nuance: Efficient detection of planets transiting active stars
Fuente:
arXiv
Guardado en:
| Autores principales: | Garcia, Lionel, Foreman-Mackey, Daniel, Murray, Catriona A., Aigrain, Suzanne, Feliz, Dax L., Pozuelos, Francisco J. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars
por: Klein, Baptiste, et al.
Publicado: (2025)
por: Klein, Baptiste, et al.
Publicado: (2025)
How do wavelength correlations affect transmission spectra? Application of a new fast and flexible 2D Gaussian process framework to transiting exoplanet spectroscopy
por: Fortune, Mark, et al.
Publicado: (2024)
por: Fortune, Mark, et al.
Publicado: (2024)
The influence of stellar activity on detecting Earth-like planets via nulling interferometry
por: Zhou, Rui-Si, et al.
Publicado: (2025)
por: Zhou, Rui-Si, et al.
Publicado: (2025)
Modelling stochastic and quasi-periodic behaviour in stellar time-series: Gaussian process regression versus power-spectrum fitting
por: O'Sullivan, Niamh K., et al.
Publicado: (2024)
por: O'Sullivan, Niamh K., et al.
Publicado: (2024)
A Gaussian process model for stellar activity in 2-D line profile time-series
por: Yu, Haochuan, et al.
Publicado: (2024)
por: Yu, Haochuan, et al.
Publicado: (2024)
The Goldilocks problem for detecting water in terrestrial planets: Constraining water abundances in the mid-IR with LIFE
por: Rugheimer, Sarah, et al.
Publicado: (2026)
por: Rugheimer, Sarah, et al.
Publicado: (2026)
Automatic search for transiting planets in TESS-SPOC FFIs with RAVEN: over 100 newly validated planets and over 2000 vetted candidates
por: Lafarga, M., et al.
Publicado: (2026)
por: Lafarga, M., et al.
Publicado: (2026)
Design, scientific goals, and performance of the SCExAO survey for planets around accelerating stars
por: Morsy, Mona El, et al.
Publicado: (2024)
por: Morsy, Mona El, et al.
Publicado: (2024)
sunset: A database of synthetic atmospheric-escape transmission spectra for nearly every transiting planet
por: Linssen, Dion, et al.
Publicado: (2024)
por: Linssen, Dion, et al.
Publicado: (2024)
Modelling stellar variability in archival HARPS data: I -- Rotation and activity properties with multi-dimensional Gaussian Processes
por: Yu, Haochuan, et al.
Publicado: (2024)
por: Yu, Haochuan, et al.
Publicado: (2024)
A multi-technique detection of an eccentric giant planet around accelerating star HD 57625
por: Barbato, D., et al.
Publicado: (2024)
por: Barbato, D., et al.
Publicado: (2024)
PLATO on the shoulders of TESS: analyzing mono-transit planet candidates in TESS data as a prior knowledge for PLATO observations
por: Magliano, Christian, et al.
Publicado: (2024)
por: Magliano, Christian, et al.
Publicado: (2024)
Prospects for the characterization of habitable planets
por: Mazevet, S., et al.
Publicado: (2023)
por: Mazevet, S., et al.
Publicado: (2023)
Long-period transiting exoplanets: advances in detection and characterization
por: Ulmer-Moll, Solène, et al.
Publicado: (2026)
por: Ulmer-Moll, Solène, et al.
Publicado: (2026)
Direct imaging characterization of cool gaseous planets
por: Min, Michiel, et al.
Publicado: (2025)
por: Min, Michiel, et al.
Publicado: (2025)
What is the maximum radius of cold planets?
por: Garfinkle, David, et al.
Publicado: (2025)
por: Garfinkle, David, et al.
Publicado: (2025)
Indirect forces in disc-planet interaction
por: Rafikov, Roman R., et al.
Publicado: (2025)
por: Rafikov, Roman R., et al.
Publicado: (2025)
Terrestrial planet formation in the era of GPU computing
por: Grimm, Simon L., et al.
Publicado: (2026)
por: Grimm, Simon L., et al.
Publicado: (2026)
CETRA: A fast, sensitive exoplanet transit detection algorithm implemented for GPUs
por: Smith, Leigh C., et al.
Publicado: (2025)
por: Smith, Leigh C., et al.
Publicado: (2025)
Inferring planet occurrence rates from radial velocities
por: Faria, J. P., et al.
Publicado: (2025)
por: Faria, J. P., et al.
Publicado: (2025)
The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems
por: Dévora-Pajares, Martín, et al.
Publicado: (2024)
por: Dévora-Pajares, Martín, et al.
Publicado: (2024)
AGNI: A radiative-convective model for lava planet atmospheres
por: Nicholls, Harrison, et al.
Publicado: (2025)
por: Nicholls, Harrison, et al.
Publicado: (2025)
Experiments reveal extreme water generation during planet formation
por: Miozzi, Francesca, et al.
Publicado: (2025)
por: Miozzi, Francesca, et al.
Publicado: (2025)
chemcomp: Modeling the chemical composition of planets formed in protoplanetary disks
por: Schneider, Aaron David, et al.
Publicado: (2023)
por: Schneider, Aaron David, et al.
Publicado: (2023)
Study of the atmospheric effects of energetic particle precipitations on giant planets with HWO
por: Chaufray, J-Y., et al.
Publicado: (2025)
por: Chaufray, J-Y., et al.
Publicado: (2025)
Unveiling habitable planets: Toy coronagraph tackles the exozodiacal dust challenge
por: Lin, Yu-Chia
Publicado: (2024)
por: Lin, Yu-Chia
Publicado: (2024)
The 3D Cosmic Shoreline for Nurturing Planetary Atmospheres
por: Berta-Thompson, Zach K., et al.
Publicado: (2025)
por: Berta-Thompson, Zach K., et al.
Publicado: (2025)
SPECULOOS: five years hunting terrestrial planets around ultra-cool dwarfs
por: Zúñiga-Fernández, Sebastián, et al.
Publicado: (2025)
por: Zúñiga-Fernández, Sebastián, et al.
Publicado: (2025)
The chemistry of star and planet formation with SKA
por: Codella, C., et al.
Publicado: (2024)
por: Codella, C., et al.
Publicado: (2024)
Predicting the detection yields of giant planets and brown dwarfs with CSST astrometry
por: Xuan, Yifan, et al.
Publicado: (2025)
por: Xuan, Yifan, et al.
Publicado: (2025)
Monte Carlo post-processing for radiation hydro simulations of accreting planets in protoplanetary disks
por: Krieger, Anton, et al.
Publicado: (2025)
por: Krieger, Anton, et al.
Publicado: (2025)
Observability of substructures in planet-forming disk in (sub)cm wavelength with SKA and ngVLA
por: Wu, Yinhao, et al.
Publicado: (2024)
por: Wu, Yinhao, et al.
Publicado: (2024)
DBNets2.0: simulation-based inference for planet-induced dust substructures in protoplanetary discs
por: Ruzza, A., et al.
Publicado: (2025)
por: Ruzza, A., et al.
Publicado: (2025)
Mercury-Opal: the GPU-accelerated version of the n-body code for planet formation Mercury-Arxes
por: Simonetti, Paolo, et al.
Publicado: (2026)
por: Simonetti, Paolo, et al.
Publicado: (2026)
Scalable Gaussian Processes for Integrated and Overlapping Measurements Via Augmented State Space Models
por: Rubenzahl, Ryan A., et al.
Publicado: (2026)
por: Rubenzahl, Ryan A., et al.
Publicado: (2026)
The NCORES Program: Precise planetary masses, null results, and insight into the planet mass distribution near the radius gap
por: Armstrong, David J., et al.
Publicado: (2025)
por: Armstrong, David J., et al.
Publicado: (2025)
Identifying rocky planets and water worlds among sub-Neptune-sized exoplanets with the Habitable Worlds Observatory
por: Hu, Renyu, et al.
Publicado: (2025)
por: Hu, Renyu, et al.
Publicado: (2025)
JWST-TST High Contrast: JWST/NIRCam observations of the young giant planet $β$ Pic b
por: Kammerer, Jens, et al.
Publicado: (2024)
por: Kammerer, Jens, et al.
Publicado: (2024)
Improving Earth-like planet detection in radial velocity using deep learning
por: Zhao, Yinan, et al.
Publicado: (2024)
por: Zhao, Yinan, et al.
Publicado: (2024)
Precise radial velocities of giant stars -- XVII. Distinguishing planets from intrinsically induced radial velocity signals in evolved stars
por: Spaeth, Dane, et al.
Publicado: (2025)
por: Spaeth, Dane, et al.
Publicado: (2025)
Ejemplares similares
-
Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars
por: Klein, Baptiste, et al.
Publicado: (2025) -
How do wavelength correlations affect transmission spectra? Application of a new fast and flexible 2D Gaussian process framework to transiting exoplanet spectroscopy
por: Fortune, Mark, et al.
Publicado: (2024) -
The influence of stellar activity on detecting Earth-like planets via nulling interferometry
por: Zhou, Rui-Si, et al.
Publicado: (2025) -
Modelling stochastic and quasi-periodic behaviour in stellar time-series: Gaussian process regression versus power-spectrum fitting
por: O'Sullivan, Niamh K., et al.
Publicado: (2024) -
A Gaussian process model for stellar activity in 2-D line profile time-series
por: Yu, Haochuan, et al.
Publicado: (2024)