Zobrazeno 1 - 10
of 94
pro vyhledávání: '"Terada, Yuka"'
Autor:
Mori, Mayuko, Ikuta, Kai, Fukui, Akihiko, Narita, Norio, de Leon, Jerome P., Livingston, John H., Ikoma, Masahiro, Kawai, Yugo, Kawauchi, Kiyoe, Murgas, Felipe, Palle, Enric, Parviainen, Hannu, Rodríguez, Gareb Fernández, Terada, Yuka, Watanabe, Noriharu, Tamura, Motohide
Detailed atmospheric characterization of exoplanets by transmission spectroscopy requires careful consideration of stellar surface inhomogeneities induced by starspots. This effect is particularly problematic for planetary systems around M-dwarfs, an
Externí odkaz:
http://arxiv.org/abs/2403.13946
Autor:
Liu, Hauyu Baobab, Muto, Takayuki, Konishi, Mihoko, Chung, Chia-Ying, Hashimoto, Jun, Doi, Kiyoaki, Dong, Ruobing, Kudo, Tomoyuki, Hasegawa, Yasuhiro, Terada, Yuka, Kataoka, Akimasa
The previous, high angular resolution 225 GHz ($\sim$1.3 mm) continuum observations on the transitional disk DM Tau have resolved an outer ring at 20-120 au radii that is weakly azimuthally asymmetric. We aimed to examine dust growth and filtration i
Externí odkaz:
http://arxiv.org/abs/2402.02900
An inner component misaligned from an outer component in a protoplanetary disk can result in the former casting shadows on the latter. We present a new instance of shadowing on the outer disk around a very low mass star, ZZ~Tau~IRS. Through the analy
Externí odkaz:
http://arxiv.org/abs/2401.02004
Magnetized exoplanets can serve as the source of auroral radio emissions, allowing us to characterize the magnetospheric properties of these planets. Successful detections of auroral radio emissions from brown dwarfs, as well as from Jupiter, suggest
Externí odkaz:
http://arxiv.org/abs/2312.15176
We examined the grain size in the dust ring encircling the 0.19~$M_\sun$ T Tauri star CIDA 1 using the Karl G. Jansky Very Large Array (JVLA) at multiple centimeter wavelengths, with a spatial resolution of 0$\farcs$2--0$\farcs$9. We detected distinc
Externí odkaz:
http://arxiv.org/abs/2308.11837
Autor:
Terada, Yuka, Liu, Hauyu Baobab, Mkrtichian, David, Sai, Jinshi, Konishi, Mihoko, Jiang, Ing-Guey, Muto, Takayuki, Hashimoto, Jun, Tamura, Motohide
The powerful, high-energy magnetic activities of young stars play important roles in the magnetohydrodynamics in the innermost parts of the protoplanetary disks. In addition, the associated UV and X-ray emission dictates the photochemistry; moreover,
Externí odkaz:
http://arxiv.org/abs/2306.09013
Autor:
Mori, Mayuko, Livingston, John H., de Leon, Jerome, Narita, Norio, Hirano, Teruyuki, Fukui, Akihiko, Collins, Karen A., Fujita, Naho, Hori, Yasunori, Ishikawa, Hiroyuki Tako, Kawauchi, Kiyoe, Stassun, Keivan G., Watanabe, Noriharu, Giacalone, Steven, Gore, Rebecca, Schroeder, Ashley, Dressing, Courtney D., Bieryla, Allyson, Jensen, Eric L. N., Massey, Bob, Shporer, Avi, Kuzuhara, Masayuki, Charbonneau, David, Ciardi, David R., Doty, John P., Esparza-Borges, Emma, Harakawa, Hiroki, Hodapp, Klaus, Ikoma, Masahiro, Ikuta, Kai, Isogai, Keisuke, Jenkins, Jon M., Kagetani, Taiki, Kimura, Tadahiro, Kodama, Takanori, Kotani, Takayuki, Krishnamurthy, Vigneshwaran, Kudo, Tomoyuki, Kurita, Seiya, Kurokawa, Takashi, Kusakabe, Nobuhiko, Latham, David W., McLean, Brian, Murgas, Felipe, Nishikawa, Jun, Nishiumi, Taku, Omiya, Masashi, Osborn, Hugh P., Palle, Enric, Parviainen, Hannu, Ricker, George R., Seager, Sara, Serizawa, Takuma, Tamura, Motohide, Teng, Huan-Yu, Terada, Yuka, Twicken, Joseph D., Ueda, Akitoshi, Vanderspek, Roland, Vievard, Sébastien, Winn, Joshua N., Zou, Yujie
We present the discovery and validation of a temperate sub-Neptune around the nearby mid-M dwarf TIC 470381900 (TOI-1696), with a radius of $3.09 \pm 0.11 \,R_\oplus$ and an orbital period of $2.5 \,\rm{days}$, using a combination of TESS and follow-
Externí odkaz:
http://arxiv.org/abs/2203.02694
Autor:
Watanabe, Noriharu, Narita, Norio, Palle, Enric, Fukui, Akihiko, Kusakabe, Nobuhiko, Parviainen, Hannu, Murgas, Felipe, Casasayas-Barris, Núria, Johnson, Marshall C., Sato, Bun'ei, Livingston, John H., de Leon, Jerome P., Mori, Mayuko, Nishiumi, Taku, Terada, Yuka, Esparza-Borges, Emma, Kawauchi, Kiyoe
WASP-33b, a hot Jupiter around a hot star, is a rare system in which nodal precession has been discovered. We updated the model for the nodal precession of WASP-33b by adding new observational points. Consequently, we found a motion of the nodal prec
Externí odkaz:
http://arxiv.org/abs/2203.02003
Autor:
Christian, Sam, Vanderburg, Andrew, Becker, Juliette, Yahalomi, Daniel A., Pearce, Logan, Zhou, George, Collins, Karen A., Kraus, Adam L., Stassun, Keivan G., de Beurs, Zoe, Ricker, George R., Vanderspek, Roland K., Latham, David W., Winn, Joshua N., Seager, S., Jenkins, Jon M., Abe, Lyu, Agabi, Karim, Amado, Pedro J., Baker, David, Barkaoui, Khalid, Benkhaldoun, Zouhair, Benni, Paul, Berberian, John, Berlind, Perry, Bieryla, Allyson, Esparza-Borges, Emma, Bowen, Michael, Brown, Peyton, Buchhave, Lars A., Burke, Christopher J., Buttu, Marco, Cadieux, Charles, Caldwell, Douglas A., Charbonneau, David, Chazov, Nikita, Chimaladinne, Sudhish, Collins, Kevin I., Combs, Deven, Conti, Dennis M., Crouzet, Nicolas, de Leon, Jerome P., Deljookorani, Shila, Diamond, Brendan, Doyon, René, Dragomir, Diana, Dransfield, Georgina, Essack, Zahra, Evans, Phil, Fukui, Akihiko, Gan, Tianjun, Esquerdo, Gilbert A., Gillon, Michaël, Girardin, Eric, Guerra, Pere, Guillot, Tristan, Habich, Eleanor Kate K., Henriksen, Andreea, Hoch, Nora, Isogai, Keisuke I, Jehin, Emmanuël, Jensen, Eric L. N., Johnson, Marshall C., Livingston, John H., Kielkopf, John F., Kim, Kingsley, Kawauchi, Kiyoe, Krushinsky, Vadim, Kunzle, Veronica, Laloum, Didier, Leger, Dominic, Lewin, Pablo, Mallia, Franco, Massey, Bob, Mori, Mayuko, McLeod, Kim K., Mékarnia, Djamel, Mireles, Ismael, Mishevskiy, Nikolay, Tamura, Motohide, Murgas, Felipe, Narita, Norio, Naves, Ramon, Nelson, Peter, Osborn, Hugh P., Palle, Enric, Parviainen, Hannu, Plavchan, Peter, Pozuelos, Francisco J., Rabus, Markus, Relles, Howard M., López, Cristina Rodríguez, Quinn, Samuel N., Schmider, Francois-Xavier, Schlieder, Joshua E., Schwarz, Richard P., Shporer, Avi, Sibbald, Laurie, Srdoc, Gregor, Stibbards, Caitlin, Stickler, Hannah, Suarez, Olga, Stockdale, Chris, Tan, Thiam-Guan, Terada, Yuka, Triaud, Amaury, Tronsgaard, Rene, Waalkes, William C., Wang, Gavin, Watanabe, Noriharu, Wenceslas, Marie-Sainte, Wingham, Geof, Wittrock, Justin, Ziegler, Carl
Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 AU) on the formation and evolution of exoplanets. We investigate these effects using new data from Gaia EDR3 and the TESS mission to
Externí odkaz:
http://arxiv.org/abs/2202.00042
Autor:
Fukui, Akihiko, Kimura, Tadahiro, Hirano, Teruyuki, Narita, Norio, Kodama, Takanori, Hori, Yasunori, Ikoma, Masahiro, Pallé, Enric, Murgas, Felipe, Parviainen, Hannu, Kawauchi, Kiyoe, Mori, Mayuko, Esparza-Borges, Emma, Bieryla, Allyson, Irwin, Jonathan, Safonov, Boris S., Stassun, Keivan G., Alvarez-Hernandez, Leticia, Béjar, Víctor J. S., Casasayas-Barris, Núria, Chen, Guo, Crouzet, Nicolas, de Leon, Jerome P., Isogai, Keisuke, Kagetani, Taiki, Klagyivik, Peter, Korth, Judith, Kurita, Seiya, Kusakabe, Nobuhiko, Livingston, John, Luque, Rafael, Madrigal-Aguado, Alberto, Morello, Giuseppe, Nishiumi, Taku, Orell-Miquel, Jaume, Oshagh, Mahmoudreza, Sánchez-Benavente, Manuel, Stangret, Monika, Terada, Yuka, Watanabe, Noriharu, Zou, Yujie, Tamura, Motohide, Kurokawa, Takashi, Kuzuhara, Masayuki, Nishikawa, Jun, Omiya, Masashi, Vievard, Sébastien, Ueda, Akitoshi, Latham, David W., Quinn, Samuel N., Strakhov, Ivan S., Belinski, Alexandr A., Jenkins, Jon M., Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua N., Charbonneau, David, Ciardi, David R., Collins, Karen A., Doty, John P., Bachelet, Etienne, Harbeck, Daniel
We report the discovery of TOI-2285b, a sub-Neptune-sized planet transiting a nearby (42 pc) M dwarf with a period of 27.3 days. We identified the transit signal from the Transiting Exoplanet Survey Satellite photometric data, which we confirmed with
Externí odkaz:
http://arxiv.org/abs/2110.10215