1 Arxiv:2401.01230V1 [Astro-Ph.Ep] 2 Jan 2024

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This work presents Depth Anything, a highly practical solution for robust monocular depth estimation. Without pursuing novel technical modules, we aim to build a

arXiv:2401.16451v1 [astro-ph.EP] 29 Jan 2024

[astro-ph/0508059] Young stars and dust in AFGL437: NICMOS/HST ...

arXiv:2401.03775v1 [astro-ph.EP] 8 Jan 2024 Draft version January 9, 2024 Typeset using LATEX twocolumn style in AASTeX62

The equation of state of hydrogen-helium (H-He) mixtures plays a vital role in the evolution and structure of gas giant planets and exoplanets. Recent equations of state that The Habitable Worlds Observatory will attempt to image Earth-sized planets in Habitable Zone orbits around nearby Sun-like stars. In this work we explore approximate analytic yield

Comments: 14 pages, 10 figures. To appear in Astronomy & Astrophysics Subjects: Earth and Planetary Astrophysics (astro-ph.EP) 1 INTRODUCTION One of the key goals of exoplanet science is the atmospheric char-acterisation of Earth-sized planets in the habitable zones of Sun-like stars. An important focus of these We present the mid-infrared (5–12 μm) phase curve of GJ 367b observed by the Mid-Infrared In-strument (MIRI) on the James Webb Space Telescope (JWST). GJ 367b is a hot (Teq = 1370

Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a Shigehisa Takakuwa,1,2 Abstract The TRAPPIST-1 system is comprised of seven Earth-sized rocky planets in small orbits around a Jupiter-sized ultracool dwarf star 12 parsec away. These planets cover an irradiation The equation of state of hydrogen-helium (H-He) mixtures plays a vital role in the evolution and structure of gas giant planets and exoplanets. Recent equations of state that account for

arXiv:2401.05923v1 [astro-ph.EP] 11 Jan 2024 2 Schulte et al. 28George Mason University, 4400 University Drive, Fairfax, VA, 22030 USA 29Department of Multi-Disciplinary Sciences,

Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO); Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR); General Relativity and Quantum arXiv:2401.10782v1 [astro-ph.EP] 19 Jan 2024 HITRAN-formatted UV line list of S2 containing transitions involving X 3Σ−

arXiv:2401.05923v1 [astro-ph.EP] 11 Jan 2024

arXiv:2401.05540v1 [astro-ph.EP] 10 Jan 2024
arXiv:2401.11815v1 [astro-ph.EP] 22 Jan 2024
GJ 367b is a dark, hot, airless sub-Earth
arXiv:2401.13293v1 [astro-ph.EP] 24 Jan 2024

Abstract page for arXiv paper 2401.00668: The structure of the stellar halo of the Andromeda galaxy explored with the NB515 for Subaru/HSC. I.: New Insights on the stellar The lifetime of mm size dust grains, such as chondrules, in the nominal solar nebula model is limited to ∼ 105 yr due to an inward drift driven by gas drag. However, isotopic Comets are primitive bodies that coalesced during solar system formation and have undergone relatively little change in the past 4.5 billion years. Thus, their compositions provide essential

[astro-ph/0412143] Adaptive Optics Imaging of the AU Microscopii ...

The recent discovery of “ultra-hot” (P < 1 day) Neptunes has come as a surprise: some of these planets have managed to retain gaseous envelopes despite being close enough

Studying the properties of desert- dwelling planets may help us understand the physical arXiv:2401.16474v1 [astro-ph.EP] 29 Jan 2024 2 Vissapragada et al. mechanisms that clear We present the mid-infrared (5–12 μm) phase curve of GJ 367b observed by the Mid-Infrared In-strument (MIRI) on the James Webb Space Telescope (JWST). GJ 367b is a hot (Teq = 1370

Citing Uranus’s suite of mysterious properties, technological readiness, and the great deal of community support, the 2023-2032 Oceans, Worlds, and Life: A Decadal Strategy for Planetary arXiv:2401.01912v1 [cs.CV] 2 Jan 2024 Shrinking Your TimeStep: Towards Low-Latency Neuromorphic Object Recognition with Spiking Neural Networks

Introduction to magnetic star-planet interactions A. Strugarek, E. Shkolnik Comments: 10 pages, 2 figures, to be published as a chapter in ‚Space Environments and their Exoplanets with short orbit period reside very close to their host stars. They transition very rapidly between diferent sectors of the circumstellar space environment along Citing Uranus’s suite of mysterious properties, technological readiness, and the great deal of community support, the 2023-2032 Oceans, Worlds, and Life: A Decadal Strategy for Planetary

A thorough inspection of known Galactic Supernova Remnants (SNRs) along the Galactic plane with SRG/eROSITA yielded the detection of the X-ray counterpart of the SNR In U(1) lattice gauge theory with compact U(1) variables, we construct the symmetry operator, i.e.\ the topological defect, for the axial U(1) noninvertible symmetry. This requires a

arXiv:2401.02574v1 [astro-ph.EP] 4 Jan 2024

arXiv:2401.03021v1 [astro-ph.EP] 5 Jan 2024 2 P. Dalba et al. long observational baselines. Nonetheless, a sample of giant exoplanets on orbits longer than 100 days has been identified

The radius valley, i.e., a dearth of planets with radii between 1.5 and 2 Earth radii, provides insights into planetary formation and evolution. Using homogenously revised planetary 1. INTRODUCTION Exoplanet discoveries have revealed a vast range of planetary architectures, many of which differ signifi- cantly from that seen in the solar system (Ford2014;

Gaussian processes and Nested Sampling Applied to Kepler’s Small Long-Period Exoplanet Candidates Michael R. B. Matesic ,1,2 Jason F. Rowe ,2 John H. Livingston ,3,4,5 Shishir The prompt emission, X-ray plateau, and X-ray flares of Gamma-ray bursts (GRB) are thought to be from internal dissipation, and the magnetar as the central engine with propeller fallback

arXiv:2401.03775v1 [astro-ph.EP] 8 Jan 2024 Draft version January 9, 2024 Typeset using LATEX twocolumn style in AASTeX62

Sub-Prime Field Planets In-Gu Shin,1 Jennifer C. Yee,1 Weicheng Zang,1,2 Cheongho Han,3 Hongjing Yang,2 Andrew Gould,4,5 Chung-Uk Lee,6 Andrzej Udalski,7 Takahiro Sumi8 Gaussian processes and Nested Sampling Applied to Kepler’s Small Long-Period Exoplanet Candidates Michael R. B. Matesic ,1,2 Jason F. Rowe ,2 John H. Livingston ,3,4,5

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