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• Rediscussion of eclipsing binaries. Paper XIX. The long-period solar-type system V454 Aurigae
  V454 Aur is an eclipsing binary system containing two solar-type stars on an orbit of relatively long period (P = 27.02 d) and large eccentricity (e = 0.381). Eclipses were detected using data from the Hipparcos satellite, and a high-quality double-lined spect…
  datacite Southworth, John 2024 置信度 0.66 Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• Characterizing Exoplanetary Atmospheres: New Views on Exoplanet Composition and Chemistry
  I review the major open science questions in exoplanet atmospheres. These are mainly focused in the areas of understanding atmospheric physics, the atmosphere as a window into other realms of planetary physics, and the atmosphere is a window into understanding…
  datacite Fortney, Jonathan J. 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
• Comparison Analysis of Starspots and Historical Sunspot Data
  Dark regions commonly appearing on the Sun’s surface are known as “sunspots.” These areas of solar activity are a result of cooled regions of magnetic flux within the Sun’s photosphere. Areas of higher solar-magnetic activity heat regions of both the photosphe…
  datacite Jack Cousins 2024 置信度 0.66 starspotssunspots
• Atmospheric properties of AF Lep b with forward modeling
  Aims. We aim to expand the atmospheric exploration of AF Lep b by modeling all available observations obtained with SPHERE at VLT (between 0.95-1.65, at 2.105, and 2.253 $μ$m, and NIRC2 at Keck (at 3.8 $μ$m) with self-consistent atmospheric models. Methods. To…
  datacite Palma-Bifani, P., Chauvin, G., Borja, D., Bonnefoy, M. 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• HARPS at 20: Evolving Through Continuous Improvements
  The High Accuracy Radial velocity Planet Searcher (HARPS), operational since October 2003, has been pioneering exoplanetary research, with over 1300 publications and more than 200 exoplanet detections, and is still in high demand. Its continued success has bee…
  datacite Lo Curto, Gaspare, Pepe, Francesco, Fleury, Michel, Hughes, Ian 等 2024 置信度 0.66
• Formation of the Hot Jupiter Core in the Early Disk
  Abstract: This paper explores hot Jupiter core formation much nearer to the star than the traditional in-situ model suggests. We propose that the protoplanetary disk and the hot Jupiter core form concurrently during a star's infancy, when cooler temperatures f…
  datacite Jan Makopa 2024 置信度 0.66 hot Jupiter formationearly stellar developmentprotoplanetary diskheadwind effectdensity enhancement
• Formation of the Hot Jupiter Core in the Early Disk
  Abstract: This paper explores hot Jupiter core formation much nearer to the star than the traditional in-situ model suggests. We propose that the protoplanetary disk and the hot Jupiter core form concurrently during a star's infancy, when cooler temperatures f…
  datacite Jan Makopa 2024 置信度 0.66 hot Jupiter formationearly stellar developmentprotoplanetary diskheadwind effectdensity enhancement
• Do Temperate Rocky Planets Around M Dwarfs have an Atmosphere ?
  Detecting an atmosphere on nearby temperate planets is one of the most important scientific objectives of the Webb mission, an endeavour in practice limited to a handful of well-characterized planets: Trappist-1d, e, f, g, LHS1140b, and the mini-Neptune K2- 18…
  datacite Doyon, Rene 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• DIAmante TESS AutoRegressive Planet Search (DTARPS): I. Analysis of 0.9 Million Light Curves
  Nearly one million light curves from the TESS Year 1 southern hemisphere extracted from Full Frame Images with the DIAmante pipeline are processed through the AutoRegressive Planet Search statistical procedure. ARIMA models remove trends and lingering autocorr…
  datacite Melton, Elizabeth J., Feigelson, Eric D., Montalto, Marco, Caceres, Gabriel A. 等 2023 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciencesFOS: Physical sciences
• Constraints on atmospheric water abundance and cloud deck pressure in the warm Neptune GJ 3470 b via CARMENES transmission spectroscopy
  Observations of cooler atmospheres of super-Earths and Neptune sized objects often show flat transmission spectra. The most likely cause of this trend is the presence of aerosols (i.e. clouds and hazes) in the atmospheres of such objects. High-resolution spect…
  datacite Dash, Spandan, Brogi, Matteo, Gandhi, Siddharth, Lafarga, Marina 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• 2200727
  Target RA (J2000): 350.916534 and deg Target Dec (J2000): -1.18929 and deg Gaia GMag: 10.72 Programme ID: CH_PR240001 PI of observing programme: Isaak Title of programme: Inspiration through space science – a CHEOPS-based education activity for high-school stu…
  datacite European Space Agency, Isaak 2024 置信度 0.66
• Cosmic Hydrogen and Ice Loss Lines
  We explain the overall equilibrium-temperature-dependent trend in the exoplanet mass-radius diagram, using the escape mechanisms of hydrogen and relevant volatiles, and the chemical equilibrium calculation of molecular hydrogen (H$_2$) break-up into atomic hyd…
  datacite Zeng, Li, Jacobsen, Stein B. 2022 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• HST astrometry of the closest Brown Dwarfs -- II. Improved parameters and constraints on a third body
  Located at less than 2pc away, Luhman16AB (WISE.J104915.57-531906.1) is the closest pair of brown dwarfs and third closest `stellar' system to Earth. An exoplanet candidate in the Luhman16 binary system was reported in 2017 based on a weak astrometric signatur…
  datacite Bedin, L. R., Dietrich, J., Burgasser, A. J., Apai, D. 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• Testing approximate infrared scattering radiative-transfer methods for hot Jupiter atmospheres
  The calculation of internal atmospheric (longwave) fluxes is a key component of any model of exoplanet atmospheres that requires radiative-transfer (RT) calculations. For atmospheres containing a strong scattering component such as cloud particles, most 1D mul…
  datacite Lee, Elspeth K. H. 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Pulsation in TESS Objects of Interest
  We report the discovery of three Transiting Exoplanet Survey Satellite Objects of Interest (TOI) with signatures of pulsation, observed in more than one sector. Our main goal is to explore how large is the variety of classical pulsators such as $δ$ Sct, $γ$ Do…
  datacite Gomes, R. L., Martins, B. L. Canto, Fontinele, D. O., Almeida, L. A. 等 2024 置信度 0.66 Solar and Stellar Astrophysics (astro-ph.SR)Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Sonora Bobcat: cloud-free, substellar atmosphere models, spectra, photometry, evolution, and chemistry
  OVERVIEW Presented here are models for non-irradiated, substellar mass objects belonging to the Sonora model series, described in Marley et al. (2021). The files presented here are model temperature-pressure structures ("structure"), emergent spectra from the …
  datacite Marley, Mark, Saumon, Didier, Morley, Caroline, Fortney, Jonathan 等 2021 置信度 0.66 brown dwarf, ultra cool dwarf, extrasolar planet, atmosphere, model, spectra, evolution, photometry
• Exoplanet Observations in Taurus Hill Observatory – Scientific Support for Research Programs
  AbstractTaurus Hill Observatory (THO) [1], observatory code A95, is an amateur observatory located in Varkaus, Finland. The observatory is maintained by the local astronomical association Warkauden Kassiopeia. THO research team has observed and measured variou…
  crossref Harri Haukka, Veli-Pekka Hentunen, Markku Nissinen, Tuomo Salmi 等 2020-10-08T10:35:58Z 置信度 0.70
• Image-Based Time-Series Representations and Transfer Learning for Enhanced Exoplanet Detection
  crossref Aseel Eljack, Ashraf Elnagar 2024-10-03T10:02:25Z 置信度 0.70
• YunMa: Advancing Atmospheric Cloud and Haze Analysis in the Next-Generation Exoplanet Data Era 
  The analysis of exoplanetary spectroscopic data, captured by next-generation instruments like Webb, emphasizes the importance of accurately modeling clouds and hazes. While retrieval studies have emerged as one of the key methods for interpreting spectroscopic…
  crossref Sushuang Ma, Yuichi Ito, Ahmed Faris Al-Refaie, Quentin Changeat 等 2024-07-03T11:09:04Z 置信度 0.70
• Ground-based photometric follow-up for exoplanet detections with the PLATO mission
  crossref H.J. Deeg, R. Alonso 2024-02-28T07:48:28Z 置信度 0.70
• Simulation of a single photon counting photonic spectrograph for exoplanet atmospheric characterization
  crossref Edwin Alexani, Donald F. Figer, Pradip Gatkine 2024-06-14T18:14:58Z 置信度 0.70
• Logistic regression to boost exoplanet detection performances
  ABSTRACT Direct imaging of exoplanets requires to separate the background noise from the exoplanet signals. Statistical methods have been recently proposed to avoid subtracting any signal of interest as opposed to initial self-subtracting methods based on angu…
  crossref Hadrien Cambazard, Nicolas Catusse, Antoine Chomez, Anne-Marie Lagrange 2024-11-29T10:49:45Z 置信度 0.70
• Research on the Methods of Exoplanet Detection and Discussion on Correlations and Flaws
  The search for exoplanets, particularly Earth-like planets, has garnered significant attention as potential second homes for human beings. Highlights of the urgency of finding alternative habitable planets due to the dire consequences of global warming and cli…
  crossref Ruidong Tian 2025-01-03T07:02:13Z 置信度 0.70
• Classification of Kepler exoplanet searching from galaxy using machine learning model
  The Kepler exoplanet mission was designed specifically to search the Milky Way galaxy for numerous small planets the size of Earth that are either in or close to the habitable zone. An exoplanet is a planet that orbits stars outside of our solar system. The da…
  crossref Sasmita Kumari Nayak 2024-01-04T23:30:14Z 置信度 0.70
• Exoplanet science with SPIRou: near-infrared precision velocimetry and spectropolarimetry
  High-precision radial-velocity measurements in the near-infrared allow one to search for exoplanet signals around the lowest-mass stars, including young ones. Because these stars can be among the most active ones, it is essential to characterize their magnetic…
  crossref Claire Moutou, Jean-François Donati, Florian Debras 2023-03-01T09:16:24Z 置信度 0.70
• Inferring Intrinsic Stellar EUV and Lyman-Alpha Fluxes and Their Effects on Exoplanet Atmospheres
  crossref Jeffrey L. Linsky, Seth Redfield 2024-04-10T08:02:01Z 置信度 0.70
• Venus as an Exoplanet: Effect of varying stellar, orbital, planetary andatmospheric properties upon composition, habitability and detectability
  The newly selected Venus missions EnVISION and VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy) offer new opportunities for studying Venus but will also contribute to furthering our knowledge of Venus as an exoplanet. Hot rocky pl…
  crossref John Lee Grenfell, Joern Helbert, Gabriele Arnold, Konstantin Herbst 等 2024-07-03T11:09:04Z 置信度 0.70
• ExoSim 2: the new exoplanet observation simulator applied to the Ariel space mission
  crossref Lorenzo V. Mugnai, Andrea Bocchieri, Enzo Pascale 2024-06-14T18:16:03Z 置信度 0.70
• Gen TSO: A General JWST Simulator for Exoplanet Times-series Observations
  Abstract Gen TSO is a noise calculator specifically tailored to simulate James Webb Space Telescope (JWST) time-series observations of exoplanets. Gen TSO enables the estimation of signal-to-noise ratios (S/Ns) for transit or eclipse depths through an interact…
  crossref Patricio E. Cubillos 2024-12-05T17:11:51Z 置信度 0.70
• Performance of PSG in retrieving exoplanet parameters from JWST data simulated with several tools
  Abstract Our research explores different methods of utilizing several known tools (petitRADTRANS, PandExo, and PSG) to simulate spectral data acquired by the James Webb Space Telescope (JWST). We specifically focus on how the choice of method affects the perfo…
  crossref H. Barbier, E. López, D. Mayorga, D. Cherres 2024-07-15T05:41:06Z 置信度 0.70
• Exploring the collinear Lagrangian points of exoplanet systems with P-R drag and oblateness
  Abstract We explore the position and stability of the collinear Lagrangian points in the Restricted Three-Body Problem (RTBP) where one primary body is radiative and the other is oblate. We examine the influence of Poynting-Robertson drag and the position and …
  crossref S. N. Hasan, Priya Hasan, Ibtesam Shaikh 2026-01-09T09:40:01Z 置信度 0.70
• Exoplanet Classification Through Machine Learning: A Comparative Analysis of Algorithms Using Kepler Data
  This study delves into the classification of exoplanets using data from the Kepler Space Telescope, comparing a suite of machine learning (ML) models to ascertain their efficacy in distinguishing confirmed planets, candidates, and false positives. With a datas…
  crossref Gregorius Airlangga 2024-09-08T07:37:18Z 置信度 0.70
• Automated Scheduling of Doppler Exoplanet Observations at Keck Observatory
  Abstract Precise Doppler studies of extrasolar planets require fine-grained control of observational cadence, i.e., the timing of and spacing between observations. We present a novel framework for scheduling a set of Doppler campaigns with different cadence re…
  crossref Luke B. Handley, Erik A. Petigura, Velibor V. Mišić, Jack Lubin 等 2024-02-21T10:59:03Z 置信度 0.70
• A continuous multiple hypothesis testing framework for optimal exoplanet detection
  crossref Nathan C. Hara, Thibault de Poyferré, Jean-Baptiste Delisle, Marc Hoffmann 2024-01-31T11:31:19Z 置信度 0.70
• End-to-end simulations of exoplanet detection with multiplexed volume Bragg gratings
  Context. Direct imaging of exoplanets greatly enhances our ability to spectroscopically detect molecules in their atmospheres, but requires both excellent angular and spectral resolution. A highly promising approach uses multiplexed transmission gratings to ac…
  crossref F. J. Fagginger Auer, C. U. Keller 2024-04-16T18:50:17Z 置信度 0.70
• Database Design for SpExoDisks: A Database and Web Portal for Spectra of Exoplanet-forming Disks
  Abstract Data access—or the availability of new and archival data for use by the larger community—is key for scientific advancement. How data is presented, searched, and formatted determines accessibility and it can be difficult to find a solution that fits th…
  crossref Caleb H. Wheeler, Natalie R. Hinkel, Andrea Banzatti 2024-12-03T12:41:27Z 置信度 0.70
• Introducing the Exoplanet Escape Factor and the Fishbowl Worlds (two conceptual tools for the search for extra terrestrial civilizations)
  The search for extraterrestrial intelligence on exoplanets is a rich field of conceptual exploration. Author introduces two definitions that could help to narrow down the possibilities that an extraterrestrial civilization may or may not have initiated explora…
  crossref Elio Rodríguez 2024-02-22T11:30:09Z 置信度 0.70
• Bound circumplanetary orbits under the influence of radiation pressure: Application to dust in directly imaged exoplanet systems
  crossref Bradley M. S. Hansen, Kevin Hayakawa 2024-03-01T15:27:14Z 置信度 0.70
• Transition from super-alfvenic to sub-alfvenic stellar wind flow passing by an exoplanet, using the example of HD 209458b
  Depending on the distance of the exoplanet from the central star and on the properties of this star, different regimes of stellar wind flow around it arise. If the exoplanet is at a distance up to the Alfven radius at which the wind speed is equal to the Alfve…
  crossref E. S. Belenkaya 2024-09-27T16:45:56Z 置信度 0.70
• Advancing Exoplanet Research with MARCOT: Innovative Photonic Lantern Integration for Enhanced Spectroscopic Capabilities
  The MARCOT-Pathfinder Telescope (MPT), situated at the Calar Alto Observatory (CAHA) in Spain, represents the integration of a state-of-the-art Multi-Mode Photonic Lantern for usage with high-resolution spectrographs, enhancing the MARCOT-Pathfinder's optical …
  crossref Marina Centenera, Pedro Amado, Jesús Aceituno, Sergio Burgos 等 2024-07-03T11:09:04Z 置信度 0.70
• From atmospheric to exoplanet formation retrievals
  With new and upcoming observing facilities (JWST and the ELTs), the exoplanet community is poised to precisely measure the chemical inventory of exoplanet atmospheres. This will allow, for the first time, to start investigating whether one of the greatest prom…
  crossref Paul Mollière, Tamara Molyarova, Bertram Bitsch, Christian Eistrup 等 2021-07-22T12:01:26Z 置信度 0.70
• Exomod: A Python Library for Exoplanet Transit Light Curve Fitting and Stacking with Background Simulation and Optimization
  Abstract From the light curve taken during exoplanet transit, important parameters such as the radius ratio of the star-planet, impact parameter, inclination, and relative tangential velocity could be derived. A module was developed in the form of a Python lib…
  crossref Rafa Nanda Akilah, Bryant Randolph, M. Khawariz Andaristiyan 2024-10-22T06:32:44Z 置信度 0.70
• Exoplanet detection limits using spectral cross-correlation with spectro-imaging
  Context. The combination of high-contrast imaging and medium- to high-resolution spectroscopy offers new possibilities for the detection and characterization of exoplanets. The so-called molecular mapping technique makes use of the difference between the plane…
  crossref A. Bidot, D. Mouillet, A. Carlotti 2023-11-15T19:49:11Z 置信度 0.70
• Lightweight design and analysis of optical cover plate for exoplanet imaging coronagraph
  crossref Lingyi Kong, Mingming Xu, Wei Guo, Jiangpei Dou 等 2024-11-04T19:57:29Z 置信度 0.70
• Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution
  Abstract Exoplanet systems are thought to evolve on secular timescales over billions of years. This evolution is impossible to directly observe on human timescales in most individual systems. While the availability of accurate and precise age inferences for in…
  crossref Stephen P. Schmidt, Kevin C. Schlaufman, Jacob H. Hamer 2024-08-06T13:16:06Z 置信度 0.70
• Thermal design of focal plane assembly of wavefront camera for exoplanet imaging corona module
  Abstract The focal plane assembly of wavefront camera is the key imaging device of wavefront detection camera and the key load of the exoplanet imaging coronagraph module. In order to ensure the imaging quality and reduce the dark current and thermal noise, it…
  crossref Chengcheng Wen, Shu Jiang, Mingming Xu, Lingyi Kong 等 2024-01-25T14:36:11Z 置信度 0.70
• Erratum: “Variability of Known Exoplanet Host Stars Observed by TESS” (2023, AJ, 166, 72)
  crossref Emilie R. Simpson, Tara Fetherolf, Stephen R. Kane, Joshua Pepper 等 2024-03-01T08:00:34Z 置信度 0.70
• Advancing Apodization Techniques: Optimizing Interferometric Apodization by Homothety for Exoplanet Detection
  Abstract New apodization techniques are emerging rapidly to enhance the coronagraphs’ rejection capabilities and refine the optics for directly detecting exoplanets. One such technique, Interferometric Apodization by Homothety (IAH), involves splitting the inc…
  crossref A. Qazbour, Y. El Azhari, J. Chafi, Z. Benkhaldoun 等 2026-01-09T09:40:01Z 置信度 0.70
• The Radiative Magneto-Hydrodynamics of Colliding Flow: Instabilities, Reconnection and Exoplanet Atmosphere Connections
  crossref Adam Frank 2024-11-27T22:07:16Z 置信度 0.70
• Exoplanets across galactic stellar populations with PLATO
  Context . The vast majority of exoplanet discoveries to date have occurred around stars in the solar neighbourhood, with chemical compositions comparable to that of the Sun. However, models suggest that planetary systems in different Galactic environments, wit…
  crossref C. Boettner, A. Viswanathan, P. Dayal 2024-11-06T14:43:19Z 置信度 0.70
• Revealing the Fate of Exoplanet Systems: Asteroseismic Identification of Host Star in the Red Clump or Red Giant Branch
  Abstract Determining the evolutionary stage of stars is crucial for understanding the evolution of exoplanetary systems. In this context, red giant branch (RGB) and red clump (RC) stars, which formed at stages in the later evolution of stars situated before an…
  crossref Wen-Xu Lin, Sheng-Bang Qian, Li-Ying Zhu 2024-08-22T18:23:03Z 置信度 0.70
• Initial Entropy and Potential Delayed Formation of the Directly Imaged Exoplanet AF Lep b
  Abstract AF Lep b is a rare directly imaged exoplanet with properties consistent with core-accretion evolution models. Using its precise dynamical mass and spectroscopically inferred bolometric luminosity alongside the Spiegel & Burrows evolution models, I…
  crossref Zhoujian 周健 Zhang 张 2024-04-30T14:52:50Z 置信度 0.70
• Distinguishing exoplanet companions from field stars in direct imaging using <i>Gaia</i> astrometry
  Direct imaging searches for exoplanets around stars detect many spurious candidates that are in fact background field stars. To help distinguish these from genuine companions, multi-epoch astrometry can be used to identify a common proper motion with the host …
  crossref Philipp Herz, Matthias Samland, Coryn A. L. Bailer-Jones 2023-12-12T19:56:42Z 置信度 0.70
• Atmospheric model intercomparison dataset on Snowball Earth and waterbelt states
  This dataset contains 2d output data and diagnosed feedback factors from different atmospheric models for the purpose of analysing the transition from a temperate climate to a waterbelt state or Snowball Earth. All models are run in a setup with aquaplanet, sl…
  datacite Hörner, Johannes, Voigt, Aiko 2025 置信度 0.66 KlimatologieClimatologyÖFOS 2012 -- NATURWISSENSCHAFTEN (1) -- Geowissenschaften (105) -- Meteorologie, Klimatologie (1052) -- Klimatologie (105204)ÖFOS 2012 -- NATURAL SCIENCES (1) -- Geosciences (105) -- Meteorology, Climatology (1052) -- Climatology (105204)climate
• First release of stellar contamination modeling and retrieval code
  Full Changelog: https://github.com/cpiaulet/stctm/commits/v1.0.0 Readme.md information from the repository (live version hosted at https://github.com/cpiaulet/stctm/blob/main/README.md): STCTM stctm (STellar ConTamination Modeling) performs spectral retrievals…
  datacite Piaulet-Ghorayeb, Caroline 2024 置信度 0.66
• Robotic Observations of Microlensing Events/Reactive Event Assessment (ROME/REA) Survey
  The Robotic Observations of Microlensing Events/Reactive Event Assessment (ROME/REA) Survey conducted time series imaging of 20 non-overlapping fields (see the ROME/REA Fields table in the Data Products and Table Columns section) in the Galactic Bulge using th…
  datacite NASA Exoplanet Archive 2024 置信度 0.66
• Star Guide: guiding citizen scientists to exoplanets
  Star Guide is an ongoing project to support exoplanet citizen science. We do this by working with existing collaborations to identify barriers to entry and pain points. In this talk, we present the results of a survey carried out early in 2024 among exoplanet …
  datacite Creaner, Oisin, Preis, Anna, Ryan, Cormac 2024 置信度 0.66
• Star Guide: guiding citizen scientists to exoplanets
  Star Guide is an ongoing project to support exoplanet citizen science. We do this by working with existing collaborations to identify barriers to entry and pain points. In this talk, we present the results of a survey carried out early in 2024 among exoplanet …
  datacite Creaner, Oisin, Preis, Anna, Ryan, Cormac 2024 置信度 0.66
• pyDANDIA v1.0
  pyDANDIA is a reduction pipeline for astronomical timeseries imaging data, based on the Difference Image Analysis technique. The package includes both the core pipeline together with data handling tools. This release represents the pyDANDIA version used to pro…
  datacite Street, Rachel, Bachelet, Etienne, Hundertmark, Markus, Tsapras, Yiannis 2025 置信度 0.66 AstronomyAstronomyAstronomy
• pyDANDIA v1.0
  pyDANDIA is a reduction pipeline for astronomical timeseries imaging data, based on the Difference Image Analysis technique. The package includes both the core pipeline together with data handling tools. This release represents the pyDANDIA version used to pro…
  datacite Street, Rachel, Bachelet, Etienne, Hundertmark, Markus, Tsapras, Yiannis 2025 置信度 0.66 AstronomyAstronomyAstronomy
• Reduced CRIRES+ spectroscopy observations of GJ 3470
  Reduced CRIRES+ spectroscopy observations of GJ 3470 from 2022-02-10 This records contains yet unpublished reduced data obtained with the CRIRES+ spectrograph at the Very Large Telescope. The time-series of observations was acquired covering a transit of the e…
  datacite Lavail, Alexis, Chabrol, Estelle 2025 置信度 0.66
• Reduced CRIRES+ spectroscopy observations of GJ 3470
  Reduced CRIRES+ spectroscopy observations of GJ 3470 from 2022-02-10 This records contains yet unpublished reduced data obtained with the CRIRES+ spectrograph at the Very Large Telescope. The time-series of observations was acquired covering a transit of the e…
  datacite Lavail, Alexis, Chabrol, Estelle 2025 置信度 0.66
• an0wen/MARDIGRAS: Automatic update and hover name
  v1.2.2 - automatic catalog update and show exoplanet name on hover Author: Artyom (Artem) Aguichine Date: 2024/12/14 Changes: The NASA Exoplanet Archive (NEA) catalog can be automatically updated by running the program with the flag "--update-nea-catalog": pyt…
  datacite Artem Aguichine 2024 置信度 0.66
• an0wen/MARDIGRAS: v1.2.0
  MARDIGRAS Mass-Radius DIaGRAm with Sliders (MARDIGRAS) is a visualization tool that allows simple and intuitive manipulation of mass-radius relationships (also known as iso-composition curves) using interactive sliders. Run the tool To run the program, downloa…
  datacite Artem Aguichine 2024 置信度 0.66
• Integration and testing of a cryogenic receiver for the Exoplanet Climate Infrared Telescope (EXCITE)
  The EXoplanet Climate Infrared TElescope (EXCITE) is an instrument designed to measure spectroscopic phase curves of extrasolar hot Jupiters from a long duration balloon platform. EXCITE will fly a moderate resolution spectrometer housed inside of a cryogenic …
  datacite Kleyheeg, Annalies, Bernard, Lee, Bocchieri, Andrea, Butler, Nat 等 2024 置信度 0.66
• The Exoplanet Climate Infrared Telescope (EXCITE): gondola pointing and stabilization qualification
  High precision sub-arcsecond pointing stability has become a capability widely utilized in the balloon-borne community, in particular for high resolution optical systems. However, many of these applications are also pushing the state-of-the-art with regards to…
  datacite Romualdez, Javier L., Bernard, Lee, Bocchieri, Andrea, Butler, Nathaniel 等 2024 置信度 0.66
• Assembly, integration, and laboratory testing of the EXCITE spectrograph
  The EXoplanet Climate Infrared TElescope (EXCITE) is a near-infrared spectrograph (0.8-3.5 µm, R∼50) designed for measuring spectroscopic phase curves of transiting hot Jupiter-type exoplanets that operates off a high-altitude balloon platform. Phase curves pr…
  datacite Bernard, Lee, Gamaunt, Johnathan, Jensen, Logan, Bocchieri, Andrea 等 2024 置信度 0.66
• Ab initio quantum dynamics as a scalable solution to the exoplanet opacity challenge: A case study of CO$_2$ in hydrogen atmosphere
  Light-matter interactions lie at the heart of our exploration of exoplanetary atmospheres. Interpreting data obtained by remote sensing is enabled by meticulous, time- and resource-consuming work aiming at deepening our understanding of such interactions (i.e.…
  datacite Wiesenfeld, Laurent, Niraula, Prajwal, de Wit, Julien, Jaïdane, Nejmeddine 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)Atomic Physics (physics.atom-ph)FOS: Physical sciencesFOS: Physical sciences
• A temperate super-Jupiter imaged with JWST in the mid-infrared
  Of the ~25 directly imaged planets to date, all are younger than 500Myr and all but 6 are younger than 100Myr. Eps Ind A (HD209100, HIP108870) is a K5V star of roughly solar age (recently derived as 3.7-5.7Gyr and 3.5$^{+0.8}_{-1.3}$Gyr). A long-term radial ve…
  datacite Matthews, E. C., Carter, A. L., Pathak, P., Morley, C. V. 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Cross-Model Validation of Coronagraphic Exposure Time Calculators for the Habitable Worlds Observatory: A Report from the Exoplanet Science Yield sub-Working Group
  Estimating the exoplanet scientific productivity of the Habitable Worlds Observatory requires estimating science exposure times. From exoplanet yields to spectral retrievals, exposure times are at the heart of our understanding of the capabilities of this futu…
  datacite Stark, Christopher C., Steiger, Sarah, Tokadjian, Armen, Savransky, Dmitry 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
• Earth Detecting Earth: At what distance could Earth's constellation of technosignatures be detected with present-day technology?
  The field of the Search for Extraterrestrial Intelligence (SETI) searches for ``technosignatures'' that could provide the first detection of life beyond Earth through the technology that an extraterrestrial intelligence (ETI) may have created. Any given SETI s…
  datacite Sheikh, Sofia Z., Huston, Macy J., Fan, Pinchen, Wright, Jason T. 等 2025 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)Earth and Planetary Astrophysics (astro-ph.EP)Popular Physics (physics.pop-ph)FOS: Physical sciences
• Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c
  Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epoch-based, modelindependent method to mitigate stellar contamination, applicable …
  datacite Arufe, Aaron Bello 2025 置信度 0.66
• Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c
  Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epoch-based, modelindependent method to mitigate stellar contamination, applicable …
  datacite Arufe, Aaron Bello 2025 置信度 0.66
• Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c
  Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epoch-based, modelindependent method to mitigate stellar contamination, applicable …
  datacite Arufe, Aaron Bello 2025 置信度 0.66
• Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c
  Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epoch-based, modelindependent method to mitigate stellar contamination, applicable …
  datacite Arufe, Aaron Bello 2025 置信度 0.66
• From Stability to Instability: Characterizing the Eccentricities of Multi-planet Systems in the California Kepler Survey as a Means of Studying Stability
  Understanding the stability of exoplanet systems is crucial for constraining planetary formation and evolution theories. We use the machine-learning stability indicator, SPOCK, to characterize the stability of 126 high-multiplicity systems from the California …
  datacite Doty, Matthew J., Weiss, Lauren M., He, Matthias Y., Petit, Antoine C. 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum
  Water has proven to be ubiquitously detected in near-infrared (NIR) transmission spectroscopy observations of hot Jupiter atmospheres, including WASP-17b. However, previous analyses of WASP-17b's atmosphere based upon Hubble Space Telescope (HST) and Spitzer d…
  datacite Louie, Dana R., Mullens, Elijah, Alderson, Lili, Glidden, Ana 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Characterizing Quadruple Eclipsing Binary Systems Through Combined TESS Photometry and Speckle Imaging During Eclipses (SIDE) Observations
  Eclipsing binary stars (EBs) have long been valued as important tools in establishing fundamental properties and relationships in stellar astrophysics. With the discovery of systems with multiple families of eclipses, the importance of EBs extends to the study…
  datacite Gabriel Hartwell 2025 置信度 0.66 photometryspeckle imagingeclipsing binarieshierarchal systems
• The GAPS Programme at TNG. LXV. Precise density measurement of TOI-1430 b, a young planet with an evaporating atmosphere
  Small-sized exoplanets in tight orbits around young stars (10-1000 Myr) give us the opportunity to investigate the mechanisms that led to their formation, the evolution of their physical and orbital properties and, especially, of their atmospheres. Thanks to t…
  datacite Nardiello, D., Murphy, J. M. Akana, Spinelli, R., Baratella, M. 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c
  Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epoch-based, model-independent method to mitigate stellar contamination, applicable…
  datacite Rathcke, Alexander D., Buchhave, Lars A., De Wit, Julien, Rackham, Benjamin V. 等 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• New Python-based Architecture for the Keck Observatory Archive
  We describe the development of the Keck Observatory Archive (KOA) Data Discovery Service, a web-based dashboard that returns metadata for wide-area queries of the entire archive in seconds. Currently in beta, this dashboard will support exploration, visualizat…
  datacite Moseley, R., Berriman, G. Bruce, Gelino, Christopher R., Good, John C. 等 2024 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciencesFOS: Physical sciences
• Analysis of Habitability and Stellar Habitable Zones from Ob- 2 served Exoplanets
  The investigation of exoplanetary habitability is integral to advancing our knowledge of 12 extraterrestrial life potential and detailing the environmental conditions of distant worlds. In this 13 analysis, we explore the properties of exoplanets situated with…
  datacite Jiang, Jonathan 2024 置信度 0.66
• Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
  In Lammer et al. 2024, we defined Earth-like Habitats (EH) as rocky planets in the habitable zone of complex life (HZCL) on which Earth-like N$_2$-O$_2$-dominated atmospheres with minor amounts of CO$_2$ can exist and derived a formula for estimating their max…
  datacite Scherf, Manuel, Lammer, Helmut, Sproß, Laurenz 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Astrophysics of Galaxies (astro-ph.GA)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciences
• Long-term stability and dynamical spacing of compact planetary systems
  Exoplanet detection surveys revealed the existence of numerous multi-planetary systems packed close to their stability limit. In this proceeding, we review the mechanism driving the instability of compact systems, originally published in Petit et al. (2020). C…
  datacite Petit, Antoine C. 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciences
• No evidence for a metallicity-dependent enhancement of distant giant companions to close-in small planets in the California Legacy Survey
  Understanding the relationship between close-in small planets (CS) and distant giants (DG) is central to understanding the formation of planetary systems like our own. Most studies of this connection have found evidence for a positive correlation, though signi…
  datacite Van Zandt, Judah, Petigura, Erik 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)FOS: Physical sciencesFOS: Physical sciences
• X-ray and UV Observations of the Young Sun HIP~67522: Evidence of Lyman-alpha Absorption Within the Planetary System
  We present ultraviolet (UV) spectroscopy of the 17 Myr, G0V star, HIP 67522. The UV spectrum is characterized by strong chromospheric and transition region emission lines. There was moderate spectral variability during the observations consisting of 15% stocha…
  datacite Froning, Cynthia S., Youngblood, Allison, Wilson, David J., Duvvuri, Girish M. 等 2025 置信度 0.66 Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• Detection and characterization of transiting exoplanets with high-precision photometric and radial velocity observations
  The study of exoplanets has revolutionized our understanding of planetary systems beyond our solar system. As of April 2024, 5 609 exoplanets have been discovered with 728 of them being well-characterized. Transiting exoplanets offer unique insight into the tr…
  datacite Psaridi, Angeliki 2024 置信度 0.66 info:eu-repo/classification/ddc/520ExoplanetsPhotometryRadial velocity
• Addressing wavelength-correlated systematics in exoplanet transmission spectroscopy: a 2D Gaussian Process approach
  Ground-based transmission spectroscopy is often dominated by systematics, which obstructs our ability to leverage the advantages of larger aperture sizes compared to space-based observations. These systematics could be time-correlated, uniform across all spect…
  datacite Manickavasaham, Lokesh, Bestha, Manjunath, Thirupathi, Sivarani, Surya, Arun 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciencesFOS: Physical sciences
• The Heliophysics Software Search Interface
  Current search capabilities for Heliophysics science software significantly lack coverage across programming languages, interoperability with generic capabilities (e.g., Google), science-specific features, and interlinking with other Heliophysics resources. Th…
  datacite Barnum, Julie, Smith, Isaiah, Ringuette, Rebecca, Renaud, Joe 等 2025 置信度 0.66
• The Heliophysics Software Search Interface
  Current search capabilities for Heliophysics science software significantly lack coverage across programming languages, interoperability with generic capabilities (e.g., Google), science-specific features, and interlinking with other Heliophysics resources. Th…
  datacite Barnum, Julie, Smith, Isaiah, Ringuette, Rebecca, Renaud, Joe 等 2025 置信度 0.66
• Searching for substellar companion candidates with Gaia. II. A catalog of 9,698 planet candidate solar-type hosts
  In a previous paper, we introduced a new tool called GaiaPMEX. It characterizes the mass and semi-major axis relative to the central star (sma) of a possible companion around any source observed with Gaia. It uses the value of RUWE, or, with both Gaia and Hipp…
  datacite Kiefer, Flavien, Lagrange, Anne-Marie, Rubini, Pascal, Philipot, Florian 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• Searching for substellar companion candidates with Gaia. I. Introducing the GaiaPMEX tool
  The Gaia mission is expected to yield the detection of several thousands of exoplanets, perhaps at least doubling the number of known exoplanets. Although the harvest is expected to occur when the astrometric time series will be published with DR4 at the eve o…
  datacite Kiefer, Flavien, Lagrange, Anne-Marie, Rubini, Pascal, Philipot, Florian 2024 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Instrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• The Sonora Substellar Atmosphere Models VI. Red Diamondback: Extending Diamondback with SPHINX for Brown Dwarf Early Evolution
  OVERVIEW Presented here are models for non-irradiated, substellar mass objects spanning ages from 1 Myr to 15 Gyr, which belong to the Sonora model series. The models are described in Davis et al. accepted. The files inlcuded here are thermal evolution tracks …
  datacite Davis, Christopher Evan, Fortney, Jonathan, Iyer, Aishwarya, Mukherjee, Sagnick 等 2025 置信度 0.66 brown dwarfyoung brown dwarfextrasolar planetevolutionphotometry
• Eksoplaneetide teke ja atmosfääriline evolutsioon
  Presentation at Annual University of Tartu Faculty of Science and Tehnology Autumn School 2024 about exoplanet atmospheres and their evolution.
  datacite Lehtmets, Alexandra 2025 置信度 0.66 ExoplanetologyAtmosphere
• Eksoplaneetide teke ja atmosfääriline evolutsioon
  Presentation at Annual University of Tartu Faculty of Science and Tehnology Autumn School 2024 about exoplanet atmospheres and their evolution.
  datacite Lehtmets, Alexandra 2025 置信度 0.66 ExoplanetologyAtmosphere
• A planetary system with a sub-Neptune planet in the habitable zone of TOI-2093
  Aims. We aim to confirm and measure the mass of the transiting planet candidate around the K5V star TOI-2093, previously announced by the Transiting Exoplanet Survey Satellite (TESS) project. Methods. We combined photometric data from 32 sectors between 2019 a…
  datacite Sanz-Forcada, J., González-Álvarez, E., Osorio, M. R. Zapatero, Caballero, J. A. 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• hipipe - VLT/HiRISE reduction pipeline
  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, Martos, Steven, Vigan, Arthur 2025 置信度 0.66 astrophysicsexoplanetsVLTspectroscopypipeline
• hipipe - VLT/HiRISE reduction pipeline
  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, Martos, Steven, Vigan, Arthur 2025 置信度 0.66 astrophysicsexoplanetsVLTspectroscopypipeline
• The Origins &amp; 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…
  datacite Bannister, Michele, Pfalzner, Susanne, Pearce, Tim, Mustill, Alexander J. 等 2025 置信度 0.66 Earth and Planetary Astrophysics (astro-ph.EP)Solar and Stellar Astrophysics (astro-ph.SR)FOS: Physical sciencesFOS: Physical sciences
• An on-sky investigation into factors limiting the performance of Keck-NIRC2 for conducting infrared high-contrast imaging
  The most common instrument used by the exoplanet/brown dwarf direct imaging community at the W.M. Keck Observatory is currently the NIRC2 near-infrared imager. We performed on-sky testing to investigate three effects which may be limiting the performance of NI…
  datacite Bowens-Rubin, Rachel, Salama, Maïssa, Nguyen, Jayke S., Thompson, William 等 2025 置信度 0.66 Instrumentation and Methods for Astrophysics (astro-ph.IM)FOS: Physical sciencesFOS: Physical sciences