Zobrazeno 1 - 10
of 1 726
pro vyhledávání: '"Jensen, Eric A"'
Autor:
Christian, Sam, Vanderburg, Andrew, Becker, Juliette, Kraus, Adam L., Pearce, Logan, Collins, Karen A., Rice, Malena, Jensen, Eric L. N., Baker, David, Benni, Paul, Bieryla, Allyson, Binnenfeld, Abraham, Collins, Kevin I., Conti, Dennis M., Evans, Phil, Girardin, Eric, Gregorio, Joao, Mazeh, Tsevi, Murgas, Felipe, Panahi, Aviad, Pozuelos, Francisco J., Relles, Howard M., Frustaglia, Fabian Rodriguez, Schwarz, Richard P., Srdoc, Gregor, Stockdale, Chris, Tan, Thiam-Guan, Waalkes, William C., Wang, Gavin, Wittrock, Justin, Zucker, Shay
Studying the relative orientations of the orbits of exoplanets and wide-orbiting binary companions (semimajor axis greater than 100 AU) can shed light on how planets form and evolve in binary systems. Previous observations by multiple groups discover
Externí odkaz:
http://arxiv.org/abs/2405.10379
Autor:
Tofflemire, Benjamin M., Prato, Lisa, Kraus, Adam L., Segura-Cox, Dominique, Schaefer, G. H., Akeson, Rachel, Andrews, Sean, Jensen, Eric L. N., Johns-Krull, Christopher M., Zanazzi, J. J., Simon, M.
Close binary systems present challenges to planet formation. As binary separations decrease, so too do the occurrence rates of protoplanetary disks in young systems and planets in mature systems. For systems that do retain disks, their disk masses an
Externí odkaz:
http://arxiv.org/abs/2403.13045
Autor:
Harris, Mallory, Dragomir, Diana, Mireles, Ismael, Collins, Karen A., Ulmer-Moll, Solène, Howell, Steve B., Stassun, Keivan G., Zhou, George, Ziegler, Carl, Bouchy, François, Briceño, César, Charbonneau, David, Collins, Kevin I., Fűűrész, Gábor, Guerrero, Natalia M., Jenkins, Jon M., Jensen, Eric L. N., Kristiansen, Martti H. K., Law, Nicholas, Lendl, Monika, Mann, Andrew W., Osborn, Hugh P., Quinn, Samuel N., Ricker, George R., Schwarz, Richard P., Seager, Sara, Ting, Eric B., Vanderspek, Roland, Watanabe, David, Winn, Joshua N.
We report the discovery of two TESS sub-Neptunes orbiting the early M dwarf TOI-904 (TIC 261257684). Both exoplanets, TOI-904 b and c, were initially observed in TESS sector 12 with twin sizes of 2.49R$_\oplus$ and 2.31R$_\oplus$, respectively. Throu
Externí odkaz:
http://arxiv.org/abs/2310.15118
Autor:
Wang, Jia-Qi, Jiang, Xiao-Jun, Zheng, Jie, Kellermann, Hanna, Riffeser, Arno, Wang, Liang, Collins, Karen A., Bieryla, Allyson, Buchhave, Lars A., Howell, Steve B., Furlan, Elise, Girardin, Eric, Gregorio, Joao, Jensen, Eric, Murgas, Felipe, Yilmaz, Mesut, Quinn, Sam, Gao, Xing, Zhou, Ruo-Yu, Grupp, Frank, Wang, Hui-Juan
We report the confirmation of a sub-Saturn-size exoplanet, TOI-1194 b with a mass about $0.456_{-0.051}^{+0.055}$ $M_{J}$, and a very low mass companion star with a mass of about $96.5\pm1.5$ $M_J$, TOI-1251 B. Exoplanet candidates provided by the Tr
Externí odkaz:
http://arxiv.org/abs/2310.12458
Autor:
Zhang, Jingwen, Weiss, Lauren M., Huber, Daniel, Jensen, Eric L. N., Brandt, Timothy D., Collins, Karen, Conti, Dennis M., Isaacson, Howard, Lewin, Pablo, Marino, Giuseppe, Massey, Bob, Murgas, Felipe, Palle, Enric, Radford, Don J., Relles, Howard M., Srdoc, Gregor, Stockdale, Chris, Tan, Thiam-Guan, Wang, Gavin
Publikováno v:
AJ, 167, 8 (2024)
The effect of stellar multiplicity on planetary architecture and orbital dynamics provides an important context for exoplanet demographics. We present a volume-limited catalog up to 300 pc of 66 stars hosting planets and planet candidates from Kepler
Externí odkaz:
http://arxiv.org/abs/2310.03299
Autor:
Kaye, Laurel, Vissapragada, Shreyas, Gunther, Maximilian N., Aigrain, Suzanne, Mikal-Evans, Thomas, Jensen, Eric L. N., Parviainen, Hannu, Pozuelos, Francisco J., Abe, Lyu, Acton, Jack S., Agabi, Abdelkrim, Alves, Douglas R., Anderson, David R., Armstrong, David J., Barkaoui, Khalid, Barragan, Oscar, Benneke, Bjorn, yd, Patricia T. Bo, Brahm, Rafael, Bruni, Ivan, Bryant, Edward M., Burleigh, Matthew R., Casewell, Sarah L., Ciardi, David, Cloutier, Ryan, Collins, Karen A., Collins, Kevin I., Conti, Dennis M., Crossfield, Ian J. M., Crouzet, Nicolas, Daylan, Tansu, Dragomir, Diana, Dransfield, Georgina, abrycky, Daniel F, Fausnaugh, Michael, Fuuresz, Gabor, Gan, Tianjun, Gill, Samuel, Gillon, Michael, Goad, Michael R, Gorjian, Varoujan, Greklek-McKeon, Michael, Guerrero, Natalia, Guillot, Tristan, Jehin, Emmanuel, Jenkins, J. S., Lendl, Monika, Kamler, Jacob, Kane, Stephen R., Kielkopf, John F., Kunimoto, Michelle, Marie-Sainte, Wenceslas, McCormac, James, Mekarnia, Djamel, Morales, Farisa Y., Moyano, Maximiliano, Palle, Enric, Parmentier, Vivien, Relles, Howard M., Schmider, Francois-Xavier, Schwarz, Richard P., Seager, S., Smith, Alexis M. S., Tan, Thiam-Guan, Taylor, Jake, Triaud, Amaury H. M. J., Twicken, Joseph D., Udry, Stephane, Vines, J. I., Wang, Gavin, Wheatley, Peter J., Winn, Joshua N.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 510, Issue 4, pp.5464-5485 (2022)
We present ground and space-based photometric observations of TOI-270 (L231-32), a system of three transiting planets consisting of one super-Earth and two sub-Neptunes discovered by TESS around a bright (K-mag=8.25) M3V dwarf. The planets orbit near
Externí odkaz:
http://arxiv.org/abs/2308.10763
Autor:
Hord, Benjamin J., Kempton, Eliza M. -R., Mikal-Evans, Thomas, Latham, David W., Ciardi, David R., Dragomir, Diana, Colón, Knicole D., Ross, Gabrielle, Vanderburg, Andrew, de Beurs, Zoe L., Collins, Karen A., Watkins, Cristilyn N., Bean, Jacob, Cowan, Nicolas B., Daylan, Tansu, Morley, Caroline V., Ih, Jegug, Baker, David, Barkaoui, Khalid, Batalha, Natalie M., Behmard, Aida, Belinski, Alexander, Benkhaldoun, Zouhair, Benni, Paul, Bernacki, Krzysztof, Bieryla, Allyson, Binnenfeld, Avraham, Bosch-Cabot, Pau, Bouchy, François, Bozza, Valerio, Brahm, Rafael, Buchhave, Lars A., Calkins, Michael, Chontos, Ashley, Clark, Catherine A., Cloutier, Ryan, Cointepas, Marion, Collins, Kevin I., Conti, Dennis M., Crossfield, Ian J. M., Dai, Fei, de Leon, Jerome P., Dransfield, Georgina, Dressing, Courtney, Dustor, Adam, Esquerdo, Gilbert, Evans, Phil, Fajardo-Acosta, Sergio B., Fiołka, Jerzy, Forés-Toribio, Raquel, Frasca, Antonio, Fukui, Akihiko, Fulton, Benjamin, Furlan, Elise, Gan, Tianjun, Gandolfi, Davide, Ghachoui, Mourad, Giacalone, Steven, Gilbert, Emily A., Gillon, Michaël, Girardin, Eric, Gonzales, Erica, Horta, Ferran Grau, Gregorio, Joao, Greklek-McKeon, Michael, Guerra, Pere, Hartman, J. D., Hellier, Coel, Hełminiak, Krzysztof G., Henning, Thomas, Hill, Michelle L., Horne, Keith, Howard, Andrew W., Howell, Steve B., Huber, Daniel, Isaacson, Howard, Isopi, Giovanni, Jehin, Emmanuel, Jenkins, Jon M., Jensen, Eric L. N., Johnson, Marshall C., Jordán, Andrés, Kane, Stephen R., Kielkopf, John F., Krushinsky, Vadim, Lasota, Sławomir, Lee, Elena, Lewin, Pablo, Livingston, John H., Lubin, Jack, Lund, Michael B., Mallia, Franco, Mann, Christopher R., Marino, Giuseppe, Maslennikova, Nataliia, Massey, Bob, Matson, Rachel, Matthews, Elisabeth, Mayo, Andrew W., Mazeh, Tsevi, McLeod, Kim K., Michaels, Edward J., Močnik, Teo, Mori, Mayuko, Mraz, Georgia, Muñoz, Jose A., Narita, Norio, Nielsen, Louise Dyregaard, Osborn, Hugh, Palle, Enric, Panahi, Aviad, Papini, Riccardo, Polanski, Alex S., Popowicz, Adam, Pozuelos, Francisco J., Quinn, Samuel N., Radford, Don J., Reed, Phillip A., Relles, Howard M., Rice, Malena, Robertson, Paul, Rodriguez, Joseph E., Rosenthal, Lee J., Rubenzahl, Ryan A., Schanche, Nicole, Schlieder, Joshua, Schwarz, Richard P., Sefako, Ramotholo, Shporer, Avi, Sozzetti, Alessandro, Srdoc, Gregor, Stockdale, Chris, Tarasenkov, Alexander, Tan, Thiam-Guan, Timmermans, Mathilde, Ting, Eric B., Van Zandt, Judah, Vignes, JP, Waite, Ian, Watanabe, Noriharu, Weiss, Lauren M., Wittrock, Justin, Zhou, George, Ziegler, Carl, Zucker, Shay
JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates are still unconfirmed and many of the best planets for atmospheric char
Externí odkaz:
http://arxiv.org/abs/2308.09617
We report the analysis of circumbinary discs formed in a radiation hydrodynamical simulation of star cluster formation. We consider both pure binary stars and pairs within triple and quadruple systems. The protostellar systems are all young (ages < $
Externí odkaz:
http://arxiv.org/abs/2306.06035
Autor:
Osborn, Hugh P., Nowak, Grzegorz, Hébrard, Guillaume, Masseron, Thomas, Lillo-Box, J., Pallé, Enric, Bekkelien, Anja, Florén, Hans-Gustav, Guterman, Pascal, Simon, Attila E., Adibekyan, V., Bieryla, Allyson, Borsato, Luca, Brandeker, Alexis, Ciardi, David R., Cameron, Andrew Collier, Collins, Karen A., Egger, Jo A., Gandolfi, Davide, Hooton, Matthew J., Latham, David W., Lendl, Monika, Matthews, Elisabeth C., Tuson, Amy, Ulmer-Moll, Solène, Vanderburg, Andrew, Wilson, Thomas G., Ziegler, Carl, Alibert, Yann, Alonso, Roi, Anglada, Guillem, Arnold, Luc, Asquier, Joel, Navascues, David Barrado y, Baumjohann, Wolfgang, Beck, Thomas, Belinski, Alexandr A., Benz, Willy, Biondi, Federico, Boisse, Isabelle, Bonfils, Xavier, Broeg, Christopher, Buchhave, Lars A., Bárczy, Tamas, Barros, S. C. C., Cabrera, Juan, Guillen, Carlos Cardona, Carleo, Ilaria, Castro-González, Amadeo, Charnoz, Sébastien, Christiansen, Jessie, Cortes-Zuleta, Pia, Csizmadia, Szilard, Dalal, Shweta, Davies, Melvyn B., Deleuil, Magali, Delfosse, Xavier, Delrez, Laetitia, Demory, Brice-Olivier, Dunlavey, Ava B., Ehrenreich, David, Erikson, Anders, Fernandes, Rachel B., Fortier, Andrea, Forveille, Thierry, Fossati, Luca, Fridlund, Malcolm, Gillon, Michaël, Goeke, Robert F., Goliguzova, Maria V., Gonzales, Erica J., Günther, M. N., Güdel, Manuel, Heidari, Neda, Henze, Christopher E., Howell, Steve, Hoyer, Sergio, Frey, Jonas Immanuel, Isaak, Kate G., Jenkins, Jon M., Kiefer, Flavien, Kiss, Laszlo, Korth, Judith, Maxted, Pierre F. L., Laskar, Jacques, Etangs, Alain Lecavelier des, Lovis, Christophe, Lund, Michael B., Luque, Rafa, Magrin, Demetrio, Almenara, Jose Manuel, Martioli, Eder, Mecina, Marko, Medina, Jennifer V., Moldovan, Daniel, Morales-Calderón, María, Morello, Giuseppe, Moutou, Claire, Murgas, Felipe, Jensen, Eric L. N., Nascimbeni, Valerio, Olofsson, Göran, Ottensamer, Roland, Pagano, Isabella, Peter, Gisbert, Piotto, Giampaolo, Pollacco, Don, Queloz, Didier, Ragazzoni, Roberto, Rando, Nicola, Rauer, Heike, Ribas, Ignasi, Ricker, George, Demangeon, Olivier D. S., Smith, Alexis M. S., Santos, Nuno, Scandariato, Gaetano, Seager, Sara, Sousa, Sergio G., Steller, Manfred, Szabó, Gyula M., Ségransan, Damien, Thomas, Nicolas, Udry, Stéphane, Ulmer, Bernd, Van Grootel, Valerie, Vanderspek, Roland, Walton, Nicholas, Winn, Joshua N.
Publikováno v:
MNRAS, Vol. 523, 2023, issue 2, pp 3069-3089
HIP 9618 (HD 12572, TOI-1471, TIC 306263608) is a bright ($G=9.0$ mag) solar analogue. TESS photometry revealed the star to have two candidate planets with radii of $3.9 \pm 0.044$ $R_\oplus$ (HIP 9618 b) and $3.343 \pm 0.039$ $R_\oplus$ (HIP 9618 c)
Externí odkaz:
http://arxiv.org/abs/2306.04450
Autor:
Page, Emma, Pepper, Joshua, Wright, Duncan, Rodriguez, Joseph E., Wittenmyer, Robert A., Kane, Stephen R., Addison, Brett, Bedding, Timothy, Bowler, Brendan P., Barclay, Thomas, Collins, Karen A., Evans, Phil, Horner, Jonathan, Jensen, Eric L. N., Johnson, Marshall C., Kielkopf, John, Mireles, Ismael, Plavchan, Peter, Quinn, Samuel N., Seager, S., Stassun, Keivan G., Striegel, Stephanie, Winn, Joshua N., Zhou, George, Ziegler, Carl
We present the discovery of TOI-1994b, a low-mass brown dwarf transiting a hot subgiant star on a moderately eccentric orbit. TOI-1994 has an effective temperature of $7700^{+720}_{-410}$ K, V magnitude of 10.51 mag and log(g) of $3.982^{+0.067}_{-0.
Externí odkaz:
http://arxiv.org/abs/2305.08836