Kepler-91b: a planet at the end of its life - Planet and giant host star properties via light-curve variations

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Table 3

Photometric data used in our spectral energy distribution fitting of Sect. 3.3.

Band	Magnitude^a	Reference

U	15.297	Everett et al. (2012)^b
B	13.986	Everett et al. (2012) ^b
V	12.884	Everett et al. (2012) ^b
g ′	13.407	KIC, Brown et al. (2011)^c
r ′	12.406	KIC, Brown et al. (2011)^c
i ′	12.104	KIC, Brown et al. (2011)^c
z ′	11.919	KIC, Brown et al. (2011)^c
Kep	12.495	Kepler, Borucki et al. (2010)
J	10.790 ± 0.026	2MASS, Cutri et al. (2003)
H	10.235 ± 0.030	2MASS, Cutri et al. (2003)
Ks	10.136 ± 0.021	2MASS, Cutri et al. (2003)
W1	10.032 ± 0.023	WISE, Wright et al. (2010)
W2	10.157 ± 0.020	WISE, Wright et al. (2010)
W3	10.049 ± 0.040	WISE, Wright et al. (2010)
W4	9.380	WISE, Wright et al. (2010)

Notes.

^(a)

We assume 1% error when no errors are provided by the catalogues.

^(b)

Johnson-like filters. More details can be found in Everett et al. (2012).

^(c)

Sloan-like filters. More details can be found in Brown et al. (2011).

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