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Point spread function

About: Point spread function is a research topic. Over the lifetime, 8963 publications have been published within this topic receiving 153354 citations.


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Journal ArticleDOI
TL;DR: In this article, the authors describe a mission-independent wavelet-based source detection algorithm called WAVDETECT, which does not require a minimum number of background counts per pixel for the accurate computation of source detection thresholds.
Abstract: Wavelets are scaleable, oscillatory functions that deviate from zero only within a limited spatial regime and have average value zero. In addition to their use as source characterizers, wavelet functions are rapidly gaining currency within the source detection field. Wavelet-based source detection involves the correlation of scaled wavelet functions with binned, two-dimensional image data. If the chosen wavelet function exhibits the property of vanishing moments, significantly non-zero correlation coefficients will be observed only where there are high-order variations in the data; e.g., they will be observed in the vicinity of sources. In this paper, we describe the mission-independent, wavelet-based source detection algorithm WAVDETECT, part of the CIAO software package. Aspects of our algorithm include: (1) the computation of local, exposure-corrected normalized (i.e. flat-fielded) background maps; (2) the correction for exposure variations within the field-of-view; (3) its applicability within the low-counts regime, as it does not require a minimum number of background counts per pixel for the accurate computation of source detection thresholds; (4) the generation of a source list in a manner that does not depend upon a detailed knowledge of the point spread function (PSF) shape; and (5) error analysis. These features make our algorithm considerably more general than previous methods developed for the analysis of X-ray image data, especially in the low count regime. We demonstrate the algorithm's robustness by applying it to various images.

448 citations

Journal ArticleDOI
TL;DR: A new code for the deep analysis of stellar elds, designed for Adaptive Optics Nyquist- sampled images with high and low Strehl ratio is described, written in IDL language and organized in the form of a self-contained widget-based application.
Abstract: We describe a new code for the deep analysis of stellar elds, designed for Adaptive Optics (AO) Nyquist- sampled images with high and low Strehl ratio. The Point Spread Function (PSF) is extracted directly from the im- age frame, to take into account the actual structure of the instrumental response and the atmospheric eects. The code is written in IDL language and organized in the form of a self-contained widget-based application, pro- vided with a series of tools for data visualization and anal- ysis. A description of the method and some applications to AO data are presented.

443 citations

Journal ArticleDOI
01 Apr 1990
TL;DR: It is shown that the introduction of the concept of coarray provides a convenient and elegant framework within which many apparently isolated techniques for point-spread function or aperture synthesis can be understood.
Abstract: Systems of two-dimensional (2-D) imaging arrays and apertures are considered from the point of view of their performance in the imaging of spatially incoherent as well as coherent source distributions. Such systems find applications in radar, sonar, and ultrasound imaging, as well as in applications such as seismology and radio astronomy. For linear imaging techniques related to beamforming and based on the Fourier transform relationship between the source distribution and the aperture plane measurements, the point spread function of the system completely characterizes its performance. This function is determined by the geometry of the physical aperture or array as well as the weighting that can be applied to measurements. It is shown that the introduction of the concept of coarray, both for receive apertures in incoherent imaging and for transmit/receive systems in reflection-mode coherent imaging, provides a convenient and elegant framework within which many apparently isolated techniques for point-spread function or aperture synthesis can be understood. In addition to this unifying role, coarray concept gives new insight into the aperture synthesis process, which allows interesting new imaging techniques to be developed, especially in coherent imaging. >

431 citations

Journal ArticleDOI
TL;DR: It is demonstrated here that the detailed time dependence of the resulting trajectory of sample points determines the relative weight and accuracy with which image information at each spatial frequency is measured, establishing theoretical limitations on image quality achievable with a given imaging method.
Abstract: The fundamental operations of nuclear magnetic resonance (NMR) imaging can be formulated, for a large number of methods, as sampling the object distribution in the Fourier spatial-frequency domain, followed by processing the digitized data (often simply by Fourier transformation) to produce a digital image. In these methods, which include reconstruction from projections, Fourier imaging, spin-warp imaging, and echo-planar imaging, controllable gradient fields determine the points in the spatial-frequency domain which are sampled at any given time during the acquisition of data (the free induction decay, or FID). The detailed time dependence of the resulting trajectory of sample points (the k trajectory) determines the relative weight and accuracy with which image information at each spatial frequency is measured, establishing theoretical limitations on image quality achievable with a given imaging method. We demonstrate here that these considerations may be used to compare the theoretical capabilities of NMR imaging methods, and to derive new imaging methods with optimal theoretical imaging properties.

429 citations

Journal ArticleDOI
TL;DR: A fluorescence microscope that creates nearly spherical focal spots of 40–45 nm (λ/16) in diameter is introduced, which unravels the interior of cells noninvasively, uniquely dissecting their sub-λ–sized organelles.
Abstract: The resolution of any linear imaging system is given by its point spread function (PSF) that quantifies the blur of an object point in the image. The sharper the PSF, the better the resolution is. In standard fluorescence microscopy, however, diffraction dictates a PSF with a cigar-shaped main maximum, called the focal spot, which extends over at least half the wavelength of light (lambda = 400-700 nm) in the focal plane and >lambda along the optical axis (z). Although concepts have been developed to sharpen the focal spot both laterally and axially, none of them has reached their ultimate goal: a spherical spot that can be arbitrarily downscaled in size. Here we introduce a fluorescence microscope that creates nearly spherical focal spots of 40-45 nm (lambda/16) in diameter. Fully relying on focused light, this lens-based fluorescence nanoscope unravels the interior of cells noninvasively, uniquely dissecting their sub-lambda-sized organelles.

420 citations


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Performance
Metrics
No. of papers in the topic in previous years
YearPapers
2023151
2022289
2021312
2020414
2019391
2018420