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/NISP :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/NISP.Y	1078.54	1086.62	1149.13	938.15	1243.54	233.25	1.48	3.82e-11	Euclid	NISP	Euclid NISP Y (full response)
Euclid/NISP.J	1362.07	1376.67	1443.98	1152.26	1595.20	355.43	272.43	4.4e-9	Euclid	NISP	Euclid NISP J (full response)
Euclid/NISP.H	1764.88	1782.52	1772.93	1497.17	2056.81	456.38	667.14	6.42e-9	Euclid	NISP	Euclid NISP H (full response)

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