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	10831.13	10914.19	10731.42	9454.41	12312.18	2258.82	1905.64	4.87e-10	Euclid	NISP	Euclid NISP Y (full response)
Euclid/NISP.J	13635.43	13785.13	13432.37	11597.55	15872.94	3685.41	1368.41	2.21e-10	Euclid	NISP	Euclid NISP J (full response)
Euclid/NISP.H	17679.62	17857.14	17440.04	15111.99	20463.09	4594.44	915.97	8.79e-11	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