“…These innovations resulted in total noise within a factor of 3 of the standard quantum limit, and an exclusion limit |g γ | 2.3 × g KSVZ γ over a 100 MHz frequency range. Further operation of this detector in the next few years will extend this frequency coverage significantly, and ongoing cavity and amplifier development [17,25] may even enable us to push down to KSVZ sensitivity. This work was supported by the National Science Foundation, under grants PHY-1362305 and PHY-1306729, by the Heising-Simons Foundation under grants 2014-181, 2014-182, and 2014-183, and by the U.S. Department of Energy through Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344.…”