Zobrazeno 1 - 10
of 87
pro vyhledávání: '"Rose, Mark E."'
Autor:
Giovinazzi, Mark R., Cale, Bryson, Eastman, Jason D., Rodriguez, Joseph E., Blake, Cullen H., Stassun, Keivan G., Beatty, Thomas G., McCrady, Nate, Vanderburg, Andrew, Kunimoto, Michelle, Kraus, Adam L., Twicken, Joseph, Dedrick, Cayla M., Horner, Jonathan, Johnson, John A., Johnson, Samson A., Plavchan, Peter, Sliski, David H., Wilson, Maurice L., Wittenmyer, Robert A., Wright, Jason T., Johnson, Marshall C., Rose, Mark E., Cornachione, Matthew
We present a new analysis of the KELT-24 system, comprising a well-aligned hot Jupiter, KELT-24~b, and a bright ($V=8.3$), nearby ($d=96.9~\mathrm{pc}$) F-type host star. KELT-24~b was independently discovered by two groups in 2019, with each reporti
Externí odkaz:
http://arxiv.org/abs/2406.04288
Autor:
Kunimoto, Michelle, Vanderburg, Andrew, Huang, Chelsea X., Davis, M. Ryleigh, Affer, Laura, Cameron, Andrew Collier, Charbonneau, David, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martnez, Ghedina, Adriano, Haywood, R. D., Lienhard, Florian, López-Morales, Mercedes, Mayor, Michel, Pepe, Francesco, Pinamonti, Matteo, Poretti, Ennio, Maldonado, Jesús, Rice, Ken, Sozzetti, Alessandro, Wilson, Thomas G., Udry, Stéphane, Baptista, Jay, Barkaoui, Khalid, Becker, Juliette, Benni, Paul, Bieryla, Allyson, Bosch-Cabot, Pau, Ciardi, David R., Collins, Karen A., Collins, Kevin I., Evans, Elise, Dupuy, Trent J., Goliguzova, Maria V., Guerra, Pere, Kraus, Adam, Lissauer, Jack J., Huber, Daniel, Murgas, Felipe, Palle, Enric, Quinn, Samuel N., Safonov, Boris S., Schwarz, Richard P., Shporer, Avi, Stassun, Keivan G., Jenkins, Jon M., Latham, David W., Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua, Essack, Zahra, Lewis, Hannah M., Rose, Mark E.
Publikováno v:
AJ, 166, 7 (2023)
We report the confirmation of three exoplanets transiting TOI-4010 (TIC-352682207), a metal-rich K dwarf observed by TESS in Sectors 24, 25, 52, and 58. We confirm these planets with HARPS-N radial velocity observations and measure their masses with
Externí odkaz:
http://arxiv.org/abs/2306.05308
Autor:
Sha, Lizhou, Vanderburg, Andrew M., Huang, Chelsea X., Armstrong, David J., Brahm, Rafael, Giacalone, Steven, Wood, Mackenna L., Collins, Karen A., Nielsen, Louise D., Hobson, Melissa J., Ziegler, Carl, Howell, Steve B., Torres-Miranda, Pascal, Mann, Andrew W., Zhou, George, Delgado-Mena, Elisa, Rojas, Felipe I., Abe, Lyu, Trifonov, Trifon, Adibekyan, Vardan, Sousa, Sérgio G., Fajardo-Acosta, Sergio B., Guillot, Tristan, Howard, Saburo, Littlefield, Colin, Hawthorn, Faith, Schmider, François-Xavier, Eberhardt, Jan, Tan, Thiam-Guan, Osborn, Ares, Schwarz, Richard P., Strøm, Paul, Jordán, Andrés, Wang, Gavin, Henning, Thomas, Massey, Bob, Law, Nicholas, Stockdale, Chris, Furlan, Elise, Srdoc, Gregor, Wheatley, Peter J., Navascués, David Barrado, Lissauer, Jack J., Stassun, Keivan G., Ricker, George R., Vanderspek, Roland K., Latham, David W., Winn, Joshua N., Seager, Sara, Jenkins, Jon M., Barclay, Thomas, Bouma, Luke G., Christiansen, Jessie L., Guerrero, Natalia, Rose, Mark E.
Hot jupiters (P < 10 d, M > 60 $\mathrm{M}_\oplus$) are almost always found alone around their stars, but four out of hundreds known have inner companion planets. These rare companions allow us to constrain the hot jupiter's formation history by ruli
Externí odkaz:
http://arxiv.org/abs/2209.14396
Autor:
Giacalone, Steven, Dressing, Courtney D., Hedges, Christina, Kostov, Veselin B., Collins, Karen A., Jensen, Eric L. N., Yahalomi, Daniel A., Bieryla, Allyson, Ciardi, David R., Howell, Steve B., Lillo-Box, Jorge, Barkaoui, Khalid, Winters, Jennifer G., Matthews, Elisabeth, Livingston, John H., Quinn, Samuel N., Safonov, Boris S., Cadieux, Charles, Furlan, E., Crossfield, Ian J. M., Mandell, Avi M., Gilbert, Emily A., Kruse, Ethan, Quintana, Elisa V., Ricker, George R., Seager, S., Winn, Joshua N., Jenkins, Jon M., Adkins, Britt Duffy, Baker, David, Barclay, Thomas, Barrado, David, Batalha, Natalie M., Belinski, Alexander A., Benkhaldoun, Zouhair, Buchhave, Lars A., Cacciapuoti, Luca, Charbonneau, David, Chontos, Ashley, Christiansen, Jessie L., Cloutier, Ryan, Collins, Kevin I., Conti, Dennis M., Cutting, Neil, Dixon, Scott, Doyon, René, Mufti, Mohammed El, Esparza-Borges, Emma, Essack, Zahra, Fukui, Akihiko, Gan, Tianjun, Gary, Kaz, Ghachoui, Mourad, Gillon, Michaël, Girardin, Eric, Glidden, Ana, Gonzales, Erica J., Guerra, Pere, Horch, Elliott P., Helminiak, Krzysztof G., Howard, Andrew W., Huber, Daniel, Irwin, Jonathan M., Isopi, Giovanni, Jehin, Emmanuël, Kagetani, Taiki, Kane, Stephen R., Kawauchi, Kiyoe, Kielkopf, John F., Lewin, Pablo, Luker, Lindy, Lund, Michael B., Mallia, Franco, Mao, Shude, Massey, Bob, Matson, Rachel A., Mireles, Ismael, Mori, Mayuko, Murgas, Felipe, Narita, Norio, O`Dwyer, Tanner, Petigura, Erik A., Polanski, Alex S., Pozuelos, Francisco J., Palle, Enric, Parviainen, Hannu, Plavchan, Peter P., Relles, Howard M., Robertson, Paul, Rose, Mark E., Rowden, Pamela, Roy, Arpita, Savel, Arjun B., Schlieder, Joshua E., Schnaible, Chloe, Schwarz, Richard P., Sefako, Ramotholo, Selezneva, Aleksandra, Skinner, Brett, Stockdale, Chris, Strakhov, Ivan A., Tan, Thiam-Guan, Torres, Guillermo, Tronsgaard, René, Twicken, Joseph D., Vermilion, David, Waite, Ian A., Walter, Bradley, Wang, Gavin, Ziegler, Carl, Zou, Yujie
Publikováno v:
AJ 163 99 (2022)
The James Webb Space Telescope (JWST) will be able to probe the atmospheres and surface properties of hot, terrestrial planets via emission spectroscopy. We identify 18 potentially terrestrial planet candidates detected by the Transiting Exoplanet Su
Externí odkaz:
http://arxiv.org/abs/2201.12661
Autor:
Vach, Sydney, Quinn, Samuel N., Vanderburg, Andrew, Kane, Stephen R., Collins, Karen A., Kraus, Adam L., Zhou, George, Medina, Amber A., Schwarz, Richard P., Collins, Kevin I., Conti, Dennis M., Stockdale, Chris, Massey, Bob, Suarez, Olga, Guillot, Tristan, Mekarnia, Djamel, Abe, Lyu, Dransfield, Georgina, Crouzet, Nicolas, Triaud, Amaury H. M. J., Schmider, François-Xavier, Agabi, Abelkrim, Buttu, Marco, Furlan, Elise, Gnilka, Crystal L., Howell, Steve B., Ziegler, Carl, Briceño, César, Law, Nicholas, Mann, Andrew W., Rudat, Alexander, Colon, Knicole D., Rose, Mark E., Kunimoto, Michelle, Günther, Maximilian N., Charbonneau, David, Ciardi, David R., Ricker, George R., Vanderspek, Roland K., Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M.
As an all-sky survey, NASA's $TESS$ mission is able to detect the brightest and rarest types of transiting planetary systems, including young planets that enable study of the evolutionary processes that occur within the first billion years. Here, we
Externí odkaz:
http://arxiv.org/abs/2111.02416
Autor:
Gilbert, Emily A., Barclay, Thomas, Quintana, Elisa V., Walkowicz, Lucianne M., Vega, Laura D., Schlieder, Joshua E., Monsue, Teresa, Cale, Bryson, Collins, Kevin I., Gaidos, Eric, Mufti, Mohammed El, Reefe, Michael, Plavchan, Peter, Tanner, Angelle, Wittenmyer, Robert A., Wittrock, Justin M., Jenkins, Jon M., Latham, David W., Ricker, George R., Rose, Mark E., Seager, S., Vanderspek, Roland K., Winn, Joshua N.
AU Mic is a young ($\sim$24 Myr), pre-Main Sequence M~dwarf star that was observed in the first month of science observations of the Transiting Exoplanet Survey Satellite (TESS) and re-observed two years later. This target has photometric variability
Externí odkaz:
http://arxiv.org/abs/2109.03924
Autor:
Osborn, Ares, Armstrong, David J., Cale, Bryson, Brahm, Rafael, Wittenmyer, Robert A., Dai, Fei, Crossfield, Ian J. M., Bryant, Edward M., Adibekyan, Vardan, Cloutier, Ryan, Collins, Karen A., Mena, E. Delgado, Fridlund, Malcolm, Hellier, Coel, Howell, Steve B., King, George W., Lillo-Box, Jorge, Otegi, Jon, Sousa, S., Stassun, Keivan G., Matthews, Elisabeth C., Ziegler, Carl, Ricker, George, Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Acton, Jack S., Addison, Brett C., Anderson, David R., Ballard, Sarah, Barrado, David, Barros, Susana C. C., Batalha, Natalie, Bayliss, Daniel, Barclay, Thomas, Benneke, Björn, Berberian Jr., John, Bouchy, Francois, Bowler, Brendan P., Briceño, César, Burke, Christopher J., Burleigh, Matthew R., Casewell, Sarah L., Ciardi, David, Collins, Kevin I., Cooke, Benjamin F., Demangeon, Olivier D. S., Díaz, Rodrigo F., Dorn, C., Dragomir, Diana, Dressing, Courtney, Dumusque, Xavier, Espinoza, Néstor, Figueira, P., Fulton, Benjamin, Furlan, E., Gaidos, E., Geneser, C., Gill, Samuel, Goad, Michael R., Gonzales, Erica J., Gorjian, Varoujan, Günther, Maximilian N., Helled, Ravit, Henderson, Beth A., Henning, Thomas, Hogan, Aleisha, Hojjatpanah, Saeed, Horner, Jonathan, Howard, Andrew W., Hoyer, Sergio, Huber, Dan, Isaacson, Howard, Jenkins, James S., Jensen, Eric L. N., Jordán, Andrés, Kane, Stephen R., Kidwell Jr., Richard C., Kielkopf, John, Law, Nicholas, Lendl, Monika, Lund, M., Matson, Rachel A., Mann, Andrew W., McCormac, James, Mengel, Matthew W., Morales, Farisa Y., Nielsen, Louise D., Okumura, Jack, Osborn, Hugh P., Petigura, Erik A., Plavchan, Peter, Pollacco, Don, Quintana, Elisa V., Raynard, Liam, Robertson, Paul, Rose, Mark E., Roy, Arpita, Reefe, Michael, Santerne, Alexandre, Santos, Nuno C., Sarkis, Paula, Schlieder, J., Schwarz, Richard P., Scott, Nicholas J., Shporer, Avi, Smith, A. M. S., Stibbard, C., Stockdale, Chris, Strøm, Paul A., Twicken, Joseph D., Tan, Thiam-Guan, Tanner, A., Teske, J., Tilbrook, Rosanna H., Tinney, C. G., Udry, Stephane, Villaseñor, Jesus Noel, Vines, Jose I., Wang, Sharon X., Weiss, Lauren M., West, Richard G., Wheatley, Peter J., Wright, Duncan J., Zhang, Hui, Zohrabi, F.
We present the bright (V$_{mag} = 9.12$), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm 0.7$ days using archival photometry and radial velocities. TOI-431b is
Externí odkaz:
http://arxiv.org/abs/2108.02310
Warm Jupiters in TESS Full-Frame Images: A Catalog and Observed Eccentricity Distribution for Year 1
Autor:
Dong, Jiayin, Huang, Chelsea X., Dawson, Rebekah I., Foreman-Mackey, Daniel, Collins, Karen A., Quinn, Samuel N., Lissauer, Jack J., Beatty, Thomas G., Quarles, Billy, Sha, Lizhou, Shporer, Avi, Guo, Zhao, Kane, Stephen R., Abe, Lyu, Barkaoui, Khalid, Benkhaldoun, Zouhair, Brahm, Rafael A., Bouchy, Francois, Carmichael, Theron W., Collins, Kevin I., Conti, Dennis M., Crouzet, Nicolas, Dransfield, Georgina, Evans, Phil, Gan, Tianjun, Ghachoui, Mourad, Gillon, Michael, Grieves, Nolan, Guillot, Tristan, Hellier, Coel, Jehin, Emmanuel, Jensen, Eric L., Jordan, Andres, Kamler, Jacob, Kielkopf, John, Mekarnia, Djamel, Nielsen, Louise D., Pozuelos, Francisco J., Radford, Don J., Schmider, Francois-Xavier, Schwarz, Richard P., Stockdale, Chris, Tan, Thiam-Guan, Timmermans, Mathilde, Triaud, Amaury H., Wang, Gavin, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Mireles, Ismael, Yahalomi, Daniel, Morgan, Edward H., Vezie, Michael, Quintana, Elisa V., Rose, Mark E., Smith, Jeffrey C., Shiao, Bernie
Warm Jupiters -- defined here as planets larger than 6 Earth radii with orbital periods of 8--200 days -- are a key missing piece in our understanding of how planetary systems form and evolve. It is currently debated whether Warm Jupiters form in sit
Externí odkaz:
http://arxiv.org/abs/2104.01970
Autor:
Guerrero, Natalia M., Seager, S., Huang, Chelsea X., Vanderburg, Andrew, Soto, Aylin Garcia, Mireles, Ismael, Hesse, Katharine, Fong, William, Glidden, Ana, Shporer, Avi, Latham, David W., Collins, Karen A., Quinn, Samuel N., Burt, Jennifer, Dragomir, Diana, Crossfield, Ian, Vanderspek, Roland, Fausnaugh, Michael, Burke, Christopher J., Ricker, George, Daylan, Tansu, Essack, Zahra, Günther, Maximilian N., Osborn, Hugh P., Pepper, Joshua, Rowden, Pamela, Sha, Lizhou, Villanueva Jr., Steven, Yahalomi, Daniel A., Yu, Liang, Ballard, Sarah, Batalha, Natalie M., Berardo, David, Chontos, Ashley, Dittmann, Jason A., Esquerdo, Gilbert A., Mikal-Evans, Thomas, Jayaraman, Rahul, Krishnamurthy, Akshata, Louie, Dana R., Mehrle, Nicholas, Niraula, Prajwal, Rackham, Benjamin V., Rodriguez, Joseph E., Rowden, Stephen J. L., Sousa-Silva, Clara, Watanabe, David, Wong, Ian, Zhan, Zhuchang, Zivanovic, Goran, Christiansen, Jessie L., Ciardi, David R., Swain, Melanie A., Lund, Michael B., Mullally, Susan E., Fleming, Scott W., Rodriguez, David R., Boyd, Patricia T., Quintana, Elisa V., Barclay, Thomas, Colón, Knicole D., Rinehart, S. A., Schlieder, Joshua E., Clampin, Mark, Jenkins, Jon M., Twicken, Joseph D., Caldwell, Douglas A., Coughlin, Jeffrey L., Henze, Chris, Lissauer, Jack J., Morris, Robert L., Rose, Mark E., Smith, Jeffrey C., Tenenbaum, Peter, Ting, Eric B., Wohler, Bill, Bakos, G. Á., Bean, Jacob L., Berta-Thompson, Zachory K., Bieryla, Allyson, Bouma, Luke G., Buchhave, Lars A., Butler, Nathaniel, Charbonneau, David, Doty, John P., Ge, Jian, Holman, Matthew J., Howard, Andrew W., Kaltenegger, Lisa, Kane, Stephen R., Kjeldsen, Hans, Kreidberg, Laura, Lin, Douglas N. C., Minsky, Charlotte, Narita, Norio, Paegert, Martin, Pál, András, Palle, Enric, Sasselov, Dimitar D., Spencer, Alton, Sozzetti, Alessandro, Stassun, Keivan G., Torres, Guillermo, Udry, Stephane, Winn, Joshua N.
We present 2,241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its two-year prime mission. We list these candidates in the TESS Objects of Interest (TOI) Catalog, which includes both new planet
Externí odkaz:
http://arxiv.org/abs/2103.12538
Autor:
Dawson, Rebekah I., Huang, Chelsea X., Brahm, Rafael, Collins, Karen A., Hobson, Melissa J., Jordán, Andrés, Dong, Jiayin, Korth, Judith, Trifonov, Trifon, Abe, Lyu, Agabi, Abdelkrim, Bruni, Ivan, Butler, R. Paul, Barbieri, Mauro, Collins, Kevin I., Conti, Dennis M., Crane, Jeffrey D., Crouzet, Nicolas, Dransfield, Georgina, Evans, Phil, Espinoza, Néstor, Gan, Tianjun, Guillot, Tristan, Henning, Thomas, Lissauer, Jack J., Jensen, Eric L. N., Sainte, Wenceslas Marie, Mékarnia, Djamel, Myers, Gordon, Nandakumar, Sangeetha, Relles, Howard M., Sarkis, Paula, Torres, Pascal, Shectman, Stephen, Schmider, François-Xavier, Shporer, Avi, Stockdale, Chris, Teske, Johanna, Triaud, Amaury H. M. J., Wang, Sharon Xuesong, Ziegler, Carl, Ricker, G., Vanderspek, R., Latham, David W., Seager, S., Winn, J., Jenkins, Jon M., Bouma, L. G., Burt, Jennifer A., Charbonneau, David, Levine, Alan M., McDermott, Scott, McLean, Brian, Rose, Mark E., Vanderburg, Andrew, Wohler, Bill
TOI-216 hosts a pair of warm, large exoplanets discovered by the TESS Mission. These planets were found to be in or near the 2:1 resonance, and both of them exhibit transit timing variations (TTVs). Precise characterization of the planets' masses and
Externí odkaz:
http://arxiv.org/abs/2102.06754