SVO Filter Profile Service

WHT :William Herschel Telescope
WHT/PFIP :The Prime Focus Imaging Platform (PFIP) or Prime Focus Camera is an optical mosaic camera for use at the prime focus of the 4.2m William Herschel Telescope. id:WHT/PFIP.a
→ GaiaXPy base XML file. You can download here the GaiaXPy base XML file for the full WHT/PFIP filter set. Please, take a look to the GaiaXPy web page and additional documentation for more information.

WHT filters: INGRID LRIS PAUCam PFIP ULTRACAM

Filter ID	λ_ref	λ_mean	λ_eff	λ_min	λ_max	W_eff	ZP_ν	ZP_λ	Obs. Facility	Instrument	Description
WHT/PFIP.RGO_U9	3600.85	3617.23	3667.55	3081.04	4113.01	561.46	1736.04	4.01e-9	WHT	PFIP	RGO U 9
WHT/PFIP.RGO_U	3687.63	3698.30	3747.16	3250.00	4110.00	437.32	1978.77	4.36e-9	WHT	PFIP	RGO U 5
WHT/PFIP.Har_B6	4287.18	4332.25	4311.10	3526.19	5714.05	1053.51	3838.53	6.26e-9	WHT	PFIP	Harris B 6
WHT/PFIP.Har_B	4291.60	4337.88	4315.12	3522.16	5727.61	1065.52	3836.48	6.24e-9	WHT	PFIP	Harris B 5
WHT/PFIP.Har_V	5456.51	5489.92	5425.16	4835.93	6647.46	983.95	3641.81	3.67e-9	WHT	PFIP	Harris V 5
WHT/PFIP.Har_R	6497.24	6596.67	6400.85	5478.29	9000.00	1628.16	3048.81	2.17e-9	WHT	PFIP	Harris R 5
WHT/PFIP.Har_I	8090.84	8136.12	8048.82	7060.28	9000.00	1644.75	2399.26	1.1e-9	WHT	PFIP	Harris I 5

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