\relax \@writefile{toc}{\contentsline {section}{\numberline {1}Executive Summary}{2}} \newlabel{executive}{{1}{2}} \@writefile{toc}{\contentsline {section}{\numberline {2}Introduction}{4}} \newlabel{intro}{{2}{4}} \@writefile{toc}{\contentsline {section}{\numberline {3}Project Status and Management}{4}} \newlabel{status}{{3}{4}} \@writefile{toc}{\contentsline {section}{\numberline {4}Toward a Japanese Participation}{5}} \newlabel{3way}{{4}{5}} \@writefile{toc}{\contentsline {section}{\numberline {5}Charges from the ACC to the ASAC}{5}} \newlabel{charges_to_asac}{{5}{5}} \@writefile{toc}{\contentsline {subsection}{\numberline {5.1}Site Statistics and Stringency}{5}} \newlabel{stringency}{{5.1}{5}} \@writefile{toc}{\contentsline {subsection}{\numberline {5.2}Early Science}{6}} \newlabel{earlyscience}{{5.2}{6}} \@writefile{toc}{\contentsline {subsection}{\numberline {5.3}Configuration Issues and The Long Baseline Array Geometry}{7}} \newlabel{configuration}{{5.3}{7}} \@writefile{toc}{\contentsline {subsection}{\numberline {5.4}Enhancements}{8}} \newlabel{enhancements}{{5.4}{8}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {5.4.1}Prioritization of the ALMA enhancements}{8}} \newlabel{prioritization}{{5.4.1}{8}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {5.4.2}Japanese proposal for the ALMA enhancements}{8}} \newlabel{japan_proposal}{{5.4.2}{8}} \@writefile{toc}{\contentsline {section}{\numberline {6}Receivers}{8}} \newlabel{receivers}{{6}{8}} \@writefile{toc}{\contentsline {section}{\numberline {7}Prototype Antennas}{9}} \newlabel{antenna}{{7}{9}} \@writefile{toc}{\contentsline {section}{\numberline {8}Software}{9}} \newlabel{software}{{8}{9}} \@writefile{toc}{\contentsline {section}{\numberline {9}Calibration}{10}} \newlabel{calibration}{{9}{10}} \@writefile{toc}{\contentsline {section}{\numberline {10}Correlator}{11}} \newlabel{correlator}{{10}{11}} \@writefile{toc}{\contentsline {section}{\numberline {11}Summary}{13}} \newlabel{Summary}{{11}{13}} \@writefile{toc}{\contentsline {section}{\numberline {A}Report of the ASAC Subcommittee on Site and Stringency}{15}} \newlabel{Site_and_Stringency}{{A}{15}} \@writefile{toc}{\contentsline {subsection}{\numberline {A.1}Introduction}{15}} \newlabel{SS_intro}{{A.1}{15}} \@writefile{toc}{\contentsline {subsection}{\numberline {A.2}Examples of Observations}{16}} \newlabel{SS_examples}{{A.2}{16}} \@writefile{toc}{\contentsline {subsection}{\numberline {A.3}Site Characteristics}{17}} \newlabel{SS_site}{{A.3}{17}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {A.3.1}Background}{17}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {A.3.2}Phase Fluctuations and Seeing}{17}} \@writefile{lot}{\contentsline {table}{\numberline {1}{\ignorespaces stability}}{18}} \newlabel{tab:stability}{{1}{18}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {A.3.3}Correlations}{18}} \@writefile{toc}{\contentsline {subsection}{\numberline {A.4}Phase correction schemes}{19}} \@writefile{toc}{\contentsline {subsubsection}{\numberline {A.4.1}Fast switching}{19}} \@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Cumulative distributions of the 225\,GHz zenith optical depths ($\tau _{225}$) measured at Chajnantor, at Mauna Kea (CSO), and at the South Pole. 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The 240 min interval suffers from a processing defect.}}{39}} \newlabel{fig:tau225-median}{{12}{39}} \@writefile{lof}{\contentsline {figure}{\numberline {13}{\ignorespaces Cumulative distributions of the maximum 225\,GHz zenith optical depths ($\tau _{225}$) measured at Chajnantor in 1996 for different sampling intervals. The 240 min interval suffers from a processing defect.}}{40}} \newlabel{fig:tau225-maximum}{{13}{40}} \@writefile{lof}{\contentsline {figure}{\numberline {14}{\ignorespaces Cumulative distributions of the maximum 11.2 GHz phase fluctuations measured at Chajnantor in 1996 for different sampling intervals. The 240 min interval suffers from a processing defect.}}{41}} \newlabel{fig:phase-maximum}{{14}{41}} \@writefile{lof}{\contentsline {figure}{\numberline {15}{\ignorespaces Joint probability distribution of $\tau (225)$ and $\phi (rms)$ with a very loose wind (pointing) requirement: that the wind speed be less than 100 m/s either day or night. 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