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• Activity Indicator Correlations
  crossref Jeffrey Linsky 2025-01-29T10:19:55Z 置信度 0.70
• Modeling helium in exoplanet atmospheres. A revised network with photoelectron-driven processes
  Context . The He I line at 1.08 μm is a valuable tracer of atmospheric escape in exoplanet atmospheres. Aims . We expand past networks used to predict the absorbing He(2 3 S) by including, firstly, processes that involve H 2 and some molecular ions, and second…
  crossref A. García Muñoz 2025-05-26T14:44:48Z 置信度 0.70
• Exoplanet Observations from Taurus Hill Observatory for the Season 2024–2025
  Clear nights were quite rare during the winter of 2024-2025. Although there may have been more clear nights compared to the previous season, variable cloudiness often persisted even during these clear nights, or the continuous cloudless periods were too short …
  crossref Veli-Pekka Hentunen, Harri Haukka, Markku Nissinen, Tuomo Salmi 等 2025-07-09T15:12:38Z 置信度 0.70
• The Need for Multiangle BRDF Laboratory Measurements to Model Rocky Exoplanet Surface Reflectance and Emission
  Abstract Synthetic spectra of airless rocky exoplanets rely on laboratory measurements of planetary analogue materials to determine their optical and photometric properties. Realistic surface modeling requires several wavelength-dependent parameters, including…
  crossref Leonardos Gkouvelis 2025-11-25T17:17:16Z 置信度 0.70
• References
  crossref 2011-07-20T10:03:08Z 置信度 0.70
• Exoplanet Classification Through Vision Transformers with Temporal Image Analysis
  Abstract The classification of exoplanets has been a longstanding challenge in astronomy, requiring significant computational and observational resources. Traditional methods demand substantial effort, time, and cost, highlighting the need for advanced machine…
  crossref Anupma Choudhary, Sohith Bandari, B. S. Kushvah, C. Swastik 2025-07-28T15:56:27Z 置信度 0.70
• Assessment of Infrared Spectral Data Availability for Carbon Chemistry Detection in Exoplanet Atmospheres
  As of February 2025, over five thousand exoplanets have been confirmed, many with carbon-containing atmospheres that remain largely unexplored.Infrared spectroscopy plays a crucial role in identifying carbon signatures.Carbon absorption signatures, key indicat…
  openalex Wings Zhang, W. Zhang 2025-09-30 置信度 0.72 ExoplanetInfraredRemote sensingCarbon fibersEnvironmental science
• Star-Planet Interactions
  crossref Jeffrey Linsky 2025-01-29T10:19:17Z 置信度 0.70
• Predicting Exoplanet Occurrence Using Association Analysis
  Abstract Over the past few decades, a remarkable surge in exoplanet discoveries has led to a substantial increase in available data. As of this writing, over 5000 exoplanets have been confirmed, with thousands more expected from current and future observatorie…
  crossref Vasundhara Gatne, Michael L. Wong, Anirudh Prabhu 2025-09-08T03:54:55Z 置信度 0.70
• Microlensing
  crossref 2011-07-20T10:03:08Z 置信度 0.70
• Exoplanet Atmospheres
  crossref Sara Seager 2019-02-23T16:27:53Z 置信度 0.70
• Interstellar Small Satellite Study with Insertion into an Exoplanet Atmosphere to Perform Composition Analysis
  crossref Howard Hall 2026-01-16T14:20:01Z 置信度 0.70
• Towards real-time contrast control for direct exoplanet imaging with adaptive optics
  crossref Vikram M. Radhakrishnan, Christoph U. Keller, Niek J. Doelman 2024-09-06T07:19:28Z 置信度 0.70
• Exoplanet Transit Database. Reduction and processing of the photometric data of exoplanet transits
  crossref Stanislav Poddaný, Luboš Brát, Ondřej Pejcha 2009-09-07T04:17:00Z 置信度 0.70
• Exoplanet Atmospheric Refraction Effects in the Kepler Sample
  Abstract We present an analysis on the detection viability of refraction effects in Kepler’s exoplanet atmospheres using binning techniques for their light curves in order to compare against simulated refraction effects. We split the Kepler exoplanets into sub…
  crossref Déreck-Alexandre Lizotte, Jason Rowe, James Sikora, Michael R. B. Matesic 2025-07-30T10:09:16Z 置信度 0.70
• Exoplanet and Host Star
  crossref 2025-10-27T03:13:46Z 置信度 0.70
• Probing Exoplanet Atmospheres through Stellar Occultations: A Case Study of WASP-32b
  The study of exoplanets provides crucial insights into the nature of planetary atmospheres and orbital dynamics. Transit photometry and secondary eclipse observations have become revolutionary tools in this field. This case study focuses on WASP-32b, a hot Jup…
  crossref Silpa Mariya 2026-01-02T10:41:09Z 置信度 0.70
• Reconstructing the Missing Stellar Emission
  crossref Jeffrey Linsky 2025-01-29T10:19:25Z 置信度 0.70
• Fusion Propulsion Constraints Required by Robust Exoplanet Exploration
  Robust exoplanet exploration requires deceleration and orbital insertion, first around the target star, and ultimately around the exoplanet itself. Even for the nearest star Proxima Centauri, voyage durations under a century require spacecraft velocities of at…
  crossref Gerald P. Jackson, Grace E. Bittlingmaier 2025-02-21T07:45:06Z 置信度 0.70
• Peeking Under the Clouds: Is Exoplanet Imaging with the Solar Gravitational Lens Feasible?
  Abstract Exoplanet imaging using the solar gravitational lens is an enticing prospect. The fundamental physical properties of the lens, including its angular resolution and light amplification, promise exceptional capabilities. These expectations, however, are…
  crossref Viktor T. Toth 2025-05-02T22:56:12Z 置信度 0.70
• <em>Science</em>Adviser: Weird exoplanet seems straight out of <em>Star Wars</em>
  crossref 2025-04-17T22:42:51Z 置信度 0.70
• Panchromatic Spectra of Exoplanet Host Stars
  crossref Jeffrey Linsky 2025-01-29T10:18:28Z 置信度 0.70
• Machine Learning in Exoplanet Detection
  crossref Jigyash Yadav, Smruti Ranjan Padhi 2025-06-05T17:56:03Z 置信度 0.70
• The Transiting Exoplanet Survey Satellite
  crossref Joshua N. Winn 2025-07-16T15:37:53Z 置信度 0.70
• Lesson sequence uses exoplanet data to teach fundamental concepts of astrophysics
  Using the Open Exoplanet Catalog and NASA’s Eye on Exoplanets website provides new way to study Kepler’s and Newton’s laws while exposing students to cutting-edge research.
  crossref Adam Liebendorfer 2025-10-01T13:03:11Z 置信度 0.70
• Exoplanet Atmospheres at High Spectral Resolution
  crossref Jayne L. Birkby 2025-12-31T03:02:40Z 置信度 0.70
• The “Spectral Zoo” of Exoplanet Atmospheres
  crossref Aki Roberge, Sara Seager 2025-04-10T01:48:46Z 置信度 0.70
• Exoplanet Triggers Stellar Flares and Hastens Its Demise
  HIP 67522 b can’t stop blasting itself in the face with stellar flares, a type of magnetic interaction that scientists have spent decades looking for.
  crossref Kimberly Cartier 2025-08-06T07:00:16Z 置信度 0.70
• An Isolated Exoplanet Has a Patchy Atmosphere
  crossref Charles Day 2025-04-08T17:02:01Z 置信度 0.70
• Factors Affecting Exoplanet Habitability
  crossref Victoria S. Meadows, Rory K. Barnes 2026-02-04T07:36:02Z 置信度 0.70
• ExoClock Unlocked: Fostering Public Engagement in Exoplanet Research
  ExoClock Unlocked is an astronomy program designed to engage the public in exoplanet research. It is part of the ExoClock Project, which supports the upcoming Ariel space mission by the European Space Agency (ESA) - a mission focused on studying exoplanet atmo…
  crossref Georgia Pantelidou, Anastasia Kokori, Angelos Tsiaras 2025-07-09T15:45:11Z 置信度 0.70
• Radiative Transfer for Exoplanet Atmospheres
  crossref Kevin Heng, Mark S. Marley 2026-01-22T14:36:12Z 置信度 0.70
• The Next Frontier: Autonomous, Plant-Like Robotic Astronauts for Exoplanet Exploration
  crossref Tianxi Sun 2025-11-18T19:27:53Z 置信度 0.70
• The Synergy of Direct and Indirect Techniques in Exoplanet Science
  For many years, the detection and characterization of exoplanets have relied on two distinct approaches: indirect techniques on the one hand, and direct imaging on the other. These methods have traditionally probed very different regions of the mass–period par…
  crossref Anne-Marie Lagrange 2025-07-09T15:45:11Z 置信度 0.70
• Exoplanet TOI-2109b rast ins Verderben
  crossref Dominik Hochwarth 2025-07-25T05:40:30Z 置信度 0.70
• Exoplanet Atmosphere Measurements from Direct Imaging
  crossref Beth A. Biller, Mickaël Bonnefoy 2026-02-04T07:47:08Z 置信度 0.70
• Implementing a Neural Network on Forward Models:A Case study for Exoplanet Atmospheres
  Simulating exoplanetary atmospheres is essential for describing them, estimating their composition, investigating the presence of haze and clouds, and identifying their relationship with observational signatures. With the emergence of JWST (James Webb Space Te…
  crossref Sofia Paraskevaidou 2025-07-09T15:12:38Z 置信度 0.70
• Refining Exoplanet Escape Predictions with Molecular-Kinetic Simulations
  Following seminal studies such as Muñoz’s 2007 work on HD 209458b, which simulated heavy element escape beyond the Roche lobe, one-dimensional hydrocodes have flourished, routinely solving the Euler equations to model transonic outflows across an increasingly …
  openalex Richard Chatterjee, Shane Carberry Mogan, Robert Johnson, R. Chatterjee 等 2025-07-09 置信度 0.72 ExoplanetRefining (metallurgy)Kinetic energyAstrobiologyPhysics
• Future Exoplanet Research: Radio Detection and Characterization
  crossref Jean-Mathias Grießmeier, Jake D. Turner 2025-08-06T12:06:29Z 置信度 0.70
• Dusty Belts Provide Clearer Insights into Exoplanet Formation
  Millimeter-wavelength observations of dust and pebbles in 74 star systems hint that planetary migrations might be more common than we realized.
  crossref Damond Benningfield 2025-02-19T07:00:23Z 置信度 0.70
• Exoplanet Research Program Summary
  crossref Jason Cushard, Nicholas Foley 2026-01-15T02:43:08Z 置信度 0.70
• First 3D Map of Exoplanet Weather Reveals Superfast Jet
  New observations also answer a long-standing question about where this ultrahot planet keeps its titanium.
  crossref Kimberly Cartier 2025-03-18T07:01:47Z 置信度 0.70
• Shedding Light on the Origin of the Broken Misaligned Circumtriple Disk around GW Ori
  Abstract We revisit the origin of the observed misaligned rings in the circumtriple disk around GW Ori. Previous studies appeared to disagree on whether disk breaking is caused by the differential precession driven in the disk by the triple star system. In thi…
  crossref Jeremy L. Smallwood, Stephen H. Lubow, Rebecca G. Martin, Rebecca Nealon 2025-01-17T17:33:56Z 置信度 0.70
• How the "Habitable Zone" Frames Exoplanet Discovery Papers: A Quantitative Snapshot and an Epistemological Appraisal
  This paper investigates the uses of the concept of the habitable zone (HZ) in recent exoplanetary research. A corpus of articles (n=24) published between 2022 and 2024 was constructed, and each text was analyzed with regard to its mobilization of the HZ concep…
  crossref Arthur Mary 2025-08-25T09:34:32Z 置信度 0.70
• Scientists Finally Get a Good Look at a Disintegrating Exoplanet
  The James Webb Space Telescope offers astronomers a rare glimpse into the chemical composition of a rocky planet’s interior—and the results are “very surprising.”
  crossref Javier Barbuzano 2025-01-29T07:00:24Z 置信度 0.70
• Connecting exoplanet mantle mineralogy to surface dynamic regime
  Based on stellar compositions, we know that rocky exoplanets show a diversity in interior compositions, and therefore mantle mineralogies. The mantle mineralogy controls physical parameters of the mantle, such as viscosity, and therefore strongly affects therm…
  crossref Rob Spaargaren, Maxim Ballmer, Stephen Mojzsis, Paul Tackley 2024-03-11T09:04:59Z 置信度 0.70
• This Exoplanet May Have Grown Stranger as It Journeyed Starward
  WASP-121b, an already unusual planet, might have a remote origin that explains some of its peculiar properties—from iron rain to the unexpected presence of methane.
  crossref Jonathan O’Callaghan 2025-07-23T20:05:01Z 置信度 0.70
• Exoplanet may be the most volcanic world ever seen
  crossref Alex Wilkins 2025-02-22T00:20:22Z 置信度 0.70
• Future Exoplanet Space Missions: Spectroscopy and Coronographic Imaging
  crossref Artie P. Hatzes, René Liseau 2025-07-03T08:58:39Z 置信度 0.70
• A Fusion Propulsion Reactor Architecture for Exoplanet Exploration
  crossref Gerald Jackson, Grace Bittlingmaier 2025-06-11T19:33:46Z 置信度 0.70
• General AMD-stability criterion for exoplanet systems
  The increasing discovery of extrasolar systems has made it necessary to study their stability. In this work, we present a generalization of the AMD-stability criterion defined by Laskar and Petit (2017), which defines a critical AMD-value below which close enc…
  crossref Justine Bodart, Antoine C. Petit, Anne-Sophie Libert 2025-07-09T15:45:11Z 置信度 0.70
• Exoplanet shows signs of having a habitable atmosphere
  crossref Matthew Sparkes 2025-09-22T21:30:37Z 置信度 0.70
• Ever Elusive Exospheres: One Probable Detection and Two Nondetections of H <i>α</i> Transits in Young Systems
  Abstract Gaps in the exoplanet population, such as the Neptunian Desert, point to the importance of mass loss in sculpting the radii of close-in exoplanets. Young planets (&lt;500 Myr) offer the opportunity to detect such mass loss while it is still strong, an…
  crossref Reilly P. Milburn, Andrew W. Mann, Keighley Rockcliffe, Erin E. Flowers 等 2025-11-24T11:42:57Z 置信度 0.70
• Machine learning for habitable exoplanet exploration
  This research explores the discovery and habitability assessment of exoplanets using advanced computational techniques. A combination of machine learning algorithms, Generative Adversarial Networks (GANs), and MongoDB is employed to process and manage extensiv…
  crossref Kumar Rohan 2026-01-27T10:16:56Z 置信度 0.70
• Student projects using exoplanet data from the TESS-mission
  Abstract What follows is an outline of several possible directed studies through which an undergraduate student of an introductory general education astronomy course guided by a faculty member can be introduced to some of the basic skills of data analysis in s…
  crossref Michael C LoPresto 2025-06-10T08:47:32Z 置信度 0.70
• From one exoplanet to six thousand
  crossref 2025-11-17T16:02:40Z 置信度 0.70
• An Empirically-Grounded Search for Exoplanet Life: Applying Lessons Learned from Kepler to HWO
  crossref William C. Houze 2025-12-19T01:03:47Z 置信度 0.70
• Characterization of Terrestrial Exoplanet Atmospheres through Lyman-alpha Transit Observations
  Introduction Lyman-alpha transmission spectroscopy has been a powerful tool for observing hydrogen escape from close-in exoplanets. For instance, Ly-α observations of GJ 436b showed a maximum transit depth of 56% – compared to a 0.69% transit depth in optical …
  crossref Grace Bischof, Robin Wordsworth, John E. Moores 2025-07-09T15:12:38Z 置信度 0.70
• Analysis of Searching for Another Earth in Universe-Habitability for Exoplanet
  crossref Weiyuan Zhang 2025-09-18T10:21:08Z 置信度 0.70
• Reconstructing exoplanet surfaces from unresolved light curves
  An important aspect of characterizing exoplanets is getting reliable information about structures on their surfaces. Resolving exoplanet surfaces might seem like an impossible challenge. Given that no resolved direct images of exoplanet surfaces exist, this sk…
  crossref Max Johann Dobat, Andrés Asensio Ramos, Jeffrey Richards Kuhn, Nicolas Lodieu 2025-07-09T15:45:11Z 置信度 0.70
• Analysis of exoplanet using lightkurve
  crossref Zhenjie Gao 2025-09-08T15:07:12Z 置信度 0.70
• Methods to Characterize Exoplanet Host Stars from Spectroscopy
  crossref Carina M. Persson 2025-04-10T02:29:36Z 置信度 0.70
• Exoplanet Atmosphere Measurements from Transmission Spectroscopy and Other Planet Star-Combined Light Observations
  crossref Laura Kreidberg 2025-02-18T12:50:46Z 置信度 0.70
• Observability of radio reflections from exoplanet ionospheres with next generation radio telescopes
  crossref Bhavesh Jaiswal, Nirupam Roy 2025-06-26T11:45:01Z 置信度 0.70
• The mid-IR view of exoplanet atmospheres
  The Mid-InfraRed Instrument (MIRI) is a joined US/EU project looking at the longest wavelength Universe accessible by the James Webb Space Telescope (JWST). With MIRI we can look at the thermal radiation from stars and planets. This unique wavelength range pro…
  crossref Michiel Min 2026-02-02T11:49:23Z 置信度 0.70
• Highlights from Exoplanet Observations by the James Webb Space Telescope
  crossref Néstor Espinoza, Marshall Perrin 2026-02-04T02:02:43Z 置信度 0.70
• Exoplanet Atmospheres at High Spectral Resolution
  High-resolution spectroscopy (HRS) has grown into one of the main techniques for characterizing the atmospheres of extrasolar planets. High spectral resolving power allows for the efficient removal of telluric and host-star contamination. Combined with the lar…
  crossref Ignas A.G. Snellen 2025-05-14T18:40:49Z 置信度 0.70
• Exoplanet characterization across the mass-radius space using machine learning
  Characterizing the internal composition of exoplanets is an essential part in understanding the diversity of observed exoplanets and the processes that govern their formation and evolution. However, the interior of an exoplanet is inaccessible to observations,…
  crossref Philipp Baumeister, Johannes Bahrenberg, Nicola Tosi, Aleeda Charly 2025-03-15T03:19:02Z 置信度 0.70
• Exploring origin of life chemistry and exoplanet biosignatures with GCMs
  Studies of exoplanet habitability involving GCMs typically consider the potential for long-lived surface liquid water&amp;#8212;or, in other words, climates that Earth-life may find survivable. However, the presence of life and remotely detectable biosignature…
  crossref Stephanie Olson, Jonathan Jernigan, Emilie Lafleche, Haleigh Brown 2024-03-09T00:35:18Z 置信度 0.70
• MIRI-LRS Spectrum of a Cold Exoplanet around a White Dwarf !
  The study of the atmosphere of exoplanets orbiting white dwarfs is a largely unexplored field. With WD 0806-661 b, we present the first deep dive into the atmospheric physics and chemistry of a cold exoplanet around a white dwarf. We observed WD 0806-661 b usi…
  crossref Maël Voyer, Quentin Changeat, Pierre-Olivier Lagage 2025-07-09T15:12:38Z 置信度 0.70
• Signal Analysis of Stellar Pulsations: The Transiting Exoplanet Survey Satellite Observations of Eclipsing Binary V477 Cyg
  The Transiting Exoplanet Survey Satellite (TESS; Ricker et al., 2015) has produced extremely accurate observations of eclipsing binary systems that contain pulsating components, particularly δ-Scuti pulsators. These binaries fall into two basic types, detached…
  crossref Dave H Hinzel 2025-05-21T15:24:54Z 置信度 0.70
• Impact of Exoplanet Science on Society: Professional Contributions, Citizen Science, and Public Perception
  crossref Hans-Jörg Deeg 2025-07-23T03:58:25Z 置信度 0.70
• The role of magnetic coupling in exoplanet atmospheres: insights from star-planet magnetic interactions
  Since the discovery in 1995 of the first exoplanet orbiting a solar-type star, more than 5,500 exoplanets have been identified, revealing a remarkable diversity of exoplanetary systems. While many of their physical parameters are now well understood, the chara…
  crossref Clémence Gourvès, Antoine Strugarek 2025-03-14T17:20:51Z 置信度 0.70
• Exoplanet and Binary Star Light Curve Demonstration
  crossref Adam C. Lark, Bradley Moser 2025-02-28T15:32:29Z 置信度 0.70
• Effects of Ocean Salinity and Planetary Obliquity on Exoplanet Climate and Complex Habitability
  crossref Kyle Batra, Stephanie Olson 2025-10-24T12:31:10Z 置信度 0.70
• Exoplanet observations and TTV, transit timing variation interesting cases
  IntroductionA group of amateur astronomers from the Sabadell Astronomical Society is using small professional telescopes to obtain exoplanets transits photometry for the ExoClock project and ARIEL mission.Through this collaboration, we have faced cases like Co…
  crossref Florence Libotte, Mercedes Correa, Antelm Ginard, Gemma Domènech 等 2025-07-09T15:12:38Z 置信度 0.70
• TRAPPIST-1 in High Resolution: Constraining Exoplanet Atmospheres Amid Systematics
  Introduction &amp; Goals Studying terrestrial planets orbiting M dwarfs is our best opportunity to identify potentially habitable worlds and search for biosignatures beyond our solar system. The TRAPPIST-1 system, hosting seven rocky, Earth-sized, transiting e…
  crossref Mathis Bouffard, René Doyon, Nicolas Cowan, Vigneshwaran Krishnamurthy 2025-07-09T15:45:11Z 置信度 0.70
• The space weather around the exoplanet GJ 436 b
  crossref A. A. Vidotto, V. Bourrier, R. Fares, S. Bellotti 等 2025-01-11T19:45:37Z 置信度 0.70
• Differentiating characteristics in exoplanet host stars
  With technological advancements now allowing for precise measurements of stars, surveys are discovering thousands of exoplanets—planets outside of our solar system. We now have data on not just the kinematics and stellar chemistry (a star’s chemical makeup and…
  crossref Daniel Adibi, Sarah Kane, Bhuvnesh Jain 2025-10-09T01:51:07Z 置信度 0.70
• Machine Learning for Exoplanet Discovery: Validating Tess Candidates and Identifying Planets in the Habitable Zone
  crossref Sarah Huang, Chen Jiang 2025-05-20T10:36:59Z 置信度 0.70
• Exoplanet Research in the Era of the Extremely Large Telescope (ELT)
  crossref Florian Rodler, Robert J. De Rosa 2025-09-05T12:36:30Z 置信度 0.70
• On the Ordering of Exoplanet Systems
  Abstract We present a comprehensive analysis of planetary radius ordering within multiplanet systems, namely their ordinal position with respect to their size in a given system, utilizing data from the NASA Exoplanet Archive. In addition, we consider not only …
  crossref Michael Lozovsky, Hagai B. Perets 2025-09-15T12:39:38Z 置信度 0.70
• Host Stars and their Effects on Exoplanet Atmospheres
  crossref Jeffrey Linsky 2025-01-29T10:09:26Z 置信度 0.70
• Detection Biases and Methodological Impacts in Exoplanet Discovery
  crossref Shaan Mirchandani, Vinay Vishwakarma 2025-09-25T17:52:28Z 置信度 0.70
• Constraining The Parameters of an Earth-Sized Exoplanet Orbiting an M3 Star
  Context. The population of rocky exoplanets is abundant, and cool stars such as M dwarfs provide a uniqueopportunity to detect these objects, which could have implications for the study of astrobiology. Both theoretical modelsand observations have shown that t…
  crossref Francis Zong Lang, Brice-Olivier Demory 2025-07-09T15:12:38Z 置信度 0.70
• Effect of ocean tidal mixing on exoplanet climates and habitability
  Due to their abundance and their observational advantages, M dwarfs offer the best chance of finding habitable planets through sheer numbers. Therefore, in the race to detect signs of life beyond the Solar System, rocky M-dwarf planets offer exciting prospects…
  crossref Maria Di Paolo, David Stevens, Manoj Joshi, Rob Hall 2024-03-09T00:35:18Z 置信度 0.70
• Exoplanet discovery with variational quantum circuits
  Abstract This manuscript addresses the automatic identification of exoplanets with the data from the Kepler mission using variational quantum circuits (VQC) implemented with the Qiskit library. The system accuracy was assessed across various configurations, in…
  crossref Alberto Regadío 2025-01-24T03:13:10Z 置信度 0.70
• Space Astrometry Missions for Exoplanet Science: Gaia and the Legacy of Hipparcos
  crossref Alessandro Sozzetti, Jos de Bruijne 2025-12-31T03:27:17Z 置信度 0.70
• Born Dry or Born Wet? A Palette of Water Growth Histories in TRAPPIST-1 Analogs and Compact Planetary Systems
  Abstract It is still unclear whether exoplanets in compact multiplanet systems such as TRAPPIST-1 are able to accrete large quantities of volatiles, grow to sufficient mass, and maintain robust atmospheres and hydrospheres. Previous estimates of water content …
  crossref Howard Chen, Matthew S. Clement, Le “Chris” Wang, Jesse T. Gu 2025-09-17T09:38:31Z 置信度 0.70
• Evaluating the Effect of Exomoons on Planetary Axial Tilt Stability and Exoplanet Habitability
  crossref Daksh Challa 2026-05-26T19:40:24Z 置信度 0.70
• Multi-method extraction of quasi-periodic exoplanet signals from noisy data in transit surveys
  The detections of exoplanets rely primarily on space-based transit surveys, such as Kepler and TESS and the coming PLATO. The detectability of an exoplanet is dominated by its Signal-to-Noise Ratio (SNR) in the lightcurve. Traditional detection approaches expl…
  crossref Yannick Eyholzer, Adrien Leleu, Slava Voloshynovskiy 2025-07-09T15:12:38Z 置信度 0.70
• Sonification of Exoplanet Transit Light Curves from the Kepler Mission
  There is a plethora of publicly accessible data on the light curves of exoplanet transits that are more often represented using visual graphs. This project aims to make the data more accessible by sonifying the light curve data, presenting it through audio mea…
  crossref Emily Liao 2026-01-05T12:40:57Z 置信度 0.70
• Ages for Exoplanet Host Stars
  crossref Jørgen Christensen-Dalsgaard, Víctor Aguirre Børsen-Koch 2025-03-21T09:57:42Z 置信度 0.70
• Potential physical foundations of exoplanet habitability
  The identification of biomarkers is one of the most intriguing challenges in modern astrophysics. Interest in this topic existed even before the discovery of exoplanets; however, the confirmation of worlds beyond our solar system has moved the discussion of bi…
  crossref Marina Rumenskikh 2026-01-26T17:31:58Z 置信度 0.70
• Exoplanet transits through the exoclock project in support of the Ariel space mission
  Any follow-up observation of the transit events, either with photometry, low or high-resolution spectroscopy, or even with polarimetry, relies on a reasonably accurate knowledge of the timing of the transit. Most observations need a certain amount of out-of-tr…
  crossref Gemma Domènech Rams, Anastasia Kokori, Angelos Tsiaras 2025-07-09T15:45:11Z 置信度 0.70
• Potassium Bromide Glass: Simulating Exoplanet Settings for Infrared Spectroscopy
  Abstract Potassium bromide (KBr) glasses are widely used in infrared spectroscopy for their optical transparency and ability to produce high-fidelity molecular spectra. They are used in astronomical studies to characterize molecular vibrations; however, their …
  crossref Paul Shapshak, Jean Schneider 2025-05-14T17:59:27Z 置信度 0.70
• Exoplanet atmospheric retrievals through different JWST/NIRISS data reduction pipelines
  Since the James Webb Space Telescope (JWST) became available in 2022, its observations of exoplanet transit spectra have revolutionized the field of exoplanet science. Its observations have enabled significant new discoveries, in particular, contributing to th…
  crossref Rafael Rianço-Silva, Giovanna Tinetti, Pedro Machado, Angelos Tsiaras 等 2025-07-09T15:12:38Z 置信度 0.70
• Rocky Planets as Heat Engines.
  europepmc 2026 置信度 0.80
• Wavelength Requirements for Life Detection via Reflected Light Spectroscopy of Rocky Exoplanets.
  europepmc 2026 置信度 0.80
• This glowing speck is a freezing exoplanet six times the size of Jupiter.
  europepmc Davide Castelvecchi 2024 置信度 0.80