Photometric segregation of dwarf and giant FGK stars using the SVO Filter Profile Service and photometric tools

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Volume 689 (September 2024)

A&A, 689 (2024) A93

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202554660e]

Table 2

Selected J-PAS filters and their characteristics.

J-PAS filter	λ_eff	λ_min	λ_max	W_eff
	(Å)	(Å)	(Å)	(Å)
J0450	4514.42	4420.83	4613.85	143.74
J0460	4608.52	4513.99	4706.85	143.95
J0470	4704.40	4608.26	4803.61	140.72
J0490	4911.15	4808.71	5009.24	148.71
J0510	5101.53	5007.49	5199.79	146.66
J0520	5207.86	5110.47	5308.04	149.27
J0530	5303.52	5206.95	5403.67	150.59
J0540	5396.85	5302.38	5496.61	149.54
J0550	5501.64	5405.61	5600.81	146.03
J0600	6009.76	5914.71	6108.40	148.38
J0610	6117.19	6021.49	6215.13	146.63
J0620	6208.79	6113.73	6307.07	147.18
J0630	6312.31	6217.88	6409.61	147.53
J0640	6410.21	6314.82	6508.32	146.51
J0650	6503.43	6412.92	6604.47	146.86

Notes. λ_eff is the effective wavelength, λ_min and λ_max are the minimum and maximum wavelength, respectively, and W_eff is the effective width. Additional information is provided on the SVO FPS webpage.

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