Herschel-PACS photometry of the five major moons of Uranus

Open Access

Table 3

Mean fluxes of the Uranian moons (Eq. (3)) calculated from a weighted mean moon-to-Uranus flux ratio (Eq. (1)) and a mean Uranus flux (Eq. (2)) over the Herschel observation campaign.

Object	n₇₀			n₁₀₀			n₁₆₀
		(10⁻³)	(Jy)		(10⁻³)	(Jy)		(10⁻³)	(Jy)
Titania	10	1.931 ± 0.0095	1.663 ± 0.008	10	1.619 ± 0.0104	1.423 ± 0.009	20	1.317 ± 0.0074	0.873 ± 0.005
Oberon	10	1.847 ± 0.0067	1.591 ± 0.006	10	1.537 ± 0.0074	1.351 ± 0.007	20	1.217 ± 0.0038	0.807 ± 0.003
Umbriel	10	1.055 ± 0.0140	0.909 ± 0.012	10	0.869 ± 0.0138	0.764 ± 0.012	20	0.613 ± 0.0187	0.406 ± 0.012
Ariel	10	0.876 ± 0.0150	0.754 ± 0.013	10	0.799 ± 0.0428	0.702 ± 0.038	20	0.294 ± 0.0171	0.195 ± 0.011
Miranda	10	0.261 ± 0.0349	0.225 ± 0.030	8	0.135 ± 0.0164	0.119 ± 0.016	–	–	–

Uranus	10		861.287 ± 0.535	10		879.061 ± 0.488	20		663.011 ± 0.403

Notes. σ_tot of the individual moon photometry was used as weight. The applied mean distance (20.024 AU) normalised Uranus flux is given in the last line. n₇₀, n₁₀₀ and n₁₆₀ give the number of reliable measurements used in the determination of .

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.