SVO Filter Profile Service

TNG :Telescopio Nazionale Galileo
TNG/NICS :NICS is the infrared camera/spectrometer designed and built for the National Telescope Galileo by the infrared group at the Arcetri Observatory in Firenze (Italy).

TNG filters: DOLORES NICS OIG TNG

Filter ID	λ_ref	λ_mean	λ_eff	λ_min	λ_max	W_eff	ZP_ν	ZP_λ	Obs. Facility	Instrument	Description
TNG/NICS.1mic	10233.44	10255.30	10208.20	9389.03	11168.39	1204.26	2070.24	5.96e-10	TNG	NICS	NICS 1mic
TNG/NICS.Js	12512.01	12539.59	12472.34	11419.10	13672.35	1561.66	1551.98	2.99e-10	TNG	NICS	NICS Js
TNG/NICS.J	12694.21	12789.08	12565.63	10678.94	14648.80	2704.28	1515.25	2.88e-10	TNG	NICS	NICS J
TNG/NICS.SW_gohss	12615.53	13298.97	11793.99	9009.00	17890.19	8022.91	1450.35	3.13e-10	TNG	NICS	NICS SW gohss
TNG/NICS.Hcont	15692.57	15693.13	15691.92	15461.03	15925.15	228.76	1095.52	1.33e-10	TNG	NICS	NICS H continuum
TNG/NICS.CH4s	15952.33	15968.05	15931.41	14571.36	17325.76	1149.85	1068.59	1.26e-10	TNG	NICS	NICS CH4 s
TNG/NICS.H	16218.66	16288.24	16129.02	14386.04	18143.84	2852.22	1046.70	1.21e-10	TNG	NICS	NICS H
TNG/NICS.FeII	16438.89	16439.63	16439.09	16171.36	16708.74	276.50	1019.99	1.13e-10	TNG	NICS	NICS FeII
TNG/NICS.CH4l	16783.94	16799.10	16764.24	15512.48	18138.68	1109.11	997.95	1.06e-10	TNG	NICS	NICS CH4 l
TNG/NICS.Kprime	21124.63	21197.90	21016.48	19033.64	23510.90	3339.73	690.71	4.69e-11	TNG	NICS	NICS Kprime
TNG/NICS.H2	21217.60	21218.38	21216.36	20903.62	21537.79	322.45	690.69	4.6e-11	TNG	NICS	NICS H2
TNG/NICS.Brg	21684.42	21685.45	21683.67	21306.72	22038.43	324.62	640.66	4.08e-11	TNG	NICS	NICS Br γ
TNG/NICS.K	21970.86	22038.01	21871.49	19899.23	24173.51	3320.48	646.03	4.05e-11	TNG	NICS	NICS K
TNG/NICS.Kcont	22741.48	22742.60	22739.81	22355.61	23133.92	366.00	612.10	3.55e-11	TNG	NICS	NICS K continuum

Filter Plots (using a common λ range)

(Plot them zoomed to their own λ range)

If your research benefits from the use of the SVO Filter Profile Service, we would appreciate if you could include the following acknowledgement in your publication:

This research has made use of the SVO Filter Profile Service (http://svo2.cab.inta-csic.es/theory/fps/) supported from the Spanish MINECO through grant AYA2017-84089

and we would appreciate if you could include the following references in your publication:

The SVO Filter Profile Service. Rodrigo, C., Solano, E., Bayo, A., 2012; https://ui.adsabs.harvard.edu/abs/2012ivoa.rept.1015R/abstract
The SVO Filter Profile Service. Rodrigo, C., Solano, E., 2020; https://ui.adsabs.harvard.edu/abs/2020sea..confE.182R/abstract