BIOS: An Algorithmically Generated Biomedical Knowledge Graph

Kavli Affiliate: Jing Wang | First 5 Authors: Sheng Yu, Zheng Yuan, Jun Xia, Shengxuan Luo, Huaiyuan Ying | Summary: Biomedical knowledge graphs (BioMedKGs) are essential infrastructures for biomedical and healthcare big data and artificial intelligence (AI), facilitating natural language processing, model development, and data exchange. For many decades, these knowledge graphs have been built […]


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Radio pulsations from a neutron star within the gamma-ray binary LS I +61$^{circ}$ 303

Kavli Affiliate: Renxin Xu | First 5 Authors: Shan-Shan Weng, Lei Qian, Bo-Jun Wang, D. F. Torres, A. Papitto | Summary: LS I +61$^{circ}$ 303 is one of the rare gamma-ray binaries, emitting most of their luminosity in photons with energies beyond 100 MeV. The $sim$26.5 d orbital period is clearly detected at many wavelengths. […]


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CHANG-ES XXV: HI Imaging of Nearby Edge-on Galaxies — Data Release 4

Kavli Affiliate: Ran Wang | First 5 Authors: Yun Zheng, Jing Wang, Judith Irwin, Jayanne English, Qingchuan Ma | Summary: We present the HI distribution of galaxies from the Continuum Halos in Nearby Galaxies – an EVLA Survey (CHANG-ES). Though the observational mode was not optimized for detecting HI, we successfully produce HI cubes for […]


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A quasar shedding its dust cocoon at redshift 2

Kavli Affiliate: Luis C. Ho | First 5 Authors: Weimin Yi, W. N. Brandt, Q. Ni, Luis C. Ho, Bin Luo | Summary: We present the first near-IR spectroscopy and joint analyses of multi-wavelength observations for SDSS J082747.14+425241.1, a dust-reddened, weak broad emission-line quasar (WLQ) undergoing a remarkable broad absorption line (BAL) transformation. The systemic […]


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Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI — Stellar Populations

Kavli Affiliate: Claudio Ricci | First 5 Authors: Rogério Riffel, Luis G. Dahmer-Hahn, Rogemar A. Riffel, Thaisa Storchi-Bergmann, Natacha Z. Dametto | Summary: We use Gemini Near-Infrared Integral Field Spectrograph (NIFS) adaptive optics assisted data-cubes to map the stellar population of the inner few hundred parsecs of a sample of 18 nearby Seyfert galaxies. The […]


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XYLayoutLM: Towards Layout-Aware Multimodal Networks For Visually-Rich Document Understanding

Kavli Affiliate: Ke Wang | First 5 Authors: Zhangxuan Gu, Changhua Meng, Ke Wang, Jun Lan, Weiqiang Wang | Summary: Recently, various multimodal networks for Visually-Rich Document Understanding(VRDU) have been proposed, showing the promotion of transformers by integrating visual and layout information with the text embeddings. However, most existing approaches utilize the position embeddings to […]


Continue.. XYLayoutLM: Towards Layout-Aware Multimodal Networks For Visually-Rich Document Understanding

XYLayoutLM: Towards Layout-Aware Multimodal Networks For Visually-Rich Document Understanding

Kavli Affiliate: Ke Wang | First 5 Authors: Zhangxuan Gu, Changhua Meng, Ke Wang, Jun Lan, Weiqiang Wang | Summary: Recently, various multimodal networks for Visually-Rich Document Understanding(VRDU) have been proposed, showing the promotion of transformers by integrating visual and layout information with the text embeddings. However, most existing approaches utilize the position embeddings to […]


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Astrophysics with the Laser Interferometer Space Antenna

Kavli Affiliate: Xian Chen | First 5 Authors: Pau Amaro Seoane, Jeff Andrews, Manuel Arca Sedda, Abbas Askar, Quentin Baghi | Summary: The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel […]


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Signature of Supersonic Turbulence in Galaxy Clusters

Kavli Affiliate: Kohei Inayoshi | First 5 Authors: Haojie Hu, Yu Qiu, Marie-Lou Gendron-Marsolais, Tamara Bogdanovic, Julie Hlavacek-Larrondo | Summary: The hot intracluster medium (ICM) is thought to be quiescent with low observed velocity dispersions. Surface brightness fluctuations of the ICM also suggest that its turbulence is subsonic with a Kolmogorov scaling relation, indicating that […]


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Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven H$α$ Filaments

Kavli Affiliate: Kohei Inayoshi | First 5 Authors: Haojie Hu, Yu Qiu, Marie-Lou Gendron-Marsolais, Tamara Bogdanovic, Julie Hlavacek-Larrondo | Summary: The hot intracluster medium (ICM) is thought to be quiescent with low observed velocity dispersions. Surface brightness fluctuations of the ICM also suggest that its turbulence is subsonic with a Kolmogorov scaling relation, indicating that […]


Continue.. Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven H$α$ Filaments