SVO Filter Profile Service

BICEP :Background Imaging of Cosmic Extragalactic Polarization (BICEP).
BICEP/BICEP2 :BICEP2 was a 26-cm refracting telescope that observed the cosmic microwave background (CMB) from the National Science Foundation's Amundsen-Scott South Pole Station from 2010-2012.id:BICEP/BICEP2.a

BICEP filters: BICEP1 BICEP2 BICEP3

Filter ID	λ_ref	λ_mean	λ_eff	λ_min	λ_max	W_eff	ZP_ν	ZP_λ	Obs. Facility	Instrument	Description
BICEP/BICEP2.220GHz_rj	1.31e+7	1.31e+7	1.29e+7	1.07e+7	1.57e+7	1.98e+6	0.00205	3.6e-22	BICEP	BICEP	BICEP2/Keck 220GHz RJ spectral response
BICEP/BICEP2.220GHz	1.31e+7	1.32e+7	1.3e+7	1.08e+7	1.6e+7	1.96e+6	0.00203	3.55e-22	BICEP	BICEP	BICEP2/Keck 220GHz spectral response
BICEP/BICEP2.150GHz_rj	2.04e+7	2.06e+7	2.01e+7	1.66e+7	2.64e+7	4.88e+6	0.000832	5.97e-23	BICEP	BICEP	BICEP2/Keck 150GHz RJ spectral response
BICEP/BICEP2.150GHz	2.06e+7	2.08e+7	2.02e+7	1.67e+7	2.65e+7	4.88e+6	0.000821	5.81e-23	BICEP	BICEP	BICEP2/Keck 150GHz spectral response
BICEP/BICEP2.95GHz_rj	3.19e+7	3.22e+7	3.14e+7	2.61e+7	4.07e+7	6.78e+6	0.000336	9.89e-24	BICEP	BICEP	BICEP2/Keck 95GHz RJ spectral response
BICEP/BICEP2.95GHz	3.21e+7	3.24e+7	3.16e+7	2.63e+7	4.08e+7	6.74e+6	0.000332	9.66e-24	BICEP	BICEP	BICEP2/Keck 95GHz spectral 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 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