HI Spectrum

HISpectrum demonstrates the necessity for integration of the weak signals received by a radio telescope

Observe the spiral galaxy NGC 2456 for 1 to 3600 seconds

Enter your observation time:
seconds

Signal to Noise ratio: 1.51651636734

no signal, too much noise

Flux Density (Jansky)HISpectrum graph

Velocity (km/sec)
You can leave a response, or trackback from your own site.

Leave a Reply