HD 117214 debris disk: scattered-light images and constraints on the presence of planets

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Table 6

References for the data of Fig. 6.

Target	Instrument	Filter	λ	Refs.
			(μm) ^(a)
HD 117214	SPHERE/IRDIS	K1	2.110	1
HR 4796 A	SPHERE/IRDIS	H	1.626	2
HD 61005	SPHERE/IRDIS	H	1.626	3
HD 191089	HST/NICMOS	F110W	1.100	4
HD 35841	GPI	H	1.647	5
HD 15115	SPHERE/IRDIS	H	1.626	6
Zodiacal	Rocket-borne	F1	0.476	7, 8
dust	photometer	F2	0.592
Saturn’s D68	Cassini/ISS	WAC clear	0.634	9
ring		NAC clear	0.651
Comet 67P	Rosetta/OSIRIS	WAC F21	0.537	10
		NAC F22	0.649

Notes. ^(a) Central or effective wavelength of filter.

References. ⁽¹⁾ This work; ⁽²⁾Milli et al. (2017); ⁽³⁾ Olofsson et al. (2016); ⁽⁴⁾ Ren et al. (2019); ⁽⁵⁾ Esposito et al. (2018); ⁽⁶⁾ Engler et al. (2019); ⁽⁷⁾ Leinert et al. (1974); ⁽⁸⁾ Leinert et al. (1976); ⁽⁹⁾ Hedman & Stark (2015); ⁽¹⁰⁾Bertini et al. (2017).

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