Using the medical image processing package, ImageJ, for astronomy
, 2006 15 pages, 6 figures; Published in ...
West, Jennifer L., Cameron, Ian D.
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The Infrared Imaging Spectrograph (IRIS) for TMT: Data Reduction System [PDF]
, 2016 IRIS (InfraRed Imaging Spectrograph) is the diffraction-limited first light instrument for the Thirty Meter Telescope (TMT) that consists of a near-infrared (0.84 to 2.4 $\mu$m) imager and integral field spectrograph (IFS). The IFS makes use of a lenslet
Chapin, Edward L. +17 more
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A Simple but Powerful Method to Reduce Background Noise in Celestial Gamma-Ray Images
The Astrophysical JournalReducing background noise is essential for clear data analysis and signal detection. In this study, we introduce a novel denoising algorithm tailored for gamma-ray astronomical data, utilizing local density sampling techniques.
H. Hedayati Kh., M. Soor, F. Akhondi
doaj +1 more source
Data Provenance and Management in Radio Astronomy: A Stream Computing Approach [PDF]
, 2011 New approaches for data provenance and data management (DPDM) are required for mega science projects like the Square Kilometer Array, characterized by extremely large data volume and intense data rates, therefore demanding innovative and highly efficient
Biem, Alain +4 more
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Long-Term Continuous Double Station Observation of Faint Meteor Showers
Sensors, 2016 Meteor detection and analysis is an essential topic in the field of astronomy. In this paper, a high-sensitivity and high-time-resolution imaging device for the detection of faint meteoric events is presented. The instrument is based on a fast CCD camera
Stanislav Vítek +3 more
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Parametric high resolution techniques for radio astronomical imaging
, 2008 The increased sensitivity of future radio telescopes will result in requirements for higher dynamic range within the image as well as better resolution and immunity to interference.
Ben-David, Chen, Leshem, Amir
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Benchmarking Dimensionality Reduction Methods for High-dimensional ALMA Image Cubes
The Astronomical JournalHigh-dimensional astronomical data cubes provide a wealth of spectral and structural information that can be used to study astrophysical and chemical processes.
Haley N. Scolati +3 more
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WFST Astrometric Calibration. I. Modeling Global Geometric Distortion with Zernike Polynomials
The Astronomical JournalAccurate modeling of geometric distortion (GD) is essential for precise astrometric calibration in wide-field imaging surveys. We present a self-calibration method based on Zernike polynomials, applied to imaging data from the Wide Field Survey Telescope
Chao Yang +23 more
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Infrared Astronomical Satellite (IRAS) Scientific Data Analysis System [PDF]
, 1980 The Jet Propulsion Laboratory's Scientific Data Analysis System will process Infrared Astronomical Satellite data and produce a catalog of perhaps a million infrared sources in the sky, as well as other vital information for astronomical ...
Duxbury, John H., Soifer, B. T.
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Influence of the Lossy Compression JPEG2000 standard on the Deformation of PSF
Acta Polytechnica, 2011 This paper deals with the influence of lossy compression algorithms on the deformation of the point spread function (PSF) of imaging systems in astronomy.
P. Páta
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