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\@writefile{toc}{\contentsline {section}{\numberline {A.}Project Description}{1}}
\@writefile{toc}{\contentsline {subsection}{\numberline {A.1}Overview}{1}}
\@writefile{toc}{\contentsline {subsection}{\numberline {A.2}Schematic of the NST}{1}}
\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces \relax \fontsize  {10}{12}\selectfont  \abovedisplayskip 10\p@ plus2\p@ minus5\p@ \abovedisplayshortskip \z@ plus3\p@ \belowdisplayshortskip 6\p@ plus3\p@ minus3\p@ \def \leftmargin \leftmargini \parsep 4.5\p@ plus2\p@ minus\p@ \topsep 9\p@ plus3\p@ minus5\p@ \itemsep 4.5\p@ plus2\p@ minus\p@ {\leftmargin \leftmargini \topsep 6\p@ plus2\p@ minus2\p@ \parsep 3\p@ plus2\p@ minus\p@ \itemsep \parsep }\belowdisplayskip \abovedisplayskip The NST equatorial mount, mirror cell, counterweights (for right ascension balance), and tower to secondary.???UPDATE???}}{2}}
\newlabel{FIG1A}{{2}{2}}
\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces \relax \fontsize  {10}{12}\selectfont  \abovedisplayskip 10\p@ plus2\p@ minus5\p@ \abovedisplayshortskip \z@ plus3\p@ \belowdisplayshortskip 6\p@ plus3\p@ minus3\p@ \def \leftmargin \leftmargini \parsep 4.5\p@ plus2\p@ minus\p@ \topsep 9\p@ plus3\p@ minus5\p@ \itemsep 4.5\p@ plus2\p@ minus\p@ {\leftmargin \leftmargini \topsep 6\p@ plus2\p@ minus2\p@ \parsep 3\p@ plus2\p@ minus\p@ \itemsep \parsep }\belowdisplayskip \abovedisplayskip Schematic of the 1.6\nobreakspace  {}m off-axis, open NST (top) and its optical layout (bottom). On the top part, the heat stop (HS) resides at the Gregorian focus with the SM mounted on a PI hexapod. The wavefront sensing system (WFS) resides immediately before M3 (along with the polarization optics for magnetic field measurements). M4 sends the light to the Coud\'e Room below. The HS, SM, M3 and M4 are not apparent in the figure. If M4 is flipped the light goes to the Nasmyth Bench where the spectrograph will reside (???REPLACE UPPER DRAWING WITH ONE HAVE A SCHEMATIC SPECTROGRAPH ON THE NASMYTH???) for which the light path is shown in red. This is where the first light observations occurred. The design was driven by competing needs for rigidity near the SM and an open light path. For more details, see \special {color push Blue}\relax $\@@underline {\hbox {\textit  {http://www.bbso.njit.edu/newtelescope}}}\mathsurround \z@ $\relax \special {color pop}.}}{3}}
\newlabel{FIG01}{{A.2}{3}}
\@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces \relax \fontsize  {10}{12}\selectfont  \abovedisplayskip 10\p@ plus2\p@ minus5\p@ \abovedisplayshortskip \z@ plus3\p@ \belowdisplayshortskip 6\p@ plus3\p@ minus3\p@ \def \leftmargin \leftmargini \parsep 4.5\p@ plus2\p@ minus\p@ \topsep 9\p@ plus3\p@ minus5\p@ \itemsep 4.5\p@ plus2\p@ minus\p@ {\leftmargin \leftmargini \topsep 6\p@ plus2\p@ minus2\p@ \parsep 3\p@ plus2\p@ minus\p@ \itemsep \parsep }\belowdisplayskip \abovedisplayskip A diffraction-limited image obtained on the NST at the Nasmyth focus (???NEED REAL FIGURE WITH R0 TO DEMONSTRATE KOLMOGOROV SEEING, ETC???).}}{3}}
\newlabel{FIG02}{{3}{3}}
\@writefile{toc}{\contentsline {subsection}{\numberline {A.3}Strehl Ratio of the Beam Feeding the Spectrograph}{3}}
\@writefile{toc}{\contentsline {subsection}{\numberline {A.4}Zeeman Splitting in the NIR}{4}}
\@writefile{toc}{\contentsline {subsection}{\numberline {A.5}Scientific Motivation: Photospheric and Chromospheric Magnetic Fields}{4}}
\@writefile{lot}{\contentsline {table}{\numberline {1}{\ignorespaces }}{5}}