One starts from the polynomial
      
      and extends one by one with
      
      until the final polynomial defining this rule is reached.
      Note: Polynomials might be truncated due to size!
      The complete polynomials are included in the download.
    
| Node (ball center) | Error (ball radius) | 
|---|---|
| 1.7320508075688772935 - 3.5221018286841338275e-133j | 2.08e-63, 2.08e-63j | 
| -0.7071067811865475244 - 6.4066659045859229582e-145j | 2.81e-63, 2.81e-63j | 
| -1.7320508075688772935 + 1.3336552496910464901e-161j | 2.08e-63, 2.08e-63j | 
| -1.2338789709326766683e-178 + 9.8710317674614133463e-178j | 4.97e-177, 4.97e-177j | 
| 0.7071067811865475244 + 0j | 1.14e-63, 1.14e-63j | 
| Weight (ball center) | Error (ball radius) | 
|---|---|
| 0.033333333333333333333 + 2.6435323705765884781e-134j | 1.49e-30, 1.95e-62j | 
| 0.3 - 2.8879657837259655288e-134j | 1.58e-29, 1.91e-61j | 
| 0.033333333333333333333 + 3.3891440648088426533e-135j | 9.12e-31, 1.22e-62j | 
| 0.33333333333333333333 + 6.7782881297254947467e-134j | 1.06e-29, 1.33e-61j | 
| 0.3 - 6.8727691230570019613e-134j | 4.69e-30, 5.39e-62j | 
All rules of Hermite (physicists') type can be downloaded here packed into a single file.