Monday | Tuesday | Wednesday | Thursday | Friday |
---|---|---|---|---|
May 19 Project Proposal |
May 20 No Class |
May 21 Exp. Design |
May 22 Research |
May 23 Reseach Data |
May 26 No School |
May 27 No School |
May 28 Data Collect |
May 29 Data Collect |
May 30 Data Collect |
Jun 2 No Class |
Jun 3 Data Analysis |
Jun 4 Data Analysis |
Jun 5 Lab Drafting |
Jun 6 No Class |
Monday | Tuesday | Wednesday | Thursday | Friday |
---|---|---|---|---|
Jun 9 Lab Drafting |
Jun 10 Lab Peer Edits? |
Jun 11 Poster |
Jun 12 No Class |
Jun 13 Lab Report Due Poster |
Jun 16 Poster Due |
Procedure written
Continue Research
Start Data Collection
Complete Data Collection
Complete Data Analysis and
Start Writing Lab
Write Lab Report
(finish by Wednesday)
Write Lab Report
(finish by Wednesday)
\documentclass{article}
\begin{document}
First document. This is a simple example, with no
extra parameters or packages included.
\end{document}
\documentclass[12pt, letterpaper]{article}
\title{My first LaTeX document}
\author{Hubert Farnsworth}
\date{August 2022}
\begin{document}
\maketitle
We have now added a title, author and
date to our first \LaTeX{} document!
\end{document}
Some of the \textbf{greatest}
discoveries in \underline{science}
were made by \textbf{\textit{accident}}.
\documentclass{article}
\usepackage{graphicx}
\graphicspath{{images/}}
\begin{document}
\begin{figure}[h]
\centering
\includegraphics[width=0.75\textwidth]{mesh}
\caption{A nice plot.}
\label{fig:mesh1}
\end{figure}
As you can see in figure \ref{fig:mesh1},
the function grows near the origin. This
example is on page \pageref{fig:mesh1}.
\end{document}
In in the middle of a block of text:
\documentclass[12pt, letterpaper]{article}
\begin{document}
In physics, the mass-energy equivalence is stated
by the equation $E=mc^2$, discovered in 1905 by Albert Einstein.
\end{document}
In physics, the mass-energy equivalence is stated by the equation
\documentclass[12pt, letterpaper]{article}
\begin{document}
The mass-energy equivalence is described by the famous equation \[ E=mc^2 \] discovered in 1905 by Albert Einstein.
In natural units ($c = 1$), the formula expresses the identity
\begin{equation}
E=m
\end{equation}
\end{document}
Symbols | and | Code | |
---|---|---|---|
\alpha A |
\nu N |
\eta H |
\tau T |
\beta B |
\xi \Xi |
\zeta Z |
\sigma \Sigma |
\gamma \Gamma |
o O |
\epsilon E |
\rho \varrho P |
\delta $\Delta |
\pi \Pi |
\chi X |
\upsilon \Upsilon |
\iota I |
\phi \Phi |
\kappa K |
\theta \Theta |
\lambda \Lambda |
\psi \Psi |
\mu M |
\omega \Omega |
E = mc^2
F_N
or F_{normal}
a = \frac{\Sigma \vec{F}}{m}
\frac{num}{dem}
\sin\theta \cos\theta \tan\theta
Write Lab Report
(finish by Wednesday)
Finish Lab Report
Start Poster