%% LaTeX template for the DDT, science, and technical justification and
%% feasibility to be submitted for short-cadence TESS observations under
%% the Director's Discretionary Targets program. This template is based on
%% the TESS GI template.
%%
%% TESS Guest Investigator Proposal DDT template 
%% (based on the Cycle 1 template)
%% V1.0
%% 2018-10-19


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\newcommand{\tess}{{\it TESS}}
\newcommand{\jwst}{{\it JWST}}
\newcommand{\kepler}{{\it Kepler}}
\newcommand{\ktwo}{{K2}}
\newcommand{\hst}{{\it HST}}
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% enter the proposal title here
\title{The Title of this DDT Proposal for Great New 2-minute Targets}

% enter the proposers, including at least one contact email, here
\author{Proposer \#1 (Institution | email), Proposer \#2 (Institution), ...}
%\date{}

\begin{document}
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\noindent{The recommended sections for a TESS DDT proposal are shown below. The PDF of the proposal is limited to 2 pages, including text, figures, and references. Target tables should be submitted as a separate machine-readable text file containing the following columns: TIC ID, relative priority (0.0-1.0,highest), keywords (separated by semicolon).


\section{DDT Justification}

Summarize why this program requires allocation of Directors Discretionary Targets for observation at 2-minute cadence. Please explain why these targets should be included before the next TESS Guest Investigator call and why they were not proposed in the previous Guest Investigator call.

\section{Scientific Justification}

Provide text and figures that justify the scientific merit of the proposed \tess\ short-cadence observations. The proposal will be reviewed by the TESS PI, a science expert selected by the TESS PI, and the science operations team. Please provide sufficient background to be understood by a broad audience of astronomers.

\section{Target Justification and Feasibility}

Summarize the target sample and demonstrate why 2-minute cadence is necessary. Demonstrate that the proposed \tess\ investigations are feasible; consider the \tess\ survey strategy, target observability, and required signal-to-noise, etc. The \tess\ Science Support Center (\href{https://heasarc.gsfc.nasa.gov/docs/tess/}{TSSC}) makes several tools available to help estimate these quantities. Indicate the expected number of sources bright than 7 magnitudes, as these may require extra-large pixel stamps.

\section{References}

List of references. 

\end{document}