地外科学 · 全部实体（第 72 / 100 页）

本页收录第 7101–7200 条，共 10000 条 · 返回 地外科学 首页

• Exoplanet Atmospheres with HST: An open science framework for the characterisation of exoplanets
  The field of exoplanets is one of the most rapidly growing, with more than 4000 new planets discovered over the past 25 years. In the last decade, we have entered in a new era, the era of exoplanet characterisation, where studies are also focused on understand…
  crossref Angelos Tsiaras 2020-10-08T11:08:36Z 置信度 0.70
• Advancements in AI Technology and Their Impact on Exoplanet Discovery
  The continuous goal of discovering extraterrestrial life has driven scientific interest in exoplanets—celestial bodies orbiting stars outside our solar system. Traditional methods of exoplanet detection, reliant on manual analysis and prone to human error, pre…
  crossref Joyce Liu 2024-09-11T12:16:37Z 置信度 0.70
• Interpretation of the Balmer-alpha line absorption in the exoplanet WASP-69 b
  In this work, the absorption in the H$\alpha$ line of the exoplanet Wasp-69 b was simulated. A three-dimensional self-consistent multifluid magnetohydrodynamic (MHD) model of the atmosphere was used to calculate the characteristic distributions of density, vel…
  crossref Ilya Miroshnichenko, S. Sharipov, M. Rumenskikh, I. Shaikhislamov 2024-12-27T23:00:12Z 置信度 0.70
• Transit Photometry as an Exoplanet Discovery Method
  crossref Hans J. Deeg, Roi Alonso 2024-09-18T13:25:02Z 置信度 0.70
• Exoplanet Ephemeris Maintenance using Ground- and Space-based Telescopes
  Ariel will require precise knowledge of the transit timings for all of its targets. However, the precision we have for each target will degrade significantly over the 8 years until launch, in some cases to the point where the error exceeds the duration of the …
  crossref Hamish Caines, Marco Rocchetto, Giorgio Savini 2020-10-08T12:24:24Z 置信度 0.70
• Exotic red flares on stars as the observational manifestation of the asteroids in exoplanet systems
  The published data on exotic red flares (RFs) obtained using optical/IR photometry was for the first time gathered and discussed in this paper. To date, the RFs have been observed: (a) in IR space missions (1–2 yr long IR brightening observed using WISE/NEOWIS…
  crossref M. Ibrahimov 2024-12-27T23:00:12Z 置信度 0.70
• 7 Exoplanet Mineralogy
  crossref Keith D. Putirka 2024-08-22T14:44:53Z 置信度 0.70
• Planetary and Solar Electromagnetic Lensing (SEL), Geometry, Astrophysics for Exoplanet Imaging
  crossref Kolemann Lutz 2024-09-20T08:30:37Z 置信度 0.70
• Exoplanet Populations and Their Dependence on Host Star Properties
  crossref Gijs D. Mulders 2024-09-18T13:13:42Z 置信度 0.70
• Impact of photochemical hazes on the thermal structure of exoplanet atmospheres
  Transit observations reveal that a significant population of the detected exoplanets has hazy atmospheres (Sing et al. 2016). Although the relative contribution of clouds and photochemical aerosols is not yet fully clarified, the impact of haze particles on th…
  crossref Panayotis Lavvas, Anthony Arfaux 2020-10-08T10:25:38Z 置信度 0.70
• Fusion Propulsion Constraints Required by Robust Exoplanet Exploration
  crossref Gerald Jackson 2024-09-10T23:20:08Z 置信度 0.70
• 1st November 1995 – The FIRST NORMAL Exoplanet
  crossref C.R. Kitchin 2024-11-04T19:24:54Z 置信度 0.70
• Rigel Exoplanet Geologist
  crossref Philip Horzempa 2023-09-01T21:14:52Z 置信度 0.70
• Importance of citizen Czech Astronomical Society for variable star and exoplanet research
  Variable Star and Exoplanet Section of Czech Astronomical Society (VSES CAS) is a citizen astronomy organization with almost century tradition in basic and advanced research on variable stars in Czech Republic. Members are formed both amateur and professional …
  crossref Katerina Honkova, Filip Walter 2020-10-08T12:24:24Z 置信度 0.70
• Icy exoplanet found to be potentially habitable
  Astronomers have discovered that the temperate exoplanet LHS 1140 b may have an atmosphere, could be covered in ice, and may even have an ocean of liquid water.
  crossref Abigail Williams 2024-10-11T14:38:07Z 置信度 0.70
• Exoplanet Imaging along a Time-Varying Focal Line Using Tethered Spacecraft
  crossref Karel Hernandez Bandrich, Steven Tragesser 2024-01-29T22:03:51Z 置信度 0.70
• No Evidence for a Metallicity-dependent Enhancement of Distant Giant Companions to Close-in Small Planets in the California Legacy Survey
  Abstract Understanding the relationship between close-in small (CS) planets and distant giants (DGs) is central to understanding the formation of planetary systems like our own. Most studies of this connection have found evidence for a positive correlation, th…
  crossref Judah Van Zandt, Erik A. Petigura 2024-11-18T16:28:36Z 置信度 0.70
• An Overview of Exoplanet Biosignatures
  crossref Edward W. Schwieterman, Michaela Leung 2024-07-01T01:36:39Z 置信度 0.70
• Study of photochemical hazes in exoplanet atmospheres: disequilibrium chemistry effects and haze feedback
  Photochemical hazes are expected to be present in exoplanet atmospheres with quantities spanning a large range of values, from quasi-non-detectable traces in clear atmospheres, to large amounts dramatically modifying their environment. Our purpose is to determ…
  crossref Anthony Arfaux, Panayotis Lavvas 2021-07-21T11:18:15Z 置信度 0.70
• Preparing for the future of direct imaging exoplanets through combining other exoplanet detection techniques
  Very little is known about giant planets and brown dwarfs at an orbital separation great than 5 AU. And yet, these are important puzzle pieces needed for constraining the uncertainties that exist in giant planet formation and evolutionary models that are plagu…
  crossref Emily Rickman 2021-07-21T17:59:21Z 置信度 0.70
• Extrasolar worlds: a review of the current state of exoplanet research in Russia and the world
  The history of the discovery and the main results of the study of extrasolar planets (exoplanets) in the world and in Russia are presented. The main emphasis is on describing the methods and results of the most successful space and ground-based research projec…
  crossref G. Valyavin, D. Gadelshin 2024-12-27T23:00:12Z 置信度 0.70
• Exoplanet TIC 468574941
  crossref Chris Woodhouse 2024-01-03T15:38:51Z 置信度 0.70
• ARTIFEX: Exoplanet atmosphere visualisation
  crossref Pieter Steyaert, Marrick Braam, Thorsten Balduin, Oriel Marshall 等 2024-06-24T23:20:35Z 置信度 0.70
• Exoplanet yield predictions for the future LIFE mission
  Context: Warm, terrestrial exoplanets represent a key component in the exoplanet population when exploring the diversity of planets and investigating the properties of potentially habitable worlds [1]. Subsequently, the LIFE Collaboration is presenting a missi…
  crossref Jens Kammerer, Felix Dannert, Sascha Quanz, Daniel Angerhausen 2021-07-21T14:54:19Z 置信度 0.70
• Exploring Factors That Influence Exoplanet Habitability
  The objective of this research is to determine which conditions influence the habitability of exoplanets. A better understanding of these attributes can help determine if life exists beyond our solar system. It also helps answer the question of whether or not …
  crossref Ian Kozloski 2025-02-14T21:15:28Z 置信度 0.70
• Exoplanet Magnetic Fields
  crossref David A. Brain, Melodie M. Kao, Joseph G. O’Rourke 2024-07-01T01:35:50Z 置信度 0.70
• Promising exoplanet may not be habitable ocean world after all
  crossref Jonathan O'Callaghan 2024-03-08T19:04:33Z 置信度 0.70
• ExoClock project: a pro-am collaboration to monitor the exoplanet ephemerides for the Ariel space mission
  ExoClock (exoclock.space) is a project aiming to monitor transiting exoplanets through regular observations using small and medium scale telescopes. The project is part of the ephemerides working group of ESA's Ariel space mission and the main scope is to maxi…
  crossref Anastasia Kokori 2021-07-22T07:54:38Z 置信度 0.70
• Monte Carlo transmission line modelling of multilayer optical coatings for performance sensitivity of exoplanet spectroscopy
  Multilayer optical coatings are widely used on the surface of optical components to enhance the transmittance of light in certain spectral regions while reducing it in other regions. Discrepancies between the measured and predicted spectral performance of opti…
  crossref Vinooja Thurairethinam, Giorgio Savini 2021-07-22T08:59:58Z 置信度 0.70
• Helium in Exoplanet Exospheres: Orbital and Stellar Influences
  Abstract Searches for helium in the exospheres of exoplanets via the metastable near-infrared triplet have yielded 17 detections and 40 nondetections. We performed a comprehensive reanalysis of published studies to investigate the influence of stellar X-ray an…
  crossref Vigneshwaran Krishnamurthy, Nicolas B. Cowan 2024-06-25T02:16:08Z 置信度 0.70
• The Kepler Mission
  crossref Michael C LoPresto 2024-11-19T14:06:17Z 置信度 0.70
• JWST reveals interior structure of puffy exoplanet WASP-107 b
  Two teams of astronomers have discovered that the exoplanet WASP-107 b is much hotter than previously thought.
  crossref Tami Freeman 2024-07-09T12:11:54Z 置信度 0.70
• Twinkle: Update on the international, collaborative exoplanet survey
  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 2021-07-21T22:05:36Z 置信度 0.70
• Exoplanet/Exomoon Astronomer
  crossref Robert H. Chen, Chelsea Chen 2024-08-14T23:48:50Z 置信度 0.70
• Exoplanet Geology: What Can We Learn from Current and Future Observations?
  OVERVIEW Nearly 30 years after the discovery of the first exoplanet around a main sequence star, thousands of planets have now been confirmed. These discoveries have completely revolutionized our understanding of planetary systems, revealing types of planets t…
  crossref Bradford J. Foley 2024-07-01T05:37:22Z 置信度 0.70
• Exoplanet Mass Measurement Program (NASA)
  crossref 2024-07-29T06:14:01Z 置信度 0.70
• The EXoplanet Climate Infrared TElescope - EXCITE
  EXCITE is a balloon-borne near-infrared spectrometer designed to observe from 0.6 to 4 micron and to perform phase-resolved spectroscopy of hot Jupiters during a Long-Duration Balloon (LDB) flight from Antarctica in 2024.  These spectral measurements …
  crossref Enzo Pascale, Nat Butler, Peter Nagler, Calvin B. Netterfield 等 2021-07-21T10:46:47Z 置信度 0.70
• ESPRESSO on VLT: An Instrument for Exoplanet Research
  crossref Jonay I. González Hernández, Francesco Pepe, Paolo Molaro, Nuno Santos 2024-09-24T15:03:00Z 置信度 0.70
• Signature of Vertical Mixing in Hydrogen-dominated Exoplanet Atmospheres
  Abstract Vertical mixing is a crucial disequilibrium process in exoplanet atmospheres, significantly impacting chemical abundance and observed spectra. While current state-of-the-art observations have detected its signatures, the effect of vertical mixing on a…
  crossref Vikas Soni, Kinsuk Acharyya 2024-12-02T10:05:57Z 置信度 0.70
• Analysis and Comparison of Three Exoplanet Searching Schemes
  In retrospect, from ancient times to the present, human beings have never stopped exploring the secrets of the universe. With this in mind, exploring the universe means the progress of human science and technology, promoting the exchange and integration of hum…
  crossref Chang Yang 2024-06-13T02:02:21Z 置信度 0.70
• The Transiting Exoplanet HAT-P-37b from the Magnificent Parallel
  crossref Héctor Noriega Mendoza 2025-03-28T07:20:21Z 置信度 0.70
• CloudFlex: A Flexible Parametric Model for the Small-scale Structure of the Circumgalactic Medium
  Abstract We present CloudFlex , an open-source tool for predicting absorption-line signatures of cool gas in galaxy halos with small-scale structure. Motivated by analyses of ∼10 4 K material in hydrodynamical simulations of turbulent, multiphase media, we mod…
  crossref Cameron B. Hummels, Kate H. R. Rubin, Evan E. Schneider, Drummond B. Fielding 2024-09-03T15:50:53Z 置信度 0.70
• Identifying Exoplanet Candidates Using WaveCeptionNet
  Abstract In this study, we propose a wavelet-transform-based light curve representation method and a CNN model based on Inception-v3 for fast classification of light curves, enabling the quick discovery of potentially interesting targets from massive data. Exp…
  crossref Huiping Liao, Guangyue Ren, Xinghao Chen, Yuxiang Li 等 2024-03-27T10:33:39Z 置信度 0.70
• Retraction: “Exoplanet Harmony: Confirming Kepler's Third Law with Kepler and TESS Discoveries” (2024, RNAAS, 8, 215)
  crossref 2024-10-15T12:44:02Z 置信度 0.70
• Transiting Exoplanet Atmospheres in the Era of JWST
  crossref Eliza M.-R. Kempton, Heather A. Knutson 2024-07-01T01:36:01Z 置信度 0.70
• 13 An Overview of Exoplanet Biosignatures
  crossref Edward W. Schwieterman, Michaela Leung 2024-08-22T14:44:53Z 置信度 0.70
• Beyond the Kepler Mission
  crossref Michael C LoPresto 2024-11-19T14:06:17Z 置信度 0.70
• Mineral and chemical detail of rocky exoplanet surfaces could be detectable
  crossref 2024-11-14T13:18:13Z 置信度 0.70
• Automated Chemical Reaction Network Generation and Its Application to Exoplanet Atmospheres
  Abstract With the advent of JWST and the spectroscopic characterization of exoplanet atmospheres in unprecedented detail, there is a demand for more complete pictures of chemical and photochemical reactions and their impacts on atmospheric composition. Traditi…
  crossref Jeehyun Yang, Renyu Hu 2024-05-07T15:33:51Z 置信度 0.70
• Observing Exoplanet Biosignatures outside the Conservative Habitable Zone
  Abstract Liquid water can exist on exoplanets in a circumstellar region significantly wider than the Conservative Habitable Zone (CHZ). In particular, tidally locked planets orbiting closer inwards than the inner CHZ border could have liquid water on their nig…
  crossref Amri Wandel 2026-01-09T09:40:01Z 置信度 0.70
• Estimating Exoplanet Mass using Machine Learning on Incomplete Datasets
  The exoplanet archive is an incredible resource of information on the properties of discovered extrasolar planets, but statistical analysis has been limited by the number of missing values. One of the most informative bulk properties is planet mass, which is p…
  crossref Florian Lalande, Elizabeth Tasker, Kenji Doya 2024-10-10T08:00:44Z 置信度 0.70
• How to identify exoplanet surfaces using atmospheric trace species in hydrogen-dominated atmospheres
  Sub-Neptunes (Rp~1.25-4 REarth) remain the most commonly detected exoplanets to date. However, it remains difficult for observations to tell whether these intermediate-sized exoplanets have surfaces and where their surfaces are located. Here we propose that th…
  crossref Xinting Yu, Julianne Moses, Jonathan Fortney, Xi Zhang 2021-07-21T11:48:26Z 置信度 0.70
• Observations of Extremely Metal-poor O Stars: Weak Winds and Constraints for Evolution Models
  Abstract Metal-poor massive stars drive the evolution of low-mass galaxies, both locally and at high redshift. However, quantifying the feedback they impart to their local surroundings remains uncertain because models of stellar evolution, mass loss, and ioniz…
  crossref O. Grace Telford, John Chisholm, Andreas A. C. Sander, Varsha Ramachandran 等 2024-10-07T08:57:38Z 置信度 0.70
• 11 Exoplanet Magnetic Fields
  crossref David A. Brain, Melodie M. Kao, Joseph G. O’Rourke 2024-08-22T14:44:53Z 置信度 0.70
• AstroFusion: A GAN-Augmented Approach for Exoplanet Detection
  crossref Aakash Suresh, Lakshmi C, Gopirajan PV, K Dhanasekaran 2024-10-08T17:35:04Z 置信度 0.70
• How does the radiative environment affect the chemistry of exoplanet atmospheres?
  The high-energy radiation environment of exoplanets can greatly affect their atmospheric chemistry through photo-chemical reactions and ionisation of the upper parts of the atmospheres. In order to analyse the chemistry of exoplanet atmospheres, it is therefor…
  crossref Nanna Bach-Møller, Christiane Helling, Martin Bødker Enghoff, Uffe Gråe Jørgensen 2024-03-11T11:16:49Z 置信度 0.70
• Determining the mass of RV exoplanet candidates using Gaia
  Mass is one of the most important parameters for determining the true nature of an astronomical object. Yet, many published exoplanets in on-line database, such as exoplanet.eu or the NASA exoplanet archive, still lacks a measurement of their true mass, in par…
  crossref Flavien Kiefer, Guillaume Hébrard, Alain Lecavelier, Eder Martoli 等 2020-10-08T15:50:02Z 置信度 0.70
• Extrasolar Geochemistry: Predicting Rocky Exoplanet Mantle Mineralogy Using Stellar Abundance Data
  crossref Rob Spaargaren, Stephen Mojzsis, Haiyang Wang, Tim Lichtenberg 等 2025-03-17T14:59:06Z 置信度 0.70
• Earth-sized Planets in Habitable Zones
  crossref Michael C LoPresto 2024-11-19T14:06:17Z 置信度 0.70
• Contamination in Exoplanet Transit Spectroscopy with a Changing Stellar Surface
  Abstract Inhomogeneities in the stellar surface can lead to differences between the actual and assumed stellar spectrum below the planet’s transit chord, causing the inferred planet transmission spectrum to have a contamination component. In this study, we pre…
  crossref Yike Qiao, Sharon X. Wang, Zitao Lin 2024-12-23T17:11:41Z 置信度 0.70
• Correction to: Retrieval study of cool, directly imaged exoplanet 51 Eri b
  crossref 2024-02-19T16:21:31Z 置信度 0.70
• Activity of the Spectral Class K2V Dwarf HD 189733 in a Hot-Jupiter Type Exoplanet
  crossref I. S. Savanov 2024-07-31T14:02:32Z 置信度 0.70
• High-temperature measurements of VUV absorption cross sections with application to warm exoplanet atmospheres
  ) IntroductionWith current observational constraints, a large fraction of observed exoplanets whose atmospheres can be studied with spectroscopy orbits closely from their host stars, receiving a high stellar flux and having elevated equilibrium temperature (Te…
  crossref Benjamin Fleury, Yves Benilan, Olivia Venot, Romeo Veillet 2024-07-03T11:09:04Z 置信度 0.70
• Habitability of an exoplanet based on stellar wind
  This paper aims to investigate the influence of stellar winds on the atmosphere of exoplanets. Stellar winds, which consist of charged particles produced by stars, can heavily alter and affect the evolution and composition of exoplanet atmospheres. This paper …
  crossref Changseok Lee 2024-07-26T03:42:22Z 置信度 0.70
• Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations
  Transmission spectroscopy is a leading method for characterising the atmospheric composition of exoplanets, but clouds and hazes in an observing target’s atmosphere frequently lead to muted or featureless spectra. Clouds and hazes also reciprocally i…
  crossref Maureen Cohen, Paul Palmer, Massimo Bollasina, Adiv Paradise 等 2024-07-03T11:09:04Z 置信度 0.70
• The effects of terrestrial exoplanet bulk composition on long-term planetary evolution
  AbstractWith more observations of terrestrial exoplanets becoming available every year, the importance of geodynamical studies focusing on exoplanets is increasing. We know from observations that stellar chemical abundances vary in the Solar neighbourhood, whi…
  crossref Robert Spaargaren, Haiyang Wang, Maxim Ballmer, Stephen Mojzsis 等 2020-10-08T12:02:39Z 置信度 0.70
• The Atmospheric Remote-sensing Infrared Exoplanet Large-survey sensitivity and performance
  The Ariel space mission will characterise spectroscopically the atmospheres of a large and diverse sample of hundreds of exoplanets. Targets will be chosen to cover a wide range of masses, densities, equilibrium temperatures and host stellar types to study the…
  crossref Enzo Pascale, Andrea Bocchieri, Paul Eccleston, Lorenzo Mugnai 等 2024-07-03T11:09:04Z 置信度 0.70
• Biases in Exoplanet Transmission Spectra Introduced by Limb-darkening Parametrization
  Abstract One of the main endeavors of the field of exoplanetary sciences is the characterization of exoplanet atmospheres on a population level. The current method of choice to accomplish this task is transmission spectroscopy, where the apparent radius of a t…
  crossref Louis-Philippe Coulombe, Pierre-Alexis Roy, Björn Benneke 2024-10-29T03:46:16Z 置信度 0.70
• Ex(o)plain: Subgroup-Level Analysis of Exoplanet Atmospheric Parameters
  crossref Alkis Koudounas, Flavio Giobergia, Elena Baralis 2024-09-24T17:26:55Z 置信度 0.70
• Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes
  Abstract Detecting exoplanet transits at X-ray wavelengths would provide a window into the effects of high-energy irradiation on the upper atmospheres of planets. However, stars are relatively dim in the X-ray, making exoplanet transit detections difficult wit…
  crossref Raven Cilley, George W. King, Lía Corrales 2024-09-26T15:55:51Z 置信度 0.70
• Model for calculating effective temperature of exoplanet in low eccentricity binary star system. Calculating the effective temperature of Kepler-47b and Kepler-453b.
  crossref Emil Musheghyan 2024-12-13T16:04:42Z 置信度 0.70
• Observations of scattered light from exoplanet atmospheres
  Optical phase curves of hot Jupiters can reveal global scattering properties. We implemented a Bayesian inference framework for optical phase curves with flux contributions from: reflected light from a potentially inhomogeneous atmosphere, thermal emission, el…
  crossref Brett M. Morris, Kevin Heng, Daniel Kitzmann 2024-05-14T07:46:29Z 置信度 0.70
• Axisymmetric High Spot Coverage on Exoplanet Host HD 189733 A
  Abstract Transmission spectroscopy is a powerful tool to study exoplanet atmospheres, which can be affected by the ability of stellar photospheric heterogeneity to mimic or mask exoplanetary spectral signatures. The canonical HD 189733 system provides a textbo…
  crossref Isaac S. Narrett, Benjamin V. Rackham, Julien de Wit 2024-02-14T10:53:31Z 置信度 0.70
• Rapid characterization of exoplanet atmospheres with the Exoplanet Transmission Spectroscopy Imager
  crossref Luke M. Schmidt, Ryan J. Oelkers, Erika Cook, Mary Anne Limbach 等 2024-12-09T03:18:51Z 置信度 0.70
• Evolution of exoplanet atmospheres:  The Mars example of geological sources and sinks in addition to solar/stellar stripping of gas
  Introduction:  Understanding exoplanet habitability and its evolution requires understanding the relative importance of the different sinks for atmospheric volatiles.  While a lot of attention is paid to stripping of atmospheric gas by stella…
  crossref Bruce Jakosky 2024-07-03T11:09:04Z 置信度 0.70
• 15 Exoplanet Geology: What Can We Learn from Current and Future Observations?
  crossref Bradford J. Foley 2024-08-22T14:44:53Z 置信度 0.70
• Biases in the Transit, Radial velocity, Gravitational Microlensing, and direct Imaging exoplanet discovery methods
  The field of extrasolar planets or exoplanets, planets in star systems outside of the solar system, is a relatively new field of astronomy emerging in the late 20th century. Since then, more exoplanet detection methods have been proposed and developed, especia…
  crossref Ruixuan He 2025-07-10T17:50:50Z 置信度 0.70
• The Nonsingular Estimator for Exoplanet Orbits: An Unscented Batch Estimation Method for Direct Imaging Measurements
  Abstract We present a new method for fitting exoplanet orbits to direct astrometric measurements, using nonlinear batch estimation and nonsingular orbital elements. Our estimation technique is based on the unscented transform, which approximates probability di…
  crossref Zvonimir Stojanovski, Dmitry Savransky 2024-06-28T17:01:33Z 置信度 0.70
• Introduction and Analysis of Exoplanet Detection Techniques
  The exoplanet study is important for exploring life's origins in the universe. With the development of astronomical observation technology, more and more exoplanets have been discovered, and the exploration of habitable planets and the study of planetary atmos…
  crossref Xiaoxi Zhao 2025-01-03T07:02:11Z 置信度 0.70
• A Survey of 12 Exoplanet-Star Systems and Their Exomoon Candidates
  crossref Connor Jackson 2025-12-18T09:55:53Z 置信度 0.70
• Synthetic light curves of exoplanet transit using nanosatellite data
  crossref A. Fuentes, M. Solar 2024-02-28T16:50:34Z 置信度 0.70
• ALDERAAN: Automated Lightcurve Detrending, Exoplanet Recovery, and Analysis of Autocorrelated Noise (v0.1.0)
  Initial release of ALDERAAN pipeline (v0.1.0) This is the version of the code used for G.J. Gilbert, E.A. Petigura, & P.M. Entrican, "Planets larger than Neptune have elevated eccentricities," PNAS 122 (11) e2405295122, https://doi.org/10.1073/pnas.2405295122 …
  datacite Gilbert, Gregory, Petigura, Erik, Entrican, Paige 2025 置信度 0.66 AstronomyAstronomy/methodsObservational astronomy
• PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-resolution Phased-resolved Spectroscopy of the Ultra-hot-Jupiter KELT-20 b.
  europepmc 2026 置信度 0.80
• Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits.
  europepmc 2025 置信度 0.80
• Mid-Devonian ocean oxygenation enabled the expansion of animals into deeper-water habitats.
  europepmc 2025 置信度 0.80
• Abundant water from primordial supernovae at cosmic dawn.
  europepmc 2025 置信度 0.80
• Quantum sensing for NASA science missions.
  The National Aeronautics and Space Administration (NASA) develops a broad range of technologies to support space-based quantum sensing and communications, uses the space environment to study fundamental quantum processes to advance our knowledge of physics, an…
  europepmc 2025 置信度 0.80
• Space Research Ethics.
  europepmc 2026 置信度 0.80
• Uncovering the integral spectral characteristics of the planetary nebula IC 4642.
  europepmc 2025 置信度 0.80
• From pixels to camera: scaling superconducting nanowire single-photon detectors for imaging at the quantum-limit.
  europepmc 2025 置信度 0.80
• Evidence for a sub-Jovian planet in the young TWA 7 disk.
  Planets are thought to form from dust and gas in protoplanetary disks, with debris disks being the remnants of planet formation. Aged a few million up to a few billion years, debris disks have lost their primordial gas, and their dust is produced by steady-sta…
  europepmc A.‐M. Lagrange, C. Wilkinson, Mathilde Mâlin, A. Boccaletti 等 2025 置信度 0.80 JovianPlanetAstrobiologyAstronomyPhysics
• Chemical Mechanical Polishing of Zerodur<sup>®</sup> Using Silica and Ceria Nanoparticles: Toward Ultra-Smooth Optical Surfaces.
  europepmc 2025 置信度 0.80
• Frequency-comb-calibrated Laser Heterodyne Radiometry for Precision Radial Velocity Measurements.
  europepmc 2025 置信度 0.80
• Predicting the diversity of photosynthetic light-harvesting using thermodynamics and machine learning.
  europepmc 2025 置信度 0.80
• Selecting optimal celestial object for space observation in the realm of complex spherical fuzzy systems.
  The sensible selection of celestial objects for observation by the James Web Space Telescope (JWST) is pivotal for the precise decision-making (DM) process, aligning with scientific priorities and instrument capabilities to maximize valuable data acquisition t…
  europepmc 2024 置信度 0.80
• Origin and Evolution of the Galilean Satellites Within the Jovian System.
  europepmc 2026 置信度 0.80
• Earth-mass planets with He atmospheres in the habitable zone of Sun-like stars.
  europepmc 2025 置信度 0.80
• Interactive symbolic regression with co-design mechanism through offline reinforcement learning.
  europepmc 2025 置信度 0.80
• The Origins & Reservoirs of Exocomets.
  Small bodies exist in distinct populations within their planetary systems. These reservoir populations hold a range of compositions, which to first order are dependent on formation location relative to their star. We provide a general overview of the nature of…
  europepmc Michele T. Bannister, Susanne Pfalzner, Tim D. Pearce, Alexander J. Mustill 等 2025 置信度 0.80 PlanetesimalExoplanetAstrobiologyDebrisSolar System
• Responsible AI Integration in Mental Health Research: Issues, Guidelines, and Best Practices.
  europepmc 2025 置信度 0.80