205 | | Leave {{{n}}} alone. |
| 205 | Leave {{{n}}} alone. Note: |
| 206 | |
| 207 | * {{{n}}}, the coefficient, is the height of the Gaussian's peak. |
| 208 | * {{{c}}} is the standard deviation, and controls the spread of the peak. Here we have it spread at 5.0E-7 Angstroms, which is essentially corresponds to the energy of a photon in a vacuum (gamma rays). This is similarly the case with {{{b}}} |
| 209 | * {{{b}}} is the position of the center of the Gaussian peak. |
| 210 | * Thus our emission is within the realm of visible light in the spectrum. |
| 211 | * We simply choose {{{x}}} based on what is recommended in the video tutorial. |