Zobrazeno 1 - 10
of 202
pro vyhledávání: '"Cooke, Benjamin"'
The determination of the full population of Resident Space Objects (RSOs) in Low Earth Orbit (LEO) is a key issue in the field of space situational awareness that will only increase in importance in the coming years. We endeavour to describe a novel
Externí odkaz:
http://arxiv.org/abs/2408.04966
Autor:
Cooke, Benjamin F., Chote, Paul, Pollacco, Don, West, Richard, Blake, James A., McCormac, James, Airey, Robert, Shrive, Billy
We present the methodology and results of a simulation to determine the recoverability of LEO objects using a blind stacking technique. The method utilises sCMOS and GPU technology to inject and recover LEO objects in real observed data. We explore t
Externí odkaz:
http://arxiv.org/abs/2305.01415
Autor:
Cooke, Benjamin
We study the comparison of computational simulations of biomolecules to experimental data. We study the convergence of these simulations to equilibrium and determine measures of variance of the data using statistical methods. We run replica-exchange
Externí odkaz:
http://hdl.handle.net/10161/923
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
Autor:
Bryant, Edward M., Bayliss, Daniel, Santerne, Alexandre, Wheatley, Peter J., Nascimbeni, Valerio, Ducrot, Elsa, Burdanov, Artem, Acton, Jack S., Alves, Douglas R., Anderson, David R., Armstrong, David J., Awiphan, Supachai, Cooke, Benjamin F., Burleigh, Matthew R., Casewell, Sarah L., Delrez, Laetitia, Demory, Brice-Olivier, Eigmüller, Philipp, Fukui, Akihiko, Gan, Tianjun, Gill, Samuel, Gillon, Michael, Goad, Michael R., Tan, Thiam-Guan, Günther, Maximilian N., Hardee, Bronwen, Henderson, Beth A., Jehin, Emmanuel, Jenkins, James S., Kosiarek, Molly, Lendl, Monika, Moyano, Maximiliano, Murray, Catriona A., Narita, Norio, Niraula, Prajwal, Odden, Caroline E., Palle, Enric, Parviainen, Hannu, Pedersen, Peter P., Pozuelos, Francisco J., Rackham, Benjamin V., Sebastian, Daniel, Stockdale, Chris, Tilbrook, Rosanna H., Thompson, Samantha J., Triaud, Amaury H. M. J., Udry, Stéphane, Vines, Jose I., West, Richard G., de Wit, Julien
HIP 41378 f is a temperate $9.2\pm0.1 R_{\oplus}$ planet with period of 542.08 days and an extremely low density of $0.09\pm0.02$ g cm$^{-3}$. It transits the bright star HIP 41378 (V=8.93), making it an exciting target for atmospheric characterizati
Externí odkaz:
http://arxiv.org/abs/2104.03159
Autor:
Tilbrook, Rosanna H., Burleigh, Matthew R., Costes, Jean C., Gill, Samuel, Nielsen, Louise D., Vines, José I., Queloz, Didier, Hodgkin, Simon T., Worters, Hannah L., Goad, Michael R., Acton, Jack S., Henderson, Beth A., Armstrong, David J., Anderson, David R., Bayliss, Daniel, Bouchy, François, Briegal, Joshua T., Bryant, Edward M., Casewell, Sarah L., Chaushev, Alexander, Cooke, Benjamin F., Eigmüller, Philipp, Gillen, Edward, Günther, Maximilian N., Hogan, Aleisha, Jenkins, James S., Lendl, Monika, McCormac, James, Moyano, Maximiliano, Raynard, Liam, Smith, Alexis M. S., Udry, Stéphane, Watson, Christopher A., West, Richard G., Wheatley, Peter J., Breytenbach, Hannes, Sefako, Ramotholo R., Thomas, Jessymol K., Alves, Douglas R.
We report the discovery of four new hot Jupiters with the Next Generation Transit Survey (NGTS). NGTS-15b, NGTS-16b, NGTS-17b, and NGTS-18b are short-period ($P<5$d) planets orbiting G-type main sequence stars, with radii and masses between $1.10-1.3
Externí odkaz:
http://arxiv.org/abs/2103.10302
Autor:
Grieves, Nolan, Nielsen, Louise D., Vines, Jose I., Bryant, Edward M., Gill, Samuel, Bouchy, François, Lendl, Monika, Bayliss, Daniel, Eigmueller, Philipp, Segransan, Damien, Acton, Jack S., Anderson, David R., Burleigh, Matthew R., Casewell, Sarah L., Chaushev, Alexander, Cooke, Benjamin F., Gillen, Edward, Goad, Michael R., Günther, Maximilian N., Henderson, Beth A., Hogan, Aleisha, Jenkins, James S., Alves, Douglas R., Jordán, Andrés, McCormac, James, Moyano, Maximiliano, Queloz, Didier, Raynard, Liam, Seidel, Julia V., Smith, Alexis M. S., Tilbrook, Rosanna H., Udry, Stephane, West, Richard G., Wheatley, Peter J.
Publikováno v:
A&A 647, A180 (2021)
We report the discovery of the massive hot Jupiter NGTS-13b by the Next Generation Transit Survey (NGTS). The V = 12.7 host star is likely in the subgiant evolutionary phase with log g$_{*}$ = 4.04 $\pm$ 0.05, T$_{eff}$ = 5819 $\pm$ 73 K, M$_{*}$ = 1
Externí odkaz:
http://arxiv.org/abs/2101.04245
Autor:
Cooke, Benjamin F., Pollacco, Don, Anderson, David R., Bayliss, Daniel, Bouchy, François, Gill, Samuel, Grieves, Nolan, Lendl, Monika, Nielsen, Louise D., Udry, Stéphane, Wheatley, Peter J.
We set out to explore how best to mitigate the number of period aliases for a transiting TESS system with two identified transits separated by a large time period on the order of years. We simulate a realistic population of doubly transiting planets
Externí odkaz:
http://arxiv.org/abs/2011.05832
Autor:
Jenkins, James S., Díaz, Matías R., Kurtovic, Nicolás T., Espinoza, Néstor, Vines, Jose I., Rojas, Pablo A. Peña, Brahm, Rafael, Torres, Pascal, Cortés-Zuleta, Pía, Soto, Maritza G., Lopez, Eric D., King, George W., Wheatley, Peter J., Winn, Joshua N., Ciardi, David R., Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Jenkins, Jon M., Beichman, Charles A., Bieryla, Allyson, Burke, Christopher J., Christiansen, Jessie L., Henze, Christopher E., Klaus, Todd C., McCauliff, Sean, Mori, Mayuko, Narita, Norio, Nishiumi, Taku, Tamura, Motohide, de Leon, Jerome Pitogo, Quinn, Samuel N., Villaseñor, Jesus Noel, Vezie, Michael, Lissauer, Jack J., Collins, Karen A., Collins, Kevin I., Isopi, Giovanni, Mallia, Franco, Ercolino, Andrea, Petrovich, Cristobal, Jordán, Andrés, Acton, Jack S., Armstrong, David J., Bayliss, Daniel, Bouchy, François, Belardi, Claudia, Bryant, Edward M., Burleigh, Matthew R., Cabrera, Juan, Casewell, Sarah L., Chaushev, Alexander, Cooke, Benjamin F., Eigmüller, Philipp, Erikson, Anders, Foxell, Emma, Gänsicke, Boris T., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Goad, Michael R., Hooton, Matthew J., Jackman, James A. G., Louden, Tom, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D., Pollacco, Don, Queloz, Didier, Rauer, Heike, Raynard, Liam, Smith, Alexis M. S., Tilbrook, Rosanna H., Titz-Weider, Ruth, Turner, Oliver, Udry, Stéphane, Walker, Simon. R., Watson, Christopher A., West, Richard G., Palle, Enric, Ziegler, Carl, Law, Nicholas, Mann, Andrew W.
About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,
Externí odkaz:
http://arxiv.org/abs/2009.12832