% STY file for Astro 504 proposal (adapted from the KPNO proposal .sty file) % First, identifying information about this style file. \def\revtex@ver{1.1} % Version number of this file. \def\revtex@date{8 Feb 95} % Revision date. \def\revtex@author{CDB} % This file's author. \def\revtex@org{KPNO} % Sponsoring organization. \def\revtex@jnl{} % Applicable journal, if specific. \def\revtex@genre{observing proposal} % Document "type". \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} \def\enddocument{\vfill\ltx@enddoc} % Supporting style files. \input{art11.sty} %\@input{times.sty} % 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 Proposer: \@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 Proposal\\Astro 504} \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 Name:\/} \@propid}}} \def\ques@font{\it} \def\instruct@font{\small\sl} % Proposal ID and receipt date will be filled in at KPNO. % % \proposalid{NUMBER} % \received{DATE} \def\received#1{\gdef\@rcptdate{#1}} \received{} \def\proposalid#1{\gdef\@propid{#1}} \proposalid{\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\vskip18pt} \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} % \affil{AFFILIATION} % \address{POSTAL ADDRESS} % \emailaddress{EMAIL ADDRESS} % \phone{TELEPHONE NUMBER} % \fax{FAX NUMBER} % \gradstudent{Y or 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\gradstudent#1{\gdef\obs@gradstudent{#1}} \def\clear@obs{\gdef\obs@name{}\gdef\obs@affil{}\gdef\obs@address{} \gdef\obs@email{}\gdef\obs@phone{}\gdef\obs@fax{}\gdef\obs@gradstudent{}} % 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 Institution: \fld@dlm \obs@affil\\ \bf Email: \fld@dlm \obs@email\\ \bf Telephone: \fld@dlm \obs@phone\\ \bf Fax: \fld@dlm \obs@fax\\ \end{tabular}\end{quote}} \def\prt@coiblock{\begin{tabbing} \makebox[.25\textwidth]{\null}\=\makebox[.25\textwidth]{\null}\= \makebox[.25\textwidth]{\null}\=\kill \hbox to.50\textwidth{\obs@tag\space% \ifx\@empty\obs@name\hrulefill\space\else\obs@name\hfill\fi}% \hbox to.25\textwidth{Grad student?\space% \ifx\@empty\obs@gradstudent\yn@rule\else\obs@gradstudent\fi\hfill}% \hbox to.25\textwidth{% \ifx\@empty\obs@email Email: \hrulefill\else\obs@email\hfill\fi}\\[.2ex] \hbox to.75\textwidth{% \ifx\@empty\obs@address Address: \hrulefill\space\else\obs@affil, \obs@address\hfill\fi}% \hbox to.25\textwidth{% \ifx\@empty\obs@phone Phone: \hrulefill\else\obs@phone\hfill\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\@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\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 Are you requesting long-term status? If `Y', please give details on the line below.}} \def\queue@head{{\ques@font Would you like these observations carried out in ``queue'' mode?}} \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\queue#1{\par$\bullet$\space\queue@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} % \lunarphase{NUMBER} % \optimaldates{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\lunarphase#1{\global\@namedef{obs\@Alph{\c@obsrun}@lunarphase}{#1}} \def\optimaldates#1{\global\@namedef{obs\@Alph{\c@obsrun}@optdates}{#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@kpnoprop{ \@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}@lunarphase} & \@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||@{\extracolsep{\fill}}*{2}{c|}} \multicolumn{1}{c}{\scriptsize Run} & \multicolumn{1}{c}{\scriptsize Telescope} & \multicolumn{1}{c}{\scriptsize Instrument, detectors, 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||@{\extracolsep{\fill}}*{4}{c|}} \multicolumn{1}{c}{\scriptsize Run} & \multicolumn{1}{c}{\scriptsize No. nights} & \multicolumn{1}{c}{\scriptsize No. days} & \multicolumn{1}{c}{\scriptsize Moon age (d)} & \multicolumn{1}{c}{\scriptsize Optimal dates} \\ \hline 1 & \obsA@numnights & \obsA@numdays & \obsA@lunarphase & \obsA@optdates \\ \hline 2 & \obsB@numnights & \obsB@numdays & \obsB@lunarphase & \obsB@optdates \\ \hline 3 & \obsC@numnights & \obsC@numdays & \obsC@lunarphase & \obsC@optdates \\ \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 % \anyother % \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.\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.\par}} \def\anyother@head{{\instruct@font If other facilities are also needed for this project, explain their role.\par}} \def\past@head{{\instruct@font List your allocation of telescope time at KPNO and CTIO during the past 2 years, 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.\par}} \def\justification{\newpage\propsection{\fbox{Scientific Justification}} \justif@head} \def\feasibility{\newpage\propsection{\fbox{Technical and Scientific Feasibility}}\feas@head} \def\anyother{\vfill\propsection{\fbox{Multi-site?}}\anyother@head} \def\thepast{\vfill\propsection{\fbox{Previous Use of KPNO Facilities}} \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@kpprophead \setcounter{secnumdepth}{0} \thispagestyle{empty}