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\@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 prime 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}}
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\@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}}
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\@writefile{toc}{\contentsline {subsection}{\numberline {A.5}Scientific Motivation: Photospheric and Chromospheric Magnetic Fields}{5}}
\@writefile{toc}{\contentsline {section}{\numberline {B.}Proposed Work}{6}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.1}Overview}{6}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.2}The CIRS Development Plan}{6}}
\@writefile{toc}{\contentsline {subsubsection}{\numberline {B.2.1}The Optical Design of CIRS}{6}}
\@writefile{toc}{\contentsline {subsubsection}{\numberline {B.2.2}Electronic, Computational and Mechanical Systems}{6}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.3}Performance Predictions}{6}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.4}Education and Research Training}{6}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.5}Data and Telescope Time}{7}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.6}Hardware and Personnel Budget}{7}}
\@writefile{toc}{\contentsline {subsection}{\numberline {B.7}Management Plan and Timelines}{7}}
\@writefile{lof}{\contentsline {figure}{\numberline {4}{\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 Gantt Chart shows the AO-308 project schedule. The chart is ``rolled-up'' because it is so detailed and would be hard to read. A complete version showing the tasks with each summary unrolled appears in the ``Supplementary Documents'' section, along with a vertical flow version of the full Gantt chart that is shown there.}}{8}}
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