Abstract: Mapping the primordial cosmic microwave background (CMB) has proven to
be an unrivaled tool for learning about cosmic history over a wide range
of timescales. Measurements made to date have contributed greatly to
our current age of "precision cosmology", but future observations at
finer angular scales still promise new features. The epoch when massive
galaxy clusters formed can be probed through the Sunyaev-Zel'dovich
effect, while the immensely earlier era of inflation influences the same
maps through the slope of their spatial power spectrum. Gravitational
lensing of the CMB itself might even be within reach of current instruments.
The Atacama Cosmology Telescope (ACT) has just begun observing the
microwave sky at 140 through 280 GHz with over 3000 detectors. ACT
exemplifies many of the technical challenges involved in measuring sky
brightness with parts-per-million accuracy, along with the technical
advances from sites like NASA-Goddard and NIST that propel the latest
CMB experiments.