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The search for habitable conditions beyond Earth is a top priority in astrophysics. The discovery of habitable exoplanets beyond our solar system will require a suite of instruments providing long-term monitoring for detection (e.g. with space and ground-based…
datacite
Mahesh, N., Bowman, J. D., Burns, J. O., Bale, S. D. 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
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In this communication, we report on the results of the second phase of the Exoplanet Imaging Data Challenge started in 2019. This second phase focuses on the characterization of point sources (exoplanet signals) within multispectral high-contrast images from g…
datacite
Cantalloube, Faustine, Christiaens, Valentin, Cantero, Carles, Cioppa, Anthony 等
2024
置信度 0.66
Exoplanet imagingExoplanet characterisationHigh-contrast imagingAdaptive OpticsCoronagraphy
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NOTT (formerly Hi-5) is the L'-band (3.5-4.0 mu m) nulling interferometer of Asgard, an instrument suite in preparation for the VLTI visitor focus. The primary scientific objectives of NOTT include characterizing (i) young planetary systems near the snow line,…
datacite
Defrère, Denis, Laugier, Romain, Martinod, Marc-Antoine, Garreau, Germain 等
2024
置信度 0.66
Nulling interferometryVLTIexoplanetsexozodiacal diskshigh contrast imaging
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Our Unified Theory of Physics is supported by more than 70 high-fidelity experimental and observational datasets spanning cosmology, quantum mechanics, gravitational physics, particle interactions, biological systems, and mathematical structures. This includes…
datacite
Elliott, Andrew, Bulyaki, Jennifer
2025
置信度 0.66
Classical physics not elsewhere classifiedGalactic astronomyGeneral relativity and gravitational wavesSolar physicsStellar astronomy and planetary systems
-
Our Unified Theory of Physics is supported by more than 70 high-fidelity experimental and observational datasets spanning cosmology, quantum mechanics, gravitational physics, particle interactions, biological systems, and mathematical structures. This includes…
datacite
Elliott, Andrew, Bulyaki, Jennifer
2025
置信度 0.66
Classical physics not elsewhere classifiedGalactic astronomyGeneral relativity and gravitational wavesSolar physicsStellar astronomy and planetary systems
-
As an archetypal M-dwarf rocky exoplanet, GJ 1132 b has a varied history of atmospheric measurements. At 1.13 $\rm R_{\oplus}$, 1.66 $\rm M_{\oplus}$, and 580 K, it orbits a bright, slowly rotating M dwarf in a 1.6-day period, making it a prime target for char…
datacite
Bennett, Katherine A., MacDonald, Ryan J., Peacock, Sarah, Perez, Junellie 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
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M dwarfs are known to host magnetic fields, impacting exoplanet studies and playing a key role in stellar and planetary formation and evolution. Observations revealed the long-term evolution of the large-scale magnetic field reconstructed with Zeeman-Doppler i…
datacite
Cristofari, P. I., Donati, J. -F., Bellotti, S., Artigau, É. 等
2025
置信度 0.66
Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
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Limb-resolved transmission spectroscopy has the potential to transform our understanding of exoplanetary atmospheres. By separately measuring the transmission spectra of the evening and morning limbs, these atmospheric regions can be individually characterized…
datacite
Murphy, Matthew M., Beatty, Thomas G., Schlawin, Everett, Bell, Taylor J. 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
-
Directly imaged exoplanets in wide orbits challenge current gas giant formation theories. They need to form quickly and acquire enough material before the disk dissipates, which cannot be accommodated by in-situ formation by core accretion. We search for wide …
datacite
Liu, Pengyu, Kenworthy, Matthew A., Biller, Beth A., Wallace, Alex 等
2025
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
-
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 (TESS) lar…
datacite
Jayaraman, Rahul, Fausnaugh, Michael, Ricker, George, Vanderspek, Roland
2025
置信度 0.66
High Energy Astrophysical Phenomena (astro-ph.HE)FOS: Physical sciencesFOS: Physical sciences
-
Large-scale photometric surveys are revolutionizing astronomy by delivering unprecedented amounts of data. The rich data sets from missions such as the NASA Kepler and TESS satellites, and the upcoming ESA PLATO mission, are a treasure trove for stellar variab…
datacite
Audenaert, Jeroen
2025
置信度 0.66
Instrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciences
-
The high-resolution spectrograph ESPRESSO, installed at the ESO Very Large Telescope in Paranal, Chile, is one of the most precise high-resolution spectrographs currently in operation. In the field of exoplanets, it plays a key role in the detection of low-amp…
datacite
Ségransan, Damien, Dumusque, Xavier, Buchschacher, Nicolas , Unger, Nicolas 等
2025
置信度 0.66
Techniques:radial velocitiesTechniques:spectroscopicAstrophysics - Solar and Stellar AstrophysicsAstrophysics - Earth and Planetary AstrophysicsPlanets and satellites:detection
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I highlight that there is a substantial number of papers (at least 11 published since 2024) which all refer to a specific type of plot as an "Allan variance" plot, when in fact they seem to be plotting the standard deviation of the residuals versus bin size. T…
datacite
Kipping, David
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
-
This dataset provides an updated grid of chemical equilibrium (CEQ) abundances for use with petitRADTRANS (Mollière et al. 2019; Nasedkin et al. 2024), an open-source package for computing exoplanet and brown dwarf spectra and conducting atmospheric retrievals…
datacite
Zhang, Zhoujian, Mollière, Paul, Fortney, Jonathan, Marley, Mark
2025
置信度 0.66
-
This dataset provides an updated grid of chemical equilibrium (CEQ) abundances for use with petitRADTRANS (Mollière et al. 2019; Nasedkin et al. 2024), an open-source package for computing exoplanet and brown dwarf spectra and conducting atmospheric retrievals…
datacite
Zhang, Zhoujian, Mollière, Paul, Fortney, Jonathan, Marley, Mark
2025
置信度 0.66
-
Our Unified Theory of Physics is supported by more than 70 high-fidelity experimental and observational datasets spanning cosmology, quantum mechanics, gravitational physics, particle interactions, biological systems, and mathematical structures. This includes…
datacite
Elliott, Andrew, B, Jennifer
2025
置信度 0.66
-
Our Unified Theory of Physics is supported by more than 70 high-fidelity experimental and observational datasets spanning cosmology, quantum mechanics, gravitational physics, particle interactions, biological systems, and mathematical structures. This includes…
datacite
Elliott, Andrew, B, Jennifer
2025
置信度 0.66
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur
2025
置信度 0.66
astrophysicsexoplanetsVLTspectroscopypipeline
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur
2025
置信度 0.66
astrophysicsexoplanetsVLTspectroscopypipeline
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur
2024
置信度 0.66
astrophysicsexoplanetsVLTspectroscopypipeline
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur
2025
置信度 0.66
astrophysicsexoplanetsVLTspectroscopypipeline
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur, Martos, Steven
2025
置信度 0.66
astrophysicsexoplanetsVLTspectroscopypipeline
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur
2024
置信度 0.66
-
This repository contains hipipe, the reduction pipeline specifically developed to calibrate and extract data generated by the HiRISE visitor instrument at the VLT. HiRISE couples the exoplanet imager SPHERE with the high-resolution spectrograph CRIRES to enabl…
datacite
Costes, Jean, Denis, Allan, Vigan, Arthur
2024
置信度 0.66
-
The dataset used in this study consists of light curves collected by the Kepler telescope, totaling 5302 light curves, each with approximately 60,000 data points. The data were sourced from NASA's Exoplanet Archive, focusing on Kepler Objects of Interest (KOIs…
datacite
Dourado Macedo, Bruno Henrique, Zalewski, Willian
2024
置信度 0.66
AstronomyExoplanetsMachine LearningAstronomical Transit
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NASA Space Apps Challenge 2024 Global Nominee: Cape Canaveral, FL - Space Force Museum Award: Galactic Problem Solver Our team, Astreaus Rupertus, developed a web application for the NASA Space Apps Challenge 2024, enabling users to explore the night sky from …
datacite
Rosen, Jay, Muszynski, Paul, Lorne, Julieth, Dickens, A'sa 等
2024
置信度 0.66
-
NASA Space Apps Challenge 2024 Global Nominee: Cape Canaveral, FL - Space Force Museum Award: Galactic Problem Solver Our team, Astreaus Rupertus, developed a web application for the NASA Space Apps Challenge 2024, enabling users to explore the night sky from …
datacite
Rosen, Jay, Muszynski, Paul, Lorne, Julieth, Dickens, A'sa 等
2024
置信度 0.66
-
Supplementary material for the paper "Cold day-side winds shape large leading streams in evaporating exoplanet atmospheres" by Nail et al. (2024). We provide the results of the 3D hydrodynamic simulation with Athena++, with key files including the input file a…
datacite
Nail, Fabienne
2023
置信度 0.66
Astronomy
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Supplementary material for the paper "Cold day-side winds shape large leading streams in evaporating exoplanet atmospheres" by Nail et al. (2024). We provide the results of the 3D hydrodynamic simulation with Athena++, with key files including the input file a…
datacite
Nail, Fabienne
2023
置信度 0.66
Astronomy
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I present the preliminary results of a comprehensive variability census of the four legacy catalogs: BD, HD, SAO, and PPM. This dedicated survey project aims to identify bright A-F type variable stars using publicly available, high-precision space photometry f…
datacite
Zhou, Ai-Ying
2025
置信度 0.66
-
I present the preliminary results of a comprehensive variability census of the four legacy catalogs: BD (+CD+SD), HD, SAO, and PPM. This dedicated survey project aims to identify bright A-F type variable stars using high-precision space photometry from the Tra…
datacite
Zhou, Ai-Ying
2025
置信度 0.66
-
I present the preliminary results of a comprehensive variability census of the four legacy catalogs: BD (+CD+SD), HD, SAO, and PPM. This dedicated survey project aims to identify bright A-F type variable stars using high-precision space photometry from the Tra…
datacite
Zhou, Ai-Ying
2025
置信度 0.66
-
Deep learning algorithms are growing in popularity in the field of exoplanetary science due to their ability to model highly non-linear relations and solve interesting problems in a data-driven manner. Several works have attempted to perform fast retrieval of …
crossref
Kai Hou Yip, Quentin Changeat, Nikolaos Nikolaou, Mario Morvan 等
2020-10-08T09:23:31Z
置信度 0.70
-
Irradiated exoplanet atmospheres, with their hot day sides and eternally dark night sides, are intrinsically three-dimensional and highly dynamical. Vigourous atmospheric motions are expected to mix the atmosphere, reducing potential chemical variations with l…
crossref
Robin Baeyens, Leen Decin, Ludmila Carone, Olivia Venot 等
2021-07-21T08:42:53Z
置信度 0.70
-
Abstract: Recent changes in the climate have sparked interest in studying molecular-electron collisions in exoplanet atmospheres and, to a greater extent, in the interstellar medium. The competitive model of quantum mechanics can be used to describe Feshbach r…
crossref
Felix Iacob
2024-12-15T01:12:59Z
置信度 0.70
-
crossref
E. V. Bekesov
2024-10-25T13:02:03Z
置信度 0.70
-
crossref
Dakotah Tyler
2025-08-25T07:51:13Z
置信度 0.70
-
The paper presents a study of the exoplanet HD 189733 b based on the multicolor photometric observations obtained by the Hubble Space Telescope as well as on the equipment of the Caucasian Mountain Observatory. It is shown that with all other parameters fixed,…
crossref
E. Bekesov
2024-12-27T23:00:12Z
置信度 0.70
-
Abstract A key goal of exoplanet spectroscopy is to measure atmospheric properties, such as abundances of chemical species, in order to connect them to our understanding of atmospheric physics and planet formation. In this new era of high-quality JWST data, it…
crossref
Matthew C. Nixon, Luis Welbanks, Peter McGill, Eliza M.-R. Kempton
2024-05-02T06:53:13Z
置信度 0.70
-
crossref
Maneet Chatterjee, Anuvab Sen, Subhabrata Roy
2024-06-11T13:28:02Z
置信度 0.70
-
Abstract In this work, we aim to model ocean and atmospheric mass loss in exoplanets with varying orbital parameters to assess the impact of simulation assumptions on conclusions on planetary habitability. In particular, we examine how altering the time at whi…
crossref
Lailyn Borum, Juliette Becker
2024-12-03T13:44:14Z
置信度 0.70
-
The study of planetary habitability has gained widespread attention, and most existing studies focused on analyzing the habitability of a single planet based on a single feature, which makes it difficult to process a large amount of planetary data quickly. In …
crossref
Haoxuan Xu, Yong Zhang
2025-08-25T19:41:59Z
置信度 0.70
-
Based on the available data on the magnetic field of the star HAT-P-11 and its closest exoplanet HAT-P-11b, as well as information on the stellar wind in this system, we construct the HAT-P-11b magnetic field magnetospheric model. We show how the value and ori…
crossref
E. S. Belenkaya, I. I. Alexeev, V. V. Kalegaev
2024-11-13T08:01:23Z
置信度 0.70
-
Abstract The current orbital geometries of exoplanet systems offer a fossilized record of the systems’ dynamical histories. A particularly rich set of dynamical mechanisms is available to exoplanets residing in multistar systems, which may have their evolution…
crossref
Malena Rice, Konstantin Gerbig, Andrew Vanderburg
2024-02-22T09:50:46Z
置信度 0.70
-
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. Contact was taken in 2022 with MuSCAT2 team who uses t…
crossref
Florence Libotte, Gareb Enoc Fernández-Rodríguez
2024-07-03T11:09:04Z
置信度 0.70
-
crossref
Rahul Gupta, James F. Steiner
2025-03-31T23:20:17Z
置信度 0.70
-
Ground-based spectrophotometric observations of transiting exoplanet atmospheres conventionally rely on correcting for instrumental and telluric systematics in the light curves by using reference stars that are simultaneously observed. However, this approach o…
crossref
Vatsal Panwar, Jean-Michel Desert, Kamen Todorov, Jacob Bean 等
2021-07-22T08:25:29Z
置信度 0.70
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IntroductionThe detection and confirmation of long-period transiting planets present significant challenges due to the infrequency of their transits. Such planets are crucial for enhancing our understanding of exoplanet formation and evolutionary dynamics. TOI…
crossref
Patricio Reller
2024-07-03T11:09:04Z
置信度 0.70
-
The Twinkle Space Mission is a space-based observatory that has been conceived to measure the atmospheric composition of exoplanets, stars and solar system objects. Twinkle’s collaborative multi-year global survey programmes will de…
crossref
Billy Edwards, Marcell Tessenyi, Ian Stotesbury, Richard Archer 等
2021-07-21T22:36:20Z
置信度 0.70
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The next generation of space telescopes is expected to deliver transmission spectra of exoplanet atmospheres with precision down to 10 parts per million (ppm). Therefore, it is required to model the astrophysical signals with even greater precision in order no…
crossref
Giuseppe Morello, Tiziano Zingales, Marine Martin-Lagarde, Rene Gastaud 等
2020-10-08T10:25:38Z
置信度 0.70
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Abstract The exchange of molecules between a planet’s interior and exterior is a major component of planetary development and atmospheric formation. Recently, detailed observational studies of exoplanet atmospheres have become possible, enabling robust testing…
crossref
Eva Stafne, Juliette Becker
2024-07-05T14:52:17Z
置信度 0.70
-
Abstract The NASA Exoplanet Archive contains published data for various stellar and planetary parameters, based on the combined work of hundreds of research teams. For cases where a parameter has been estimated multiple times, the opportunity exists to compare…
crossref
Shruti Subramaniyan, Harsh Mehta, Mark R. Swain, Geoffrey Bryden 等
2024-03-13T03:40:05Z
置信度 0.70
-
crossref
C.A. Wolfe, T.D. Robinson
2024-08-02T10:29:55Z
置信度 0.70
-
crossref
Felipe Meza-Obando, Juan Luis Crespo-Mariño
2025-02-17T18:30:01Z
置信度 0.70
-
The work carried out an analysis and interpretation of light curves obtained with observing with the HST telescope the transit of the exoplanet HD 189733 b across the disk of the star. Observations were carried out in a wide range of wavelengths 5500–10500 Å, …
crossref
E. V. Bekesov
2024-12-25T17:15:25Z
置信度 0.70
-
crossref
A. García Muñoz, A. Asensio Ramos, A. Faure
2024-04-05T18:11:58Z
置信度 0.70
-
Abstract Aerosol opacity has emerged as a critical factor controlling transmission and emission spectra. We provide a simple guideline for the effects of aerosol morphology on opacity and residence time in the atmosphere, as it pertains to transit observations…
crossref
Sanaz Vahidinia, Sarah E. Moran, Mark S. Marley, Jeffrey N. Cuzzi
2024-08-30T16:08:46Z
置信度 0.70
-
Abstract Transmission spectroscopy is still the preferred characterization technique for exoplanet atmospheres, although it presents unique challenges that translate into characterization bottlenecks when robust mitigation strategies are missing. Stellar conta…
crossref
Benjamin V. Rackham, Julien de Wit
2024-07-19T08:47:07Z
置信度 0.70
-
Deep learning algorithms are growing in popularity in the field of exoplanetary science due to their ability to model highly non-linear relations and solve interesting problems in a data-driven manner. Several works have attempted to perform fast retrievals of…
crossref
Kai Hou Yip, Quentin Changeat, Nikolaos Nikolaou, Mario Morvan 等
2021-07-21T10:46:47Z
置信度 0.70
-
Absorption of stellar X-ray and extreme ultraviolet (EUV) radiation in the upper atmosphere of close-in exoplanets can give rise to hydrodynamic outflows, which may lead to the gradual shedding of their primordial light element envelopes. Excess absorption by …
crossref
Federico Biassoni, Andrea Caldiroli, Elena Gallo, Francesco Haardt 等
2023-12-13T14:55:40Z
置信度 0.70
-
crossref
I. S. Savanov
2025-03-14T12:12:47Z
置信度 0.70
-
Abstract The rising number of exoplanet discoveries and advances in machine learning (ML) techniques present new possibilities for exploring and understanding the characteristics of worlds beyond our solar system. This research examines the exoplanet dataset b…
crossref
M. Mousavi-Sadr, G. Gozaliasl, D. M. Jassur
2026-01-09T09:40:01Z
置信度 0.70
-
crossref
Sebastian Johannes Spicker, Alexander Küpper
2024-02-22T21:17:09Z
置信度 0.70
-
Abstract The presence of a planetary companion around its host star has been repeatedly linked with stellar properties, affecting the likelihood of substellar object formation and stability in the protoplanetary disc, thus presenting a key challenge in exoplan…
crossref
Miguel A Zammit, Josef Borg, Kristian Zarb Adami
2024-06-12T00:47:14Z
置信度 0.70
-
With the exploitation of resources and environmental pollution, the Earth has suffered countless damages. As a result, there are more and more environmental problems such as the greenhouse effect and desertification. People only have one home, one Earth, so if…
crossref
Helin Yang
2025-01-03T07:02:36Z
置信度 0.70
-
Abstract We propose a measure, the joint differential entropy of eigencolors, for determining the spatial complexity of exoplanets using only spatially unresolved light-curve data. The measure can be used to search for habitable planets, based on the premise o…
crossref
Gary Segal, David Parkinson, Stuart Bartlett
2024-02-16T09:42:57Z
置信度 0.70
-
Astronomers have identified over five thousand extrasolar planets since the discovery of the first solar-like star in 1995. These systems exhibit greater diversity than our solar system, providing insights into their formation and evolution. To understand thes…
crossref
Huanyu Ye
2024-04-28T05:41:03Z
置信度 0.70
-
crossref
Michael C LoPresto
2024-11-19T14:06:17Z
置信度 0.70
-
crossref
Zhuoxi Huo
2025-01-31T21:02:44Z
置信度 0.70
-
Abstract The Galileo spacecraft had distant encounters with Earth in 1990 and 1992. Limited Solid State Imager (SSI) data acquired during these encounters has been previously presented, but the majority of the data from these Earth flybys have not been present…
crossref
Ryder H. Strauss, Tyler D. Robinson, David E. Trilling, Ryan Cummings 等
2024-02-01T09:26:31Z
置信度 0.70
-
Exoplanets are celestial bodies outside our solar system, orbiting stars other than our sun. They come in various sizes, compositions, and distances from their host stars. Scientists detect exoplanets by observing the dimming of a star's light as a planet pass…
crossref
Preeti Kalra, Abhendra PratapSingh, Arushi Gupt, Kartik Gupta 等
2023-12-26T05:25:44Z
置信度 0.70
-
Within the Young Suns Exoplanet Survey (YSES) we are observing a homogeneous sample of 70 solar-mass members of the approximately 16 Myr-old Lower Centaurus-Crux subgroup of the Scorpius-Centaurus association to search for sub-stellar companions.High-contrast …
crossref
Matthew Kenworthy, Alexander Bohn, Christian Ginski, Maddalena Reggiani 等
2021-07-21T08:42:53Z
置信度 0.70
-
Abstract We present the progress of work to streamline and simplify the process of exoplanet observation by citizen scientists. International collaborations such as ExoClock and Exoplanet Watch enable citizen scientists to use small telescopes to carry out tra…
crossref
Oisín Creaner, Anna Preis, Cormac Ryan, Nika Gorchakova
2026-01-20T09:38:19Z
置信度 0.70
-
Abstract Salt clouds are predicted to be common on warm exoplanets, but their optical properties are uncertain. The Exoplanet Cloud Ensemble Scattering System (ExCESS), a new apparatus to measure the scattering intensity and degree of linear polarization for a…
crossref
Colin D. Hamill, Alexandria V. Johnson, Peter Gao
2024-08-27T11:14:22Z
置信度 0.70
-
Context. Interpreting the observations of exoplanet atmospheres to constrain physical and chemical properties is typically done using Bayesian retrieval techniques. Since these methods require many model computations, a compromise must be made between the mode…
crossref
F. Ardévol Martínez, M. Min, D. Huppenkothen, I. Kamp 等
2024-01-08T12:51:24Z
置信度 0.70
-
crossref
Kole Lutz
2025-01-31T21:02:44Z
置信度 0.70
-
Abstract Depending on the distance of the exoplanet from the central star and the properties of this star, different regimes of stellar wind flow around it arise. If the exoplanet is located at a distance up to the Alfvén radius, where the wind speed is equal …
crossref
E. S. Belenkaya
2024-07-04T11:02:33Z
置信度 0.70
-
ABSTRACT In this paper, we explore the detectability of polycyclic aromatic hydrocarbons (PAHs) under diverse planetary conditions, aiming to identify promising targets for future observations of planetary atmospheres. Our primary goal is to determine the mini…
crossref
Rosa Arenales-Lope, Karan Molaverdikhani, Dwaipayan Dubey, Barbara Ercolano 等
2024-11-27T02:10:46Z
置信度 0.70
-
crossref
Saima Khan, Md. Abidur Rahman Khan
2024-09-28T19:40:21Z
置信度 0.70
-
Transmission spectroscopy with the James Webb Space Telescope (JWST) is revealing growing chemical complexity in giant exoplanet atmospheres. Of particular interest is sulfur, which had essentially no observational constraints before JWST. Recent work has show…
datacite
Triantafillides, Anastasia, Beatty, Thomas G., Nixon, Matthew C., Bell, Taylor J. 等
2026
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
-
Recent astronomical observations, in particular from the Kepler and TESS missions and their related follow-ups, have revealed an abundance of exoplanets in the size range between Neptune (4 Earth radii) and Earth (1 Earth radii ), as well as a low occurrence r…
datacite
Zeng, Li, Werner, Stephanie C., Jacobsen, Stein B., Mamonova, Elena 等
2026
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
-
As the only known habitable (and inhabited) planet in the universe, Earth informs our search for life elsewhere. Future telescopes like the Habitable Worlds Observatory (HWO) will soon look for life on rocky worlds around Sun-like stars, so it is critical that…
datacite
Gilbert-Janizek, Samantha, Barnes, Rory K., Driscoll, Peter E., Wogan, Nicholas F. 等
2026
置信度 0.66
Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
-
We report on the goals, design, and ongoing development of the Netherlands EXoplanet Testbed (NEXT), a high-contrast imaging testbed under construction in Leiden. NEXT is designed to develop and validate technologies and algorithms for extreme adaptive optics …
datacite
Landman, Rico, Haffert, Sebastiaan, Desdoigts, Louis, Mars, Matthijs 等
2026
置信度 0.66
Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciences
-
Small-scale dark matter (DM) structure encodes key information about the particle nature of DM and therefore provides a sensitive test of competing models. Yet, it remains hidden from electromagnetic surveys and is instead inferred through its gravitational ef…
datacite
Daniel, Matthias, Xue, Xiao, Pardo, Kris, Sagunski, Laura
2026
置信度 0.66
Cosmology and Nongalactic Astrophysics (astro-ph.CO)General Relativity and Quantum Cosmology (gr-qc)FOS: Physical sciences
-
datacite
Morello, Giuseppe
2026
置信度 0.66
ExoplanetologySpectroscopyStellar astronomy
-
datacite
Morello, Giuseppe
2026
置信度 0.66
ExoplanetologySpectroscopyStellar astronomy
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Debris disks are characterized by the dusty, gas-depleted environment bearing non-primordial dust grains which are constantly generated by continuous collisions between planetesimals. High-contrast imaging in the near-infrared allows to measure the intensity d…
datacite
Bhowmik, Trisha
2020
置信度 0.66
debris diskshigh-contrast imagingSPHEREexoplanet
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Debris disks are characterized by the dusty, gas-depleted environment bearing non-primordial dust grains which are constantly generated by continuous collisions between planetesimals. High-contrast imaging in the near-infrared allows to measure the intensity d…
datacite
Bhowmik, Trisha
2020
置信度 0.66
debris diskshigh-contrast imagingSPHEREexoplanet
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A periodic transit-like signal is detected in the Kepler light curve of KIC 7259722. Transit Least Squares (TLS) analysis reveals a stable period of \(P \approx 9.6~\mathrm{days}\) across multiple quarters. Transit modeling with a Mandel--Agol model yields \(R…
datacite
NuanDong, Xia
2026
置信度 0.66
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Initial release of code accompanying the paper "Supervised Machine Learning Methods with Uncertainty Quantification for Exoplanet Atmospheric Retrievals from Transmission Spectroscopy" by Forestano et al.
datacite
Roy T. Forestano, Konstantin T. Matchev, Katia Matcheva, Eyup B. Unlu
2026
置信度 0.66
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Initial release of code accompanying the paper "Supervised Machine Learning Methods with Uncertainty Quantification for Exoplanet Atmospheric Retrievals from Transmission Spectroscopy" by Forestano et al.
datacite
Roy T. Forestano, Konstantin T. Matchev, Katia Matcheva, Eyup B. Unlu
2026
置信度 0.66
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Brown dwarfs and young giant exoplanet are subject to variability and colour changes as the L/T transition. Clouds are expected to be the main driver of the L/T. Using a three-dimensional Global Climate Model, we show that clouds play a major role in shaping t…
datacite
Maio, Francesco, Bonnefoy, M., Chauvin, G., Lacour, S. 等
2026
置信度 0.66
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Brown dwarfs and young giant exoplanet are subject to variability and colour changes as the L/T transition. Clouds are expected to be the main driver of the L/T. Using a three-dimensional Global Climate Model, we show that clouds play a major role in shaping t…
datacite
Maio, Francesco, Bonnefoy, M., Chauvin, G., Lacour, S. 等
2026
置信度 0.66
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Stellar rotation offers a powerful probe of stellar evolution, age, and magnetic activity in low-mass stars. As stars age, magnetized winds extract angular momentum, causing their rotation rates to slow—a process that forms the basis of gyrochronology. This te…
datacite
Boyle, Andrew
2026
置信度 0.66
stellar rotationopen clusters
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Stellar rotation offers a powerful probe of stellar evolution, age, and magnetic activity in low-mass stars. As stars age, magnetized winds extract angular momentum, causing their rotation rates to slow—a process that forms the basis of gyrochronology. This te…
datacite
Boyle, Andrew
2026
置信度 0.66
stellar rotationopen clusters
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Rocky exoplanets that orbit very near their Roche limits may assume non-spherical equilibrium shapes. These unusual planet geometries are dependent upon the planet composition, so accurately predicting the tidal distortion of a particular exoplanet requires de…
datacite
Price, Ellen M., Rogers, Leslie, Vanderburg, Andrew, Dang, Lisa 等
2026
置信度 0.66
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Rocky exoplanets that orbit very near their Roche limits may assume non-spherical equilibrium shapes. These unusual planet geometries are dependent upon the planet composition, so accurately predicting the tidal distortion of a particular exoplanet requires de…
datacite
Price, Ellen M., Rogers, Leslie, Vanderburg, Andrew, Dang, Lisa 等
2026
置信度 0.66
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The Universal Particle Law: A Cosmic Architecture for Life Imagine a single, fundamental clock—a heartbeat lasting exactly one second—that echoes from the inside of a proton to the edge of the galaxy. That is the central claim of the Universal Particle Law (UP…
datacite
Beardsley, Ian
2026
置信度 0.66
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The atmospheric composition of rocky exoplanets offers an important tool for constraining the properties of the interior of this type of planet, beyond what is possible from measurements of their mass and radius alone. However, the interpretation of these obse…
datacite
Steinmeyer, Marie-Luise, Noack, Lena, Baumeister, Philipp, Hamano, Keiko 等
2026
置信度 0.66
ExoplanetsExoplanet atmospheresExoplanet atmospheric evolutionExoplanet observationExtrasolar rocky planets
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Sub-Neptune-sized exoplanets are the most common class discovered by transit surveys, yet their detailed exploration has just begun. Their demographics have inspired models of planetary formation and evolution, though the sample is naturally biased toward the …
datacite
Morello, G., Pelaez-Torres, A., Pozuelos, F. J., Dévora-Pajares, M. 等
2026
置信度 0.66
methods: observationaltechniques: high angular resolutiontechniques: photometrictechniques: spectroscopicplanets and satellites: detection