Short-term variability of a sample of 29 trans-Neptunian objects and Centaurs

Free Access

Issue		A&A Volume 522, November 2010


Article Number		A93
Number of page(s)		43
Section		Planets and planetary systems
DOI		https://doi.org/10.1051/0004-6361/200912340
Published online		05 November 2010

Online material

Table 1

Dates, geometric and photometric data of the observations.

	Fig. A.1 Lomb periodogram of 2003 FY₁₂₈.
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	Fig. A.2 Rotational phase curve for 2003 FY₁₂₈ obtained by using a spin period of 8.54 h (upper plot) and a spin period of 17.08 h (lower plot). The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.3 Rotational phase curves for 2003 MW₁₂ obtained by using different spin periods; 5.9 h (upper plot) and 7.87 h (lower plot). In both case, we present a single peak lightcurve. The dash lines are a Fourier Series fits of the photometric data. Different symbols correspond to different dates.
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	Fig. A.4 Lomb periodogram of 2003 MW₁₂.
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	Fig. A.5 Rotational phase curve for 2003 OP₃₂ obtained by using a spin period of 4.05 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.6 Lomb periodogram of 2003 OP₃₂.
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	Fig. A.7 Rotational phase curves for 2004 SB₆₀ obtained by using different spin periods: 6.09 h (upper plot) and 8.1 h (lower plot). In both cases, we present a single peak lightcurve. The dash lines are a Fourier Series fits of the photometric data. Different symbols correspond to different dates.
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	Fig. A.8 Lomb periodogram of 2004 SB₆₀.
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	Fig. A.9 Lomb periodogram of 2005 CB₇₉.
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	Fig. A.10 Rotational phase curve for 2005 CB₇₉ obtained by using a spin period of 6.76 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.11 Lomb periodogram of 2005 RN₄₃.
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	Fig. A.12 Rotational phase curves for 2005 RN₄₃ obtained by using different spin periods: 5.62 h (upper plot) and 7.32 h (lower plot). In both case, we present a single peak lightcurve. The dash lines are a Fourier Series fits of the photometric data. Different symbols correspond to different dates.
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	Fig. A.13 Lomb periodogram of 2005 RR₄₃.
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	Fig. A.14 Rotational phase curve for 2005 RR₄₃ obtained by using a spin period of 7.87 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.15 Lomb periodogram of Quaoar.
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	Fig. A.16 Rotational phase curve for Quaoar obtained by using a spin period of 8.84 h for the single peak lightcurve (upper plot) and a spin period of 17.68 h (lower plot) for the double lightcurve. The dash lines are a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.17 Lomb periodogram of Varuna.
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	Fig. A.18 Rotational phase curve for Varuna obtained by using a spin period of 6.3418 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.19 Lomb periodogram of 2002 AW₁₉₇.
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	Fig. A.20 Rotational phase curve for 2002 AW₁₉₇ obtained by using a spin period of 8.78 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.21 Lomb periodogram of 2002 TX₃₀₀.
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	Fig. A.22 Rotational phase curve for 2002 TX₃₀₀ obtained by using a spin period of 8.16 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.23 Lomb periodogram of Makemake.
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	Fig. A.24 Rotational phase curve for Makemake obtained by using a spin period of 7.65 h. The thick line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.25 Lomb periodogram of 2001 YH₁₄₀.
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	Fig. A.26 Rotational phase curve for 2001 YH₁₄₀ obtained by using a spin period of 13.2 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.27 Lomb periodogram of Orcus.
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	Fig. A.28 Rotational phase curve for Orcus obtained by using a spin period of 10.47 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.29 Lomb periodogram of 2002 VE₉₅.
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	Fig. A.30 Rotational phase curve for 2002 VE₉₅ obtained by using a spin period of 9.97 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.31 Lomb periodogram of 2003 AZ₈₄.
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	Fig. A.32 Rotational phase curve for 2003 AZ₈₄ obtained by using a spin period of 6.79 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.33 Lomb periodogram of 2003 VS₂.
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	Fig. A.34 Rotational phase curve for 2003 VS₂ obtained by using a spin period of 7.42 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.35 Lomb periodogram of 2004 UX₁₀.
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	Fig. A.36 Rotational phase curve for 2004 UX₁₀ obtained by using a spin period of 5.68 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.37 Lomb periodogram of Haumea.
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	Fig. A.38 Rotational phase curve for Haumea obtained by using a spin period of 3.92 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.39 Lomb periodogram of 2005 RM₄₃.
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	Fig. A.40 Rotational phase curve for 2005 RM₄₃ obtained by using a spin period of 6.71 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.41 Lomb periodogram of Typhon.
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	Fig. A.42 Rotational phase curve for Typhon obtained by using a spin period of 9.67 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.43 Lomb periodogram of 1996 TL₆₆.
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	Fig. A.44 Rotational phase curve for 1996 TL₆₆ obtained by using a spin period of 12 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.45 Lomb periodogram of Okyrhoe.
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	Fig. A.46 Rotational phase curves for Okyrhoe obtained by using different spin periods: 4.86 h (upper plot) and 6.08 h (lower plot). In both cases, we present a single peak lightcurve . The dash lines are a Fourier Series fits of the photometric data. Different symbols correspond to different dates.
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	Fig. A.47 Lomb periodogram of 2005 UJ₄₃₈.
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	Fig. A.48 Rotational phase curve for 2005 UJ₄₃₈ obtained by using a spin period of 4.16 h for the single peak lightcurve (upper plot) and a spin period of 8.32 h for the double peak lightcurve (lower plot). The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.49 Lomb periodogram of 2007 UL₁₂₆ (or 2002 KY₁₄).
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	Fig. A.50 Rotational phase curves for 2007 UL₁₂₆ (2002 KY₁₄) obtained by using different spin periods: 3.56 h for the single peak lightcurve and 7.12 h for the double peak lightcurve. The dash lines are a Fourier Series fits of the photometric data. Different symbols correspond to different dates.
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	Fig. A.51 Rotational phase curves for 2007 UL₁₂₆ (2002 KY₁₄) obtained by using different spin periods: 4.2 h for a single peak lightcurve and 8.4 h for the double peak lightcurve. The dash lines are a Fourier Series fits of the photometric data. Different symbols correspond to different dates.
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	Fig. A.52 Lomb periodogram of Amycus.
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	Fig. A.53 Rotational phase curve for Amycus obtained by using a spin period of 9.76 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.54 Lomb periodogram of 2003 CO₁.
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	Fig. A.55 Rotational phase curve for 2003 CO₁ obtained by using a spin period of 4.51 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.56 Lomb periodogram of 2003 WL₇.
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	Fig. A.57 Rotational phase curve for 2003 WL₇ obtained by using a spin period of 8.24 h. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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	Fig. A.58 Lomb periodogram of 1999 TZ₁.
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	Fig. A.59 Rotational phase curve for 1999 TZ₁ obtained by using a spin period of 5.211 h (upper plot) for the single peak lightcurve and 10.422 h (lower plot) for the double peak lightcurve. The dash line is a Fourier Series fit of the photometric data. Different symbols correspond to different dates.
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© ESO, 2010

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