measurements come from this dataset (labeled “SN”), and the fluxes are given in Table \[bcddata\].

We have expanded this existing optical/NIR photometry with new observations from the WIYN[^2] 3.5-m telescope at KPNO. Complete details of the observations, reductions, and calibrations are given in @janowiecki14. In short, the Minimosaic and OPTIC (Orthogonal Parallel Transfer Imaging Camera) imagers were used to obtain optical observations and the WHIRC [WIYN High Resolution Infrared Camera, @meixner10] imager was used to obtain NIR observations. Observations were taken between November 2008 and April 2010, and were calibrated with catalog measurements from Sloan Digital Sky Survey (SDSS) and Two Micron All Sky Survey (2MASS) of stars in the fields with our targets. Table \[bcdobs\] shows which flux measurements come from our recent WIYN observations (labeled “W”), and our complete set of fluxes and uncertainties are reported in Table \[bcddata\].

We also have calibrated narrow band Ha observations of the BCD sample which are used to determine SFRs from the standard prescription of @kennicutt98. These [H$\alpha$ ]{}fluxes were measured from narrow-band imaging [@salzerelston92], and the calibrated [H$\alpha$ ]{} luminosities are given in Table \[bcdha\], along with metallicity values from the literature for the BCD sample. Distances in Table \[bcdha\] 