Presentation Content for the BAROSpection seminar
Stars are AMAZING!!!

Behold the Power of STARS

Light & Matter and Electromagnetism
- What is Light?
- Electromagnetic Waves
- Photons & Matter
- What is a Blackbody

- Electromagnetic Spectrum
- Modeling a Black Body
- Waves & Particles
- Class Jupyter Notebook - Light Basics
Spectroscopy
- What is Spectroscopy
- Types of Spectra
- Continuous Spectrum
- Absorption Spectrum
- Emission Spectrum
- Source of Spectral Lines
- Calculating Balmer’s Constant
- Doppler Effect on Spectral Lines
- Jupyter Notebook - Absorption & Emission Spectra
Star Properties
- Star Types
- What can you learn from Star Spectra
- HertzSprung Russell Diagram (HRD)
- HRD Explorer
- Plot an HRD for Sun’s 100 Parsec neighbourhood
- Final Project - Mystery Stars & HRD
- HRD Presentation
Obtain Live Spectra from the BARO Telescope
- Spectral Grating configuration on BARO
- Selecting Targets in the Solar Neiborhood
- Create Target List for Hot & Cool Stars & Nebulae
- Schedule to obtain Spectra
- Calibrate using RSpec
Analyze & Publish Spectral Images using RSpec
- Annotated HR Diagram
- Use RSpec to Analyze Spectral Lines
- Measure Wavelenghts & Frequencies
- Measure Shift in Spectral Lines
- Compare against NIST Standard
- Publish your results in a Jupyter Notebook
- Post examples to RSpec website