Results 21 to 30 of about 9,374,373 (212)
Exoplanets prediction in multiplanetary systems [PDF]
Publications of the Astronomical Society of Australia, 2021 AbstractWe present the results of a search for additional exoplanets in all multiplanetary systems discovered to date, employing a logarithmic spacing between planets in our Solar System known as the Titius–Bode (TB) relation. We use the Markov Chain Monte Carlo method and separately analyse 229 multiplanetary systems that house at least three or more ...M. Mousavi-Sadr, G. Gozaliasl, D.M. Jassur +2 moreopenaire +3 more sourcesexoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series [PDF]
, 2021 What's Changed
Adding test and fixing deprecated unit parameters by @dfm in https://github.com/exoplanet-dev/exoplanet/pull/211
Removing old ValueError in Keplerian orbit that should never be hit by @dfm in https://github.com/exoplanet-dev/exoplanet ...Savel, Arjun, Morris, Brett M., Bouma, Luke G., Luger, Rodrigo, Brandt, Timothy D., Hey, Daniel R., Gilbert, Emily, David, Trevor, Agol, Eric, Savel, Arjun B., Hey, Daniel, Foreman-Mackey, Daniel, Bouma, Luke, Price-Whelan, Adrian, Gordon, Tyler A., Barclay, Thomas, Brandt, Timothy, Morris, Brett, Czekala, Ian, Gilbert, Emily A., David, Trevor J., Dong, Jiayin, Price-Whelan, Adrian M., Hedges, Christina, Gordon, Tyler, Czekala, Ian; id_orcid, Tyler Gordon, Eric Agol, Ian Czekala, Brett Morris, Christina Hedges, Jiayin Dong, Daniel Foreman-Mackey, Emily Gilbert, Daniel Hey, Luke Bouma, Adrian Price-Whelan, Arjun Savel, Thomas Barclay, Trevor David, Timothy Brandt, Rodrigo Luger +41 morecore +2 more sourcesIs there an exoplanet in the Solar system? [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2016 Abstract We investigate the prospects for the capture of the proposed Planet 9 from other stars in the Sun's birth cluster. Any capture scenario must satisfy three conditions: the encounter must be more distant than ∼150 au to avoid perturbing the Kuiper belt; the other star must have a wide-orbit planet (a ≳ 100 au); the planet must be ...Mustill, Alexander J.,, Raymond, Sean N., Davies, Melvyn B., +2 moreopenaire +3 more sourcesThe Science of Exoplanets and Their Systems [PDF]
Astrobiology, 2013 A scientific forum on "The Future Science of Exoplanets and Their Systems," sponsored by Europlanet and the International Space Science Institute (ISSI) and co-organized by the Center for Space and Habitability (CSH) of the University of Bern, was held during December 5 and 6, 2012, in Bern, Switzerland.Lammer, Helmut, Blanc, Michel, Benz, Willy, Fridlund, Malcolm, Foresto, Vincent Coudé Du, Güdel, Manuel, Rauer, Heike, Udry, Stephane, Bonnet, Roger-Maurice, Falanga, Maurizio, Charbonneau, David, Helled, Ravit, Kley, Willy, Linsky, Jeffrey, Elkins-Tanton, Linda T., Alibert, Yann, Chassefière, Eric, Encrenaz, Therese, Hatzes, Artie P., Lin, Douglas, Liseau, Rene, Lorenzen, Winfried, Raymond, Sean N. +22 moreopenaire +7 more sourcesAnalysis of the exoplanet containing system Kepler-91 [PDF]
Astrophysics and Space Science, 2015 We have applied the graphical user interfaced close binary system analysis program WinFitter to an intensive study of Kepler 91 using all the available photometry from the NASA Exoplanet Archive (NEA) at the Caltech website: http://exoplanetarchive.ipac.caltech.edu . Our fitting function for the tidal distortion derives from the relevant Radau equation Budding, E., Püsküllü, Ç., Demircan, O., Rhodes, M., Budding, Edwin, Püsküllü, Çağlar, Rhodes, Michael, Demircan, Osman, Erdem, A., Erdem, Ahmet +9 moreopenaire +7 more sourcesPLANETESIMAL COMPOSITIONS IN EXOPLANET SYSTEMS [PDF]
The Astrophysical Journal, 2012 We have used recent surveys of the composition of exoplanet host stars to investigate the expected composition of condensed material in planetesimals formed beyond the snow line in the circumstellar nebulae of these systems. Of the major solid forming elements, we find that, as for the Sun, the C and O abundances (and particularly the C/O abundance ...Johnson, T.V., Mousis, O., Lunine, J.I., Madhusdhan, N. +3 moreopenaire +3 more sourcesexoplanet-dev/exoplanet: exoplanet v0.4.5
, 2021 0.5.0 (2021-05-04)
Adds high-level, pure-Theano/Aesara implementation of RegularGridInterpolator to replace compiled version #167
Moves compiled Ops to exoplanet-core making exoplanet a pure-Python package #171
Moves ReboundOp and ReboundOrbit to ...emilygilbert, Dan Foreman-Mackey, Eric Agol, Christina Hedges, Tom Barclay, Ian Czekala, Luke Bouma, Rodrigo Luger, Adrian Price-Whelan, Timothy D Brandt, Arjun Savel +10 morecore +1 more sourceExoplanet imaging data challenge: benchmarking the various image processing methods for exoplanet detection [PDF]
, 2020 The Exoplanet Imaging Data Challenge is a community-wide effort meant to offer a platform for a fair and common comparison of image processing methods designed for exoplanet direct detection. For this purpose, it gathers on a dedicated repository (Zenodo)Desgrange, Célia, Schreiber, Laura, Bonse, M. J., Bonse, Markus Johannes, Fuhrmann, T., Cantalloube, Faustine, Dino Mesa, Kenworthy, M., Samland, Matthias, Nasedkin, E., Ruffio, J.-B., Henning, Th., Tiffany Meshkat, Bonse, Markus, Jensen-Clem, R., André Müller, Sébastien Piérard, Schmidt, Dirk, Marc Van Droogenbroeck, Michael Bottom, Regis Bacher, Henning, Thomas H., Flasseur, O., Adaptive Optics Systems VII, Kenworthy, Matthew, Jean-Baptiste Ruffio, Bottom, Michael, Desgrange, C., Célia Desgrange, Mawet, D., Absil, Olivier, Pairet, Benoit, Müller, Andreas, Cantero Mitjans, Carles, Markus Bonse, Benoit Pairet, Bottom, M., Müller, A., Bacher, Raphael, Van Droogenbroeck, Marc, Stone, Jordan, Stone, J., Fuhrmann, Thomas, Mouillet, David, Samland, M., Flasseur, Olivier, Cantero, Carles, Henning, Thomas, Jensen-Clem, Rebecca, Ruffio, Jean-Baptiste, Piérard, Sébastien, Müller, André, Mouillet, D., Meshkat, T., Mesa, Dino, Vernet, Elise, Gomez Gonzalez, Carlos, Olivier Absil, Carles Cantero, Meshkat, Tiffany, Pairet, B., Cantalloube, F., Mesa, D., Bacher, Regis, Carl-Henrik Dahlqvist, Matthias Samland, Thomas H. Henning, Gomez-Gonzalez, Carlos, Dahlqvist, Carl-Henrik, Faustine Cantalloube, Matthew Kenworthy, Bacher, R., Nasedkin, Evert, Carlos Gomez-Gonzalez, Olivier Flasseur, Thomas Fuhrmann, Rebecca Jensen-Clem, Evert Nasedkin, Dimitri Mawet, Mawet, Dimitri, Jordan Stone, David Mouillet +81 morecore +1 more sourceCorrelations between the stellar, planetary, and debris components of exoplanet systems observed by Herschel [PDF]
, 2014 J.P.M., C.E., J.M. and B.M. are partially supported by Spanish grant AYA 2011-26202. This work was supported by the European Union through ERC grant number no.Lestrade, J.-F., Olofsson, G., G. Olofsson, G. Bryden, C. Eiroa, Horner, J., Eiroa, C., J. Sanz-Forcada, Meeus, G., Pilbratt, G.L., Moro-Martin, Amaya, Lestrade, J. -F., Meeus, Gwendolyn, White, G.J., Olofsson, Goran, Kennedy, G., Ivison, R. J., A. Moro-Martín, Sanz-Forcada, J., Wyatt, M.C., G. Meeus, Lestrade, J-E, J. P. Marshall, Ivison, Robert J., Marshall, J.P., Greaves, J. S., J. S. Greaves, Eiroa, Carlos, J. Horner, Greaves, J.S., G. Kennedy, Maldonado, J., R. J. Ivison, Sibthorpe, B., White, Glenn J., Wyatt, Mark C., Wyatt, M. C., Matthews, B., Del Burgo, C., Moro-Martín, A., Montesinos, B., Kennedy, G. M., J.-F. Lestrade, del Burgo, Carlos, J. Maldonado, Pilbratt, G. L., Olofsson, Göran,, Bryden, G., B. Sibthorpe, Marshall, J. P., Forcada, Jorge Sanz, White, G. J., Mora, A., B. Matthews, B. Montesinos, Maldonado, Jesús, C. del Burgo, Ivison, R.J., G. L. Pilbratt, M. C. Wyatt, Lestrade, Jean-François, Matthews, B. C., A. Mora, G. J. White, Horner, Jonathan, Lestrade J, Wyatt MC, Ivison RJ, Eiroa C, Olofsson G, White GJ, Marshall JP, del Burgo C, Kennedy G, Maldonado J, Meeus G, Matthews B, Bryden G, Sibthorpe B, Montesinos B, Sanz-Forcada J, Pilbratt GL, Horner J, Mora A, Greaves JS, Moro-Martín A +85 morecore +1 more sourceTesting exoplanet evaporation with multitransiting systems [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 ABSTRACT The photoevaporation model is one of the leading explanations for the evolution of small, close-in planets and the origin of the radius-valley. However, without planet mass measurements, it is challenging to test the photoevaporation scenario. Even if masses are available for individual planets, the host star’s unknown EUV/X-ray Owen, JE, Estrada, BCopenaire +3 more sources