Zobrazeno 1 - 10
of 1 482
pro vyhledávání: '"Díaz, P. R."'
Autor:
Xiao, Guang-Yao, Feng, Fabo, Shectman, Stephen A., Tinney, C. G., Teske, Johanna K., Carter, B. D., Jones, H. R. A., Wittenmyer, Robert A., Díaz, Matías R., Crane, Jeffrey D., Wang, Sharon X., Bailey, J., O'Toole, S. J., Feinstein, Adina D., Rice, Malena, Essack, Zahra, Montet, Benjamin T., Shporer, Avi, Butler, R. Paul
Giant planets on long period orbits around the nearest stars are among the easiest to directly image. Unfortunately these planets are difficult to fully constrain by indirect methods, e.g., transit and radial velocity (RV). In this study, we present
Externí odkaz:
http://arxiv.org/abs/2409.08067
Autor:
Li, Zhexing, Kane, Stephen R., Brandt, Timothy D., Fetherolf, Tara, Robertson, Paul, Zhao, Jinglin, Dalba, Paul A., Wittenmyer, Robert A., Butler, R. Paul, Diaz, Matias R., Howell, Steve B., Bailey, Jeremy, Carter, Brad, Furlan, Elise, Gnilka, Crystal L., Jones, Hugh R. A., O'Toole, Simon, Tinney, Chris
Multi-planet systems exhibit a diversity of architectures that diverge from the solar system and contribute to the topic of exoplanet demographics. Radial velocity (RV) surveys form a crucial component of exoplanet surveys, as their long observationa
Externí odkaz:
http://arxiv.org/abs/2401.17415
Autor:
Osborne, H. L. M., Van Eylen, V., Goffo, E., Gandolfi, D., Nowak, G., Persson, C. M., Livingston, J., Weeks, A., Pallé, E., Luque, R., Hellier, C., Carleo, I., Redfield, S., Hirano, T., Gili, M. Garbaccio, Alarcon, J., Barragán, O., Casasayas-Barris, N., Díaz, M. R., Esposito, M., Jenkins, J. S., Knudstrup, E., Murgas, F., Orell-Miquel, J., Rodler, F., Serrano, L., Stangret, M., Albrecht, S. H., Alqasim, A., Cochran, W. D., Deeg, H. J., Fridlund, M., Hatzes, A., Korth, J., Lam, K. W. F.
We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V=10.8), which hosts a small transiting planet recently discovered by the Transiting Exoplanet Survey Satellite (TESS). We collected 122 high-resolution HARPS
Externí odkaz:
http://arxiv.org/abs/2310.14908
Autor:
Vines, Jose I., Jenkins, James S., Berdiñas, Zaira, Soto, Maritza G., Díaz, Matías R., Alves, Douglas R., Tuomi, Mikko, Wittenmyer, Robert A., de Leon, Jerome Pitogo, Peña, Pablo, Lissauer, Jack J., Ballard, Sarah, Bedding, Timothy, Bowler, Brendan P., Horner, Jonathan, Jones, Hugh R. A., Kane, Stephen R., Kielkopf, John, Plavchan, Peter, Shporer, Avi, Tinney, C. G., Wright, Hui Zhang Duncan J., Addison, Brett, Mengel, Matthew W., Okumura, Jack, Samadi-Ghadim, Anya
Very little is known about the young planet population because the detection of small planets orbiting young stars is obscured by the effects of stellar activity and fast rotation which mask planets within radial velocity and transit data sets. The f
Externí odkaz:
http://arxiv.org/abs/2210.07945
Autor:
Serrano, Luisa Maria, Gandolfi, Davide, Mustill, Alexander J., Barragán, Oscar, Korth, Judith, Dai, Fei, Redfield, Seth, Fridlund, Malcolm, Lam, Kristine W. F., Díaz, Matías R., Grziwa, Sascha, Collins, Karen A., Livingston, John H., Cochran, William D., Hellier, Coel, Bellomo, Salvatore E., Trifonov, Trifon, Rodler, Florian, Alarcon, Javier, Jenkins, Jon M., Latham, David W., Ricker, George, Seager, Sara, Vanderspeck, Roland, Winn, Joshua N., Albrecht, Simon, Collins, Kevin I., Csizmadia, Szilárd, Daylan, Tansu, Deeg, Hans J., Esposito, Massimiliano, Fausnaugh, Michael, Georgieva, Iskra, Goffo, Elisa, Guenther, Eike, Hatzes, Artie P., Howell, Steve B., Jensen, Eric L. N., Luque, Rafael, Mann, Andrew W., Murgas, Felipe, Osborne, Hannah L. M., Palle, Enric, Persson, Carina M., Rowden, Pam, Rudat, Alexander, Smith, Alexis M. S., Twicken, Joseph D., Van Eylen, Vincent, Ziegler, Carl
It is commonly accepted that exoplanets with orbital periods shorter than 1 day, also known as ultra-short period (USP) planets, formed further out within their natal protoplanetary disk, before migrating to their current-day orbits via dynamical int
Externí odkaz:
http://arxiv.org/abs/2204.13573
We study the emergence of quasicrystal configurations produced purely by quantum fluctuations in the ground-state phase diagram of interacting bosonic systems. By using a variational mean-field approach, we determine the relevant features of the pair
Externí odkaz:
http://arxiv.org/abs/2110.12299
Autor:
Trifonov, Trifon, Brahm, Rafael, Espinoza, Nestor, Henning, Thomas, Jordán, Andrés, Nesvorny, David, Dawson, Rebekah I., Lissauer, Jack J., Lee, Man Hoi, Kossakowski, Diana, Rojas, Felipe I., Hobson, Melissa J., Sarkis, Paula, Schlecker, Martin, Bitsch, Bertram, Bakos, Gaspar Á., Barbieri, Mauro, Bhatti, Waqas, Butler, R. Paul, Crane, Jeffrey D., Nandakumar, Sangeetha, Díaz, Matías R., Shectman, Stephen, Teske, Johanna, Torres, Pascal, Suc, Vincent, Vines, Jose I., Wang, Sharon X., Ricker, George R., Shporer, Avi, Vanderburg, Andrew, Dragomir, Diana, Vanderspek, Roland, Burke, Christopher J., Daylan, Tansu, Shiao, Bernie, Jenkins, Jon M., Wohler, Bill, Seager, Sara, Winn, Joshua N.
TOI-2202 b is a transiting warm Jovian-mass planet with an orbital period of P=11.91 days identified from the Full Frame Images data of five different sectors of the TESS mission. Ten TESS transits of TOI-2202 b combined with three follow-up light cu
Externí odkaz:
http://arxiv.org/abs/2108.05323
Autor:
Sha, Lizhou, Huang, Chelsea X., Shporer, Avi, Rodriguez, Joseph E., Vanderburg, Andrew, Brahm, Rafael, Hagelberg, Janis, Matthews, Elisabeth C., Ziegler, Carl, Livingston, John H., Stassun, Keivan G., Wright, Duncan J., Crane, Jeffrey D., Espinoza, Néstor, Bouchy, François, Bakos, Gáspár Á., Collins, Karen A., Zhou, George, Bieryla, Allyson, Hartman, Joel D., Wittenmyer, Robert A., Nielsen, Louise D., Plavchan, Peter, Bayliss, Daniel, Sarkis, Paula, Tan, Thiam-Guan, Cloutier, Ryan, Mancini, Luigi, Jordán, Andrés, Wang, Sharon, Henning, Thomas, Narita, Norio, Penev, Kaloyan, Teske, Johanna K., Kane, Stephen R., Mann, Andrew W., Addison, Brett C., Tamura, Motohide, Horner, Jonathan, Barbieri, Mauro, Burt, Jennifer A., Díaz, Matías R., Crossfield, Ian J. M., Dragomir, Diana, Drass, Holger, Feinstein, Adina D., Zhang, Hui, Hart, Rhodes, Kielkopf, John F., Jensen, Eric L. N., Montet, Benjamin T., Ottoni, Gaël, Schwarz, Richard P., Rojas, Felipe, Nespral, David Lopez Fdez, Torres, Pascal, Mengel, Matthew W., Udry, Stéphane, Zapata, Abner, Snoddy, Erin, Okumura, Jack, Ricker, George R., Vanderspek, Roland K., Latham, David W., Winn, Joshua N., Seager, Sara, Jenkins, Jon M., Colón, Knicole D., Henze, Christopher E., Krishnamurthy, Akshata, Ting, Eric B., Vezie, Michael, Villanueva, Steven
Publikováno v:
AJ 161 (2021) 82
We report the discovery of two short-period Saturn-mass planets, one transiting the G subgiant TOI-954 (TIC 44792534, $ V = 10.343 $, $ T = 9.78 $) observed in TESS sectors 4 and 5, and one transiting the G dwarf K2-329 (EPIC 246193072, $ V = 12.70 $
Externí odkaz:
http://arxiv.org/abs/2010.14436
Autor:
Mayer, T., Werner, H., Schmid, F., Diaz-Pardo, R., Fujii, J., Vobornik, I., Back, C. H., Kronseder, M., Bougeard, D.
Publikováno v:
Phys. Rev. Materials 5, 014202 (2021)
The challenge of parasitic bulk doping in Bi-based 3D topological insulator materials is still omnipresent, especially when preparing samples by molecular beam epitaxy (MBE). Here, we present a heterostructure approach for epitaxial BSTS growth. A th
Externí odkaz:
http://arxiv.org/abs/2010.06532
Autor:
Ment, Kristo, Irwin, Jonathan, Charbonneau, David, Winters, Jennifer G., Medina, Amber, Cloutier, Ryan, Díaz, Matías R., Jenkins, James S., Ziegler, Carl, Law, Nicholas, Mann, Andrew W., Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Goeke, Robert F., Levine, Alan M., Rojas-Ayala, Bárbara, Rowden, Pamela, Ting, Eric B., Twicken, Joseph D.
We present the discovery of TOI 540 b, a hot planet slightly smaller than Earth orbiting the low-mass star 2MASS J05051443-4756154. The planet has an orbital period of $P = 1.239149$ days ($\pm$ 170 ms) and a radius of $r = 0.903 \pm 0.052 R_{\rm Ear
Externí odkaz:
http://arxiv.org/abs/2009.13623