Observational detection of eight mutual eclipses and occultations between the satellites of Uranus

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Table 3:

Best-fit estimates of the parameters of the mutual events successfully observed in this work.
Date	Event	Obs.	Midtime	Impact parameter	Albedo	Relative speed on	Mean rms
(DDMMYY)	type	site	(UT)	(km)	ratio	impact plane (km s^-1)	of fit
040507	4O2P	FTS	19:09:53 $\pm$ 3	400 $\pm$ 70	$1.229 ^a \pm 0.1$	7.078^a	0.031
050807	4O2P	FTN	13:53:49 $\pm$ 30	850 $\pm$ 30	$1.238^a \pm 0.1$	1.225^a	0.019
140807	2O4P	ATH1	01:34:25 $\pm$ 28	750 $\pm$ 160	$0.813^a \pm 0.1$	5.765^a	0.083
220807	2E5T	FTN	15:03:37 $\pm$ 5	0 $\pm$ 60	$0.410 \pm 0.025$ (0.617)	3.647^a	0.039
240807	1O2P	FTN	12:24:04 $\pm$ 30	840 $\pm$ 30	$1.833^a \pm 0.1$	2.210^a	0.018
121007	4E5T	FTN	09:51:53 $\pm$ 2	$\rm 410^{+150}_{-410}$	$\rm 1.271^{+0.55}_{-0.28}$ (0.759)	5.179^a	0.042
301107	1E5T	FTN	08:53:58 $\pm$ 2	$\rm 310^{+90}_{-130}$	$\rm0.830^{+0.22}_{-0.14}$ (1.216)	7.403^a	0.040
301107	3E4P	SALT	18:47:36 $\pm$ 5	260 $\pm$ 150	$1.113^a \pm 0.1$	1.992^a	0.032

^a These parameters have been assumed and kept fixed during the fitting process.

Source LaTeX | All tables | In the text

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