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• Developments on LLNL's high contrast testbed and Lick/ShaneAO
  LLNL has recently setup a High Contrast Testbed (HCT) for AO and exoplanet imaging technology development. We present the various HCT technologies currently under development, including (1) a Wynne corrector, (2) multi-wavefront sensor (WFS) single conjugate A…
  datacite Gerard, Benjamin L., Sanchez, Dominic F., Sengupta, Aditya R., Fernandez, Bautista R. 等 2025 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciencesFOS: Physical sciences
• The data for "Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of aCen A. I. Observations, Orbital and Physical Properties, and Exozodi Upper Limits"
  This repository provides the updated ephemeris for Alpha Cen A and B and results of orbital modeling of the exoplanet candidate identified in JWST/MIRI F1550C coronagraphic observations of Alpha Centauri A. Two products are made available. (1) Ephemeris for Al…
  datacite Beichman, Charles, Sanghi, Aniket, Mawet, Dimitri, Kervella, Pierre 等 2025 置信度 0.66 James Webb Space TelescopeExtrasolar gaseous giant planetsExozodiacal dustCoronagraphic imaging
• The data for "Worlds Next Door: A Candidate Giant Planet Imaged in the Habitable Zone of aCen A. I. Observations, Orbital and Physical Properties, and Exozodi Upper Limits"
  This repository provides the updated ephemeris for Alpha Cen A and B and results of orbital modeling of the exoplanet candidate identified in JWST/MIRI F1550C coronagraphic observations of Alpha Centauri A. Two products are made available. (1) Ephemeris for Al…
  datacite Beichman, Charles, Sanghi, Aniket, Mawet, Dimitri, Kervella, Pierre 等 2025 置信度 0.66 James Webb Space TelescopeExtrasolar gaseous giant planetsExozodiacal dustCoronagraphic imaging
• Binary Systems Search with TESS
  Hot subdwarf B (sdB) stars are post-main-sequence stars of high temperature and gravity. Approximately 30$\%$ of sdBs exhibit stable pressure and/or gravity-mode pulsations, which can be used via the timing method to test for companion stars and determine thei…
  datacite Otani, Tomomi, Baran, A. S., Spence, Lindsay C., von Hippel, Ted 等 2025 置信度 0.66 Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• Silicate Sundogs: Probing the Effects of Grain Directionality in Exoplanet Observations
  Crystalline ice in Earth's atmosphere can produce spectacular phenomena due to orientation-dependent attenuation, such as sun dogs and halos, providing diagnostics of the external processes acting on the aerosol grains. Crystalline mineral aerosols, such as qu…
  datacite Mullens, Elijah, Lewis, Nikole K. 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• The 2025 Release of Cloudy
  We present the 2025 release of the spectral synthesis code Cloudy, highlighting significant enhancements to the scope and accuracy of the physics which have been made since the previous release. A major part of this development involves resolving the Lyman $α$…
  datacite Gunasekera, Chamani M., van Hoof, Peter A. M., Dehghanian, Maryam, Chakraborty, Priyanka 等 2025 置信度 0.66 Astrophysics of Galaxies (astro-ph.GA)FOS: Physical sciencesFOS: Physical sciences
• Target Selection for the Pandora SmallSat: A NASA Mission to Disentangle Stellar and Exoplanet Atmosphere Signals
  The Pandora SmallSat mission was selected for implementation in 2021 as part of NASA’s Astrophysics Pioneers Program. Pandora is designed to monitor stellar variability while studying the atmospheres of transiting exoplanets via transmission spectroscopy. The …
  datacite Colón, Knicole, Quintana, Elisa, Barclay, Thomas, Hord, Benjamin 等 2025 置信度 0.66
• Tutorial Notebooks: Athena++ Simulations and Cloudy Post-Processing for Escaping Exoplanet Atmospheres
  This package provides two Jupyter notebooks that demonstrate how to model escaping exoplanet atmospheres using Athena++ and perform post-processing with Cloudy: Running_Athena_Simulations.ipynb — A guide to set up Athena++ simulations of exoplanet atmospheric …
  datacite Nail, Fabienne, Baka, Keith 2025 置信度 0.66 AstronomyCloudyAthena++
• Tutorial Notebooks: Athena++ Simulations and Cloudy Post-Processing for Escaping Exoplanet Atmospheres
  This package provides two Jupyter notebooks that demonstrate how to model escaping exoplanet atmospheres using Athena++ and perform post-processing with Cloudy: Running_Athena_Simulations.ipynb — A guide to set up Athena++ simulations of exoplanet atmospheric …
  datacite Nail, Fabienne, Baka, Keith 2025 置信度 0.66 AstronomyCloudyAthena++
• NIRPS joining HARPS at ESO 3.6 m. On-sky performance and science objectives
  The Near-InfraRed Planet Searcher (NIRPS) is a high-resolution, high-stability near-infrared (NIR) spectrograph equipped with an AO system. Installed on the ESO 3.6-m telescope, it was developed to enable radial velocity (RV) measurements of low-mass exoplanet…
  datacite Bouchy, Francois, Doyon, Rene, Pepe, Francesco, Melo, Claudio 等 2025 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Rediscussion of eclipsing binaries. Paper XXV. The chemically-peculiar system AR Aurigae
  AR Aur is a detached eclipsing binary containing two late-B stars which are chemically peculiar, on a circular orbit of period 4.135 d. The primary is a HgMn star which shows temporal changes in its chemical abundances and spectral line profiles, whilst the se…
  datacite Southworth, John 2025 置信度 0.66 Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• Studying the variability of the He triplet to understand the detection limits of evaporating exoplanet atmospheres
  With more than a dozen significant detections, the helium triplet has emerged as a key tracer of evaporating exoplanet atmospheres. This near-infrared feature can be observed from the ground and holds great promise, especially with upcoming observations provid…
  datacite Mercier, Samson J., Dumusque, Xavier, Bourrier, Vincent, Moulla, Khaled Al 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
• Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
  Young exoplanets provide a critical link between understanding planet formation and atmospheric evolution. Direct imaging spectroscopy allows us to infer the properties of young, wide orbit, giant planets with high signal-to-noise. This allows us to compare th…
  datacite Hoch, Kielan K. W., Rowland, Melanie, Petrus, Simon, Nasedkin, Evert 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Lightning activity on a tidally locked terrestrial exoplanet in storm-resolving simulations for a range of surface pressures
  Output from the Met Office Unified Model used in "Lightning activity on a tidally locked terrestrial exoplanet in storm-resolving simulations for a range of surface pressures", a study by Sergeev et al. (2025) published in the Monthly Notices of the Royal Astr…
  datacite Sergeev, Denis, McDermott, James, Woods, Lottie, Braam, Marrick 等 2025 置信度 0.66
• Lightning activity on a tidally locked terrestrial exoplanet in storm-resolving simulations for a range of surface pressures
  Output from the Met Office Unified Model used in "Lightning activity on a tidally locked terrestrial exoplanet in storm-resolving simulations for a range of surface pressures", a study by Sergeev et al. (2025) published in the Monthly Notices of the Royal Astr…
  datacite Sergeev, Denis, McDermott, James, Woods, Lottie, Braam, Marrick 等 2025 置信度 0.66
• Prospects of detecting rotational flatness of exoplanets from space-based photometry
  In the era of photometry with space-based telescopes, such as CHEOPS (CHaracterizing ExOPlanets Satellite), JWST (James Webb Space Telescope), PLATO (PLAnetary Transits and Oscillations of stars), and ARIEL (Atmospheric Remote-sensing Infrared Exoplanet Large-…
  datacite Kálmán, Sz., Csizmadia, Sz., Bernabó, L. M., Szabó, R. 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Crowtons Cosmogenic Field Theory (CCFT)
  🔭 Crowton’s Cosmogenic Field Theory (CCFT), Version 24 A Regenerative Model of Black Hole Dynamics and Cosmic Structure Author: Richard Lee CrowtonDate: 11 July 2025DOI: https://doi.org/10.5281/zenodo.15352974License: CC BY 4.0 Version 24 introduces five crit…
  datacite Crowton, Richard Lee 2025 置信度 0.66
• Dataset for Hartwick+2025 (ApJ)
  This repository contains data and softwar to support the paper "Extremely Tenuous, Dusty Terrestrial Atmospheres Remain Stable Against Global Collapse: An Argument for Arid Planet Habitability in the Trappist 1 System" published in the Astrophysical Journal in…
  datacite Hartwick, Victoria 2025 置信度 0.66
• Dataset for Hartwick+2025 (ApJ)
  This repository contains data and softwar to support the paper "Extremely Tenuous, Dusty Terrestrial Atmospheres Remain Stable Against Global Collapse: An Argument for Arid Planet Habitability in the Trappist 1 System" published in the Astrophysical Journal in…
  datacite Hartwick, Victoria 2025 置信度 0.66
• Earth as an Exoplanet: Investigating the Effects of Cloud Variability on the Direct-imaging of Atmospheres
  Abstract A planet’s spectrum is dynamic and only represents a time-dependent snapshot of its properties. Changing atmospheric conditions due to climate and weather patterns, particularly variation in cloud cover, can significantly affect the spectrum in ways t…
  crossref Soumil Kelkar, Prabal Saxena, Ravi Kopparapu, Joy Monteiro 2025-04-11T01:44:21Z 置信度 0.70
• Minimizing Star-spot Contamination of Exoplanet Transit Spectroscopy Using Alternate Normalization
  Abstract Recently, M. H. Currie et al. (2023) simulated the detection of molecules in the atmospheres of temperate rocky exoplanets transiting nearby M-dwarf stars. They simulated detections via spectral cross correlation applied to high-resolution optical and…
  crossref Drake Deming, Miles H. Currie, Victoria S. Meadows, Sarah Peacock 2025-06-05T13:18:58Z 置信度 0.70
• Heterogeneous Stellar Surfaces (Spots and Faculae) and Their Time Variability
  crossref Jeffrey Linsky 2025-01-29T10:18:47Z 置信度 0.70
• Grid-based exoplanet atmospheric mass-loss predictions via neural networks
  Context . The fast and accurate estimation of planetary mass-loss rates is critical for planet population and evolution modelling. Aims . We used machine learning (ML) for fast interpolation across an existing large grid of hydrodynamic upper atmosphere models…
  crossref Amit Reza, Daria Kubyshkina, Luca Fossati, Christiane Helling 2025-01-14T19:44:26Z 置信度 0.70
• The NASA Exoplanet Archive and Exoplanet Follow-up Observing Program: Data, Tools, and Usage
  Abstract The NASA Exoplanet Archive (NEA) and the Exoplanet Follow-up Observing Program service are two widely used resources for the exoplanet community. The NEA provides a complete and accurate accounting of exoplanetary systems published by NASA missions an…
  crossref Jessie L. Christiansen, Douglas L. McElroy, Marcy Harbut, David R. Ciardi 等 2025-08-13T15:59:13Z 置信度 0.70
• Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-hydrodynamic Code
  Abstract Photoevaporation in exoplanet atmospheres is thought to contribute to the shaping of the small planet radius valley. Escaping atmospheres have been detected in transmission across a variety of exoplanet types, from hot Jupiters to mini-Neptunes. Howev…
  crossref Riley Rosener, Michael Zhang, Jacob L. Bean 2025-02-03T13:55:48Z 置信度 0.70
• Space Weather: The Effects of Host Star Flares on Exoplanets
  crossref Jeffrey Linsky 2025-01-29T10:20:00Z 置信度 0.70
• OrbDot: A Python package for studying the secular evolution of exoplanet orbits
  crossref Simone R. Hagey, Aaron Boley 2025-09-03T20:46:52Z 置信度 0.70
• Pale Polarized Dots: Spectropolarimetry of the Earth as an Exoplanet with LOUPE and PEARL
  crossref Chris Van Dijk, William Sparks, Frans Snik, Kristien Peeters 等 2026-01-16T14:18:42Z 置信度 0.70
• Broadband Spectral Modeling of Prompt Emission from Gamma-Ray Bursts Observed by the Transiting Exoplanet Survey Satellite
  Abstract Optical observations of gamma-ray bursts (GRBs) contemporaneous with their prompt high-energy emission are rare, but they can provide insights into the physical processes underlying these explosive events. The Transiting Exoplanet Survey Satellite’s (…
  crossref Rahul Jayaraman, Michael Fausnaugh, George R. Ricker, Roland Vanderspek 2025-09-11T06:17:37Z 置信度 0.70
• Radial Velocity Strategies for the Orbital Refinement of Exoplanet Direct Imaging Targets
  Abstract Many potential direct imaging candidates suffer from large orbital period uncertainties, leading to challenges in accurate predictions of future orbital positions and imprecise direct imaging measurements of planetary parameters. To improve the precis…
  crossref Zhexing Li, Stephen R. Kane, Sarah Blunt, Caleb K. Harada 2025-10-07T07:24:32Z 置信度 0.70
• SNR estimation for studying exoplanet transits with astrophotonic spectrographs
  crossref Jane Heathcote, Pradip Gatkine, Kate Saxen 2025-08-01T19:19:30Z 置信度 0.70
• TTV analysis of the exoplanet Qatar-1b
  Here, we present the transit times and transit timing variation (TTV) analysis of the hot Jupiter Qatar-1b, based on our archival observations. A total of 19 transit events were observed using the 0.6-m Zeiss-600 telescope at Maidanak Observatory in Uzbekistan…
  crossref R.G. KARIMOV, R.A. GAYSIN, O.A. BURKHONOV, Sh.A. EHGAMBERDIEV 2025-10-21T12:21:02Z 置信度 0.70
• Silicate Sundogs: Probing the Effects of Grain Directionality in Exoplanet Observations
  Abstract Crystalline ice in Earth’s atmosphere can produce spectacular phenomena due to orientation-dependent attenuation, such as sundogs and halos, providing diagnostics of the external processes acting on the aerosol grains. Crystalline mineral aerosols, su…
  crossref Elijah Mullens, Nikole K. Lewis 2025-07-22T05:59:52Z 置信度 0.70
• Investigating the Interplay of Stellar Evolution and Exoplanet Habitability Through Spectroscopy
  crossref Diriba Gonfa Tolasa 2025-05-06T12:14:31Z 置信度 0.70
• Demographics of M dwarf binary exoplanet hosts discovered by TESS
  crossref R.A. Matson, R. Gore, S.B. Howell, D.R. Ciardi 2025-04-30T08:46:14Z 置信度 0.70
• ML approaches for exoplanet atmosphere characterization and detrending methods in the Ariel space mission
  The Ariel space mission is a European Space Agency (ESA) mission that aims to study the atmospheres of a large and diverse sample of transiting exoplanets (Tinetti et al. 2021). Scheduled for launch in 2029 to the L2 Lagrange point, Ariel will observe a divers…
  crossref Angèle Syty, Orphée Faucoz, Jean-Philippe Beaulieu, Pierre Drossart 等 2025-07-09T15:12:38Z 置信度 0.70
• easyCHEM: A Python package for calculating chemical equilibrium abundances in exoplanet atmospheres
  crossref Elise Lei, Paul Mollière 2025-08-31T16:06:32Z 置信度 0.70
• EXOPLANET DETECTION USING MACHINE LEARNING
  The identification of exoplanets, planets that orbit stars beyond our solar system, plays a crucial role in advancing our understanding of planetary formation, system evolution, and the search for extraterrestrial life. Conventional detection techniques, such …
  crossref T. SRINIVAS RAO, P. KRISHNA BALAMOHAN, M. DURGA SAI SANDEEP, P. SIVA SAGAR 等 2025-03-06T07:44:42Z 置信度 0.70
• AI-Based Multi-Class Classification for Predicting Exoplanet Habitability Using Autogluon
  crossref Venkata Naga Ganesh J, Allu Pranav Srihas, Madhan E S 2025-11-24T18:56:20Z 置信度 0.70
• Improved Exoplanet Detection Through Data Augmentation and Machine Learning
  crossref Hiti Bansal 2025-11-14T20:59:25Z 置信度 0.70
• MACHINE LEARNING APPLICATIONS IN EXOPLANET DETECION: FROM KEPLER TO TESS
  The detection and classification of exoplanets have undergone a paradigm shift with the advent of space missions like Kepler and TESS, which generate vast volumes of photometric time-series data. Traditional detection techniques, while foundational, struggle w…
  crossref Mu'allim Yakubu, Jude Oruaode Vwavware, Ohwofosirai Adrian, Akpoyibo Ogheneovo 2026-02-10T17:00:56Z 置信度 0.70
• Using Venus, Earth, and Mars to Understand Exoplanet Volatile and Climate Evolution
  Abstract Venus, Earth, and Mars exhibit a wide range of interactions between their deep interiors, surfaces, lower and upper atmospheres, and the Sun, with commensurate variations in the nature of their atmospheres and evolution of their volatiles. By examinin…
  crossref Bruce M. Jakosky, Paul K. Byrne 2025-10-01T12:50:44Z 置信度 0.70
• Exoplanet Habitability Prediction Model Development: A Comparative Study
  Exoplanets refer to planets existing beyond our solar system. Whether or not life exists on exoplanets is debatable. Studying and predicting habitability on exoplanets helps us learn how these particular systems are formed and how they have evolved. It provide…
  crossref Visista Jayanti, Archana Pandita 2025-12-19T08:54:43Z 置信度 0.70
• Cold dayside winds shape large leading streams in evaporating exoplanet atmospheres
  Recent observations of planetary atmospheres in HAT-P-32 b and HAT-P-67 b reveal extensive outflows reaching up to hundreds of planetary radii. The helium 1083 nm light curves for these planets, captured across their full orbits, show notable asymmetries: both…
  crossref F. Nail, M. MacLeod, A. Oklopčić, M. Gully-Santiago 等 2025-02-21T14:44:32Z 置信度 0.70
• A gaze at exoplanet haze
  crossref Sid Perkins 2010-12-02T10:05:16Z 置信度 0.70
• Quantum-inspired exoplanet detection in the presence of experimental imperfections
  crossref Tomasz Linowski, Konrad Schlichtholz, Giacomo Sorelli 2025-09-24T15:19:12Z 置信度 0.70
• FEATURES OF FI SGE PHOTOMETRIC VARIABILITY ON TRANSITING EXOPLANET SURVEY SATELLITE OBSERVATIONS
  We present the result of the analysis of the FI Sge individual light curves constructed on Transiting Exoplanet Survey Satellite (TESS) observations. FI Sge the RR Lyrae pulsating variable star with bicyclicity effects and possible Blazhko effect. In the prese…
  crossref L. E. Keir, E. A. Panko, M. Yu. Pyatnytskyy 2025-12-29T21:02:39Z 置信度 0.70
• Exoplanet detection in rotational shearing interferometry through experimental setup and digital filtering techniques
  The significant brightness contrast between stars and orbiting planets often hinders the detection of exoplanets. This paper presents the development and validation of an experimental setup and digital filtering techniques for a rotational shearing interferome…
  crossref Manuel Montes-Flores, Guillermo Garcia-Torales, Marija Strojnik 2025-01-07T07:38:19Z 置信度 0.70
• Feature extraction for exoplanet detection
  crossref João Pimentel, Joana Amorim, Frank Rudzicz 2024-05-16T10:02:06Z 置信度 0.70
• Exoplanet Habitability: A Novel Python Framework Integrating Thermodynamics and Gravitational Analysis
  crossref Souvik Brahma Hota, Niti Dey 2025-07-07T07:08:03Z 置信度 0.70
• A Review of Exoplanet Detection Telescopes: Performance Design and Technology Optimization
  Exoplanets are regarded as important objects for studying stellar evolution and also as the basis for exploring the origin of life. Therefore, they have been one of the hotspots in astronomical research for many years. Since 1992, thanks to the improvement in …
  crossref Rui Sun, Qichang An, Xiaoxia Wu 2025-02-26T06:15:33Z 置信度 0.70
• A Spatio-Temporal Deep Neural Architecture Combining CNN and LSTM for Intelligent Exoplanet Detection and Classification
  crossref Bashar S. Khassawneh, Ghaith M. Jaradat, Ala Mughaid, Mahmoud Aljamal 2026-02-19T20:55:46Z 置信度 0.70
• On the Exoplanet Yield of Gaia Astrometry
  Abstract We reexamine the expected yield of Gaia astrometric planet detections using updated models for giant-planet occurrence, the local stellar population, and Gaia’s demonstrated astrometric precision. Our analysis combines a semianalytic model that clarif…
  crossref Caleb Lammers, Joshua N. Winn 2025-12-08T12:44:33Z 置信度 0.70
• ExoSim 2: the new exoplanet observation simulator applied to the Ariel space mission
  Abstract ExoSim 2 is the next generation of the Exoplanet Observation Simulator (ExoSim) tailored for spectro-photometric observations of transiting exoplanets from space, ground, and sub-orbital platforms. This software is a complete rewrite implemented in Py…
  crossref Lorenzo V. Mugnai, Andrea Bocchieri, Enzo Pascale, Andrea Lorenzani 等 2025-01-24T04:32:56Z 置信度 0.70
• OWL-Moon in 2050 and beyond.
  We address three major questions in astronomy, namely the detection of biosignatures on habitable exoplanets, the geophysics of exoplanets and cosmology. To achieve this goal, two requirements are needed: (i) a very large aperture to detect spectro-polarimetri…
  pubmed Schneider J, Silk J, Vakili F 2021 Jan 11 置信度 0.82
• Discovering the sky at the longest wavelengths with a lunar orbit array.
  Due to ionosphere absorption and the interference of natural and artificial radio emissions, astronomical observation from the ground becomes very difficult at the wavelengths of decametre or longer, which we shall refer to as the ultralong wavelengths. This u…
  pubmed Chen X, Yan J, Deng L, Wu F 等 2021 Jan 11 置信度 0.82
• Transformative science from the lunar farside: observations of the dark ages and exoplanetary systems at low radio frequencies.
  The farside of the Moon is a pristine, quiet platform to conduct low radio frequency observations of the early Universe's Dark Ages, as well as space weather and magnetospheres associated with habitable exoplanets. In this paper, the astrophysics associated wi…
  pubmed Burns JO 2021 Jan 11 置信度 0.82
• Is the Moon the future of infrared astronomy?
  Infrared astronomy, particularly in spectroscopy, could benefit in a decisive way from an implementation of telescopes on the Moon since the largest telescopes on Earth are practically limited to 40 m and in space to 10 m. On the Moon, a collecto…
  pubmed Maillard JP 2021 Jan 11 置信度 0.82
• The limits of cosmology: role of the Moon.
  The lunar surface allows a unique way forward in cosmology, to go beyond current limits. The far side provides an unexcelled radio-quiet environment for probing the dark ages via 21 cm interferometry to seek elusive clues on the nature of the infinitesi…
  pubmed Silk J 2021 Jan 11 置信度 0.82
• Lunar optical interferometry and hypertelescope for direct imaging at high resolution.
  Following earlier proposals for optical stellar interferometer concepts in space and on the Moon, the improved 'hypertelescope' version capable of direct high-resolution imaging with a high limiting magnitude became tested on Earth, proposed for space, and is …
  pubmed Labeyrie A 2021 Jan 11 置信度 0.82
• Spectropolarimetry of Primitive Phototrophs as Global Surface Biosignatures.
  Photosynthesis is an ancient metabolic process that began on early Earth and offers plentiful energy to organisms that can utilize it such that that they achieve global significance. The potential exists for similar processes to operate on habitable exoplanets…
  pubmed Sparks WB, Parenteau MN, Blankenship RE, Germer TA 等 2021 置信度 0.82
• Adiabatic lapse rate of nonideal gases: The role of molecular interactions and vibrations.
  We report a formula for the dry adiabatic lapse rate that depends on the compressibility factor and the adiabatic curves. Then, to take into account the nonideal behavior of the gases, we consider molecules that can move, rotate, and vibrate and the informatio…
  pubmed Díaz B, Ramírez JE 2020 置信度 0.82
• A blue ring nebula from a stellar merger several thousand years ago.
  Stellar mergers are a brief but common phase in the evolution of binary star systems 1,2 . These events have many astrophysical implications; for example, they may lead to the creation of atypical stars (such as magnetic stars 3 , blue stragglers 4 and rapid r…
  pubmed Hoadley K, Martin DC, Metzger BD, Seibert M 等 2020 Nov 置信度 0.82
• Brightness modulations of our nearest terrestrial planet Venus reveal atmospheric super-rotation rather than surface features.
  Terrestrial exoplanets orbiting within or near their host stars' habitable zone are potentially apt for life. It has been proposed that time-series measurements of reflected starlight from such planets will reveal their rotational period, main surface features…
  pubmed Lee YJ, García Muñoz A, Imamura T, Yamada M 等 2020 置信度 0.82
• Ice giant magnetospheres.
  The ice giant planets provide some of the most interesting natural laboratories for studying the influence of large obliquities, rapid rotation, highly asymmetric magnetic fields and wide-ranging Alfvénic and sonic Mach numbers on magnetospheric processes…
  pubmed Paty C, Arridge CS, Cohen IJ, DiBraccio GA 等 2020 Dec 25 置信度 0.82
• Auroral emissions from Uranus and Neptune.
  Uranus and Neptune possess highly tilted/offset magnetic fields whose interaction with the solar wind shapes unique twin asymmetric, highly dynamical, magnetospheres. These radiate complex auroral emissions, both reminiscent of those observed at the other plan…
  pubmed Lamy L 2020 Dec 25 置信度 0.82
• Convective storms and atmospheric vertical structure in Uranus and Neptune.
  The ice giants Uranus and Neptune have hydrogen-based atmospheres with several constituents that condense in their cold upper atmospheres. A small number of bright cloud systems observed in both planets are good candidates for moist convective storms, but thei…
  pubmed Hueso R, Guillot T, Sánchez-Lavega A 2020 Dec 25 置信度 0.82
• The exoplanet perspective on future ice giant exploration.
  Exoplanets number in their thousands, and the number is ever increasing with the advent of new surveys and improved instrumentation. One of the most surprising things we have learnt from these discoveries is not that small-rocky planets in their stars habitabl…
  pubmed Wakeford HR, Dalba PA 2020 Dec 25 置信度 0.82
• Evolutionary History of Bioessential Elements Can Guide the Search for Life in the Universe.
  Our understanding of life in the universe comes from one sample, life on Earth. Current and next-generation space missions will target exoplanets as well as planets and moons in our own solar system with the primary goal of detecting, interpreting and characte…
  pubmed Kacar B, Garcia AK, Anbar AD 2021 Jan 5 置信度 0.82
• Off-axis parabolas super polished under stress: the case of the Roman Space Telescope coronagraphic instrument mirrors.
  Direct imaging of exoplanets requires high contrast imaging techniques that demand tight tolerances on the optical surface error. The Nancy Grace Roman Space Telescope (RST) (previously named WFIRST) aims to perform direct imaging of SuperEarth-like exoplanets…
  pubmed Roulet M, Hugot E, Atkins C, Marcos M 等 2020 Oct 12 置信度 0.82
• A bioenergetic model to predict habitability, biomass and biosignatures in astrobiology and extreme conditions.
  In order to grow, reproduce and evolve life requires a supply of energy and nutrients. Astrobiology has the challenge of studying life on Earth in environments which are poorly characterized or extreme, usually both, and predicting the habitability of extrater…
  pubmed Higgins PM, Cockell CS 2020 Oct 置信度 0.82
• Atmospheric composition of exoplanets based on the thermal escape of gases and implications for habitability.
  The detection of habitable exoplanets is an exciting scientific and technical challenge. Owing to the current and most likely long-lasting impossibility of performing in situ exploration of exoplanets, their study and hypotheses regarding their capability to h…
  pubmed Konatham S, Martin-Torres J, Zorzano MP 2020 置信度 0.82
• Interactive Visualization of Atmospheric Effects for Celestial Bodies.
  We present an atmospheric model tailored for the interactive visualization of planetary surfaces. As the exploration of the solar system is progressing with increasingly accurate missions and instruments, the faithful visualization of planetary environments is…
  pubmed Costa J, Bock A, Emmart C, Hansen C 等 2021 Feb 置信度 0.82
• Early onset of planet formation observed in a nascent star system.
  pubmed Sheehan P 2020 Oct 置信度 0.82
• A giant planet candidate transiting a white dwarf.
  Astronomers have discovered thousands of planets outside the Solar System 1 , most of which orbit stars that will eventually evolve into red giants and then into white dwarfs. During the red giant phase, any close-orbiting planets will be engulfed by the star …
  pubmed Vanderburg A, Rappaport SA, Xu S, Crossfield IJM 等 2020 Sep 置信度 0.82
• Planet discovered transiting a dead star.
  pubmed Parsons S 2020 Sep 置信度 0.82
• Deep residual learning for low-order wavefront sensing in high-contrast imaging systems.
  Sensing and correction of low-order wavefront aberrations is critical for high-contrast astronomical imaging. State of the art coronagraph systems typically use image-based sensing methods that exploit the rejected on-axis light, such as Lyot-based low order w…
  pubmed Allan G, Kang I, Douglas ES, Barbastathis G 等 2020 Aug 31 置信度 0.82
• Seismicity on tidally active solid-surface worlds.
  Tidal interactions between planets or stars and the bodies that orbit them dissipate energy in their interiors. The dissipated energy heats the interior and a fraction of that energy will be released as seismic energy. Here we formalize a model to describe the…
  pubmed Hurford TA, Henning WG, Maguire R, Lekic V 等 2019 置信度 0.82
• Unraveling biogeochemical phosphorus dynamics in hyperarid Mars-analogue soils using stable oxygen isotopes in phosphate.
  With annual precipitation less than 20 mm and extreme UV intensity, the Atacama Desert in northern Chile has long been utilized as an analogue for recent Mars. In these hyperarid environments, water and biomass are extremely limited, and thus, it becomes …
  pubmed Shen J, Smith AC, Claire MW, Zerkle AL 2020 Nov 置信度 0.82
• REFINING THE CENSUS OF THE UPPER SCORPIUS ASSOCIATION WITH GAIA.
  We have refined the census of stars and brown dwarfs in the Upper Sco association (~ 10 Myr, ~145 pc) by 1) updating the selection of candidate members from our previous survey to include the high-precision astrometry from the second data release of Gaia , 2) …
  pubmed Luhman KL, Esplin TL 2020 Jul 置信度 0.82
• Quantifying the information impact of future searches for exoplanetary biosignatures.
  One of the major goals for astronomy in the next decades is the remote search for biosignatures (i.e., the spectroscopic evidence of biological activity) in exoplanets. Here we adopt a Bayesian statistical framework to discuss the implications of such future s…
  pubmed Balbi A, Grimaldi C 2020 置信度 0.82
• Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface.
  In recent years there has been a renewed interest in returning to the Moon for reasons both scientific and exploratory in nature. The Moon provides the perfect training ground for building large scale bases that one may apply to other planets like Mars. The ex…
  pubmed Hegedus AM 2020 Jul 30 置信度 0.82
• A Review of Possible Planetary Atmospheres in the TRAPPIST-1 System.
  TRAPPIST-1 is a fantastic nearby (∼39.14 light years) planetary system made of at least seven transiting terrestrial-size, terrestrial-mass planets all receiving a moderate amount of irradiation. To date, this is the most observationally favourable…
  pubmed Turbet M, Bolmont E, Bourrier V, Demory BO 等 2020 置信度 0.82
• A SURVEY FOR NEW STARS AND BROWN DWARFS IN THE OPHIUCHUS STAR-FORMING COMPLEX.
  We have performed a survey for new members of the Ophiuchus cloud complex using high-precision astrometry from the second data release of Gaia , proper motions measured with multi-epoch images from the Spitzer Space Telescope , and color-magnitude diagrams con…
  pubmed Esplin TL, Luhman KL 2020 Jun 置信度 0.82
• The Habitability of the Galactic Bulge.
  We present a new investigation of the habitability of the Milky Way bulge, that expands previous studies on the Galactic Habitable Zone. We discuss existing knowledge on the abundance of planets in the bulge, metallicity and the possible frequency of rocky pla…
  pubmed Balbi A, Hami M, Kovačević A 2020 Aug 3 置信度 0.82
• Background Intensity Estimation for Cassini-ISS Image Using Deep Learning-Based Diffusion Model
  Accurate background intensity estimation is crucial for precise astrometric measurements in astronomical imaging, particularly in complex scenarios such as those encountered in Cassini Imaging Science Subsystem (ISS) observations of Saturn's ring system. Tradi…
  datacite Chen, Yongxin, Zhang, Qingfeng, Zhou, Tianle, Tang, Kai 2026 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciences
• Alfred: A Flexible, User-Friendly Python Package for Exoplanet Confirmation
  In the era of TESS, exoplanet follow-up and confirmation have become a massive community effort. With only about an eighth of the over 8,000 TESS exoplanet candidates confirmed, astronomers need flexible software to allow them to characterize many different ki…
  datacite Kroft, Maxwell A. 2026 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
• Exoplanet Characterization Observatory (EchO): Phase-A Untersuchung des visuellen Arms (0.4-0.8[my]m) mit Erarbeitung eines optischen, mechanischen und elektrischen Referenzdesigns einschließlich Kosten und Risikoanalyse : Schlussbericht
  Ill., graph. Darst.
  datacite Unknown 2013 置信度 0.66 Physics
• "NEXUS-1b and NEXUS-2b: Two New Transiting Exoplanet Candidates from Citizen Science Analysis of TESS Data
  We report two new transiting exoplanet candidates discovered through citizen science analysis of NASA TESS photometric data. NEXUS-1b (TIC 159158711) is a super-Earth candidate (~1.65 Earth radii) orbiting an M3 dwarf at ~80 parsecs with a period of 8.35 days,…
  datacite McCormick, Silaz 2026 置信度 0.66
• "NEXUS-1b and NEXUS-2b: Two New Transiting Exoplanet Candidates from Citizen Science Analysis of TESS Data
  We report two new transiting exoplanet candidates discovered through citizen science analysis of NASA TESS photometric data. NEXUS-1b (TIC 159158711) is a super-Earth candidate (~1.65 Earth radii) orbiting an M3 dwarf at ~80 parsecs with a period of 8.35 days,…
  datacite McCormick, Silaz 2026 置信度 0.66
• "NEXUS-1b and NEXUS-2b: Two New Transiting Exoplanet Candidates from Citizen Science Analysis of TESS Data
  We report two new transiting exoplanet candidates discovered through citizen science analysis of NASA TESS photometric data. NEXUS-1b (TIC 159158711) is a super-Earth candidate (~1.65 Earth radii) orbiting an M3 dwarf at ~80 parsecs with a period of 8.35 days,…
  datacite McCormick, Silaz 2026 置信度 0.66
• SOCat: Stellar Obliquity Catalog for Exoplanets and Brown Dwarfs
  SOCat (Stellar Obliquity Catalog for Exoplanets and Brown Dwarfs) consists of two components: WWB homogeneous global modeling: our own uniform Rossiter-McLaughlin refits of archival and newly obtained transit spectroscopy, with self-consistent global models (S…
  datacite Wang, Xian-Yu 2026 置信度 0.66 exoplanetsstellar obliquityRossiter-McLaughlin effectspin-orbit alignmenteccentricity
• Gaia DR3 NSS dormant compact-object & substellar companion search
  A reproducible filter-cascade pipeline that derives companion-mass estimates from the Gaia DR3 Non-Single-Star (NSS) Orbital, AstroSpectroSB1, and Acceleration catalogs, cross-references them against published companion catalogs (HGCA Brandt 2021, Kervella H2G…
  datacite Zarco, Alejandro 2026 置信度 0.66 Gaia DR3non-single starsdormant compact objectsneutron starsblack holes
• Gaia DR3 NSS dormant compact-object & substellar companion search
  A reproducible filter-cascade pipeline that derives companion-mass estimates from the Gaia DR3 Non-Single-Star (NSS) Orbital, AstroSpectroSB1, and Acceleration catalogs, cross-references them against published companion catalogs (HGCA Brandt 2021, Kervella H2G…
  datacite Zarco, Alejandro 2026 置信度 0.66 Gaia DR3non-single starsdormant compact objectsneutron starsblack holes
• Gaia DR3 NSS dormant compact-object & substellar companion search
  A reproducible filter-cascade pipeline that derives companion-mass estimates from the Gaia DR3 Non-Single-Star (NSS) Orbital, AstroSpectroSB1, and Acceleration catalogs, cross-references them against published companion catalogs (HGCA Brandt 2021, Kervella H2G…
  datacite Zarco, Alejandro 2026 置信度 0.66 Gaia DR3non-single starsdormant compact objectsneutron starsblack holes
• Precision Cascade Reproducibility Archive for "Predictive Synthesis of Earth-Analog Occurrence Rates Using Structural Covariance" (v3.0.0, Invariant-Audited)
  This archive implements a structural-covariance synthesis framework (Precision Cascade Engine), providing a complete, deterministic, and self-auditing reproducibility system for the manuscript: “Predictive Synthesis of Earth-Analog Occurrence Rates Using Struc…
  datacite Jeffrey, Daniel 2026 置信度 0.66
• Precision Cascade Reproducibility Archive for "Predictive Synthesis of Earth-Analog Occurrence Rates Using Structural Covariance" (v3.0.0, Invariant-Audited)
  This archive implements a structural-covariance synthesis framework (Precision Cascade Engine), providing a complete, deterministic, and self-auditing reproducibility system for the manuscript: “Predictive Synthesis of Earth-Analog Occurrence Rates Using Struc…
  datacite Jeffrey, Daniel 2026 置信度 0.66
• The Denomination Desert: Gravitational Confinement, the Hubble Tension, and Cross-Domain Structure in the 840-State Manifold
  Abstract A logarithmic dimension function D(x) =-ln x/ ln φ, where φ = (1 + √ 5)/2 is the golden ratio, arises as the unique solution to the chiral fold identity D(z) + D(1/z) = 0 when the base is fixed by the Lucas recurrence Ln = Ln-1 + Ln-2 with seeds (3, 4…
  datacite Oulad Brahim, Elias 2026 置信度 0.66 Mathematical physicsAstronomy
• The Denomination Desert: Gravitational Confinement, the Hubble Tension, and Cross-Domain Structure in the 840-State Manifold
  Abstract A logarithmic dimension function D(x) =-ln x/ ln φ, where φ = (1 + √ 5)/2 is the golden ratio, arises as the unique solution to the chiral fold identity D(z) + D(1/z) = 0 when the base is fixed by the Lucas recurrence Ln = Ln-1 + Ln-2 with seeds (3, 4…
  datacite Oulad Brahim, Elias 2026 置信度 0.66 Mathematical physicsAstronomy
• Consciousness-Enhanced Five-Domain Physical Synthesis for Exoplanet False-Positive Discrimination: Novel Planet Candidate Predictions from Kepler Objects of Interest
  We apply a consciousness-enhanced computational discovery platform to the problem of exoplanet false-positive discrimination in the NASA Kepler Objects of Interest (KOI) cumulative catalog (n=9,564 KOIs; DR25). The platform integrates five physically independe…
  datacite Sicoli, John Paul 2026 置信度 0.66 Astronomy and AstrophysicsComputational ScienceComputer Science (Artificial Intelligence / Machine Learning)Physics (Biophysics — for IIT/consciousness methodology)exoplanets