YY Hya and its interstellar environment | Astronomy & Astrophysics (A&A)

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Table A.2

Overview of the photometric bands, used effective wavelengths, λ_eff, calibration zero points, ZP, and the interstellar extinction, A_λ. In addition, an overview of the magnitudes as used in the SED fitting (see text) is given.

band	λ_eff	ZP	A_λ		< m_λ >		amplitude	phase
	[nm]	[Jy]	[mag]	[mag]	[mag]	[mag]	[mag]	[0,1]	[mag]
GALEX FUV	154.9	521	.261					0.38	14.142	13.88
GALEX NUV	230.5	789	.284					0.38	14.440	14.16
Gaia BP	502.1	3393	.112	14.577	14.077	13.576	1.002			14.46
CRTS V	561.8	2690	.0975	14.378	13.897	13.416	0.963			14.28
Gaia G	583.6	2835	.0975	14.374	13.912	13.449	0.925			14.28
PTF R	612.2	3042	.0887	14.387	13.955	13.524	0.864			14.30
Gaia RP	758.9	2485	.0659	13.958	13.534	13.110	0.847			13.89
DENIS I_c	786.2	2442	.0618					0.12	13.474	13.74
	786.2	2442	.0618					0.88	13.443	13.71
DENIS J	1221.	1588	.0293					0.12	13.115	13.21
	1221.	1588	.0293					0.88	13.143	13.24
2MASS J	1235.	1594	.0288					0.78	12.867	13.20
2MASS H	1662.	1024	.0178					0.78	12.518	12.85
DENIS K_s	2147.	667	.0118					0.12	12.809	12.91
	2147.	667	.0118					0.88	12.660	12.77
2MASS K_s	2159.	666	.0117					0.78	12.392	12.72
WISE W1	3353.	310	.0061	12.845	12.523	12.201	0.644			12.84
WISE W2	4603.	172	.0047	12.805	12.444	12.084	0.722			12.80

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