Luminous blue variables: An imaging perspective on their binarity and near environment

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Volume 587 (March 2016)

A&A, 587 (2016) A115

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Table 3

List of instruments used.

Star	NACO	VISIR	Spitzer archive
	13,27,54 mas	75 mas	(IRAC 0.6″, MIPS 1.2″)

Pistol Star	K-S13/S27, Lp-L27	PAH2, SiC, NeII*	IRAC1, 2, 3, 4
WR102ka	problem		IRAC1, 2, 3, 4
WR102ka			MIPS24
LBV1806-20	K-S27, Lp-L27		IRAC1, 2, 3, 4
LBV1806-20			MIPS24
HD 168625	3.74/4.05/Lp-L54	PAH1, PAH2	IRAC1, 2, 3, 4
HD 168625	K-S27, Lp-L27	SiC, NeII	MIPS24
HD 168607	K-S27, Lp-L27		IRAC1, 2, 3, 4
HD 168607			MIPS24
MWC930	K-S27, Lp-L27^*
MWC314	K-S27, Lp-L27		IRAC1, 2, 3, 4
HD 152234		PAH1, SiC, NeII
WR102e	K-S13/S27, Lp-L27		IRAC1, 2, 3, 4
HD 164794	K-S27, Lp-L27		IRAC1, 2, 3, 4
HD 164794			MIPS24

Star	WISE-archive	HST-archive	other
	(1.38″)	25,50,100 mas	archive

Pistol Star	1,2,3^,4^	yes	2MASS^**
WR102ka	1,2,3,4	no	SINFONI^***
LBV1806-20	1, 2, 3, 4	yes	N/A
HD 168625	1, 2, 3*, 4	yes	N/A
HD 168607	1, 2, 3, 4	yes	N/A
MWC930	1, 2, 3, 4	yes	N/A
MWC314	1, 2, 3, 4	no	swift^, EMMI^
HD 152234	1, 2, 3, 4	no	N/A
WR102e	1, 2, 3^,4^	yes	N/A
HD 164794	1, 2, 3, 4	yes^*	VISIR^*

Notes. The pixel size in angular units (mas or arcsec) of the cameras is indicated. The filters and NACO cameras (S13, S27, L27, L54) are mentioned. The central wavelength of each filter is provided in Table 4.

^(*)

Too faint, saturated, not used (insufficient resolution or not deep enough).

^(**)

Skrutskie et al. (2006).

^(***)

SINFONI, scale 250 mas × 150 mas, data presented in Oskinova et al. (2013).

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