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Search features of digital libraries
Published 2000-01-01“…Traditional on-line search services such as Dialog, DataStar and Lexis provide a wide range of search features (boolean and proximity operators, truncation, etc). …”
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Volcanic Ash Region Path Planning Based on Improved A-Star Algorithm
Published 2022-01-01“…The verification results show that the improved A-star algorithm optimizes the flight path planning in the volcanic ash area and has the advantages of less search nodes, a small search range, and short computing time.…”
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Long-term Evolution of Sco X-1: Implications for the Current Spin Frequency and Ellipticity of the Neutron Star
Published 2025-01-01“…Our estimation of current ν values can improve the CW search sensitivity.…”
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Detecting the Black Hole Candidate Population in M51’s Young Massive Star Clusters: Constraints on Accreting Intermediate-mass Black Holes
Published 2025-01-01“…Jansky Very Large Array to search for any evidence of accreting black holes in young massive star clusters in the nearby galaxy M51. …”
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Upper Limits on Stellar Companions to the Kepler-34 and Kepler-35 Systems
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COSMIC’s Large-scale Search for Technosignatures during the VLA Sky Survey: Survey Description and First Results
Published 2025-01-01“…To test this postprocessing pipeline, we searched toward 511 stars from the Gaia catalog with coherent beams. …”
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A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at z = 4–6
Published 2025-01-01“…We obtained JWST/NIRCam grism spectroscopy and ALMA 1.2 mm continuum map along 25 independent quasar sightlines, covering a total survey area of ∼35 arcmin ^2 where we search for dusty star-forming galaxies (DSFGs) at z = 0–7. …”
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Exoplanet science with SPIRou: near-infrared precision velocimetry and spectropolarimetry
Published 2023-03-01“…High-precision radial-velocity measurements in the near-infrared allow one to search for exoplanet signals around the lowest-mass stars, including young ones. …”
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A Hybrid Dynamic Path-Planning Method for Obstacle Avoidance in Unmanned Aerial Vehicle-Based Power Inspection
Published 2025-01-01“…In the sampling-point search, a target-biased search strategy is introduced to guide the random tree growth toward the target point, while an attractive function is added to enhance search efficiency. …”
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Revisiting Near-infrared Features of Kilonovae: The Importance of Gadolinium
Published 2025-01-01“…The observation of the kilonova AT2017gfo and investigations of its light curves and spectra confirmed that neutron star mergers are sites of r -process nucleosynthesis. …”
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A Multiple-detection-heads Machine Learning Algorithm for Detecting White Dwarfs
Published 2025-01-01“…White dwarfs (WDs) are the ultimate stage for approximately 97% of stars in the Milky Way and are crucial for studying stellar evolution and galaxy structure. …”
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3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
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An HST Transmission Spectrum of the Closest M Dwarf Transiting Rocky Planet LTT 1445Ab
Published 2025-01-01“…In doing so, we uncover an ultraviolet (UV) flare on the neighboring star LTT 1445C that is completely invisible at optical wavelengths; we report one of the first simultaneous near-UV/optical spectra of an M dwarf flare. …”
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LAMOST Reveals Long-lived Protoplanetary Disks
Published 2025-01-01“…In this work, we perform a systematic search for aged young stellar objects still surrounded by protoplanetary disks in the M-star catalog from the LAMOST archive. …”
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Adverse Reactions Caused by Biomaterials Used in Dentistry
Published 2023-07-01“…The equation used for the search was: (Biocompatible Dental Materials) and (Side Effects). …”
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Direct imaging of exoplanets: Legacy and prospects
Published 2023-06-01“…Understanding how giant and terrestrial planets form and evolve, what is their internal structure and that of their atmosphere, represents one of the major challenges of modern astronomy, which is directly connected to the ultimate search for life at the horizon 2030–2050. However, several astrophysical (understanding of the formation and physics of giant and terrestrial exoplanets), biological (identification of the best biomarkers) and technological (technical innovations for the new generations of telescopes and instruments) obstacles must be overcome. …”
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