0.90 | 7.28 | 11.80 ± 0.11 | |
(ϕ = 82.4°) | KS | 24.05 | 0.96 | −0.24 | 0.54 | 23.25 | 1.04 | 7.43 | 11.60 ± 0.15 |
MAR 11 | J | 28.19 | 1.30 | −0.43 | 0.37 | 27.61 | 1.31 | 5.79 | 12.74 ± 0.12 |
H | 27.88 | 1.13 | −0.37 | 0.10 | 27.31 | 1.11 | 5.85 | 12.24 ± 0.10 | |
(ϕ = 83.9°) | KS | 27.74 | 1.56 | −0.15 | 1.85 | 27.12 | 2.11 | 6.10 | 12.08 ± 0.20 |
MAR 12 | J | 32.57 | 1.22 | 0.27 | 0.39 | 31.92 | 1.23 | 5.73 | 11.13 ± 0.11 |
H | 31.69 | 1.14 | 0.23 | 0.36 | 31.07 | 1.16 | 5.69 | 11.20 ± 0.11 | |
(ϕ = 84.5°) | KS | 27.35 | 1.06 | 0.24 | 0.51 | 26.81 | 1.10 | 5.70 | 11.58 ± 0.12 |
MAR 13 | J | 29.60 | 1.11 | 0.21 | 0.44 | 29.13 | 1.13 | 5.13 | 11.12 ± 0.13 |
H | 28.73 | 1.03 | 0.21 | 0.36 | 28.27 | 1.04 | 5.13 | 11.22 ± 0.10 | |
(ϕ = 85.2°) | KS | 28.36 | 1.06 | 0.18 | 0.46 | 27.92 | 1.09 | 5.10 | 11.29 ± 0.11 |
MAR 14 | J | 27.37 | 1.02 | 0.21 | 0.46 | 27.02 | 1.05 | 4.64 | 11.86 ± 0.17 |
H | 26.03 | 0.94 | 0.23 | 0.36 | 25.69 | 0.95 | 4.66 | 11.41 ± 0.10 | |
(ϕ = 85.6°) | KS | 26.19 | 0.98 | 0.19 | 0.56 | 25.85 | 1.02 | 4.62 | 11.27 ± 0.20 |
MAR 15 | J | 28.10 | 1.11 | 0.19 | 0.59 | 27.73 | 1.15 | 4.68 | 11.84 ± 0.12 |
H | 27.28 | 1.01 | 0.26 | 0.38 | 26.91 | 1.02 | 4.75 | 11.37 ± 0.10 | |
(ϕ = 85.9°) | KS | 26.87 | 1.05 | 0.29 | 0.46 | 26.49 | 1.08 | 4.77 | 11.25 ± 0.19 |
Notes. (a) Observed degree of linear polarization of the cometin percent; (b)standard deviation of P in percent; (c) electric vector position angle in degrees; (d)standard deviation of θP in degrees; (e) P relative to the scattering plane in percent (see Eq. (5)); (f) standard deviation of Pr in percent; (g) polarization angle with regard to the perpendicular direction of the scattering plane in degrees (see Eq. (6)); (h) apparent magnitude of the IRSF data; and (i)position angle of the scattering plane.
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