%   Template for applications for observing time at Calar Alto
%
%          Updated version Jan. 17, 2011   (U. Thiele)
%
%            requires dsaz0112.sty
%
%   Changes with respect to previous versions:
%
%   to template0102.tex / dsaz0102.sty :
%       -- 1.23m-telescope removed
%       -- PMAS as new CAHA instrument
%   to template0702.tex / dsaz0702.sty :
%       -- OMEGA2000 as a new instrument
%   to template0103.tex / dsaz0103.sty :
%       -- none thus far
%   to template0703.tex / dsaz0703.sty
%       arguments extended for \instrumentation in case of
%                                      OMEGA Cass and PMAS
%   to template0104.tex / dsaz0104.sty
%       OMEGA-prime has been removed from offered instruments
%
%   to template0107.tex / dsaz0107.sty
%       -- New section 9b.: Comments on target sample 
%       -- Target list limited to 30 entries
%
%   to template0707.tex / dsaz0707.sty
%       -- Page 3a is now logistics page
%
%   to template0110.tex / dsaz0110.sty
%       -- New section on page 2: Strategic relevance for MPIA
%
%   to template0111.tex / dsaz0111.sty
%       -- OMEGA-Cass removed 
%       -- CAFE added
%
%   to template0711.tex / dsaz0711.sty
%       -- New column in publications list
%       -- Instrument sheet modified
%       -- New section 9c.: Comment on archive
%
%
%   ************************************************************
%   * This template contains explicit instructions as to how   *
%   * to fill in the LaTeX-commands (comments + examples).     *
%   *                                                          *
%   *       Please follow these instructions carefully!        *
%   *                                                          *
%   * Since this LaTeX-file is automatically analysed to       *
%   * collect the statistical information and prepare the      *
%   * applications for the referees you must not manipulate    *
%   * this file (e.g. omit or permutate commands).             *
%   * Do not concatenate two commands into one line!           *
%   * Commands not needed have to be supplied with an empty    *
%   * argument (e.g. \SchedulingConstraints{} ).               *
%   ************************************************************
%
%  General Information:
%
%  Only proposals written in English are accepted!
%
%  The Style-File and the Template-File were tested with LaTeX 2e
%  (Version 2000/06/01) or TeX-Version 3.14159.
%
%  To create an empty form, empty calls {} have to be selected.
%
%  Comments always refer to the argument or group of arguments
%  of the  *** PREVIOUS *** line.
%
%  Forced linebreaks (\\ or empty line) do not work with most commands.
%  Please use the command \newline instead!
%
%  Type size and page format must not be changed, especially
%  not within the scientific justification!
%  The given number of pages and arrangement are checked! If your pages
%  overflow the space provided, a LaTeX-error will occur.
%
%  The list of publications and the citations from the scientific
%  justification can (but do not have to) be created by LaTeX-command
%  \cite{label} (see item publications). A mixture of manual entries
%  and the use of \cite{label}, though, is not possible.
%
%  Some frequent symbols are defined in the style-file:
%     \etal \privcom \eg \ie \ibidem \dito
%
%  Units for math-mode (in rm-Font)
%     \GHz \MHz \Hz \pc \kpc \Mpc \cm \sec \Kelvin \Jy \mJy \microJy
%
%====================================================================
%
\documentclass{article}
\usepackage[dvips]{graphicx}
\usepackage{ifthen}
\usepackage{dsaz0112}
%
\begin{document}
%
%\TestRun
%               Activate this command to create a test run
%               checking your LaTeX file at CAHA.
%               Do not forget to de-activate this command for
%               actual submission!!!
%
%               No records will be kept at CAHA for test runs,
%               even if they are successful!
%
% ========================== p a g e  1 =============================
%
%                     Group, from which the application originates
%                     Comment/uncomment as appropriate
%
\RDSapplication       % German institute other than MPIA
%                         RDS = Rat Deutscher Sternwarten
%\MPIAapplication%     % MPIA
%\SPANISHapplication   % Spanish institute
%\OTHER                % all others
%
\noServiceMode         % visitor mode
%\PartlyServiceMode    % partly in service mode
%\ServiceMode          % full service mode
%
%           please select the appropriate mode for your application
%           and comment out the other one.
%
\AutumnApplication{2012}
%
\TelThreePointFive{}{}
%\TelTwoPointTwo{}{}
%               {flag}{proposal reference ID}
%
%                          select only one telescope per application!
%
% -------------------------------------------------------------------
%                         Types of applications
% -------------------------------------------------------------------
%
% The type of your application - if applicable - is specified in
% the above command for the telescope selection as the 1. argument,
% perhaps together with the reference number of the previously
% submitted application as a 2. argument. If none of the cases
% described below is applicable, leave both arguments empty.
%
% MPIA or IAA guaranteed time: G
% ==============================
%
% Requests for MPIA or IAA guaranteed time must be flagged with a G. 
% If you apply for MPIA time please fill in the
% \subsection*{Strategic relevance for MPIA} (see below). 
%
% Long term projects (> 2 semesters): P, L
% ========================================
% Applications for PhD thesis work and long projects may be flagged,
% PhD thesis with a P, other long term projects with an L in the 1.
% argument to the telescope call above. If this flag is used, for both
% an additional page (item 8e) has to be filled in below, describing
% the current / planned logistics of the project. Is this an application
% to continue observations from previous semesters, please quote the
% reference number of the former application in the 2. argument.
%
% The purpose of flagging PhD programs is to request a particularly
% thorough initial application with an outline of all anticipated
% observations. In return, PhD programs can then usually expect
% subsequent approval within the framework of the initial request,
% as long as a satisfactory update on the PhD student's progress
% is provided in subsequent applications. Such a bonus will, however,
% not be given for long-term projects, which have to compete again fully
% with all other proposals currently submitted. For the latter the
% flag is intended to help the referees judging the overall project
% and its needs.
%
% Instrumental tests: I
% =====================
% Requests for observing time to test and commission a new
% instrument must be flagged with an I. Such an application must
% not be mixed with scientific observations and justification
% of this science. For the latter a separate proposal has to
% be submitted.
% Since January 2004 the CAHA director decides on time for instrumental
% tests
%
% Repetitive applications: W, T, C, R
% ===================================
% If a previous run has been lost due to weather or technical problems,
% the re-submitted proposal should be flagged. W indicates loss due to
% weather, T due to technical difficulties. Indicate the reference
% number of the previous application in the 2. argument.
% If you re-submit an application to continue a project (less than 3
% semesters in total duration) you may flag it with an C. Re-submission
% of a previously rejected application may be flagged with an R. Both
% should include the reference number of the former application in the
% 2. argument.
%
% Example:
% \TelThreePointFive{C}{H00-3.5-64} is a re-submission of an application
% analogous to application 64 at the 3.5m-telescope in autumn
% semester 2000.
%
% Multiple applications: M
% ========================
% Projects requiring different telescopes or instruments while using
% the SAME SCIENTIFIC JUSTIFICATION under item 8 for organizational
% reasons have to provide separate applications for each combination
% telescope/instrument needed. However, the detailed scientific
% justification may be provided only in one of these applications,
% in the other a short reference to the application with the full
% scientific justification is sufficient.
%
%    In order to make it easier to relate them to each other, in the
%    applications belonging together the first flag in the telescope
%    call always has to be given as M.
%
% Example:
% A project needs optical as well as infrared observations.
% Then, two applications should be submitted, for which the telescopes
% e.g. \TelThreePointFive{M}{} and \TelTwoPointTwo{M}{} are specified.
% One of these contains the scientific justification.
%
% In applications, for which a special type is indicated as outlined
% above, a leading M in the 1. telescope argument signals, that for
% this type multiple applications are submitted.
%
% Example:
% \TelThreePointFive{MC}{S96-3.5-64} is the application to continue
% the project with the quoted reference number, together with which
% a further application is submitted,
% e.g. \TelTwoPointTwo{MC}{S96-2.2-28}.
%
% ---------------------------------------------------------------------
%
% Please, be careful when filling in the proposal, and provide complete
% information regarding previous applications. Help the TAC by supplying
% the requested info (accurate and complete).
%
% ---------------------------------------------------------------------
%
\Applicant{}{}{}
        % Title Name Surname of the principal investigator (P.I.)
        %             ( =addressee of correspondence)
{}
        % Institute
{}
        % Street
{}{}
        % ZIP-code Town
{}
        % Country
{}
        % complete e-mail address
        %
        % Not only give Smith.
        % No space or TeX-format are to be used within this string
        % because our procedure for the acceptance of the applications
        % does use this string to send the confirmation to the P.I. !
        %
\Collaborators{}{}
        % collaborators: Name(s)  Institute(s)
{}{}
        %                Name(s)  Institute(s)
\Observers{}
           {}
        % Name(s) of the applicants/collaborators who will
        % perform the observation.
\Category{}    % category
        % Please choose ONE category that comes closest to your
        % application by giving the corresponding letter
        % in the argument.
        %
        % This is an IMPORTANT INFORMATION needed for the
        % the allocation of the referees. Please choose
        % it carefully!
        %
        % A = Cosmology, intergalactic medium,
        %     clusters of galaxies, galaxies
        % B = active galactic nuclei
        % C = interstellar medium, star formation, milky way
        % D = massive / hot stars
        % E = low-mass / cold stars
        % F = solar system
        % G = instrumentation
\KeyWord{}
        % unique keyword to mark the application
        % (used to identify the application on the instrumentation
        % sheet in addition to the P.I.'s name)
\Title{}
        % Only one line!
\Abstract{}
        % The length of the abstract must not change the page layout!
\Method{}  % Instrument
       {}
        % observing method to be applied
        %       (e.g. long-slit  spectroscopy)
\FluxLevel{}    % from
          {}    % to
          {}    % unit of measurement of the brightness given
                %  (e.g. K-mag, Jy at 660nm)
%
% The following information has to contain the SUM of the time
% applied for as a (real) number (e.g. 3.5 or 0.2) to facilitate
% the electronic processing of the data.
% Further details (e.g. 3 x 1/2 night) are to be specified under
% item 11 with the command \SchedulingConstraints !
%
\Nights{} % no restriction  % number of nights applied for
       {} % grey            %       (without weather corrections!)
       {} % dark            %     please specify only ONE of these!
       {} % already awarded for this project (leave empty if none).
       {} % nights expectedly needed to finish this project,
          %        in addition to the present application.
          %   ----> leave empty if you do not intend to submit further
          %         proposals in future semesters for this project.
          % Only integer/real numbers (no blanks, no LaTeX-code) !
%
% Please, be careful when filling in the proposal, and provide complete
% information regarding previous applications. Help the TAC by supplying
% the requested info (accurate and complete).
%
% Specifically, supply the number of formerly granted nights for 
% programmes directly related to the present application.
%
\ObsTimeRange{}{}
        % best date range for observations {from} {to}
        % Format to ease electronic processing: dd.mm.yy (no blanks !)
        %
        % examples:
        %  {15.11.99}{15.5.00}  i.e. no limit in  WS99
        %  {1.2.00}{15.4.00}    i.e. beginning Feb. - mid-Apr. 2000
        %
        % Any scheduling constraints should be given under item 11.
\LST{}{}
%       Optimum range in local sideral time (LST) in hours {from}{to}
%       Format to ease electronic processing: hh:mm
%                 (e.g. {5:30}{10:00}, no blanks allowed!)
%
% ========================== p a g e  2 =============================
%
\begin{ObservingProgram}
%
%  Scientific justification
%  A maximum of 1 page text (no changes to font size should be made!)
%  An additional page is at your disposal for pictures and tables to
%  support your application!
%
%  Please describe the following:
%
%     -- outline of astrophysical problem
%     -- scientific aim of the observations and what the novelty is,
%     -- own previous work in this context,
%     -- only in case of MPIA GTO proposals: Strategic relevance for MPIA
%        (in this case please uncomment the corresponding subsection line)
%     -- layout of the observation.
%
%  In the last point please explain specifically how the
%  observations planned will lead to the projected aim, i.e. the
%  answer to the scientific questions.
%
%  For long-term projects, nights allocated thus far have to be given
%  (item 13) as well as the number of nights needed to finish the
%  programme (item 6). Especially the results reached so far have to
%  be presented under item 8.
%
%  When wording your application, please take into consideration the
%  following: Our committee consists of only 7 referees (HST has
%  about 10x as many!). Its is, therefore, evident that we do not
%  always have a specialist for each and every small area of interest.
%  For this reason you should present aim and previous work in such a
%  way that any experienced astrophysicist can follow your arguments
%  (e.g. do not use unusual abbreviations, known to only a chosen few).
%  Papers not yet published should be handed in as preprints (2 copies,
%  one for each referee). As there is a large number of applications to
%  be surveyed it is unreasonable to have to consult the web to be able
%  to understand the background and previous work of an application!
%  Reference to papers in preprint-servers, therefore, is pointless.
%
%  Please do not change the layout of the scientific justification section
%
\subsection*{Astrophysical context}
\subsection*{Immediate aim}
\subsection*{Previous work}
%\subsection*{Strategic relevance for MPIA}  %Only for MPIA GTOs
\subsection*{Layout of observations}
\end{ObservingProgram}
%
% ========================== p a g e  3 =============================
%
% This page is only for pictures and tables in support of the
% application. It must not be used for additional text!
%
% The following lines give an example of how to insert a single-column
% picture. Pictures that expand over both columns can be inserted
% likewise, with only the caption remaining single-column. When using
% the LaTeX-commando \begin{figure*} allowing a two-column caption,
% unfortunately an unwanted page-break occurs.
% Therefore please do not use this feature!
%
% Do not use a path to the PostScript-File. This will obviously
% not work during the LaTeX run at CAHA!
%
%\begin{SupportingMaterial}
%\begin{figure}
%\includegraphics[width=8.3cm,angle=0,clip=true]{image1.eps}
%\caption{\label{image1}Text for image 1}
%\end{figure}
%\end{SupportingMaterial}
%
% ========================== p a g e  3a ===========================
%
% Description of the current logistics for PhD thesis work
%             and status report of long-term projects
%             or large programmes (more than 10 nights per semester)
%
%\begin{Logistics}
%
%\end{Logistics}
%
% ========================== p a g e  3b =============================
%
% Backup project:
% Projects with special observing requirements (exceptionally good
% seeing, photometric conditions etc.) have to present a fully
% adequate backup programme (for details see
%        http://www.caha.es/CAHA/Applications)
%
% The same comments as under item 8 above are applicable.
%
%\begin{BackupProgramm}
%\subsection*{Astrophysical context}
%\subsection*{Immediate aim}
%\subsection*{Previous work}
%\subsection*{Layout of observations}
%\end{BackupProgramm}
%
% ========================== p a g e  3c =============================
%
% This page is only for pictures and tables supporting the
% backup programme. It must not be used for additional text!
%
%\begin{BackupSupportingMaterial}
%\begin{figure}
%\includegraphics[width=8.3cm,angle=0,clip=true]{image1.eps}
%\caption{\label{image1}}
%\end{figure}
%\end{BackupSupportingMaterial}
%
% ========================== p a g e  4 ==============================
%
% If you wish to use a different heading instead of the brightness in
% the 4th column of the object table below (something more
% characteristic for your application, e.g. the redshift) you may
% change the text of the column-heading via the command
%   \def\HeadLine{new heading}, e.g.
%   \def\HeadLine{redshift\newline of the  QSOs},
% which you insert here (before the \begin{Targets} command).
%
%\def\HeadLine{}
%
\begin{Targets}
%
%--------------------------------------------------------------------
%  List only those objects scheduled for observation during the span
%  of time applied for.
%
%  Please limit the number of targets to a maximum of 30. If 
%  the actual list is longer, provide a subsample that includes 
%  the most representative examples and covers the whole RA range. 
%
%  Pay attention to observability and good use of the night!
%--------------------------------------------------------------------
%
% Examples of format
%        (footnotes to the table are possible with \footnote{}):
%
% Name & \RA{h}{m}{s}{fract s} & \DEC{d}{'}{"} & mag & priority \\
%      & \RA{}{}{}{} & \DEC{}{}{} & & \\
%
\end{Targets}
%
\CommentsSample{}
%
%--------------------------------------------------------------------
%       Comments on the selection of the target sample.
%       Please indicate, if not done in the general description,
%       why these special targets have been selected, and in case
%       they have been studied already by other groups, why
%       it is justified to re-observe them.
%--------------------------------------------------------------------
%
\CommentsArchive{}
%
%--------------------------------------------------------------------
%       Please verify whether data of your selected objects,
%       taken in a similar observing configuration, are already
%       available in the Calar Alto archive:
%             http://caha.sdc.cab.inte-csic/calto
%       If so, please justify why new observations are necessary.
%--------------------------------------------------------------------
%
% ========================== p a g e  5 =============================
%
\TimeJustification{}
%       Justification for the amount of time applied for.
%       Please indicate also why this special telescope/
%       instrument is needed or particularly suitable.
%
\SchedulingConstraints{}
%       Leave empty if there are no restrictions.
%
%       Otherwise, give the constraints and/or restrictions
%       which are important for scheduling your observations.
%       Please be brief here!
%       Examples:
%               Before 3.5m-observations !
%               Not between ... and ... !
%               Simultaneously to HST-observations at ... !
%
\ObsExperience{}
%       Observational experience regarding the project applied for
%
\begin{Publications}
            % Results and publications of campaigns during
            % the past three years in form of a table (see example).
            % ***** Please remain within the given format ******
            % In the last column indicate the corresponding
            % reference under item 14 and there under item
            % \BibliographieListen in argument #2 list the full
            % quotation (including title).
            %
            % With the optional command \StatusOfProjects a short
            % summary of projects carried out during the last years on
            % Calar Alto may be added to the table in support of this
            % application.
% Columns of table:
% Tel. & instrument & proposal ID & period & nights & success [%] & publications
% Example:
% 3.5m &   PMAS     & F11-3.5-099 & Jan 11 &   3    &   33\%  & \cite{CA-1}\\
% 2.2m &   CAFOS    & H10-2.2-099 & Jul 10 &   5    &   85\%  & \cite{CA-2}\\
%
%\StatusOfProjects{}
%
% Please, be careful when filling in the proposal, and provide complete
% information regarding previous applications. Help the TAC by supplying
% the requested info (accurate and complete).
%
\end{Publications}
%
%
% ========================== p a g e  6 =============================
%
\BibliographyLists{auto}{}{}
%\BibliographyLists{manuell}{}{}
%
% ------------------------------------------------------------------
% The bibliographical details in argument 2 and 3 of this call above
% refer to item 8 resp. 13 of the application.
%
% If as first argument {auto} is used, all references within the
% text are carried out via LaTeX-command \cite{label}. The references
% have then to be given as second and third argument as follows:
%
% 2. argument =
%      references relating to scientific justification (item 8):
%{\bibitem{label}{reference}
% \bibitem{label}{reference}
%    ...
%}{
% These two brackets separate the 2nd and 3rd argument.
% 3. argument =
%      references to past observations on Calar Alto (item 13):
%\bibitem{label}{reference}
%\bibitem{label}{reference}
%    ...
%}%  closes 3rd argument
%
% When using the Auto-Modus the entries to (8) receive
% consecutive numbers <100, those to (13) numbers >99.
%
% Example:
%
% If the text gives: "... produces  $H_0=10$ \cite{Mei76} ...",
% insert in the 2. argument of \BibliographyLists the following:
% {    ...
%\bibitem{Mei76}{Meier (1976): {\em The Hubble-constant},
%        A\&A {\bf 123}, 1024}
%      ...    }
%
% If the references are inserted manually into the text and the
% literature list is formatted manually, the call has to be as
% follows:
%
%\BibliographyLists{manual}{references to 8}{references to 13}
%
% In this case the applicant has to take care of the necessary
% cross-references himself. The information under item 8 will
% automatically be separated by a horizontal line from those
% under item 13.
%
% Example:
%\BibliographyLists{manual}%
%{Meier (1976): {\em the Hubble-constant}, A\&A {\bf 123}, 1024\\
% Schmidt (1963): {\em Identification of 3C\,273}, Nature {\bf 197}, 10
%}{Ich (1997): {\em the XYZ-constant}, ApJ {\bf 123}, 987\\
% Ich und Du (1998): {\em Die Entfernung zu M\,31}, PASP {\bf 145}, 12}
%
% A T T E N T I O N:
% ================
%
% A mixture of the two modi in the arguments 2 und 3 is not possible!
% That is either  ** ALL **  citations (in the scientific justification
% as well as those papers going back to observations on Calar Alto) are
% done by \cite{mark} or ** ALL **  citations and references are
% inserted manually.
%
% ========================== p a g e  7 =============================
%
%\TravelFunding{}
%       Uncomment if you intend to apply for travel funds from DFG.
%       The argument remains empty if only one observer will apply
%       for travel funds at the DFG.
%
%       The deadlines for DFG funding are:
%             15.11. for the spring semester
%             15.05. for the autumn semester
%
%       !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
%       ! Please, DEFINITELY give as argument the reason if it is !
%       ! planned to apply for travel funds for TWO OBSERVERS!    !
%       !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
%
%  Applicants from Max Planck institutes cannot apply for DFG funding!
%
\noTravelFunding
%       Comment out, if you will apply for DFG funds.
%
%
% >>>> Please note that the observing data will be made public by the Virtual
%      Observatory (VO), Madrid, after a proprietary period of one year after
%      the end of the observation. This does not apply for IAA and MPIA
%      guaranteed time. 
%
% ========================== p a g e  8 =============================
%
\MinimumObservingRequirements
        {}  % worst tolerable seeing ["],  e.g. {2.5}
        {}  % minimum transparency [%],  e.g. {50}
        {}  % maximum airmass,  e.g. {1.5}
        {}  % photometric conditions required [yes/no]
        {/} % maximum moon phase [0-1 in units of illuminated fraction]
            %   / min. distance to object [degrees],  e.g. {0.8/30}
        {/} % min./max. time difference between individual observations
            %   in case of service observation [days/days], e.g. {2/10}
\Instrumentation{}{}{}{}{}{}{}
%               THE ARGUMENTS HAVE CHANGED ! (see below)
%               Specification of instrumentation
%               Note that always 7 arguments have to be given!
%               Arguments not needed have to be given as {} !
%
%               Possible arguments are listed below ---
%               behind \EndOfApplication --- !
%
\EndOfApplication

 The rest of this file will not be processed by LaTeX!

In the following we provide

   -- list of all valid entries for \Instrumentation

   -- frame for your bibliographic data base entries

++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++

Possible combinations for the arguments in \Instrumentation

              --> Capitalization is important! <--

Each column for an argument stands for one component.
The sequence of the information has to strictly remain as given here!

The applicant himself is responsible for correct placement of the
marks on page 8 ! Mistakes, inconsistencies in the style-file and
possible misunderstandings of the following information are not excluded.
I therefore ask for feed-back when problems arise (uthiele@caha.es)!

When gratings/grisms or own instrumentation is required, the grating/grism has
to be specified as text explicitly or the instrument has to be characterized
shortly.

3.5m-telescope:
===============

argument_1      argument_2      argument_3      argument_4     argument_5 


{LAICA}         {filters}

{OMEGA 2000}    {filters}

{TWIN}          {mirror}        {blue grating}  {red grating}
                {beamsplitter}

{MOSCA}         {filters}       {grisms}

{PMAS}          {PPAK}          {}              {grating}
                {LensArray}     {0.5}           {grating}
                {LensArray}     {0.75}          {grating}
                {LensArray}     {1.0}           {grating}

{OWN}           {description}

2.2m-Teleskop:
==============

{CAFOS}         {standard}      {filters}       {grisms}   
                % Standard = neither Polarizer nor Etalon
                {eta}           {filters}       {grisms}
                {pol}           {filters}       {grisms}
                                

{MAGIC}         {WideField}
                {HighResolution}      {R270}

{CAFE}
{BUSCA}         {filters}
{ASTRALUX}      {filters}

{OWN}           {description}


++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++