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    Finding Lensed Radio Sources with the Very Large Array Sky Survey by Michael N. Martinez, Yjan A. Gordon, Keith Bechtol, Gillian Cartwright, Peter S. Ferguson, Miranda Gorsuch

    Published 2025-01-01
    “…Lensed radio sources have proven difficult to identify, in large part due to the limited depth and angular resolution of the previous generation of radio sky surveys, and, as such, only a few dozen lensed radio sources are known. …”
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    A new proposal for an easy-to-calibrate DNI clear-sky model: a performance analysis and validation in different geographical locations by César D. Sánchez-Segura, Manuel I. Peña Cruz

    Published 2025-01-01
    “…Derived from the above, in this work a new easy-calibration methodology was developed to obtain a functional clear sky model for any day of the year and any geographical location. …”
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    VoxelSky-3D: A Weather Radar Visualization Prototype for Air Traffic Control by Zhenhao Zhan, Tek-Yong Lim, Kannan Ramakrishnan

    Published 2025-01-01
    “…This paper presents VoxelSky-3D, a new 3D weather radar visualization prototype for civil aviation air traffic control. …”
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    COSMIC’s Large-scale Search for Technosignatures during the VLA Sky Survey: Survey Description and First Results by C. D. Tremblay, J. Sofair, L. Steffes, T. Myburgh, D. Czech, P. B. Demorest, R. A. Donnachie, A. W. Pollak, M. Ruzindana, Siemion A. P. V., S. S. Varghese, S. Z. Sheikh

    Published 2025-01-01
    “…Jansky Very Large Array (VLA) in New Mexico in order to search for signals throughout the Galaxy consistent with our understanding of artificial radio emissions. …”
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    « Et que fais-tu de cinq cents millions d’étoiles ? » by Samuel Challéat, Thomas Poméon

    Published 2020-07-01
    “…Under the effect of light pollution, darkness and the starry sky are among those objects that have become rare, and we are assessing what they provide now that they seem to be eluding us. …”
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    A Study of NOAA-20 VIIRS Band M1 (0.41 µm) Striping over Clear-Sky Ocean by Wenhui Wang, Changyong Cao, Slawomir Blonski, Xi Shao

    Published 2024-12-01
    “…Our results indicate that the prelaunch-measured polarization sensitivity and the polarization correction method work well and can effectively reduce striping over clear-sky ocean scenes by up to ~2% at near nadir zones. …”
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    Spread Sea Clutter Suppression in HF Hybrid Sky-Surface Wave Radars Based on General Parameterized Time-Frequency Analysis by Zhuo-qun Wang, Ya-jun Li, Jun-nan Shi, Peng-fei Wang, Ai-hua Liu, Xin-fan Xia, De-hong Chen

    Published 2020-01-01
    “…Firstly, the radar configuration and sea clutter broadening model are introduced based on the newly developed integrated HF sky-surface wave experimental system. …”
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    « Motionless Monotony »: New Nowheres in Irish Photography by Colin Graham

    Published 2014-06-01
    “…Places are closer together because the distances between them take less time to traverse. In this process of acceleration and psychic contraction the marks and traces of road-building and faster human movement necessitate the appearance of new landscapes, strips of nowhere places; verges, wastelands, unfinished building sites, ‘open’ areas, suburban spaces. …”
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    Enhancing environmental models with a new downscaling method for global radiation in complex terrain by A. Druel, J. Ruffault, H. Davi, A. Chanzy, O. Marloie, M. De Cáceres, A. Olioso, F. Mouillot, C. François, K. Soudani, N. K. Martin-StPaul

    Published 2025-01-01
    “…The influences of surrounding mountains' shade on direct radiation and the “bowl” (deep valley) effect (or sky-view factor) on diffuse radiation are then considered. …”
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    Galaxies Lighting Up: Discovery of Seventy New Turn-on Changing-look Active Galactic Nuclei by Qian Yang, Paul J. Green, Xue-Bing Wu, Michael Eracleous, Linhua Jiang, Yuming Fu

    Published 2025-01-01
    “…Based on their bright state Eddington ratios, turn-on CL AGN are associated with lower accretion rates compared to turn-off CL AGN or typical Sloan Digital Sky Survey quasars with similar redshift and magnitude distributions, even though turn-on CL AGN have lower BH masses. …”
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