Results 41 to 50 of about 5,542,325 (204)
High-resolution magnetic susceptibility and % CaCO3 records (5 to 10 cm sampling interval) are used to track astronomical cycles from a Lower Berriasian record from central Tunisia.
Hamdi Omar +4 more
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Robotic fiber positioner (RFP) arrays are essential for multiobject spectroscopic telescopes. To improve the survey efficiency, they are densely arranged on the focal planes with overlapped patrol areas, guaranteeing full coverage and increasing the ...
Zengxiang Zhou +6 more
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Astronomia ex machina: a history, primer and outlook on neural networks in astronomy
In this review, we explore the historical development and future prospects of artificial intelligence (AI) and deep learning in astronomy. We trace the evolution of connectionism in astronomy through its three waves, from the early use of multilayer ...
Michael J. Smith, James E. Geach
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Bayesian Doppler Imaging: Simultaneous Inference of Surface Maps and Geometric Parameters
We present a fully Bayesian, pixel-based Doppler imaging framework that enables the simultaneous inference of surface brightness maps and geometric parameters, including the inclination i and equatorial rotation velocity v _rot , from high-resolution ...
Yamato Ureshino +3 more
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Empirical modeling of tropospheric delays with uncertainty [PDF]
Accurate modeling of tropospheric delay is important for high-precision data analysis of space geodetic techniques, such as the Global Navigation Satellite System (GNSS).
J. Wang +6 more
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The Influence of Acquisition Techniques on the Compilation of Astronomical Data [PDF]
With the increasing use of electronic rather than photographic data collection, and on-line minicomputers at the telescope, two factors will necessitate a reconsideration of the way in which data are stored at the telescope.1) Many of the electronic data collecting methods produce data in a final or semifinal (digital) form and usually with a large ...
openaire +1 more source
A Hierarchical Point-spread Function Reconstruction Method
Reconstruction of the point-spread function (PSF) plays an important role in many areas of astronomy, including photometry, astrometry, galaxy morphology, and shear measurement.
Pedro Alonso, Jun Zhang, Cong Liu
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Primary beam calibration for commensal telescopes utilizing offset optics
IntroductionAccurate primary beam calibration is essential for precise brightness measurements in radio astronomy. The VLA Low-band Ionosphere and Transient Experiment (VLITE) faces challenges in calibration due to the offset Cassegrain optics used in ...
Emil Polisensky +3 more
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EMU:Evolutionary Map of the Universe [PDF]
EMU is a wide-field radio continuum survey planned for the new Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep (rms ∼10Jy/beam) radio continuum survey of the entire Southern sky at 1.3GHz ...
Ian Smail +279 more
core +1 more source
Commercial flatbed scanners have the potential to deliver a quick and efficient means of capturing the scientific content of spectra recorded on photographic plates.
T. J. Davidge
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