
BKV: Measurements of Bmode Polarization at Degree Angular Scales and
150 GHz by Keck Array
The Keck Array and BICEP2 Collaborations, ApJ 811, 126, 2015
 20150202: Posted BICEP2/Keck Array combined data products.
Data Products  

BK_bandpowers_20150130.txt  Text file containing bandpowers and statistical uncertainties of combined BICEP2 and Keck Array maps, corresponding to Figure 9 of Keck Array/BICEP2 2015 V. 
BK_bandpowers_sample_20150129.txt  Text file containing bandpowers and statistical uncertainties of combined BICEP2 and Keck Array maps including sample variance consistent with the signal we observe. 
BK_bandpower_window_functions.tgz BK_bpwf_bin1_20150129.txt BK_bpwf_bin2_20150129.txt BK_bpwf_bin3_20150129.txt BK_bpwf_bin4_20150129.txt BK_bpwf_bin5_20150129.txt BK_bpwf_bin6_20150129.txt BK_bpwf_bin7_20150129.txt BK_bpwf_bin8_20150129.txt BK_bpwf_bin9_20150129.txt 
Bandpower window functions for each ℓ bin. 
BK_likelihood_bandpowers_20150129.txt BK_bpcm_nosysuncer_20150129.txt 
Data necessary for constructing approximate bandpower likelihoods following the method of Hamimeche & Lewis (2008). See Section 9.1 of Barkats et al. 
BK_camb_planck_params_20150129.ini BK_camb_planck_lensed_uK_20150129.txt BK_cl_expected_lensed_20150129.txt 
Theoretical power spectra for the lensedΛCDM model, described in Section 5.1 of BICEP2 I. Includes the model parameters, the unbinned spectra calculated by CAMB (March 2013 version) and the binned expectation values of the bandpowers. Note that these are nearly identical to the theoretical spectra provided with the BICEP2 2014 release, except that the accuracy of the CAMB lensing calculation has been increased and the bandpower window functions of Keck Array are slightly different. 