Hot pixel (telescopes) explained

A hot pixel or bright dot defect is a pixel that outputs many more electrons than others at the same input signal in a charge-coupled device (CCD) or CMOS sensor. In the simulated image,[1] the hot pixels are the sources of the salt-and-pepper noise. In the definition of the HST ACS, A pixel above 0.14 e¯/pixel/second is considered a "hot" pixel.[2]

A warm pixel is a pixel that has negative bias values. In the definition of the Hubble Space Telescope, a pixel below the hot pixels range but above 0.06 e¯/pixel/second is considered a "warm" pixel.

See also

References

  1. Hroch . Filip . 2000-02-23 . The robust detection of stars on CCD images . Experimental Astronomy. 9 . 4 . 251–259 . 10.1023/A:1008195518637 . astro-ph/0002435 . 13504731 .
  2. Web site: 4.3 Dark Current, Hot Pixels, and Cosmic Rays - HST User Documentation . 2023-03-09 . hst-docs.stsci.edu.