Zobrazeno 1 - 10
of 1 957
pro vyhledávání: '"HENning, Thomas"'
Autor:
Mâlin, Mathilde, Boccaletti, Anthony, Perrot, Clément, Baudoz, Pierre, Rouan, Daniel, Lagage, Pierre-Olivier, Waters, Rens, Güdel, Manuel, Henning, Thomas, Vandenbussche, Bart, Absil, Olivier, Barrado, David, Charnay, Benjamin, Choquet, Elodie, Cossou, Christophe, Danielski, Camilla, Decin, Leen, Glauser, Adrian M., Pye, John, Olofsson, Goran, Glasse, Alistair, Patapis, Polychronis, Royer, Pierre, Scheithauer, Silvia, Serabyn, Eugene, Tremblin, Pascal, Whiteford, Niall, van Dishoeck, Ewine F., Ostlin, Göran, Ra, Tom P., Wright, Gillian
The newly accessible mid-infrared (MIR) window offered by the James Webb Space Telescope (JWST) for exoplanet imaging is expected to provide valuable information to characterize their atmospheres. In particular, coronagraphs on board the JWST Mid-Inf
Externí odkaz:
http://arxiv.org/abs/2501.00104
Autor:
Vlasblom, Marissa, Temmink, Milou, Grant, Sierra L., Kurtovic, Nicolas, Sellek, Andrew D., van Dishoeck, Ewine F., Güdel, Manuel, Henning, Thomas, Lagage, Pierre-Olivier, Barrado, David, Garatti, Alessio Caratti o, Glauser, Adrian M., Kamp, Inga, Lahuis, Fred, Olofsson, Göran, Arabhavi, Aditya M., Christiaens, Valentin, Gasman, Danny, Jang, Hyerin, Morales-Calderón, Maria, Perotti, Giulia, Schwarz, Kamber, Tabone, Benoît
Radial drift of icy pebbles can have a large impact on the chemistry of the inner regions of protoplanetary disks. Compact dust disks ($\lesssim$50 au) are suggested to have a higher (cold) H$_2$O flux than more extended disks, likely due to efficien
Externí odkaz:
http://arxiv.org/abs/2412.12715
Autor:
Ducrot, Elsa, Lagage, Pierre-Olivier, Min, Michiel, Gillon, Michael, Bell, Taylor J., Tremblin, Pascal, Greene, Thomas, Dyrek, Achrene, Bouwman, Jeroen, Waters, Rens, Gudel, Manuel, Henning, Thomas, Vandenbussche, Bart, Absil, Olivier, Barrado, David, Boccaletti, Anthony, Coulais, Alain, Decin, Leen, Edwards, Billy, Gastaud, Rene, Glasse, Alistair, Kendrew, Sarah, Olofsson, Goran, Patapis, Polychronis, Pye, John, Rouan, Daniel, Whiteford, Niall, Argyriou, Ioannis, Cossou, Christophe, Glauser, Adrian M., Krause, Oliver, Lahuis, Fred, Royer, Pierre, Scheithauer, Silvia, Colina, Luis, van Dishoeck, Ewine F., Ostlin, Goran, Ray, Tom P., Wright, Gillian
The first JWST/MIRI photometric observations of TRAPPIST-1 b allowed for the detection of the thermal emission of the planet at 15 $\mu m$, suggesting that the planet could be a bare rock with a zero albedo and no redistribution of heat. These observ
Externí odkaz:
http://arxiv.org/abs/2412.11627
Autor:
Vítková, Michaela, Brahm, Rafael, Trifonov, Trifon, Kabáth, Petr, Jordán, Andrés, Henning, Thomas, Hobson, Melissa J., Eberhardt, Jan, Pinto, Marcelo Tala, Rojas, Felipe I., Espinoza, Nestor, Schlecker, Martin, Jones, Matías I., Moyano, Maximiliano, Eyheramendy, Susana, Ziegler, Carl, Lissauer, Jack J., Vanderburg, Andrew, Collins, Karen A., Wohler, Bill, Watanabe, David, Ricker, George R., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Skarka, Marek
We present a joint analysis of TTVs and Doppler data for the transiting exoplanet system TOI-4504. TOI-4504 c is a warm Jupiter-mass planet that exhibits the largest known transit timing variations (TTVs), with a peak-to-node amplitude of $\sim$ 2 da
Externí odkaz:
http://arxiv.org/abs/2412.05609
Autor:
Martinez, Romy Rodriguez, Eastman, Jason D., Collins, Karen, Rodriguez, Joseph, Charbonneau, David, Quinn, Samuel, Latham, David W., Ziegler, Carl, Brahm, Rafael, Fairnington, Tyler, Ulmer-Moll, Solene, Stassun, Keivan, Suarez, Olga, Guillot, Tristan, Hobson, Melissa, Winn, Joshua N., Kanodia, Shubham, Schlecker, Martin, Butler, R. P., Crane, Jeffrey D., Shectman, Steve, Teske, Johanna K., Osip, David, Beletsky, Yuri, Battley, Matthew P., Psaridi, Angelica, Figueira, Pedro, Lendl, Monika, Bouche, Francois, Udry, Stephane, Kunimoto, Michelle, Mekarnia, Dejamel, Abe, Lyu, Trifonov, Trifonov, Pinto, Marcelo T., Eberhardt, Jan, Espinoza, Nestor, Henning, Thomas, Jordan, Andres, Rojas, Felipe I., Barkaoui, Khalid, Relles, Howard M., Srdoc, Gregor, Collins, Kevin I., Seager, Sara, Shporer, Avi, Vezie, Michael, Hedges, Christina L., Mireles, Ismael
We present the detection and characterization of TOI-4994b (TIC 277128619b), a warm Saturn-sized planet discovered by the NASA Transiting Exoplanet Survey Satellite (TESS). TOI-4994b transits a G-type star (V = 12.6 mag) with a mass, radius, and effe
Externí odkaz:
http://arxiv.org/abs/2412.02769
Autor:
Pinto, Marcelo Tala, Jordán, Andrés, Acuña, Lorena, Jones, Matías, Brahm, Rafael, Reinarz, Yared, Eberhardt, Jan, Espinoza, Néstor, Henning, Thomas, Hobson, Melissa, Rojas, Felipe, Schlecker, Martin, Trifonov, Trifon, Bakos, Gaspar, Boyle, Gavin, Csubry, Zoltan, Hartmann, Joel, Knepper, Benjamin, Kreidberg, Laura, Suc, Vincent, Teske, Johanna, Butler, R. Paul, Crane, Jeffrey, Schectman, Steve, Thompson, Ian, Osip, Dave, Ricker, George, Collins, Karen A., Watkins, Cristilyn N., Bieryla, Allyson, Stockdale, Chris, Wang, Gavin, Zambelli, Roberto, Seager, Sara, Winn, Joshua, Rose, Mark E., Rice, Malena, Essack, Zahra
We report the discovery and characterization of three new transiting giant planets orbiting TOI-6628, TOI-3837 and TOI-5027, and one new warm sub-Saturn orbiting TOI-2328, whose transits events were detected in the lightcurves of the Transiting Exopl
Externí odkaz:
http://arxiv.org/abs/2412.02069
Autor:
Nozari, Parisa, Sadavoy, Sarah, Chapillon, Edwige, Mason, Brian, Friesen, Rachel, Lowe, Ian, Stanke, Thomas, Di Francesco, James, Henning, Thomas, Zhang, Qizhou, Stutz, Amelia
It is widely assumed that dust opacities in molecular clouds follow a power-law profile with an index, $\beta$. Recent studies of the Orion Molecular Cloud (OMC) 2/3 complex, however, show a flattening in the spectral energy distribution (SED) at $ \
Externí odkaz:
http://arxiv.org/abs/2411.12693
Autor:
Liu, Yao, Roussel, Hélène, Linz, Hendrik, Fang, Min, Wolf, Sebastian, Kirchschlager, Florian, Henning, Thomas, Yang, Haifeng, Du, Fujun, Flock, Mario, Wang, Hongchi
Publikováno v:
A&A 692, A148 (2024)
ALMA surveys have suggested that protoplanetary disks are not massive enough to form the known exoplanet population, under the assumption that the millimeter continuum emission is optically thin. In this work, we investigate how the mass determinatio
Externí odkaz:
http://arxiv.org/abs/2411.00277
Autor:
Saunders, Nicholas, Grunblatt, Samuel K., Huber, Daniel, Ong, J. M. Joel, Schlaufman, Kevin C., Hey, Daniel, Li, Yaguang, Butler, R. P., Crane, Jeffrey D., Shectman, Steve, Teske, Johanna K., Quinn, Samuel N., Yee, Samuel W., Brahm, Rafael, Trifonov, Trifon, Jordán, Andrés, Henning, Thomas, Sing, David K., MacGregor, Meredith, Page, Emma, Rapetti, David, Falk, Ben, Levine, Alan M., Huang, Chelsea X., Lund, Michael B., Ricker, George R., Seager, S., Winn, Joshua N., Jenkins, Jon M.
We present the discovery of TOI-7041 b (TIC 201175570 b), a hot Saturn transiting a red giant star with measurable stellar oscillations. We observe solar-like oscillations in TOI-7041 with a frequency of maximum power of $\nu_{\rm max} = 218.50\pm2.2
Externí odkaz:
http://arxiv.org/abs/2410.11037
Autor:
Ricciardi, Giulia, van Terwisga, Sierk E., Roccatagliata, Veronica, Hacar, Alvaro, Henning, Thomas, Del Pozzo, Walter
Aims. The goal of this work is to comprehensively characterize the impact of stellar multiplicity on Class II disks in the L1641 and L1647 regions of Orion A (~1-3 Myr), part of the Survey of Orion Disks with ALMA (SODA). We characterize the protoste
Externí odkaz:
http://arxiv.org/abs/2409.11485