excrete
发表于 2025-3-25 06:26:00
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Enliven
发表于 2025-3-25 11:19:24
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ENACT
发表于 2025-3-25 15:40:54
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insurgent
发表于 2025-3-25 18:11:43
Tomographic Imaging of Stellar Surfaces and Interacting Binary Systems,ps allow us to study surface activity, spot and magnetic field variability and map irradiation patterns on secondaries of cataclysmic variable systems (CVs). During the past few years, magnetic fields have been detected and studied on stars throughout the Hertzsprung-Russell diagram. Spectropolarime
Omniscient
发表于 2025-3-25 23:23:25
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Exuberance
发表于 2025-3-26 00:08:09
Astronomy at High Angular Resolution978-3-319-39739-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
Aggrandize
发表于 2025-3-26 08:13:53
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合群
发表于 2025-3-26 11:44:40
H.-J. Cantow,G. Dall’Asta,H. A. Stuarty Imaging is a passive observing technique with individual integration times comparable to the atmospheric coherence time. Thanks to the advent of essentially noise free “Electron multiplying CCD” detectors, Lucky Imaging saw a renewed interest in the past decade. It is now routinely used at a numbe
Communal
发表于 2025-3-26 14:55:33
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intelligible
发表于 2025-3-26 19:40:43
H.-G. Elias,R. Bareiss,J. G. Wattersonux, zero read-noise regime and offering superior calibration in the bright regime. Since adaptive optics has become commonplace on large telescopes, the key advantage of aperture-mask interferometry is in calibration, particularly of low spatial-frequency phase aberrations that cause quasi-static sp