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.

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	10635.07	9405.72	12037.04	2171.10	1928.71	5.11e-10	Euclid	NISP	NISP Y approximate filter
Euclid/NISP0.Blue	11028.60	11154.97	10872.33	9253.29	12961.67	2850.67	1844.81	4.68e-10	Euclid	NISP	NISP Blue approximate filter
Euclid/NISP0.J	13580.16	13709.84	13406.11	11625.79	15650.13	3444.23	1364.48	2.28e-10	Euclid	NISP	NISP J approximate filter
Euclid/NISP0.Red	15300.81	15620.35	14877.99	12153.91	18762.96	5852.62	1126.38	1.53e-10	Euclid	NISP	NISP Red approximate filter
Euclid/NISP0.H	17588.51	17754.46	17366.17	15104.71	20316.79	4550.76	919.27	9.14e-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 Spanish Virtual Observatory (https://svo.cab.inta-csic.es) project 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