SVO Filter Profile Service

Euclid :Euclid is an ESA mission to map the geometry of the Universe and better understand the mysterious dark matter and dark energy
Euclid/NISP0 :The Near Infrared Spectrometer and Photometer (NISP) instrument is composed of a matrix of 4x4 2040x2040 18-micron pixel TIS detectors, covering a field of view of 0.53 deg².id:Euclid/NISP0.a

Euclid filters: NISP NISP0 VIS

Filter ID	λ_ref	λ_mean	λ_eff	λ_min	λ_max	W_eff	ZP_ν	ZP_λ	Obs. Facility	Instrument	Description
Euclid/NISP0.Y	10718.85	10789.10	10633.90	9405.72	12037.04	2171.10	1930.93	5.04e-10	Euclid	NISP	NISP Y approximate filter
Euclid/NISP0.Blue	11028.59	11154.97	10870.81	9253.29	12961.67	2850.68	1869.38	4.61e-10	Euclid	NISP	NISP Blue approximate filter
Euclid/NISP0.J	13580.17	13709.84	13404.97	11625.79	15650.13	3444.22	1373.63	2.23e-10	Euclid	NISP	NISP J approximate filter
Euclid/NISP0.Red	15300.81	15620.35	14875.36	12153.91	18762.96	5852.62	1167.14	1.49e-10	Euclid	NISP	NISP Red approximate filter
Euclid/NISP0.H	17588.51	17754.46	17364.93	15104.71	20316.79	4550.76	922.11	8.94e-11	Euclid	NISP	NISP H approximate filter

Filter Plots

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 "Carlos Rodrigo", funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00

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