% MDMPROP.STY -- MDM observing proposal form. % First, identifying information about this style file. \def\revtex@ver{2.3} % Version number of this file. \def\revtex@date{11 Apr 2007} % Revision date. \def\revtex@author{Jules} % This file's author. \def\revtex@org{Columbia} % Sponsoring organization. \def\revtex@jnl{} % Applicable journal, if specific. \def\revtex@genre{observing proposal} % Document "type". % provide compatibility with previous versions \newcommand{\lunarphase}{\lunardays} \typeout{\revtex@org\space \ifx\revtex@jnl\@empty\else\revtex@jnl\space\fi \revtex@genre\space substyle, v\revtex@ver\space <\revtex@date>.} \def\revtex@pageid{\xdef\@thefnmark{\null} \@footnotetext{\revtex@org\space \ifx\revtex@jnl\@empty\else\revtex@jnl\space\fi \revtex@genre\space \LaTeX\ macros v\revtex@ver.}} \let\ltx@enddoc=\enddocument \def\enddocument{\vfill\revtex@pageid\ltx@enddoc} % Supporting style files. \@input{art11.sty} %\@input{times.sty} %\def\normalsize{\ifx\@currsize\normalsize \rm \else \@normalsize\fi} % Page design/layout macros. Page sizes are at the end of the file. \def\baselinestretch{0.98} % Tighten up baselines a little. \def\ps@mdmprophead{\def\@oddfoot{}\def\@evenfoot{} \def\@oddhead{\hbox to\textwidth{\small\sl Proposal \#\@propid \ifx\@empty\@rcptdate\relax\else, received \@rcptdate\fi \hfill Page \thepage}}\let\@evenhead\@oddhead \def\chaptermark##1{\markright {{\ifnum \c@secnumdepth>\m@ne \@chapapp\ \thechapter. \ \fi ##1}}}} \def\prop@head{Observing Time Request\\MDM Observatory} \newdimen\prop@idboxwidth \def\prop@idbox{\prop@idboxwidth\textwidth \advance\prop@idboxwidth by-2.3\fboxsep \fbox{\hbox to\prop@idboxwidth{ \ifx\@rcptdate\@empty{\it Date:\/} \today \else{\it Date received:\/} \@rcptdate\fi\hfil % {\it Institution:\/} \@taccategory \hspace{1.4cm} {\it Proposal number:\/} \@propid }}} \def\ques@font{\it} \def\instruct@font{\small\sl} % Proposal ID will be filled in by Jules. % % \proposalid{NUMBER} % \received{DATE} \def\received#1{\gdef\@rcptdate{#1}} \received{} \def\proposalid#1{\gdef\@propid{#1}} \proposalid{\hspace{1in}} \def\taccategory#1{\gdef\@taccategory{#1}} \taccategory{\hspace{1in}} % 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. % % \title{TEXT} \def\title#1{\null\vspace{-2\headheight}\vspace{-\headsep} \begin{center}\large\bf\prop@head\end{center}\prop@idbox\par \vspace*{.2in} \def\@tempa{#1}\ifx\@empty\@tempa \makebox[\textwidth]{\large{\bf TITLE:} \hrulefill}\par \makebox[\textwidth]{\hrulefill}\par \else{{\large{\bf TITLE:}} \@tempa}\fi} \def\abstract{\par\vspace{0ex}\vbox to2.35in\bgroup\noindent {\bf Abstract of Scientific Justification:}\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} % \emailaddress{EMAIL ADDRESS} % \atthetelescope{Y/N} % % 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\address#1{\gdef\obs@address{#1}} \def\emailaddress#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\gradstudent#1{\gdef\obs@gradstudent{#1}} % for compatibility (ignored) \def\permaddress#1{\gdef\obs@permaddress{#1}} % for future use (ignored) \def\atthetelescope#1{\gdef\obs@present{#1}} \def\clear@obs{\gdef\obs@name{}\gdef\obs@affil{}\gdef\obs@address{} \gdef\obs@email{}\gdef\obs@phone{}\gdef\obs@fax{}\gdef\obs@invstatus{} \gdef\obs@gradstudent{}\gdef\obs@permaddress{}} % 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 bitch about the overfull hbox. \def\yn@rule{\rule{0.3in}{0.4pt}} \newcount\@maxnumcois \@maxnumcois=3 \def\prt@piblock{\begin{quote}\begin{tabular}{ll} \bf Principal Investigator: \fld@dlm \obs@name\\ \bf Email: \fld@dlm \obs@email\\ \bf Present?: \fld@dlm \obs@present\\ \end{tabular}\end{quote}} \def\prt@coiblock{\begin{tabbing} \makebox[.25\textwidth]{\null}\=\makebox[.25\textwidth]{\null}\= \makebox[.25\textwidth]{\null}\=\kill \hbox to.35\textwidth{\obs@tag\space% \ifx\@empty\obs@name\hrulefill\space\else\obs@name\hfill\fi} \hbox to.50\textwidth{% \ifx\@empty\obs@email Email: \hrulefill\else\hfill\obs@email\fi} %\\[.2ex] \hbox to.135\textwidth{% \ifx\@empty\obs@present Present? \hrulefill\else\hfill\obs@present\fi}% \end{tabbing}} % 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@coiblock} \newenvironment{CoI}{\clear@obs\stepcounter{CoI}}{\ifnum\c@CoI>\@maxnumcois \relax\else\vspace*{-5ex}\prt@coiblock\fi} % Questions for first page. % % \thesis{Y or N} % \longterm{Y or N} % \longtermdetails{BRIEF DETAILS} % \queue{Y or N} % \unusabledates{BRIEF DETAILS} \def\chk@setblank#1{\def\@mdmtmpa{#1}\ifx\@empty\@mdmtmpa \def\@mdmtmpa{\yn@rule}\fi\mbox{\@mdmtmpa}} \def\chk@setblankline#1{\def\@mdmtmpa{#1}\ifx\@empty\@mdmtmpa \def\@mdmtmpa{\rule{\textwidth}{0.4pt}}\fi \par\makebox[\textwidth][l]{\@mdmtmpa}} \def\thesis@head{{\ques@font Is this proposal part of a PhD thesis?}} % If `Y', you must send a letter; see instructions.}} \def\longterm@head{{\ques@font Requesting long-term status? If `Y', please give \# of semesters and nights on the next line.}} \def\mode@head{{\ques@font Enter `C' for classical run, or `Q' for proxy queue on the 2.4m with OSMOS, or `R' for robotic on the 1.3m with MIRAGE.}} \def\undates@head{{\ques@font List dates you cannot use for non-astronomical reasons on the next line.}} \def\thesis#1{\par$\bullet$\space\thesis@head\quad\chk@setblank{#1}} \def\longterm#1{\par$\bullet$\space\longterm@head\quad\chk@setblank{#1} \gdef\@longterm{#1}} \def\longtermdetails#1{\def\@tempa{N}\ifx\@longterm\@tempa\relax\else \chk@setblankline{#1}\fi} \def\mode#1{\par$\bullet$\space\mode@head\quad\chk@setblank{#1}} \def\unusabledates#1{\par$\bullet$\space\undates@head\par\chk@setblankline{#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=3\par\prt@obsruns\par\fi} % Observing run parameters to be specified by the investigators. % % \telescope{IDENT} % \instrument{IDENT(S)} % \numnights{NUMBER} % \numdays{NUMBER} % removed from printed table % \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\numdays#1{\global\@namedef{obs\@Alph{\c@obsrun}@numdays}{#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} % This one is not actually used. It is work in progress... \def\obsblock@mdmprop{ \@whilenum\c@obsrun <3 \do {\typeout{Run \the\c@obsrun.} \@arabic{\c@obsrun} & \@nameuse{obs\@Alph{\c@obsrun}@telid} & \@nameuse{obs\@Alph{\c@obsrun}@inst} \\ \global\advance\c@obsrun by\@ne} & \@nameuse{obs\@Alph{\c@obsrun}@numnights} & \@nameuse{obs\@Alph{\c@obsrun}@numdays} & \@nameuse{obs\@Alph{\c@obsrun}@lunardays} & \@nameuse{obs\@Alph{\c@obsrun}@optdates} & \@nameuse{obs\@Alph{\c@obsrun}@accdates} } % Note that I am taking serious advantage of the requirement that only % three of these blocks may be specified: I am explicitly printing % three sets of obsrun data and three sets only. \def\prt@obsruns{\begin{center}{\small\bf\obsrun@head}\\[1ex] \setcounter{obsrun}{1} \begin{tabular*}{1.0\textwidth} {|c||c|l@{\extracolsep{\fill}}c|} \multicolumn{1}{c}{\scriptsize Run} & \multicolumn{1}{c}{\scriptsize Telescope} & \multicolumn{1}{c}{\scriptsize Instrument, detectors, grisms, gratings, filters, camera optics, etc.}\\ \hline 1 & \obsA@telid & \obsA@inst &\\ \hline 2 & \obsB@telid & \obsB@inst &\\ \hline 3 & \obsC@telid & \obsC@inst &\\ \hline \end{tabular*}\\ \vspace{2ex} \begin{tabular*}{1.0\textwidth} {|c||c|c|@{\extracolsep{\fill}}*{2}{c|}} \multicolumn{1}{c}{\scriptsize Run} & \multicolumn{1}{c}{\scriptsize No. nights} & \multicolumn{1}{c}{\scriptsize Moon age (d)} & \multicolumn{1}{c}{\scriptsize Optimal dates} & \multicolumn{1}{c}{\scriptsize Acceptable dates}\\ \hline 1 & \obsA@numnights & \obsA@lunardays & \obsA@optdates & \obsA@accdates \\ \hline 2 & \obsB@numnights & \obsB@lunardays & \obsB@optdates & \obsB@accdates \\ \hline 3 & \obsC@numnights & \obsC@lunardays & \obsC@optdates & \obsC@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). % % \justification % \feasibility % \whymdm % \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 Try to include overall significance to astronomy.\par}} \def\feas@head{{\instruct@font List objects, coordinates, and magnitudes (or surface brightness, if appropriate), desired S/N, wavelength coverage and resolution. Justify the number of nights requested as well as the specific telescope, instruments, and lunar phase. Indicate the optimal detector, as well as acceptable alternates. If you've requested long-term status, justify why this is necessary for successful completion of the science.\par}} \def\whymdm@head{{\instruct@font If other optical/IR facilities are being used for this project, explain the role that MDM observations will play. \par}} \def\past@head{{\instruct@font List your allocations of telescope time at MDM during the past 3 years, together with the current status of the project (cite publications where appropriate). Mark with an asterisk those allocations of time related to the current proposal. For ongoing projects, are they achieving their goals?\par}} \def\justification{\newpage\propsection{\fbox{Scientific Justification}} \justif@head} \def\feasibility{\newpage\propsection{\fbox{Technical and Scientific Feasibility}}\feas@head} \def\whymdm{\vfill\propsection{\fbox{Why MDM?}}\whymdm@head} \def\thepast{\vfill\propsection{\fbox{How is it Going?}} \past@head} \def\relatedwork#1{\fbox{$\star$}\space#1} % **************************************** % * 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. \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\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\ion#1#2{#1$\;${\small\rm\@Roman{#2}}\relax} % Initialization. \textwidth 6.5in \textheight 9.0in \oddsidemargin \z@ \evensidemargin \z@ \topmargin \z@ \headheight .2in \headsep .2in \footheight \z@ \parindent \z@ \parskip 1ex \voffset=-0.25in %\hoffset=-0.25in \ps@mdmprophead \setcounter{secnumdepth}{0} \thispagestyle{empty}