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.id:Euclid/NISP.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/NISP.Y	10785.39	10866.24	10688.60	9381.52	12435.44	2332.48	1916.10	4.94e-10	Euclid	NISP	Euclid NISP Y (full response)
Euclid/NISP.J	13620.63	13766.64	13422.62	11522.58	15951.97	3554.06	1370.25	2.21e-10	Euclid	NISP	Euclid NISP J (full response)
Euclid/NISP.H	17648.80	17825.15	17410.63	14971.70	20568.14	4563.68	918.35	8.84e-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