Category: 2. Space

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  • A young gas giant and hidden substructures in a protoplanetary disk

    A young gas giant and hidden substructures in a protoplanetary disk

  • Keppler, M. et al. Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70. Astron. Astrophys. 617, A44 (2018).

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  • Haffert, S. Y. et al. Two…

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  • Author Correction: Co-precession of a curved jet and compact accretion disk in M87

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  • Methanetetrol and the final frontier in ortho acids

    Methanetetrol and the final frontier in ortho acids

  • Wilke, E. Zur kenntnis wäßriger kohlensäurelösungen. Z. Anorg. Allg. Chem. 119, 365–379 (1922).

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  • Tieckelmann, H. & Post, H. W. The preparation of methyl, ethyl, propyl, and butyl…

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  • A solar C/O ratio in planet-forming gas at 1 au in a highly irradiated disk

    A solar C/O ratio in planet-forming gas at 1 au in a highly irradiated disk

  • Gardner, J. P. et al. The James Webb Space Telescope mission. Publ. Astron. Soc. Pac. 135, 068001 (2023).

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  • Kamp, I. et al. The chemical inventory of the inner regions of…

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  • The biggest black hole smashup ever detected challenges physics theories

    The biggest black hole smashup ever detected challenges physics theories

    Senior physics writer Emily Conover has a Ph.D. in physics from the University of Chicago. She is a two-time winner of the D.C. Science Writers’ Association Newsbrief award and a winner of the Acoustical Society of America’s…

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  • The Second and Third Data Releases from the UKIRT Hemisphere Survey

    This paper describes the second and third data releases (DR2 and DR3, respectively) from the ongoing United Kingdom Infrared Telescope Hemisphere Survey (UHS). DR2 is primarily comprised of the K-band portion of the UHS survey, and was released…

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  • ABYSS. III. Observing Accretion Activity in Young Stars Through Empirical Veiling Measurements

    Stellar accretion plays an important role in the early stages of stellar evolution, particularly in Classical T Tauri Stars (CTTSs). Accretion of a CTTS can be related to different physical parameters such as effective temperature (Teff), age,…

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  • Deep Reinforcement Learning for Efficient Scheduling of Ground-based Astronomical Observations

    Ground-based astronomical observations face inherent challenges from weather changes, target visibility window constraints, and observational requirements. Enhancing the efficiency and effectiveness of telescope operations has long been a key…

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  • Semiempirical versus Theoretical Stellar Population Models: A Comparison with Star Clusters

    Stellar population synthesis (SPS) models are a key tool for deriving the age, metallicity, radial velocity, and reddening of star clusters from their integrated spectra. Using a sample of 129 star clusters with high-quality spectra, we analyze…

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