Although the telescope name is for historic reasons called HATCREEK, they are really the 6m BIMA antennae, but while this array was operational at the Hat Creek site in Northern California. The following UV variables were specificially used for this array, although some of them moved to CARMA as well:
atten(nants) cable(nants) corbit corbw(2) corfin(4) cormode coropt cortaper delay(nants) carma delay0(nants) dewpoint focus(nants) freqif ivalued(nants) lo1 carma lo2 phaselo1(nants) carma phaselo2(nants) carma phasem1(nants) carma rmspath carma srv2k(nants) tau230 carma temp(nants, ntemp themt(nants) tif2(nants) tpower(nants, ntpower) tsis(nants)