Zobrazeno 1 - 10
of 121
pro vyhledávání: '"Vines, Jose I"'
Autor:
Henderson, Beth A., Casewell, Sarah L., Jordán, Andrés, Brahm, Rafael, Henning, Thomas, Gill, Samuel, Mayorga, L. C., Ziegler, Carl, Stassun, Keivan G., Goad, Michael R., Acton, Jack, Alves, Douglas R., Anderson, David R., Apergis, Ioannis, Armstrong, David J., Bayliss, Daniel, Burleigh, Matthew R., Dragomir, Diana, Gillen, Edward, Günther, Maximilian N., Hedges, Christina, Hesse, Katharine M., Hobson, Melissa J., Jenkins, James S., Jenkins, Jon M., Kendall, Alicia, Lendl, Monika, Lund, Michael B., McCormac, James, Moyano, Maximiliano, Osborn, Ares, Pinto, Marcelo Tala, Ramsay, Gavin, Rapetti, David, Saha, Suman, Seager, Sara, Trifonov, Trifon, Udry, Stéphane, Vines, Jose I., West, Richard G., Wheatley, Peter J., Winn, Joshua N., Zivave, Tafadzwa
We report the discovery of the most eccentric transiting brown dwarf in the brown dwarf desert, TOI02490b. The brown dwarf desert is the lack of brown dwarfs around main sequence stars within $\sim3$~AU and is thought to be caused by differences in f
Externí odkaz:
http://arxiv.org/abs/2408.04475
Autor:
Nabbie, Emma, Huang, Chelsea X., Burt, Jennifer A., Armstrong, David J., Mamajek, Eric E., Adibekyan, Vardan, Sousa, Sérgio G., Lopez, Eric D., Thorngren, Daniel P., Fernández, Jorge, Li, Gongjie, Jenkins, James S., Vines, Jose I., da Silva, João Gomes, Wittenmyer, Robert A., Bayliss, Daniel, Briceño, César, Collins, Karen A., Dumusque, Xavier, Horne, Keith D., Keniger, Marcelo F., Law, Nicholas, Lillo-Box, Jorge, Liu, Shang-Fei, Mann, Andrew W., Nielsen, Louise Dyregaard, Osborn, Ares, Relles, Howard M., Rodrigues, José J., Bell, Juan, Srdoc, Gregor, Stockdale, Chris, Strøm, Paul A., Gardner-Watkins, Cristilyn N., Wheatley, Peter J., Wright, Duncan J., Zhou, George, Ziegler, Carl, Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua W., Jenkins, Jon M., Fausnaugh, Michael, Kunimoto, Michelle, Osborn, Hugh P., Quinn, Samuel N., Wohler, Bill
The recent discoveries of Neptune-sized ultra-short period planets (USPs) challenge existing planet formation theories. It is unclear whether these residents of the Hot Neptune Desert have similar origins to smaller, rocky USPs, or if this discrete p
Externí odkaz:
http://arxiv.org/abs/2407.04225
Autor:
Gill, Samuel, Bayliss, Daniel, Ulmer-Moll, Solène, Wheatley, Peter J., Brahm, Rafael, Anderson, David R., Armstrong, David, Apergis, Ioannis, Alves, Douglas R., Burleigh, Matthew R., Butler, R. P., Bouchy, François, Battley, Matthew P., Bryant, Edward M., Bieryla, Allyson, Crane, Jeffrey D., Collins, Karen A., Casewell, Sarah L., Carleo, Ilaria, Claringbold, Alastair B., Dalba, Paul A., Dragomir, Diana, Eigmüller, Philipp, Eberhardt, Jan, Fausnaugh, Michael, Günther, Maximilian N., Grieves, Nolan, Goad, Michael R., Gillen, Edward, Hagelberg, Janis, Hobson, Melissa, Hedges, Christina, Henderson, Beth A., Hawthorn, Faith, Henning, Thomas, Jones, Matías I., Jordán, Andrés, Jenkins, James S., Kunimoto, Michelle, Krenn, Andreas F., Kendall, Alicia, Lendl, Monika, McCormac, James, Moyano, Maximiliano, Torres-Miranda, Pascal, Nielsen, Louise D., Osborn, Ares, Otegi, Jon, Osborn, Hugh, Quinn, Samuel N., Rodriguez, Joseph E., Ramsay, Gavin, Schlecker, Martin, Shectman, Stephen A., Seager, Sara, Tilbrook, Rosanna H., Trifonov, Trifon, Teske, Johanna K., Udry, Stephane, Vines, Jose I., West, Richard R., Wohler, Bill, Winn, Joshua N., Wang, Sharon X., Zhou, George, Zivave, Tafadzwa
Discovering transiting exoplanets with relatively long orbital periods ($>$10 days) is crucial to facilitate the study of cool exoplanet atmospheres ($T_{\rm eq} < 700 K$) and to understand exoplanet formation and inward migration further out than ty
Externí odkaz:
http://arxiv.org/abs/2405.07367
Autor:
O'Brien, Sean M., Schwamb, Megan E., Gill, Samuel, Watson, Christopher A., Burleigh, Matthew R., Kendall, Alicia, Anderson, David R., Vines, José I., Jenkins, James S., Alves, Douglas R., Trouille, Laura, Ulmer-Moll, Solène, Bryant, Edward M., Apergis, Ioannis, Battley, Matthew P., Bayliss, Daniel, Eisner, Nora L., Gillen, Edward, Goad, Michael R., Günther, Maximilian N., Henderson, Beth A., Heo, Jeong-Eun, Jackson, David G., Lintott, Chris, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D., Osborn, Ares, Saha, Suman, Sefako, Ramotholo R., Stephens, Andrew W., Tilbrook, Rosanna H., Udry, Stéphane, West, Richard G., Wheatley, Peter J., Zivave, Tafadzwa, Lim, See Min, Sainio, Arttu
Publikováno v:
AJ 167 (2024) 238
We present the results from the first two years of the Planet Hunters NGTS citizen science project, which searches for transiting planet candidates in data from the Next Generation Transit Survey (NGTS) by enlisting the help of members of the general
Externí odkaz:
http://arxiv.org/abs/2404.15395
Autor:
Henderson, Beth A., Casewell, Sarah L., Goad, Michael R., Acton, Jack S., Günther, Maximilian N., Nielsen, Louise D., Burleigh, Matthew R., Belardi, Claudia, Tilbrook, Rosanna H., Turner, Oliver, Howell, Steve B., Clark, Catherine A., Littlefield, Colin, Barkaoui, Khalid, Alves, Douglas R., Anderson, David R., Bayliss, Daniel, Bouchy, Francois, Bryant, Edward M., Dransfield, George, Ducrot, Elsa, Eigmüller, Philipp, Gill, Samuel, Gillen, Edward, Gillon, Michaël, Hawthorn, Faith, Hooton, Matthew J., Jackman, James A. G., Jehin, Emmanuel, Jenkins, James S., Kendall, Alicia, Lendl, Monika, McCormac, James, Moyano, Maximiliano, Pedersen, Peter Pihlmann, Pozuelos, Francisco J., Ramsay, Gavin, Sefako, Ramotholo R., Timmermans, Mathilde, Triaud, Amaury H. M. J., Udry, Stephane, Vines, Jose I., Watson, Christopher A., West, Richard G., Wheatley, Peter J., Zúñiga-Fernández, Sebastián
We report the discovery of a brown dwarf orbiting a M1 host star. We first identified the brown dwarf within the Next Generation Transit Survey data, with supporting observations found in TESS sectors 11 and 38. We confirmed the discovery with follow
Externí odkaz:
http://arxiv.org/abs/2402.09943
Autor:
Hawthorn, Faith, Gill, Sam, Bayliss, Daniel, Osborn, Hugh P., Pelisoli, Ingrid, Rodel, Toby, Darnbrook, Kaylen Smith, Wheatley, Peter J., Anderson, David R., Apergis, Ioan nis, Battley, Matthew P., Burleigh, Matthew R., Casewell, Sarah L., Eigmüller, Philipp, Günther, Maximilian N., Jenkins, James S., Lendl, Monika, Moyano, Maximiliano, Osborn, Ares, Ramsay, Gavin, Ulmer-Moll, Solène, Vines, Jose I., West, Richard
Discovering transiting exoplanets with long orbital periods allows us to study warm and cool planetary systems with temperatures similar to the planets in our own Solar system. The TESS mission has photometrically surveyed the entire Southern Eclipti
Externí odkaz:
http://arxiv.org/abs/2310.17268
Autor:
Smith, Gareth D., Gillen, Edward, Hodgkin, Simon T., Alves, Douglas R., Anderson, David R., Battley, Matthew P., Burleigh, Matthew R., Casewell, Sarah L., Gill, Samuel, Goad, Michael R., Henderson, Beth A., Jenkins, James S., Kendall, Alicia, Moyano, Maximiliano, Ramsay, Gavin, Tilbrook, Rosanna H., Vines, Jose I., West, Richard G., Wheatley, Peter J.
We present a study of rotation across 30 square degrees of the Orion Star-forming Complex, following a $\sim$200 d photometric monitoring campaign by the Next Generation Transit Survey (NGTS). From 5749 light curves of Orion members, we report period
Externí odkaz:
http://arxiv.org/abs/2305.04621
Autor:
Psaridi, Angelica, Bouchy, François, Lendl, Monika, Akinsanmi, Babatunde, Stassun, Keivan G., Smalley, Barry, Armstrong, David J., Howard, Saburo, Ulmer-Moll, Solène, Grieves, Nolan, Barkaoui, Khalid, Rodriguez, Joseph E., Bryant, Edward M., Suárez, Olga, Guillot, Tristan, Evans, Phil, Attia, Omar, Wittenmyer, Robert A., Yee, Samuel W., Collins, Karen A., Zhou, George, Galland, Franck, Parc, Léna, Udry, Stéphane, Figueira, Pedro, Ziegler, Carl, Mordasini, Christoph, Winn, Joshua N., Seager, Sara, Jenkins, Jon M., Twicken, Joseph D., Brahm, Rafael, Jones, Matías I., Abe, Lyu, Addison, Brett, Briceño, César, Briegal, Joshua T., Collins, Kevin I., Daylan, Tansu, Eigmüller, Phillip, Furesz, Gabor, Guerrero, Natalia M., Hagelberg, Janis, Heitzmann, Alexis, Hounsell, Rebekah, Huang, Chelsea X., Krenn, Andreas, Law, Nicholas M., Mann, Andrew W., McCormac, James, Mékarnia, Djamel, Mounzer, Dany, Nielsen, Louise D., Osborn, Ares, Reinarz, Yared, Sefako, Ramotholo R., Steiner, Michal, Strøm, Paul A., Triaud, Amaury H. M. J., Vanderspek, Roland, Vanzi, Leonardo, Vines, Jose I., Watson, Christopher A., Wright, Duncan J., Zapata, Abner
Publikováno v:
A&A 675, A39 (2023)
While the sample of confirmed exoplanets continues to increase, the population of transiting exoplanets around early-type stars is still limited. These planets allow us to investigate the planet properties and formation pathways over a wide range of
Externí odkaz:
http://arxiv.org/abs/2303.15080
Autor:
Magliano, Christian, Covone, Giovanni, Dobal, Richa, Cacciapuoti, Luca, Tonietti, Luca, Giacalone, Steven, Vines, Jose I., Inno, Laura, Jenkins, James S., Lissauer, Jack J., Bieryla, Allyson, Oliva, Fabrizio, Pagano, Isabella, Kostov, Veselin, Ziegler, Carl, Ciardi, David R., Gonzales, Erica J., Dressing, Courtney D., Buchhave, Lars A., Howell, Steve B., Matson, Rachel A., Matthews, Elisabeth, Rotundi, Alessandra, Alves, Douglas, Fiscale, Stefano, Ienco, Riccardo M., Pena, Pablo, Gallo, Francesco, Tomajoli, Maria T. Muscari
We statistically validated a sample of hot Neptune candidates applying a two-step vetting technique using DAVE and TRICERATOPS. We performed a systematic validation of 250 transit-like events in the Transiting Exoplanet Survey Satellite (TESS) archiv
Externí odkaz:
http://arxiv.org/abs/2211.08490
Autor:
Jackson, David G., Watson, Christopher A., de Mooij, Ernst J. W., Acton, Jack S., Alves, Douglas R., Anderson, David R., Armstrong, David J., Bayliss, Daniel, Belardi, Claudia, Bouchy, François, Bryant, Edward M., Burleigh, Matthew R., Casewell, Sarah L., Costes, Jean C., Eigmüller, Phillip, Goad, Michael R., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Hawthorn, Faith, Henderson, Beth A., Jackman, James A. G., Jenkins, James S., Lendl, Monika, Kendall, Alicia, McCormac, James, Moyano, Maximiliano, Nielsen, Louise. D., Osborn, Ares, Sefako, Ramotholo R., Smith, Alexis M. S., Tilbrook, Rosanna H., Turner, Oliver, Udry, Stéphane, Vines, Jose I., West, Richard G., Wheatley, Peter J., Worters, Hannah
We report the discovery of three new hot Jupiters with the Next Generation Transit Survey (NGTS) as well as updated parameters for HATS-54b, which was independently discovered by NGTS. NGTS-23b, NGTS-24b and NGTS-25b have orbital periods of 4.076, 3.
Externí odkaz:
http://arxiv.org/abs/2211.01044