% GEMPHASE1_US13B.STY -- NOAO/Gemini observing proposal form.

% First, identifying information about this style file.

\def\revtex@ver{1.02}		% Version number of this file.
\def\revtex@date{15 Aug 12}	% Revision date.
\def\revtex@author{DJB/KAO}	% This file's author.
\def\revtex@org{NOAO/Gemini}		% Sponsoring organization.
\def\revtex@genre{observing proposal}	% Document "type".

% \ifundefined sequence
\def\ifundefined#1{\expandafter\ifx\csname#1\endcsname\relax}

% maximum number of Co-Investigators to print.
% can be changed in form, e.g. \setmaxnumcois{10}
\newcount\maxnumcois \maxnumcois=6
\def\setmaxnumcois#1{\gdef\maxnumcois{#1}}

%
\def\geminidata#1#2{}{}


\def\revtex@pageid{\xdef\@thefnmark{\null}
    \@footnotetext{\revtex@org\space
    \revtex@genre\space \LaTeX\ macros v\revtex@ver.}}

\let\ltx@enddoc=\enddocument
\def\enddocument{\vfill\revtex@pageid\ltx@enddoc}

% Page design/layout macros.  Page sizes are at the end of the file.

\def\baselinestretch{0.98}	% Tighten up baselines a little.

\def\ps@kpprophead{\def\@oddfoot{}\def\@evenfoot{}
    \def\@oddhead{\hbox to\textwidth{\small\sl \prop@phead
	\ifx\@empty\@rcptdate\phantom{, received Dec 31 1999}
        \else, received \@rcptdate\fi
	\hfill Section 2.Page \thepage
        \hfill \prop@pidbox}}\let\@evenhead\@oddhead
    \def\chaptermark##1{\markright {{\ifnum \c@secnumdepth>\m@ne
	\@chapapp\ \thechapter. \ \fi ##1}}}}


\def\prop@idbox{ \ifx\@empty\@propid{
	\hfill\phantom{\framebox[1.7in][c]{\LARGE\bf/}}
    }\else{
	\hfill\framebox[1.7in][c]{\LARGE\bf \@propid/\@sciencecategorynum }
    }\fi
}

\def\prop@oldidbox{ \ifx\@empty\@oldpropid{
	\phantom{\framebox[2.2in][c]{\bf/}}
    }\else{
	\framebox[2.2in][c]{\bf Resubmission of \@oldpropid }
    }\fi
}


\def\prop@pidbox{ \ifx\@empty\@propid{
	\hfill\framebox[1.2in][c]{{\small\sl\ This box blank.}
        \phantom{\large\bf/}}
    }\else{
	\hfill\framebox[1.2in][c]{\large\bf \@propid/\@sciencecategorynum}
    }\fi
}

\def\@thesistrue{Y}
\def\@issurvey{Survey}

\def\prop@info{\begin{tabbing}
    % first line
    \hbox to.34\textwidth{\large\bf\prop@head\hfill}%
    \hbox to.30\textwidth{%
	\ifx\@proposaltype\@empty{\hfill}%
	\else{\hfill{\it \@proposaltype\ proposal}\hfill}\fi}%
    \hbox to.36\textwidth{%
        {\bf Panel:} \hspace{0.21in} 
	\ifx\@panelassignment\@empty{\instruct@font For office use.}%
	\else{\@panelassignment}\fi%
	\hfill}%
    \\

    % second line
    \hbox to.34\textwidth{%
	\ifx\@rcptdate\@empty{\it Date:\/} \today%
	\else{Date received:} \@rcptdate\fi\hfill}%
    \hbox to.30\textwidth{%
    	\ifx\@thesis\@thesistrue{\hfill{\it Thesis}\hfill}%
	\else{\hfill}\fi}%
    \hbox to.36\textwidth{{\bf Category:} \@sciencecategory\hfill}%
\end{tabbing}}


\def\ques@font{\it}
\def\instruct@font{\small\sl}

% Proposal ID and receipt date will be filled in at NOAO.
%
%    \proposalid{NUMBER}
%    \received{DATE}

\def\received#1{\gdef\@rcptdate{#1}} \received{}
\def\proposalid#1{\gdef\@propid{#1}} \proposalid{}
\def\pastid#1{\gdef\@oldpropid{#1}} \pastid{}
\def\observatory#1{\gdef\@observatory{#1}} \observatory{}
\def\proposaltype#1{\gdef\@proposaltype{#1}} \proposaltype{}
\def\thesis#1{\gdef\@thesis{#1}} \thesis{}
\def\sciencecategory#1{\gdef\@sciencecategory{#1}} \sciencecategory{}
\def\sciencecategorynum#1{\gdef\@sciencecategorynum{#1}} \sciencecategorynum{}
\def\panelassignment#1{\gdef\@panelassignment{#1}} \panelassignment{}

% Below is the markup that the observing team needs to supply.
% Instructions for filling in the form using these commands are in
% a template proposal form file as LaTeX comments.

\def\prop@head{NOAO/Gemini Observing Proposal}
\def\prop@phead{NOAO/Gemini Proposal}

\def\title#1{
    \vspace*{-6\headheight}\prop@oldidbox  \prop@idbox
    \vspace*{0.5in}
    \prop@info\par
    \vspace*{0.1in}
    \def\@savetitle{#1}\ifx\@empty\@savetitle
    \makebox[\textwidth]{\Large{\bf TITLE:} \hrulefill}\par
    \makebox[\textwidth]{\hrulefill}\par
    \else{\LARGE\bf\@savetitle}\fi
}
    

\def\abstract{\par\vspace{0ex}\vbox to2.50in\bgroup\noindent
{\bf Abstract of Scientific Justification}
{\small\sl (will be made publicly available for accepted proposals)}{\bf :}\\
\parindent\z@}
\let\ltx@endabstract=\endabstract
\def\endabstract{\ltx@endabstract\vfil\egroup\vspace{\fill}}

% Observer identification.  These items are buffered so that they can be
% specified in any order, subject only to the restriction that the observer
% name be given first.  The same commands are used to identify the PI as
% well as the co-investigators; the formatting is controlled separately,
% and differences arise in the use of LaTeX environments, below.
%
% Each member of the observing team is identified with several bits of
% information.
%
%    \name{OBSERVER NAME}
%    \affil{AFFILIATION}
%    \address{POSTAL ADDRESS}
%    \email{EMAIL ADDRESS}
%    \phone{TELEPHONE NUMBER}
%    \fax{FAX NUMBER}
%    \invstatus{P, T, G, U, or O}
%
% Note that the fax number does not print on the form.  There is not
% enough room on the cover page the way it is currently laid out.

\def\name#1{\gdef\obs@name{#1}}
\def\affil#1{\gdef\obs@affil{#1}}
\def\department#1{\gdef\obs@department{#1}}
\def\address#1{\gdef\obs@address{#1}}
\def\citycode#1{\gdef\obs@citycode{#1}}
\def\city#1{\gdef\obs@city{#1}}
\def\state#1{\gdef\obs@state{#1}}
\def\zipcode#1{\gdef\obs@zipcode{#1}}
\def\country#1{\gdef\obs@country{#1}}
\def\email#1{\gdef\obs@email{#1}}
\def\phone#1{\gdef\obs@phone{#1}}
\def\fax#1{\gdef\obs@fax{#1}}
\def\invstatus#1{\gdef\obs@invstatus{#1}}

\def\clear@obs{	\gdef\obs@name{} \gdef\obs@affil{} \gdef\obs@department{}
		\gdef\obs@address{} \gdef\obs@citycode{} \gdef\obs@city{} 
		\gdef\obs@state{} \gdef\obs@zipcode{} \gdef\obs@country{} 
		\gdef\obs@email{}  \gdef\obs@phone{}
		\gdef\obs@fax{} \gdef\obs@invstatus{} }

% Formatting of PI and CO-I data are controlled by the next two macros.

% Now here is some dicey stuff.  We want to solve a variety of problems with
% one form and one set of macros, stemming from the need to print rational
% forms, whether or not anything has been filled in electronically.  In
% other words, if somebody runs a *blank* electronic form through LaTeX,
% a usable form should emerge from the laser printer, with blanks in the
% appropriate places, etc.  If the form is filled in electronically, the
% rules should be replaced with the stuff the user fills in.
%
% Fine.  Except that real estate on the first page is quite limited, and
% we also need a way of letting the user who fills in information with the
% editor know when he/she is being verbose.  We achieve this by forcing
% certain pieces of information into boxes of fixed size.  These contain
% either an \hrulefill, or text supplied by the author.  If too much text
% is provided, TeX will complain about the overfull hbox.

\def\yn@rule{\rule{0.3in}{0.4pt}}


\def\prt@invline{
    \hbox to.35\textwidth{\obs@tag\space%
	\ifx\@empty\obs@name\hrulefill\space\else\obs@name\hfill\fi}%
    \hbox to.14\textwidth{{\bf Status:}\space%
	\ifx\@empty\obs@invstatus\hrulefill\else\obs@invstatus\fi\hfill}%
    \hbox to.51\textwidth{{\bf Affil.:}\space%
	\ifx\@empty\obs@affil\hrulefill\else\obs@affil\hfill\fi}
}

\def\prt@piblock{\begin{tabbing}
    % first line
    \prt@invline
    \\

    % second line
    \hbox to1.00\textwidth{%
	\def\@blankadd{1}%
	\ifx\@empty\obs@department\else\def\@blankadd{0}\fi
	\ifx\@empty\obs@address\else\def\@blankadd{0}\fi
	\ifx\@empty\obs@city\else\def\@blankadd{0}\fi
	\ifx\@empty\obs@state\else\def\@blankadd{0}\fi
	\ifx\@empty\obs@zipcode\else\def\@blankadd{0}\fi
	\ifx\@empty\obs@country\else\def\@blankadd{0}\fi
	\ifnum\@blankadd=1
	    {\bf Address:\hrulefill}%
	\else
	    \obs@department\ifx\@empty\obs@department\else,\space\fi
	    \obs@address\ifx\@empty\obs@address\else,\space\fi
	    \obs@citycode\ifx\@empty\obs@citycode\else\space\fi
	    \obs@city\ifx\@empty\obs@city\else,\space\fi
	    \obs@state\space\obs@zipcode\space\obs@country\hfill
        \fi}
    \\

    % third line
    \hbox to.46\textwidth{%
	Email:\space%
	\ifx\@empty\obs@email\hrulefill\else\obs@email\hfill\fi}%
    \hbox to.54\textwidth{%
	\space\space%
	Phone:\space%
	    \ifx\@empty\obs@phone\hrulefill\else\obs@phone\hfill\fi%
	\space\space%
	FAX:\space%
	    \ifx\@empty\obs@fax\hrulefill\else\obs@fax\fi}%
    \\
    \\

    % separator
    \hbox to1.0\textwidth{\hfill\rule[10pt]{4.5in}{0.01in}\hfill}%
    \end{tabbing}}

\def\prt@coiblock{\begin{tabbing}\prt@invline\end{tabbing}}
\def\prt@xcoiblock{\marginpar{\tiny\obs@name}}

% Principal investigator and co-investigator environments.

% Note that after the first three CoI blocks, I quit printing the CoI
% information.  This is not especially nice.  It would be better if the
% names (and possibly the grad student status) of the additional CoIs
% were listed on the proposal form someplace.  Since the cover page is
% so full at this point, my sense is that these would have to be collected
% into end notes somehow.  This would be hard to program, and so it should
% be deemed a very necessary requirement.  Perhaps some other display
% format would be acceptable, one that would require less programming.

\newcounter{CoI}
\def\obs@tag{{\bf CoI:}}

\newenvironment{PI}{\clear@obs}{\def\obs@tag{{\bf PI:}}\prt@piblock}

\newenvironment{CoI}{\clear@obs\stepcounter{CoI}}{\ifnum\c@CoI>\maxnumcois
    \prt@xcoiblock\else\vspace*{-6.3ex}\prt@coiblock\fi}

%

\def\chk@setblank#1{\def\@kptmpa{#1}\ifx\@empty\@kptmpa
    \def\@kptmpa{\yn@rule}\fi\mbox{\@kptmpa}}

\def\chk@setblankline#1{\def\@kptmpa{#1}\ifx\@empty\@kptmpa
    \def\@kptmpa{\rule{\textwidth}{0.4pt}}\fi
    \par\makebox[\textwidth][l]{\@kptmpa}}


\def\undates@head {{\bf Scheduling constraints and non-usable dates} %
{\it (up to four lines).}}

\def\unusabledates#1{\undates@head\par\def\@kptmpa{#1}
    \ifx\@empty\@kptmpa{\par
	\makebox[\textwidth]{\hrulefill}
	\makebox[\textwidth]{\hrulefill}
	\makebox[\textwidth]{\hrulefill}
	\makebox[\textwidth]{\hrulefill}\par}
    \else{
	\@kptmpa
    }\fi
}



\def\ra@head {{\par\bf R.A. range of principal targets (hours): }}
\def\dec@head {{\par\bf Dec. range of principal targets (degrees): }}
%\def\pid@head {{\par\bf Previous ID of this observing proposal: }}

\def\targetsra#1{\ra@head #1}
\def\targetsdec#1{\dec@head #1}
%\def\pastid#1{\pid@head #1}

\def\pp@head {{\par\bf Proprietary Period: }}
\def\proprietaryperiod#1{\pp@head #1}

\def\btyn@head {{\par\bf Consider for Band 3? }}
\def\bandthreeyn#1{\btyn@head #1}

\def\classicalyn@head {{\par\bf Request Classical Observing? }}
\def\classical#1{\classicalyn@head #1}


% Observing run environment.  This is used to describe observing parameters
% in a very succinct manner, to be presented in an abbreviated form on the
% first page.  I have chosen to use multiple \begin{obsrun}-\end{obsrun}
% groupings, as opposed to a repeating set of parameter identifying macros.

\newcounter{obsrun}
\newenvironment{obsrun}{\stepcounter{obsrun}}%
    {\ifnum\c@obsrun=6\par\prt@obsruns\par\fi}

% Observing run parameters to be specified by the investigators.
%
%   \telesope{IDENT}
%   \instrument{IDENT(S)}
%   \numnights{NUMBER}
%   \lunardays{NUMBER}
%   \optimaldates{RANGE}
%   \acceptabledates{RANGE}

% These are pretty amazing-looking.  They are fake "arrays", actually.

\def\telescope#1{\global\@namedef{obs\@Alph{\c@obsrun}@telid}{#1}}
\def\instrument#1{\global\@namedef{obs\@Alph{\c@obsrun}@inst}{#1}}
\def\numnights#1{\global\@namedef{obs\@Alph{\c@obsrun}@numnights}{#1}}
\def\lunardays#1{\global\@namedef{obs\@Alph{\c@obsrun}@lunardays}{#1}}
\def\optimaldates#1{\global\@namedef{obs\@Alph{\c@obsrun}@optdates}{#1}}
\def\acceptabledates#1{\global\@namedef{obs\@Alph{\c@obsrun}@accdates}{#1}}

\def\obsrun@head{Summary of observing runs requested for this project}
\def\orth@font{\small}

\def\prt@obsruns{\begin{center}{\bf\obsrun@head}\\[1ex]
    \setcounter{obsrun}{1}
    \begin{tabular}{|c||l|l|c|c|c|c|}
    \multicolumn{1}{c}{\orth@font Run} &
    \multicolumn{1}{c}{\orth@font Telescope} &
    \multicolumn{1}{c}{\orth@font Instrument} &
    \multicolumn{1}{c}{\orth@font No. Nights} &
    \multicolumn{1}{c}{\orth@font Moon} &
    \multicolumn{1}{c}{\orth@font Optimal months} &
    \multicolumn{1}{c}{\orth@font Accept. months}\\
    \hline
    1 & \obsA@telid & \obsA@inst & \obsA@numnights & 
    \obsA@lunardays & \obsA@optdates & \obsA@accdates\\
    \hline
    2 & \obsB@telid & \obsB@inst & \obsB@numnights & 
    \obsB@lunardays & \obsB@optdates & \obsB@accdates\\
    \hline
    3 & \obsC@telid & \obsC@inst & \obsC@numnights & 
    \obsC@lunardays & \obsC@optdates & \obsC@accdates\\
    \hline
    4 & \obsD@telid & \obsD@inst & \obsD@numnights & 
    \obsD@lunardays & \obsD@optdates & \obsD@accdates\\
    \hline
    5 & \obsE@telid & \obsE@inst & \obsE@numnights & 
    \obsE@lunardays & \obsE@optdates & \obsE@accdates\\
    \hline
    6 & \obsF@telid & \obsF@inst & \obsF@numnights & 
    \obsF@lunardays & \obsF@optdates & \obsF@accdates\\
    \hline
    \end{tabular}
    \end{center}}


% The scientific justification and the proposed observing program are
% typeset (printed) as they are specified by the author.  Specific
% observations are summarized in the "obsrun" environment (above).
%
%    \sciencejustification
%    \expdesign
%    \otherfacilities
%    \manplan
%    \whyctio
%    \thepast

\newenvironment{references}{\subsubsection*{References}}{\relax}
\let\reference=\par

\def\propsection{\@startsection{section}{1}{\z@}
    {7pt plus 4pt minus 2pt}{-1em}{\normalsize\bf}}
\def\subsection{\@startsection{subsection}{2}{\z@}
    {-3.25ex plus -1ex minus -.2ex}{1.5ex plus .2ex}{\normalsize\bf}}

\def\justif@head{{\instruct@font Be sure to include overall significance
    to astronomy. For standard proposals limit text to one page with 
    figures, 
    captions and references on no more than two additional pages.\par}}

\def\feas@head{{\instruct@font 
\ifx\@proposaltype\@issurvey{
    Describe the survey experimental design and the observations planned 
    in detail.  Justify choice of telescope, instrument, and sensitivity 
    goals in terms of the survey science goals.  A key part of the survey 
    proposal process is to justify the total duration of the program both 
    in terms of the number of nights and the number and distribution of 
    observing runs required.  Please show explicitly how on-target exposure 
    time, setup, and calibration requirements determine these parameters. 
    {\it Please do not include any allowance for bad weather.} Based on a 
    clear understanding of your observational strategy as outlined in 
    this section, we will evaluate the need for augmenting the allocation 
    to allow for bad weather.}
\else{
    Describe your overall observational program.
    How will these observations contribute toward the accomplishment
    of the goals outlined in the science justification?
    If you've requested long-term status, justify why this is necessary
    for successful completion of the science. 
    (Limit text to one page)}\fi
}\par}




\def\mplan@head{{\instruct@font
Describe the overall organizational plan for conducting the proposed survey,
including data reduction and analysis, preparation of survey deliverables,
and staffing requirements.
List the roles and responsibilities of the Co-Is with their anticipated time commitments directed to achieving the goals of the survey. 
You may also wish to detail external sources
of support that will be used in the program.  Please detail any use
of non-NOAO observational facilities that are required to achieve the
overall goals of the survey program.
    \par}}

\def\ofac@head{{\instruct@font (1) Describe how the proposed observations 
    complement data from
    non-Gemini facilities, including those available through NOAO.  For each of these other facilities, indicate 
    the nature of the observations (yours or those of others), and 
    describe the importance of the observations proposed here in the 
    context of the entire program. (2) Do you currently have a grant 
    that would provide resources to support the data processing, analysis, 
    and publication of the observations proposed here?
    \par}}

\def\whyctio@head{{\instruct@font (For CTIO proposals only.)
    Explain why access to the southern hemisphere is needed to achieve your
    scientific goals.\par}}

\def\dataacc@head{{\instruct@font  Describe the data products (reduced 
observations, single or stacked images, spectra, object catalogues, and 
so on) to be releases, as well as the timeline and mechanism of their 
release to the community.  Please differentiate between intermediate 
products  developed during the execution of the survey versus the 
final products likely to be produced after the full observations 
have been obtained.\par}}

\def\ltd@head{{\instruct@font If you are requesting long term status, 
    list the observing runs (telescope, instrument, number of nights) 
    requested in subsequent semesters to complete the project. 
    \par}}

\def\specreq@head{{\instruct@font Describe briefly any special or 
    non-standard usage of instrumentation.\par}}

\def\techjust@head{{\instruct@font Describe the observations to be made during
    this observing run.  Justify the specific telescope, the exposure times, and the constraints requested (seeing, cloud cover, sky brightness, and, if appropriate, water vapor and airmass limit).\par}}

\def\sched@head{{\instruct@font If there are scheduling constraints or non-usable dates for your program, please describe below.  Note that you do not need to list all dates that meet your observing condition requirements; only list scheduling constraints that you think merit special attention from the queue or classical schedule coordinator. \par}}

\def\bandthreeplan@head{{\instruct@font  If applying for queue time and it is acceptable for the proposal to be scheduled in Band 3, describe the changes to be 
made to allow it to be successful in Band 3 (limit text to half a page).  Band 3 observations are used to fill the queue when no Band 1 or 2 programs are available.  Successful Band 3 programs generally use poorer than median observing conditions, have targets away from the most popular regions of the sky, do not require strict timing or other constraints, and do not require special instrument configurations.   \par}}

\def\classicalbackup@head{{\instruct@font If applying for classically scheduled time, describe the program you will pursue should the weather be worse than the requested observing conditions (limit text to half a page).   \par}}

\def\justifyduplications@head{{\instruct@font If your targets have been previously observed by Gemini using similar or identical setups to those proposed here, justify the duplication below.  Duplicate observations can be identified through a search of the Gemini Science Archive.\par}}

\def\past@head{{\instruct@font List allocations of telescope time on 
    facilities available through NOAO to the PI during the last 2 years 
    for regular proposals, and at any time in the past for survey proposals 
    (including participation of the PI as a Co-I on previous NOAO surveys), 
    together with the current status of the data (cite publications where 
    appropriate).  Mark with an asterisk those allocations of time related 
    to the current proposal.  Please include original proposal semesters 
    and ID numbers when available.\par}}

\def\sciencejustification{\newpage\propsection{\fbox{Scientific Justification}}
    \justif@head}
\def\expdesign{\newpage\propsection{\fbox{Experimental Design}}\feas@head}
%\def\sexpdesign{\newpage\propsection{\fbox{Experimental Design}}\sfeas@head}
\def\manplan{\vfill\propsection{\fbox{Management Plan}}\mplan@head}
\def\otherfacilities{\vfill\propsection{\fbox{Use of Other Facilities or Resources}}\ofac@head}
\def\longtermdetails{\vfill\propsection{\fbox{Long-term Details}}\ltd@head}
\def\dataaccess{\vfill\propsection{\fbox{Release of Data}}\dataacc@head}
\def\whyctio{\vfill\propsection{\fbox{Why CTIO?}}\whyctio@head}
\def\specialrequest{\propsection{\fbox{Special Instrument Requirements}}
    \specreq@head}
\def\thepast{\vfill\propsection{\fbox{Previous Use of NOAO Facilities}}
    \past@head}
\def\technicaldescription{\newpage\propsection{\fbox{Technical Description}}
    \techjust@head}
\def\scheduling{\propsection{\fbox{Scheduling Constraints}}
    \sched@head}
\def\bandthreeplan{\propsection{\fbox{Band 3 Plan}}
    \bandthreeplan@head}
\def\classicalbackup{\propsection{\fbox{Classical Backup Program}}
    \classicalbackup@head}
\def\justifyduplications{\propsection{\fbox{Justify Target Duplications}}
    \justifyduplications@head}

\def\relatedwork#1{\fbox{$\star$}\space#1}


% RUN DETAILS PAGE

\def\cleart@obsi {
    \gdef\obs@filters{} \gdef\obs@grating{} \gdef\obs@order{} 
    \gdef\obs@crossdisperser{} \gdef\obs@slit{} \gdef\obs@multislit{}
    \gdef\obs@wstart{} \gdef\obs@wend{} \gdef\obs@cable{} 
    \gdef\obs@corrector{} \gdef\obs@collimator{} \gdef\obs@adc{}
    \gdef\obs@dispersers{} \gdef\obs@focalplaneunits{}
    \gdef\obs@adaptiveoptics{} \gdef\obs@cameras{}
    \gdef\obs@disperserorders{} \gdef\obs@polarimetry{}
    
}

\def\filters#1{\gdef\obs@filters{#1}}
\def\grating#1{\gdef\obs@grating{#1}}
\def\order#1{\gdef\obs@order{#1}}
\def\crossdisperser#1{\gdef\obs@crossdisperser{#1}}
\def\slit#1{\gdef\obs@slit{#1}}
\def\multislit#1{\gdef\obs@multislit{#1}}
\def\wstart#1{\gdef\obs@wstart{#1}}
\def\wend#1{\gdef\obs@wend{#1}}
\def\cable#1{\gdef\obs@cable{#1}}
\def\corrector#1{\gdef\obs@corrector{#1}}
\def\collimator#1{\gdef\obs@collimator{#1}}
\def\adc#1{\gdef\obs@adc{#1}}
\def\adaptiveoptics#1{\gdef\obs@adaptiveoptics{#1}}
\def\cameras#1{\gdef\obs@cameras{#1}}
\def\dispersers#1{\gdef\obs@dispersers{#1}}
\def\focalplaneunits#1{\gdef\obs@focalplaneunits{#1}}
\def\cameras#1{\gdef\obs@cameras{#1}}
\def\disperserorders#1{\gdef\obs@disperserorders{#1}}
\def\polarimetry#1{\gdef\obs@polarimetry{#1}}

\def\runid#1#2{
    \vfill
    \newpage
    \begin{center}
    {\large\bf Observing Run Details for Run #1: #2}
    \end{center}
}

\def\ic@font{\footnotesize}
\def\gic@font{\bf}
\newenvironment{configuration}{\cleart@obsi}{
    \vfill
    \footnotesize
    \begin{center}\fbox{\large\bf Instrument Configuration}\end{center}
    \begin{tabbing}
    \hbox to0.35\textwidth{{\ic@font Filters: }\obs@filters\hfill}
    \hbox to0.30\textwidth{{\ic@font Slit: }\obs@slit\hfill}
    \hbox to0.35\textwidth{{\ic@font Fiber cable: }\obs@cable\hfill}
    \\
    \hbox to0.35\textwidth{{\ic@font Grating/grism: }\obs@grating\hfill}
    \hbox to0.30\textwidth{{\ic@font Multislit: }\obs@multislit\hfill}
    \hbox to0.35\textwidth{{\ic@font Corrector: }\obs@corrector\hfill}
    \\
    \hbox to0.35\textwidth{{\ic@font Order: }\obs@order\hfill}
    \hbox to0.30\textwidth{{\ic@font $\lambda_{start}$: }
	\obs@wstart\hfill}
    \hbox to0.35\textwidth{{\ic@font Collimator: }\obs@collimator\hfill}
    \\
    \hbox to0.35\textwidth{{\ic@font Cross disperser: }
	\obs@crossdisperser\hfill}
    \hbox to0.30\textwidth{{\ic@font $\lambda_{end}$:\hspace{4pt} }
	\obs@wend\hfill}
    \hbox to0.35\textwidth{{\ic@font Atmos.~disp.~corr.: }
	\obs@adc\hfill}
    \end{tabbing}
    \vfill
}

\def\@bandthreetrue{Y}
\def\gembandthree#1{\gdef\@gembandthree{#1}}
\def\gbtnumhours#1{\gdef\@gbtnumhours{#1}}
\def\gbtimagequality#1{\gdef\@gbtimagequality{#1}}
\def\gbtskybackground#1{\gdef\@gbtskybackground{#1}}
\def\gbtwatervapor#1{\gdef\@gbtwatervapor{#1}}
\def\gbtcloudcover#1{\gdef\@gbtcloudcover{#1}}
\def\gbtcomment#1{\gdef\@gbtcomment{#1}}

\newenvironment{resources}{\cleart@obsi}{

    \vfill
    \begin{center}\fbox{\large\bf Band 3 Information}\end{center}
	\medskip
	{\bf Consider for Band 3?}  ~~~\@gembandthree\\\mbox{}
     	\ifx\@gembandthree\@bandthreetrue{ 

	{\bf Minimum required time for a useable band 3 allocation:}
		~~~~\@gbtnumhours\\\mbox{}

	{\bf Use the following conditions for band 3 only:}\\\mbox{}
	{\bf Image Quality:}~\@gbtimagequality \hfill
	{\bf Sky Background:}~\@gbtskybackground \hfill
	{\bf Water Vapor:}~\@gbtwatervapor \hfill
	{\bf Cloud Cover:}~\@gbtcloudcover\\\mbox{}

	{\bf Band 3 Consideration Comments (50 words):\hfill}\\\mbox{}
	\@gbtcomment

	}
	\else
	\fi

    \vfill
    \footnotesize
    \begin{center}\fbox{\large\bf Instrument Resources}\end{center}
    {\gic@font AO: }\obs@adaptiveoptics\\
    {\gic@font Cameras: }\obs@cameras\\
    {\gic@font Filters: }\obs@filters\\
    {\gic@font Dispersers: }\obs@dispersers\\
    {\gic@font Disperser Orders: }\obs@disperserorders\\
    {\gic@font Focal Plane Units: }\obs@focalplaneunits\\
    {\gic@font Polarimetry: }\obs@polarimetry
    \vfill
}


\def\obs@head{Target Table for \@nameuse{instrname@\@instrid}}

\def\@instrid{default}
\newenvironment{targettable}[1]{\cleart@obst%
    \def\@instrname{#1}\def\obs@list{}}%
    {\vfill\pagebreak[3]\begin{center}\small\bf\obs@head\\[1.8ex]%
    \footnotesize\tabcolsep2\p@%
    \nopagebreak[4]\samepage%
    \begin{tabular}{\@nameuse{pream@default}}%
    \@nameuse{obshead@\@instrid}\\\hline\\[-1.8ex]%
    \obs@list\end{tabular}\end{center}}

\newenvironment{geminitargettable}[1]{\cleart@gobst%
    \def\@instrname{#1}\def\gobs@list{}}%
    {\vfill\pagebreak[3]\begin{center}\small\bf\obs@head\\[1.8ex]%
    \footnotesize\tabcolsep2\p@%
    \nopagebreak[4]\samepage%
    \begin{tabular}{\@nameuse{pream@gemini}}%
    \@nameuse{obshead@gemini}\\\hline\\[-1.8ex]%
    \gobs@list\end{tabular}\end{center}}



% Observing parameters.  Not all of these are needed for each instrument
% combination.
%
%    \objid{OBJECT ID}
%    \object{OBJECT NAME}
%    \ra{RIGHT ASCENSION}
%    \dec{DECLINATION}
%    \epoch{COORDINATE EPOCH}
%    \magnitude{MAGNITUDE}
%    \filter{FILTER}
%    \exptime{EXPOSURE TIME}
%    \nexposures{NUMBER OF EXPOSURES}
%    \moondays{DAYS FROM NEW MOON}
%    \skycond{SKY CONDITION}
%    \seeing{SEEING LIMIT}
%    \obscomment{COMMENT}

\def\cleart@obst {
    \gdef\obs@objid{} \gdef\obs@object{} \gdef\obs@ra{} \gdef\obs@dec{}
    \gdef\obs@epoch{} \gdef\obs@magnitude{} \gdef\obs@filter{} 
    \gdef\obs@exptime{} \gdef\obs@nexposures{} \gdef\obs@moondays{}
    \gdef\obs@skycond{} \gdef\obs@seeing{} \gdef\obs@obscomment{}
}

\def\cleart@gobst {
    \gdef\obs@objid{} \gdef\obs@object{} \gdef\obs@ra{} \gdef\obs@dec{}
    \gdef\obs@epoch{} \gdef\obs@magnitude{} 
    \gdef\obs@obstime{} 
    \gdef\obs@guidestars{} 
    \gdef\obs@skybackground{} \gdef\obs@watervapor{}
    \gdef\obs@cloudcover{} \gdef\obs@imagequality{}
    \gdef\obs@gemcomment{}
}

\def\cleart@gobsline {
    \gdef\obs@guidestars{} \gdef\obs@gemcomment{}
}


\def\obsblock@add{
    \ifx\obs@list\@empty
        \@temptokena=\expandafter{\obs@list}
    \else \@temptokena=\expandafter{\obs@list\\}\fi
    \xdef\obs@list{\the\@temptokena\@nameuse{obsblock@\@instrid}}}

\def\gobsblock@add{
    \ifx\gobs@list\@empty
        \@temptokena=\expandafter{\gobs@list}
    \else \@temptokena=\expandafter{\gobs@list\\}\fi
    \xdef\gobs@list{\the\@temptokena\@nameuse{obsblock@gemini}}
    \cleart@gobsline}

\def\objid#1{\gdef\obs@objid{#1}}
\def\object#1{\gdef\obs@object{#1}}
\def\ra#1{\gdef\obs@ra{#1}}
\def\dec#1{\gdef\obs@dec{#1}}
\def\epoch#1{\gdef\obs@epoch{#1}}
\def\magnitude#1{\gdef\obs@magnitude{#1}}
\def\filter#1{\gdef\obs@filter{#1}}
\def\exptime#1{\gdef\obs@exptime{#1}}
\def\nexposures#1{\gdef\obs@nexposures{#1}}
\def\moondays#1{\gdef\obs@moondays{#1}}
\def\skycond#1{\gdef\obs@skycond{#1}}
\def\seeing#1{\gdef\obs@seeing{#1}}
\def\obscomment#1{\gdef\obs@obscomment{#1}\obsblock@add}

\def\obstime#1{\gdef\obs@obstime{#1}}
\def\guidestars#1{\gdef\obs@guidestars{#1}}
\def\skybackground#1{\gdef\obs@skybackground{#1}}
\def\watervapor#1{\gdef\obs@watervapor{#1}}
\def\cloudcover#1{\gdef\obs@cloudcover{#1}}
\def\imagequality#1{\gdef\obs@imagequality{#1}}
\def\gemcomment#1{\gdef\obs@gemcomment{#1}}
\def\endtarget{\gobsblock@add}

\def\instrname@default{\@instrname}
\def\pream@default{ccccccccccccl}
\def\pream@gemini{cccccccccccccl}

\def\obshead@default{
{\shortstack{Obj\\ID}} & {Object} & {$\alpha$} & {$\delta$} & {Epoch} &
{Mag.} & {Filter} & {\shortstack{Exp.\\time}} &
{\shortstack{\# of\\exp.}} &
{\shortstack{Lunar\\days}} & {Sky} & {Seeing} & {Comment}
}

\def\obshead@gemini{
{\shortstack{Obj\\ID}} & {Object} & {$\alpha$} & {$\delta$} & {Epoch} &
{Mag.} & {\shortstack{Obs.\\time}} &
{\shortstack{WFS\\stars}} &
{\shortstack{IQ\\\%}} &
{\shortstack{SB\\\%}} &
{\shortstack{WV\\\%}} &
{\shortstack{CC\\\%}} &
{Comment}
}

\def\obsblock@default{
\obs@objid & \obs@object & \obs@ra & \obs@dec & \obs@epoch &
\obs@magnitude & \obs@filter & \obs@exptime & \obs@nexposures &
\obs@moondays & \obs@skycond & \obs@seeing & \obs@obscomment
}

\def\obsblock@gemini{
\obs@objid & \obs@object & \obs@ra & \obs@dec & \obs@epoch &
\obs@magnitude & \obs@obstime & 
\obs@guidestars & 
\obs@imagequality & \obs@skybackground& \obs@watervapor & \obs@cloudcover & 
\obs@gemcomment
}




%  ****************************************
%  *           EPS INCLUSIONS             *
%  ****************************************

% Include Rokicki's epsf.sty file explicitly.

\@ifundefined{epsfbox}{\input{epsf.sty}}{\relax}

% Simplified EPS inclusion macros so we can see how this goes...
% These are layered on Rokicki's dvips material, and are dependent
% on the author's use of that DVI driver.
%
%    \plotone{EPSFILE}
%    \plottwo{EPSFILE}{EPSFILE}
%    \plotfiddle{EPSFILE}{VSIZE}{ROT}{HSF}{VSF}{HTRANS}{VTRANS}
%
% \plotone inserts the plot in a space that is \columnwidth wide; the
% plot is scaled so the horizontal dimension fits in the text width,
% and the vertical dimension is scaled to maintain the aspect ratio.
% \plottwo inserts two plots next to each other in one \columnwidth,
% sort of like "two-up" mode.
%
%    EPSFILE    name of file with EPS
%
% The following arguments are for the \plotfiddle macro which formats
% the \special itself, prepares vspace, etc.  This completely bypasses
% Rokicki's macros that attempt to rationalize the EPS BoundingBox with
% the LaTeX page dimensions.
%
%    VSIZE      vertical white space to allow for plot
%    ROT        rotation angle
%    HSF        horiz scale factor
%    VSF        vert scale factor
%    HTRANS     horiz translation
%    VTRANS     vert translation

%\epsfverbosetrue

\def\eps@scaling{.95}
\def\epsscale#1{\gdef\eps@scaling{#1}}

\def\plotone#1{\centering \leavevmode
    \epsfxsize=\eps@scaling\columnwidth \epsfbox{#1}}

\def\plottwo#1#2{\centering \leavevmode
    \epsfxsize=.45\columnwidth \epsfbox{#1} \hfil
    \epsfxsize=.45\columnwidth \epsfbox{#2}}

\def\plotfiddle#1#2#3#4#5#6#7{\centering \leavevmode
    \vbox to#2{\rule{0pt}{#2}}
    \special{psfile=#1 voffset=#7 hoffset=#6 vscale=#5 hscale=#4 angle=#3}}

% Conveniences - compatible with AASTeX v4.0.

\def\deg{\hbox{$^\circ$}}
\def\sun{\hbox{$\odot$}}
\def\earth{\hbox{$\oplus$}}
\def\lesssim{\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$}}}\hbox{$<$}}}}
\def\gtrsim{\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$}}}\hbox{$>$}}}}
\def\sq{\hbox{\rlap{$\sqcap$}$\sqcup$}}
\def\arcdeg{\hbox{$^\circ$}}
\def\arcmin{\hbox{$^\prime$}}
\def\arcsec{\hbox{$^{\prime\prime}$}}
\def\fd{\hbox{$.\!\!^{\rm d}$}}
\def\fh{\hbox{$.\!\!^{\rm h}$}}
\def\fm{\hbox{$.\!\!^{\rm m}$}}
\def\fs{\hbox{$.\!\!^{\rm s}$}}
\def\fdg{\hbox{$.\!\!^\circ$}}
\def\farcm{\hbox{$.\mkern-4mu^\prime$}}
\def\farcs{\hbox{$.\!\!^{\prime\prime}$}}
\def\fp{\hbox{$.\!\!^{\scriptscriptstyle\rm p}$}}
\def\micron{\hbox{$\mu$m}}
\let\la=\lesssim			% For Springer A&A compliance...
\let\ga=\gtrsim
\def\case#1#2{\hbox{$\frac{#1}{#2}$}}
\def\slantfrac#1#2{\hbox{$\,^#1\!/_#2$}}
\def\onehalf{\slantfrac{1}{2}}
\def\onethird{\slantfrac{1}{3}}
\def\twothirds{\slantfrac{2}{3}}
\def\onequarter{\slantfrac{1}{4}}
\def\threequarters{\slantfrac{3}{4}}
\def\ubvr{\hbox{$U\!BV\!R$}}            
\def\ub{\hbox{$U\!-\!B$}}               
\def\bv{\hbox{$B\!-\!V$}}               
\def\vr{\hbox{$V\!-\!R$}}               
\def\ur{\hbox{$U\!-\!R$}}
\def\ion#1#2{#1$\;${\small\rm\@Roman{#2}}\relax}

\let\jnl@style=\rm
\def\ref@jnl#1{{\jnl@style#1}}
\def\aj{\ref@jnl{AJ}}                   
\def\araa{\ref@jnl{ARA\&A}}             
\def\apj{\ref@jnl{ApJ}}                 
\def\apjl{\ref@jnl{ApJ}}                
\def\apjs{\ref@jnl{ApJS}}               
\def\ao{\ref@jnl{Appl.~Opt.}}           
\def\apss{\ref@jnl{Ap\&SS}}             
\def\aap{\ref@jnl{A\&A}}                
\def\aapr{\ref@jnl{A\&A~Rev.}}          
\def\aaps{\ref@jnl{A\&AS}}              
\def\azh{\ref@jnl{AZh}}                 
\def\baas{\ref@jnl{BAAS}}               
\def\jrasc{\ref@jnl{JRASC}}             
\def\memras{\ref@jnl{MmRAS}}            
\def\mnras{\ref@jnl{MNRAS}}             
\def\pra{\ref@jnl{Phys.~Rev.~A}}        
\def\prb{\ref@jnl{Phys.~Rev.~B}}        
\def\prc{\ref@jnl{Phys.~Rev.~C}}        
\def\prd{\ref@jnl{Phys.~Rev.~D}}        
\def\pre{\ref@jnl{Phys.~Rev.~E}}        
\def\prl{\ref@jnl{Phys.~Rev.~Lett.}}    
\def\pasp{\ref@jnl{PASP}}               
\def\pasj{\ref@jnl{PASJ}}               
\def\qjras{\ref@jnl{QJRAS}}             
\def\skytel{\ref@jnl{S\&T}}             
\def\solphys{\ref@jnl{Sol.~Phys.}}      
\def\sovast{\ref@jnl{Soviet~Ast.}}      
\def\ssr{\ref@jnl{Space~Sci.~Rev.}}     
\def\zap{\ref@jnl{ZAp}}                 
\def\nat{\ref@jnl{Nature}}              
\def\iaucirc{\ref@jnl{IAU~Circ.}}
\def\aplett{\ref@jnl{Astrophys.~Lett.}}
\def\apspr{\ref@jnl{Astrophys.~Space~Phys.~Res.}}
\def\bain{\ref@jnl{Bull.~Astron.~Inst.~Netherlands}}
\def\fcp{\ref@jnl{Fund.~Cosmic~Phys.}}
\def\gca{\ref@jnl{Geochim.~Cosmochim.~Acta}}
\def\grl{\ref@jnl{Geophys.~Res.~Lett.}}
\def\jcp{\ref@jnl{J.~Chem.~Phys.}}      
\def\jgr{\ref@jnl{J.~Geophys.~Res.}}    
\def\jqsrt{\ref@jnl{J.~Quant.~Spec.~Radiat.~Transf.}}
\def\memsai{\ref@jnl{Mem.~Soc.~Astron.~Italiana}}
\def\nphysa{\ref@jnl{Nucl.~Phys.~A}}
\def\physrep{\ref@jnl{Phys.~Rep.}}
\def\physscr{\ref@jnl{Phys.~Scr}}
\def\planss{\ref@jnl{Planet.~Space~Sci.}}
\def\procspie{\ref@jnl{Proc.~SPIE}}
\let\astap=\aap
\let\apjlett=\apjl
\let\apjsupp=\apjs
\let\applopt=\ao

% Initialization.

\textwidth 6.5in
\textheight 9.0in
\oddsidemargin \z@
\evensidemargin \z@
\topmargin \z@
\headheight .2in
\headsep .2in
%\footheight \z@
\parindent \z@
%\parskip 1ex
\addtolength{\parskip}{1 ex}

\voffset=-0.25in
%\hoffset=-0.25in

\ps@kpprophead
\setcounter{secnumdepth}{0}

\thispagestyle{empty}