The CHIRP algorithm was developed to process data collected by the very-long-baselineEvent Horizon Telescope, the international collaboration that in 2019 captured the black hole image of M87* for the first time. CHIRP was not used to produce the image,[6] but was an algebraic solution for the extraction of information from radio signals producing data by an array of radio telescopes scattered around the globe.[3][7] Stable sources (that don't change over short periods of time) can also gain signal by integrating the change at each location with the rotation of the earth.[3]: 915 Because the radio telescopes used in the project produce vast amounts of data, which contain gaps, the CHIRP algorithm is one of the ways to fill the gaps in the collected data.[8][9]
Evaluation
For reconstruction of such images which have sparse frequency measurements the CHIRP algorithm tends to outperform CLEAN, BSMEM (BiSpectrum Maximum Entropy Method), and SQUEEZE, especially for datasets with lower signal-to-noise ratios and for reconstructing images of extended sources. While the BSMEM and SQUEEZE algorithms may perform better with hand-tuned parameters, tests show CHIRP can do better with less user expertise.[10]
^ abKatherine L. Bouman, Michael D. Johnson, Daniel Zoran, Vincent L. Fish, Sheperd S. Doeleman, William T. Freeman (June 2016). "Computational Imaging for VLBI Image Reconstruction". IEEE Conference on Computer Vision and Pattern Recognition (CVPR). June 2016: 913–922. arXiv:1512.01413. Bibcode:2016cvpr.conf..913B – via Proceedings CVPR 2016 open access by Computer Vision Foundation.{{cite journal}}: CS1 maint: multiple names: authors list (link)
^ACM (Association for Computing Machinery), TechNews (June 6, 2016). "A Method to Image Black Holes". ACM News Service. Archived from the original on April 13, 2019. Retrieved April 13, 2019.