![2.3.2 Early PSF/LSF model‣ 2.3 Calibration models ‣ Chapter 2 Astrometric and photometric pre-processing ‣ Part II Gaia data processing ‣ Gaia Data Release 2 Documentation release 1.2 2.3.2 Early PSF/LSF model‣ 2.3 Calibration models ‣ Chapter 2 Astrometric and photometric pre-processing ‣ Part II Gaia data processing ‣ Gaia Data Release 2 Documentation release 1.2](https://gea.esac.esa.int/archive/documentation/GDR2/Data_processing/chap_astpre/sec_cu3pre_cali/cu3/Figures/Pre/LsfPsf/FOV1_ROW4_AF5_2D_PSF.png)
2.3.2 Early PSF/LSF model‣ 2.3 Calibration models ‣ Chapter 2 Astrometric and photometric pre-processing ‣ Part II Gaia data processing ‣ Gaia Data Release 2 Documentation release 1.2
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Figure 4 from A postprocessing method for spatially variant point spread function compensation | Semantic Scholar
![PDF] A postprocessing method for spatially variant point spread function compensation | Semantic Scholar PDF] A postprocessing method for spatially variant point spread function compensation | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/bd60b771262980cff6f27ae159d7496dbeef489f/12-Figure1-1.png)
PDF] A postprocessing method for spatially variant point spread function compensation | Semantic Scholar
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Track of the PSF centroid of the original simulated star (black) and... | Download Scientific Diagram
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Point spread function estimation from projected speckle illumination | Light: Science & Applications
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Fluorescence microscopy point spread function model accounting for aberrations due to refractive index variability within a specimen
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Deconvolution with shift-variant PSF: (a) simulation of an observation... | Download Scientific Diagram
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