Explainer · 0:39 · silent, with on-screen words
Watch noise melt away as 1, 4, 16 and 64 frames of the Southern Cross are stacked, and see the signal-to-noise ratio grow as the square root of the number of frames.
Shows a simulated 32° by 18° field around the Southern Cross: real star places and magnitudes (Yale Bright Star Catalogue), seeded random noise in every frame.
From the lesson Your First Astrophoto Session.
A silent explainer with a simulated image, said so on screen. It shows a 32° by 18° patch of sky around the Southern Cross with 67 stars where the Yale Bright Star Catalogue puts them and as bright as it says, with fresh random noise in every frame, and averages 1, 2, 4 ... 64 frames.
The signal-to-noise ratio of a magnitude 5.0 star, measured on the stacked pixels (its signal over the measured noise of the background): 1 frame 1.5, 2 frames 2.1, 4 frames 3.0, 8 frames 4.3, 16 frames 6.0, 32 frames 8.4, 64 frames 12.0. It grows as the square root of the number of frames: 4 frames double it, 16 frames quadruple it.