As of 14 August there are 39 antennas at the ALMA AOS. Recent deliveries have included: DA50, relocated to the AOS Pad A045, AIV delivery #42, DA48, relocated to the AOS Pad A046, AIV delivery #43, and DA49, relocated to the AOS Pad A029, AIV delivery #44. There is a webcam on DA41 which provides an inside-the-array realtime view ( http://www.alma.cl/cams/da41/) from pad A003. Three conditional acceptances have occurred recently, for DV23, DA53 and CM12. DV23 will be relocated from the Vertex camp to the OSF Technical Facility, on Sunday, where it will join DA53, DV22, CM12, CM09, DV07, and DV06. With 39 antennas, the 32 inputlimits of the dual quadrant correlator have been surpassed. Work continues on the ACA correlator (there are 11 antennas in the ACA currently). The correlator will be shut down on 3 September for reconfiguration to its final four quadrant configuration. Stations out to 5km are delivered but acceptance awaits connection to the Permanent Power Supply (PPS). The permanent power system is necessary in order to use any pads outside the present configuration. Commissioning of larger, cycle 1 configurations, awaits implementation of the PPS. On the receiver from, production of the Band 6 cartridges is finishing. NA FEIC delivery 20, of FE057, has been made; that FE was shipped 8 Aug. There are a number of deficiencies in the cartridge area in the antennas at the AOS, which are being addressed--25 are fully available for B3, B7 and B9. There is an AIV+ plan for installation of the Band 4, 8 and 10 cartridges which are not in Front Ends in Chile at the OSF. Computing reports progress in the bulk data implementation, with successful tests on the OSF Interferometer, to be repeated today at the AOS. A precise acceptance plan for R9.1.0 to allow restart of Cycle 0 observation on 3 October is currently being developed. Analysis of Cycle 1 proposal submission last-(15)minute problem suggests its cause to be mostly configuration, although memory use is not entirely understood. Early Science Block 21 has been progressing quite well and is benefiting from the good weather (for example, Monday night Weather: pwv 0.4-1.1 mm, wind 6 m/s; several B9 projects were run), despite a range of problems, including lost data and power breakdowns. As many as 25 12m antennas have operated in the array on occasion. Observations of objects that required the compact configuration have been resumed, though the spacings available do not quite mimic those in the compact configuration advertised for Cycle 0. CSV has been focused on the ACA commissioning and software testing. SV data has been acquired for new targets: RXCJ1347-1145 (Band 3 continuum) and Mars (Bands 3, 6 and 7, methane lines) while data reduction on these and previously observed targets (HD163296, Io, Uranus, Arp220) is ongoing.