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۱. مبانی نظری: تانسور ۱۶۵ بعدی و میدان Ξ ارتباط با تمدنهای فرازمینی از طریق امواج الکترومغناطیسی کلاسیک به دلیل محدودیت سرعت نور ($c$) شکست خورده است. متد حمزه بر پایه غیرمحلی بودن (Non-locality) و مشتقات فراکتالی بنا شده است. فرمول بنیادین آگاهی حمزه: $$D_t^…
datacite
JALALI, SEYED RASOUL
2025
置信度 0.66
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Latest related work: De Jesus, Elias. (2025). Fundamental Constants from Logical Geometry: Deriving α, me, and Mp/me from the RTLI Framework. Zenodo. https://doi.org/10.5281/zenodo.17977094 This research note applies the Relational Threshold and Latent Interac…
datacite
De Jesus, Elias
2025
置信度 0.66
• Fine-Structure Constant • RTLI Framework • Structural Transition Cost • Gravitational Lensing • Radial Acceleration Relation (RAR) • Zero-Stiffness Mode • Cosmological Relaxation • Renormalization Structure • Cross-Scale Coupling • Emergent Constants • Structural Coherence • Variance Filtering • Relational Physics • Hypothesis-Generating Analysis
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Latest related work: De Jesus, Elias. (2025). Fundamental Constants from Logical Geometry: Deriving α, me, and Mp/me from the RTLI Framework. Zenodo. https://doi.org/10.5281/zenodo.17977094 This research note applies the Relational Threshold and Latent Interac…
datacite
De Jesus, Elias
2025
置信度 0.66
• Fine-Structure Constant • RTLI Framework • Structural Transition Cost • Gravitational Lensing • Radial Acceleration Relation (RAR) • Zero-Stiffness Mode • Cosmological Relaxation • Renormalization Structure • Cross-Scale Coupling • Emergent Constants • Structural Coherence • Variance Filtering • Relational Physics • Hypothesis-Generating Analysis
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This is a basic reproduction package for the paper "Chasing the storm: Investigating the application of high-contrast imaging techniques in producing precise exoplanet light curves" by Sutlieff et al. (2025). It aims to provide the most important data products…
datacite
Sutlieff, Ben J., Doelman, David S., Birkby, Jayne L., Kenworthy, Matthew A. 等
2025
置信度 0.66
Astronomyplanets and satellites: atmospheresexoplanetsmethods: observationaltechniques: imaging spectroscopy
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This is a basic reproduction package for the paper "Chasing the storm: Investigating the application of high-contrast imaging techniques in producing precise exoplanet light curves" by Sutlieff et al. (2025). It aims to provide the most important data products…
datacite
Sutlieff, Ben J., Doelman, David S., Birkby, Jayne L., Kenworthy, Matthew A. 等
2025
置信度 0.66
Astronomyplanets and satellites: atmospheresexoplanetsmethods: observationaltechniques: imaging spectroscopy
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Hemispherical reflectance data from Paragas et al. (2025). Citation: @article{Paragas_2025, doi = {10.3847/1538-4357/ada9eb}, url = {https://doi.org/10.3847/1538-4357/ada9eb}, year = {2025}, month = {mar}, publisher = {The American Astronomical Society}, volum…
datacite
Nicholls, Harrison
2025
置信度 0.66
surface_albedos
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Hemispherical reflectance data from Paragas et al. (2025). Citation: @article{Paragas_2025, doi = {10.3847/1538-4357/ada9eb}, url = {https://doi.org/10.3847/1538-4357/ada9eb}, year = {2025}, month = {mar}, publisher = {The American Astronomical Society}, volum…
datacite
Nicholls, Harrison
2025
置信度 0.66
surface_albedos
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The nearby star Fomalhaut is orbited by a compact source, Fomalhaut b, which has previously been interpreted as either a dust-enshrouded exoplanet or a dust cloud generated by the collision of two planetesimals. Such collisions are rarely observed but their de…
datacite
Kalas, Paul, Wang, Jason J., Millar-Blanchaer, Maxwell A., Ren, Bin B. 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
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Pandora is a SmallSat mission designed to observe exoplanet atmospheres and stellar activity. Funded by the NASA Science Mission Directorate (SMD) Astrophysics Division through the Pioneers program, Pandora is a collaboration between NASA centers Goddard and A…
openalex
Wiser, Lindsey, Dotson, Jessie, Greene, Thomas, Barclay, Thomas 等
2024
置信度 0.72
ExoplanetProject commissioningNeptuneTelescopePhysics
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Title SDT Law of Mutual Occlusive Gravitation (Steradian Form): Theory, Examples, and 7,400-day Earth–Sun–Jupiter Analysis Description This deposit introduces the Spatial Displacement Theory (SDT) Law of Mutual Occlusive Gravitation in steradian form and provi…
datacite
Harvey, James
2025
置信度 0.66
-
Stellar magnetic activity, manifested through spots (faculae and flares), fundamentally shapes the exoplanets' environments. For low-mass stars in particular, where most habitable-zone planets reside, the variable magnetic phenomena can dominate atmospheric ch…
datacite
Majidi, Fatemeh Zahra, Biazzo, Katia, Tsantaki, Maria, Bayo, Amelia 等
2025
置信度 0.66
Instrumentation and Methods for Astrophysics (astro-ph.IM)Earth and Planetary Astrophysics (astro-ph.EP)High Energy Astrophysical Phenomena (astro-ph.HE)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciences
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The search for free-floating planets (FFPs) is a key science driver for upcoming microlensing surveys like the Nancy Grace Roman Galactic Exoplanet Survey. These rogue worlds are typically detected via short-duration microlensing events, the characterization o…
datacite
Smyth, Nolan, Perreault-Levasseur, Laurence, Hezaveh, Yashar
2025
置信度 0.66
Instrumentation and Methods for Astrophysics (astro-ph.IM)Earth and Planetary Astrophysics (astro-ph.EP)Astrophysics of Galaxies (astro-ph.GA)FOS: Physical sciencesFOS: Physical sciences
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IMPORTANT: Original tag v1.5.1 from 08-11-2025. Reindexed in December for integration with Zenodo. No major changes between August and December 2025. What's Changed Upgrade to account for residual exozodi in snr calc by @curriem in https://github.com/eleonoraa…
datacite
ALEI, ELEONORA, Currie, Miles, Stark, Christopher, Roberge, Aki 等
2025
置信度 0.66
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ستون فقرات تمدن فرا-کوانتومی: نسل هفتم محاسبات و اینترنت بینهایت ($\text{Net}\infty$) ۱. مق��مه: گذار از محدودیتهای کلاسیک به فرا-کوانتوم در حالی که نسلهای پیشین محاسبات کوانتومی با مشکلاتی نظیر زمان همدوسی (Coherence Time) کوتاه، نرخ خطای بالا و محدودیتها…
datacite
JALALI, SEYED RASOUL
2025
置信度 0.66
-
ستون فقرات تمدن فرا-کوانتومی: نسل هفتم محاسبات و اینترنت بینهایت ($\text{Net}\infty$) ۱. مقدمه: گذار از محدودیتهای کلاسیک به فرا-کوانتوم در حالی که نسلهای پیشین محاسبات کوانتومی با مشکلاتی نظیر زمان همدوسی (Coherence Time) کوتاه، نرخ خطای بالا و محدودیتهای…
datacite
JALALI, SEYED RASOUL
2025
置信度 0.66
-
James C. Hanlon III – December 2025 – CC-BY-4.0 Public data from pulsars, dying suns, and nebulae reveal the same eight perfect-square frequencies previously measured in embryos and water—no new physics, no parameters. Raw periods are noise; the ladder lives i…
datacite
James c Hanlon III
2025
置信度 0.66
-
Public data from pulsars, dying suns, and nebulae reveal the same eight perfect-square frequencies previously measured in embryos and water—no new physics, no parameters. Raw periods are noise; the ladder lives in the residual beats after stripping dominant mo…
datacite
James C Hanlon III
2025
置信度 0.66
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Celestial Resonance Echoes – Survey 1 The Universal Eight-Key Resonance Ladder in Stellar and Exoplanetary Systems James C. Hanlon III – December 2025 – CC-BY-4.0 Public Kepler, TESS, and Gaia light curves (2018–2025) reveal the identical eight-key resonance l…
datacite
James c Hanlon III
2025
置信度 0.66
-
Celestial Resonance Echoes – Survey 1 The Universal Eight-Key Resonance Ladder in Stellar and Exoplanetary Systems James C. Hanlon III – December 2025 – CC-BY-4.0 Public Kepler, TESS, and Gaia light curves (2018–2025) reveal the identical eight-key resonance l…
datacite
James C Hanlon III
2025
置信度 0.66
-
Few spectra of directly-imaged exoplanets have been obtained in the mid-infrared (> 3 $μ$m). This region is particularly rich in molecular spectral signatures, whose measurements can help recover atmospheric parameters and provide a better understanding of …
datacite
Houllé, M., Millour, F., Berio, P., Scigliuto, J. 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciencesFOS: Physical sciences
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It was only thirty years ago that the first extrasolar planet, or exoplanet, orbiting a Sun-like star was discovered. Since then (as of October 2025), 6,022 have been confirmed across 4,490 planetary systems, 1,013 of which host multiple planets. Whilst these …
datacite
Palethorpe, Larissa
2025
置信度 0.66
ExoplanetsTransit photometryRadial velocity measurementsRadius valleyPlanetary evolution
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We propose a coherence-augmented formulation of the three-body problem within Relational Field Theory (RFT). Each pairwise interaction carries a small, causal memory state Hij whose real part Rij = ℜHij modulates the Newtonian force by a symmetric factor 1 + ε…
datacite
Svancara, Clinton
2025
置信度 0.66
-
We present TRMH-8.0, the first dynamic habitability index based on temporal multi-harmonic resonance with a Möbius-type phase twist. Applied to the 187 conservatively habitable exoplanets (NASA Exoplanet Archive, Dec 2025) and incorporating real JWST transmiss…
datacite
Valdivia Muñoz, Joel
2025
置信度 0.66
exoplanets, habitability, JWST, TESS, dynamic index, Möbius resonance, astrobiology
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We present TRMH-8.0, the first dynamic habitability index based on temporal multi-harmonic resonance with a Möbius-type phase twist. Applied to the 187 conservatively habitable exoplanets (NASA Exoplanet Archive, Dec 2025) and incorporating real JWST transmiss…
datacite
Valdivia Muñoz, Joel
2025
置信度 0.66
exoplanets, habitability, JWST, TESS, dynamic index, Möbius resonance, astrobiology
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The version of the TIRAMISU code used to produce the models presented in the paper "TIRAMISU: Non-LTE radiative transfer for molecules in exoplanet atmospheres", published in ApJ (2025). Archives of the GitHub release are provided here.
openalex
Bowesman, Charles, Yurchenko, Sergey, Al-Refaie, Ahmed, Tennyson, Jonathan
2025
置信度 0.72
ExoplanetRadiative transferPhysicsAstrobiologyMolecule
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The version of the TIRAMISU code used to produce the models presented in the paper "TIRAMISU: Non-LTE radiative transfer for molecules in exoplanet atmospheres", published in ApJ (2025). Archives of the GitHub release are provided here.
openalex
Bowesman, Charles, Yurchenko, Sergey, Al-Refaie, Ahmed, Tennyson, Jonathan
2025
置信度 0.72
ExoplanetRadiative transferPhysicsAstrobiologyMolecule
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3I/ATLAS, also known as C2025 N1 (ATLAS), is the third known macroscopic interstellar object to pass through our Solar System. We report serendipitous Transiting Exoplanet Survey Satellite (TESS) observations of 3I/ATLAS taken between 2025-05-07 and 2025-06-02…
datacite
Martinez-Palomera, Jorge, Tuson, Amy, Hedges, Christina, Dotson, Jessie 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)Astrophysics of Galaxies (astro-ph.GA)FOS: Physical sciencesFOS: Physical sciences
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Captain Exoplanet v1.0.0 - Initial Public Release Live Demo Hunt for exoplanets with AI. Main Features Browser-based interface: Easily classify exoplanet candidates using any modern browser. Next.js + FastAPI stack: Frontend built in React (Next.js), backend i…
openalex
Zayed, Gamal, Leśniowski, Marcin, Sant, Yatharth Mahesh, Pasumarthi, Babu sree Harsha 等
2025
置信度 0.72
DeconfusionDirect ImagingExoplanet DetectionCitizen Science/InstrumentationCitizen Science/classification
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Captain Exoplanet v1.0.0 - Initial Public Release Live Demo Hunt for exoplanets with AI. Main Features Browser-based interface: Easily classify exoplanet candidates using any modern browser. Next.js + FastAPI stack: Frontend built in React (Next.js), backend i…
openalex
Zayed, Gamal, Leśniowski, Marcin, Sant, Yatharth Mahesh, Pasumarthi, Babu sree Harsha 等
2025
置信度 0.72
DeconfusionDirect ImagingExoplanet DetectionCitizen Science/InstrumentationCitizen Science/classification
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We present the description of the instruments and the first results of the PRime-focus Infrared Microlensing Experiment (PRIME). PRIME is the first dedicated near-infrared (NIR) microlensing survey telescope located at the South African Astronomical Observator…
datacite
Sumi, Takahiro, Buckley, David A. H., Kutyrev, Alexander S., Tamura, Motohide 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)Astrophysics of Galaxies (astro-ph.GA)Instrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciences
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Captain Exoplanet v1.0.0 – Initial Public Release Live Demo Hunt for exoplanets with AI. Main Features Browser-based interface: Easily classify exoplanet candidates using any modern browser. Next.js + FastAPI stack: Frontend built in React (Next.js), backend i…
datacite
Zayed, Gamal, Leśniowski, Marcin, Sant, Yatharth Mahesh, Harsha, Pasumarthi Pabu Sree 等
2025
置信度 0.66
Photometry/methodsDeconfusionDirect ImagingExoplanetologyExoplanet Detection
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OVERVIEW V2 UPDATE: The evolution code's atmospheric boundary condition now has a "weighted transition region" across Teff 2000 - 2400 K (where both the original Sonora Diamondback and new SPHINX grids have modeled atmospheres). This differs from V1, where the…
datacite
Davis, Christopher Evan, Fortney, Jonathan, Iyer, Aishwarya, Mukherjee, Sagnick 等
2025
置信度 0.66
brown dwarfyoung brown dwarfextrasolar planetevolutionphotometry
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OVERVIEW V2 UPDATE: The evolution code's atmospheric boundary condition now has a "weighted transition region" across Teff 2000 - 2400 K (where both the original Sonora Diamondback and new SPHINX grids have modeled atmospheres). This differs from V1, where the…
datacite
Davis, Christopher Evan, Fortney, Jonathan, Iyer, Aishwarya, Mukherjee, Sagnick 等
2025
置信度 0.66
brown dwarfyoung brown dwarfextrasolar planetevolutionphotometry
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# RESUMEN CIENTÍFICO: ## DEMOSTRACIÓN MATEMÁTICA DE LAS CONEXIONES ENTRE EL CALENDARIO MAYA Y LAS COORDENADAS GALÁCTICAS MODERNAS **Autor**: Joel Emiliano Valdivia Muñoz **Fecha**: 23 de noviembre de 2025 **Palabras clave**: Calendario maya, coordenadas galáct…
datacite
Valdivia Muñoz, Joel Emiliano
2025
置信度 0.66
-
# RESUMEN CIENTÍFICO: ## DEMOSTRACIÓN MATEMÁTICA DE LAS CONEXIONES ENTRE EL CALENDARIO MAYA Y LAS COORDENADAS GALÁCTICAS MODERNAS **Autor**: Joel Emiliano Valdivia Muñoz **Fecha**: 23 de noviembre de 2025 **Palabras clave**: Calendario maya, coordenadas galáct…
datacite
Valdivia Muñoz, Joel Emiliano
2025
置信度 0.66
-
import numpy as npimport pandas as pdimport matplotlib.pyplot as pltimport seaborn as snsimport tensorflow as tffrom tensorflow.keras import layers, modelsfrom tensorflow.keras.layers import MultiHeadAttention, LayerNormalization, Dropout, GlobalAveragePooling…
datacite
Valdivia Muñoz, Joel Emiliano
2025
置信度 0.66
-
import numpy as npimport pandas as pdimport matplotlib.pyplot as pltimport seaborn as snsimport tensorflow as tffrom tensorflow.keras import layers, modelsfrom tensorflow.keras.layers import MultiHeadAttention, LayerNormalization, Dropout, GlobalAveragePooling…
datacite
Valdivia Muñoz, Joel Emiliano
2025
置信度 0.66
-
This study presents a full 4.1-billion-year forward-time planetary evolution model reconstructing the emergence of Earth’s first lithosphere. Using a unified multiphysics framework—integrating relativistic gravitational response, mantle thermochemical gradient…
datacite
Slawson, Drew
2025
置信度 0.66
early Earth lithosphere formation proto-plate boundaries mantle convection planetary evolution geodynamics crustal segmentation mantle thermal gradients planetary interiors tectonic emergence multiphysics modeling curvature-response physics mantle structure evolution
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This study presents a full 4.1-billion-year forward-time planetary evolution model reconstructing the emergence of Earth’s first lithosphere. Using a unified multiphysics framework—integrating relativistic gravitational response, mantle thermochemical gradient…
datacite
Slawson, Drew
2025
置信度 0.66
early Earth lithosphere formation proto-plate boundaries mantle convection planetary evolution geodynamics crustal segmentation mantle thermal gradients planetary interiors tectonic emergence multiphysics modeling curvature-response physics mantle structure evolution
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Files to reproduce the figures of the paper "Modelling the Milky Way's exoplanet population based on cosmological galaxy simulations", Padois et al. 2025 (https://arxiv.org/abs/2511.14704). Code available at https://github.com/cpadois/glxsimu_to_exoplanets_pap…
openalex
Padois, Chloé
2025
置信度 0.72
Milky WayExoplanetPhysicsPopulationGalaxy
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Files to reproduce the figures of the paper "Modelling the Milky Way's exoplanet population based on cosmological galaxy simulations", Padois et al. 2025 (https://arxiv.org/abs/2511.14704). Code available at https://github.com/cpadois/glxsimu_to_exoplanets_pap…
openalex
Padois, Chloé
2025
置信度 0.72
Milky WayExoplanetPhysicsPopulationGalaxy
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Understanding how the Universe evolved from diffuse primordial gas into the rich cosmic web we observe today is one of the great challenges of modern astrophysics. Quasar absorption lines — the imprints left by intervening gas on the light from distant quasars…
datacite
Berg, Trystyn, D’Odorico, Valentina, Boera, Elisa, Calderone, Giorgio 等
2025
置信度 0.66
-
This study presents a full-lifespan (4.6 billion years) forward-time simulation of a terrestrial-class planet, Lumenis Prime, modeled using a unified relativistic–topological physics framework. The simulation integrates relativistic gravitational fields, magne…
datacite
Slawson, Drew
2025
置信度 0.66
planetary formation terrestrial planet evolution emergent physics relativistic geophysics mantle convection core dynamo modeling atmospheric evolution climate-band stability hydrospheric development exoplanet analogues unified physics simulation geodynamic modeling planetary habitability
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This study presents a full-lifespan (4.6 billion years) forward-time simulation of a terrestrial-class planet, Lumenis Prime, modeled using a unified relativistic–topological physics framework. The simulation integrates relativistic gravitational fields, magne…
datacite
Slawson, Drew
2025
置信度 0.66
planetary formation terrestrial planet evolution emergent physics relativistic geophysics mantle convection core dynamo modeling atmospheric evolution climate-band stability hydrospheric development exoplanet analogues unified physics simulation geodynamic modeling planetary habitability
-
SPARTA (Simple, fast, barebones, utilitarian — Spartan) is a lightweight yet powerful pipeline for reducing and analyzing JWST time-series exoplanet data. It provides streamlined processing modules with minimal dependencies, designed for clarity, reproducibili…
datacite
Xue, Qiao, Zhang, Michael
2025
置信度 0.66
-
The transit method is pivotal for exoplanet detection and radius determination by measuring periodic dips in stellar brightness. However, systematic biases, particularly from unaccounted-for limb darkening (LD) and stellar activity in simplified public data pr…
crossref
Ruilin Ma
2025-10-28T14:31:08Z
置信度 0.70
-
The TESS Science Processing Operation Center searches for transiting planets in 160,000 targets selected from the full frame images (FFI) each observing sector. The pipeline detects several thousand potential transit signals, or threshold- crossing events (TCE…
crossref
Makaila Jennings, Douglas A. Caldwell
2026-04-14T19:55:59Z
置信度 0.70
-
Abstract With the advancement of observational techniques, over one million stars have been observed to search for exoplanets. The vast amounts of light curve data generated necessitate an automated, rapid, and efficient method for screening exoplanet candidat…
crossref
Dapeng Xie, Ying Wang, Fuyao Liu, Wei Sun
2025-08-02T22:51:01Z
置信度 0.70
-
crossref
Jeffrey Linsky
2025-01-29T10:18:59Z
置信度 0.70
-
crossref
Jeffrey Linsky
2025-01-29T10:18:23Z
置信度 0.70
-
Magma worlds, due to their hot, extended atmospheres are readily characterized spectroscopically by ground- and space-based telescopes, such as JWST. As yet, the lack of direct observations means that the nature and composition of these planets’ atmo…
crossref
Maggie Thompson, Paolo Sossi, Dan Bower, Sylvain Petitgirard 等
2024-03-09T03:12:10Z
置信度 0.70
-
Abstract The size distribution of planets with radii between 1 R ⊕ and 4 R ⊕ peaks near 1.4 R ⊕ and 2.2 R ⊕ , with a dip around 1.8 R ⊕ —the so-called “radius valley.” Recent statistical analyses suggest that planets within this valley (1.5 < R < 2 R ⊕ )…
crossref
Sho Shibata, Andre Izidoro
2025-06-18T12:03:57Z
置信度 0.70
-
The Ariel space mission is set to perform spectroscopic characterization of the atmospheres of a broad and diverse selection of hundreds of exoplanets. The target list is designed to span a wide array of planetary masses, densities, equilibrium temperatures, a…
crossref
Enzo Pascale, Andrea Bocchieri, Paul Eccleston, Lorenzo Mugnai 等
2025-07-09T15:45:11Z
置信度 0.70
-
ABSTRACT The third Gaia data release (DR3) contains ∼170 000 astrometric orbit solutions of two-body systems located within ∼500 pc of the Sun. Determining component masses in these systems, in particular of stars hosting exoplanets, usually hinges on incorpor…
crossref
Johannes Sahlmann, Pablo Gómez
2025-01-09T02:27:21Z
置信度 0.70
-
Planets are assembled from the same material as their parent stars. Therefore, stellar chemical abundance measurements provide important constraints on the formation, composition, and interior structure of exoplanets. M dwarfs are the most prolific hosts of lo…
crossref
Yutong Shan, Petra Hatalova, Hugo Tabernero, Anina Timmermann 等
2024-03-11T11:16:49Z
置信度 0.70
-
Abstract In this work, we apply an exploratory joint Bayesian transit detector, previously evaluated using Kepler data, to the 2 minutes simple aperture photometry light-curve data in the continuous viewing zone for the Transiting Exoplanet Survey Satellite (T…
crossref
Jamila S. Taaki, Athol J. Kemball, Farzad Kamalabadi
2025-06-05T08:48:21Z
置信度 0.70
-
This is the age of exoplanets. Thousands of planets around other suns have been discovered, upending settled science. Unlike spectacular imagery of other phenomena (e.g., nebulae), exoplanets are difficult to `directly' image, and exoplanet scientific imagery …
crossref
Ceridwen Dovey
2025-09-01T08:53:22Z
置信度 0.70
-
ABSTRACT Stellar activity manifests differently across wavelengths, causing flux variability that can obscure planetary transits. While transit observations are typically performed in the visible and infrared bands, where stellar flux is relatively stable, sho…
crossref
Tisyagupta Pyne, Belur Ravindra, Ravinder K Banyal
2025-12-10T13:12:48Z
置信度 0.70
-
Abstract In an era when we are charting multiple planets per system, one might wonder the extent to which “missing” (or failing to detect) a planet can skew our interpretation of the system architecture. We address this question with a simple experiment: start…
crossref
C. Alexander Thomas, Lauren M. Weiss, Matthias Y. He
2025-04-28T17:15:30Z
置信度 0.70
-
Introduction: As we enter the next chapter in our characterization of exoplanet atmospheres with state-of-the-art telescopes such as the James Webb Space Telescope, the efficacy of our atmospheric retrieval pipelines is more important than ever. At present, th…
crossref
Lily Robinthal, Tyler D. Robinson, Tommi Koskinen, Franck Montemessin 等
2025-07-09T15:45:11Z
置信度 0.70
-
crossref
Yu-Chia Lin
2025-09-18T15:45:09Z
置信度 0.70
-
Abstract Science yield studies will drive the development of future direct imaging telescopes, such as the Habitable Worlds Observatory. These studies rely on a metric called completeness, which represents the fraction of planets from an assumed planet populat…
crossref
Corey Spohn, Dmitry Savransky, Christopher C. Stark
2025-11-26T17:31:08Z
置信度 0.70
-
crossref
Jonathan Tennyson, Sergei N. Yurchenko
2025-07-16T08:38:07Z
置信度 0.70
-
Introduction The identification of habitable exoplanets is an important challenge in modern space science, requiring the combination of planetary and stellar parameters to assess conditions that support life. Methods Using a dataset of 5867 exoplanets from the…
crossref
Prasenjit Banerjee, Asis Kumar Chattopadhyay
2025-12-01T06:26:52Z
置信度 0.70
-
crossref
Syeda Saarah Fatema, S R Mani Sekhar
2025-09-04T18:16:35Z
置信度 0.70
-
Context. Revealing the internal composition and structure of giant planets is fundamental for understanding planetary formation. However, the bulk composition can only be inferred through interior models. As a result, advancements in modelling aspects are esse…
crossref
S. Howard, R. Helled, S. Müller
2024-12-12T14:45:07Z
置信度 0.70
-
Astronomical observations have provided an extensive body of evidence for the existence of disequilibrium chemistry in many exoplanet atmospheres, and this departure from a chemical equilibrium composition may have an impact on the temperature of the atmospher…
crossref
Marcelino Agúndez
2025-06-13T14:43:49Z
置信度 0.70
-
crossref
Corey Spohn, Sarah Steiger, Alex R. Howe
2025-12-11T23:09:16Z
置信度 0.70
-
crossref
Jeffrey Linsky
2025-01-29T10:19:40Z
置信度 0.70
-
crossref
Pooja Illangarathne, Janani Harischandra, Kanishka Hewageegana
2025-08-04T18:34:06Z
置信度 0.70
-
crossref
Jeffrey Linsky
2025-01-29T10:09:26Z
置信度 0.70
-
crossref
Sebastián Zúñiga-Fernández, Artem Burdanov, Laetitia Delrez, Michaël Gillon 等
2025-04-25T05:20:21Z
置信度 0.70
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The possible presence of dimethyl sulfide (DMS) in the atmosphere of the exoplanet K2‑18b—an ocean‑bearing Hycean world candidate—has intensified the interest in its potential habitability. This sulfur compound, primarily produced by marine life on Earth, is c…
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José Antonio de Freitas Pacheco De Freitas Pacheco
2025-08-27T07:29:22Z
置信度 0.70
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The photospheric manifestations of stellar magnetic activity, such as starspots, introduce contaminations in exoplanet transit observations. For instance, occulted starspots cause 'bumps' in the transit lightcurve that can change the shape of the ingress and e…
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Andre O. Kovacs, Adriana Valio
2025-07-09T15:12:38Z
置信度 0.70
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Giovanna Tinetti
2012-12-05T22:49:44Z
置信度 0.70
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2011-07-20T10:03:08Z
置信度 0.70
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Abstract Most Sun-like and higher-mass stars reside in systems that include one or more gravitationally bound stellar companions. These systems offer an important probe of planet formation in the most common stellar systems, while also providing key insights i…
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Joseph E. Hand, Konstantin Gerbig, Malena Rice
2025-05-14T12:06:20Z
置信度 0.70
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This study evaluates the possibility of efficient radio emission generation in the bow shock region of hot Jupiter–type exoplanets. As a source of energetic electrons, the shock drift acceleration mechanism at a quasi-perpendicular shock is proposed. Electrons…
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A. A. Kuznetsov
2026-02-24T11:41:22Z
置信度 0.70
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M. Deleuil, C. Moutou, P. Bordé
2016-04-28T10:14:15Z
置信度 0.70
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Jeffrey Linsky
2025-01-29T10:17:58Z
置信度 0.70
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Abstract A main source of bias in transmission spectroscopy of exoplanet atmospheres is magnetic activity of the host star in the form of stellar spots, faculae, or flares. However, the fact that main-sequence stars have a chromosphere and a corona and that th…
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Volker Perdelwitz, Adam Chaikin-Lifshitz, Aviv Ofir, Oded Aharonson
2025-02-19T07:36:41Z
置信度 0.70
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With the trend of technology advancement and environmental resource depletion, scientists make a hard effort to explore exoplanets that have ideal conditions for new colonization. Although the telescope becomes innovative, it is capable of detecting longer exp…
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Kecheng Wang
2025-11-05T13:56:51Z
置信度 0.70
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2011-07-20T10:03:08Z
置信度 0.70
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2019-02-23T16:27:53Z
置信度 0.70
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2011-07-20T10:03:08Z
置信度 0.70
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Aims. We investigated the potential of polarimetric observations in the optical wavelength range for the detection of exomoons and the characterization of exoplanet-exomoon systems. Methods. Using the three-dimensional Monte Carlo radiative transfer code POLAR…
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M. B. Michaelis, M. Lietzow-Sinjen, S. Wolf
2025-04-01T18:48:25Z
置信度 0.70
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The discovery and study of exoplanets have made tremendous strides, particularly with the aid of Artificial Intelligence (AI). The surge in data from space missions like Kepler, TESS, and the upcoming James Webb Space Telescope has necessitated the development…
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Gautam Saikia
2025-01-30T06:00:52Z
置信度 0.70
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Ground based telescopes have been proven efficient enough for successful follow-up observations of exoplanets for more than 20 years now. In the field of exoplanets we have entered the era of characterisation, where the confirmation of exoplanets is not enough…
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Anastasia Kokori
2025-07-09T15:45:11Z
置信度 0.70
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We considers the properties of the TOI-3568 system, which has a super-Neptune-type planet and which by its properties falls into the region of the sub-Jovian desert. TOI-3568 is a poorly studied dwarf of the spectral class K. On the base of archival measuremen…
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I. S Savanov
2025-11-14T14:59:56Z
置信度 0.70
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With the first exoplanet JWST and Cheops data available, and ARIEL in the near future, we are expecting to get a lot of time-varying measurements of exoplanets (e.g. phase curves and 3D eclipse maps), giving us unprecedented information about their climate. Ho…
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Nicolas Iro, Thomas Fauchez, Thaddeus Komacek, Emily Rauscher 等
2024-03-11T11:16:49Z
置信度 0.70
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2018-03-04T15:16:02Z
置信度 0.70
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Sara Seager
2019-11-01T09:02:01Z
置信度 0.70
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Since the discovery of 51 Pegasi b in 1995, exoplanet research has evolved from serendipitous radial-velocity detections to large-scale surveys employing transit photometry, microlensing, astrometry, and high-contrast direct imaging. Each technique probes diff…
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Xiaotong Wang
2025-11-19T15:57:58Z
置信度 0.70
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2019-02-23T16:27:53Z
置信度 0.70
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2018-03-04T15:16:02Z
置信度 0.70
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Abstract Atmospheric retrievals are essential tools for interpreting exoplanet transmission and eclipse spectra, enabling quantitative constraints on the chemical composition, aerosol properties, and thermal structure of planetary atmospheres. The James Webb S…
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Yoav Rotman, Luis Welbanks, Michael R. Line, Peter McGill 等
2025-08-18T08:25:01Z
置信度 0.70
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2018-08-28T07:09:34Z
置信度 0.70
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2018-03-04T15:16:02Z
置信度 0.70
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The detection of exoplanets, the characterization of their atmospheres, and the study of exoplanet formation mechanisms are major current challenges in astrophysics. High-contrast direct imaging (HCI) is one of the observational techniques of choice to address…
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Théo Bodrito, Olivier Flasseur, Julien Mairal, Jean Ponce 等
2025-07-09T15:45:11Z
置信度 0.70
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Abstract High-resolution spectroscopy ( R > 25,000) has opened new opportunities to characterize exoplanet atmospheres from the ground. By resolving individual lines in planetary emission and transmission spectra, one can sensitively probe the chemical inve…
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Ruizhe Wang, Ryan J. MacDonald, Neale P. Gibson, Nikole K. Lewis
2025-05-22T08:42:51Z
置信度 0.70