Zobrazeno 1 - 10
of 73 364
pro vyhledávání: '"Fukui, A"'
Autor:
Ghachoui, M., Rackham, B. V., Dévora-Pajares, M., Chouqar, J., Timmermans, M., Kaltenegger, L., Sebastian, D., Pozuelos, F. J., Eastman, J. D., Burgasser, A. J., Murgas, F., Stassun, K. G., Gillon, M., Benkhaldoun, Z., Palle, E., Delrez, L., Jenkins, J. M., Barkaoui, K., Narita, N., de Leon, J. P., Mori, M., Shporer, A., Rowden, P., Kostov, V., Fűrész, G., Collins, K. A., Schwarz, R. P., Charbonneau, D., Guerrero, N. M., Ricker, G., Jehin, E., Fukui, A., Kawai, Y., Hayashi, Y., Esparza-Borges, E., Parviainen, H., Clark, C. A., Ciardi, D. R., Polanski, A. S., Schleider, J., Gilbert, E. A., Crossfield, I. J. M., Barclay, T., Dressing, C. D., Karpoor, P. R., Softich, E., Gerasimov, R., Davoudi, F.
We present the validation of two TESS super-Earth candidates transiting the mid-M dwarfs TOI-6002 and TOI-5713 every 10.90 and 10.44 days, respectively. The first star (TOI-6002) is located $32.038\pm0.019$ pc away, with a radius of $0.2409^{+0.0066}
Externí odkaz:
http://arxiv.org/abs/2408.00709
Autor:
Fukui, Toshizumi, Hasegawa, Masaru
We describe singularities of distance squared functions on singular surfaces in $\mathbb{R}^3$ parameterized by smooth map-germs $\mathcal{A}$-equivalent to one of $S_k$, $B_k$, $C_k$ and $F_4$ singularities in terms of extended geometric language vi
Externí odkaz:
http://arxiv.org/abs/2408.00231
Autor:
Dai, Fei, Howard, Andrew W., Halverson, Samuel, Orell-Miquel, Jaume, Palle, Enric, Isaacson, Howard, Fulton, Benjamin, Price, Ellen M., Plotnykov, Mykhaylo, Rogers, Leslie A., Valencia, Diana, Paragas, Kimberly, Greklek-McKeon, Michael, Barrientos, Jonathan Gomez, Knutson, Heather A., Petigura, Erik A., Weiss, Lauren M., Lee, Rena, Brinkman, Casey L., Huber, Daniel, Steffansson, Gudmundur, Masuda, Kento, Giacalone, Steven, Lu, Cicero X., Kite, Edwin S., Hu, Renyu, Gaidos, Eric, Zhang, Michael, Rubenzahl, Ryan A., Winn, Joshua N., Han, Te, Beard, Corey, Holcomb, Rae, Householder, Aaron, Gilbert, Gregory J., Lubin, Jack, Ong, J. M. Joel, Polanski, Alex S., Saunders, Nicholas, Van Zandt, Judah, Yee, Samuel W., Zhang, Jingwen, Zink, Jon, Holden, Bradford, Baker, Ashley, Brodheim, Max, Crossfield, Ian J. M., Deich, William, Edelstein, Jerry, Gibson, Steven R., Hill, Grant M., Jelinsky, Sharon R, Kassis, Marc, Laher, Russ R., Lanclos, Kyle, Lilley, Scott, Payne, Joel N., Rider, Kodi, Robertson, Paul, Roy, Arpita, Schwab, Christian, Shaum, Abby P., Sirk, Martin M., Smith, Chris, Vandenberg, Adam, Walawender, Josh, Wang, Sharon X., Shin-Ywan, Wang, Wishnow, Edward, Wright, Jason T., Yeh, Sherry, Caballero, Jos. A., Morales, Juan C., Murgas, Felipe, Nagel, Evangelos, Reiners, Ansgar, Schweitzer, Andreas, Tabernero, Hugo M., Zechmeister, Mathias, Spencer, Alton, Ciardi, David R., Clark, Catherine A., Lund, Michael B., Caldwell, Douglas A., Collins, Karen A., Schwarz, Richard P., Barkaoui, Khalid, Watkins, Cristilyn N., Shporer, Avi, Narita, Norio, Fukui, Akihiko, Srdoc, Gregor, Latham, David W., Jenkins, Jon M., Ricker, George R., Seager, Sara, Vanderspek, Roland
TOI-6255~b (GJ 4256) is an Earth-sized planet (1.079$\pm0.065$ $R_\oplus$) with an orbital period of only 5.7 hours. With the newly commissioned Keck Planet Finder (KPF) and CARMENES spectrographs, we determined the planet's mass to be 1.44$\pm$0.14
Externí odkaz:
http://arxiv.org/abs/2407.21167
Autor:
Vach, Sydney, Zhou, George, Huang, Chelsea X., Mann, Andrew W., Barber, Madyson G., Bieryla, Allyson, Latham, David W., Collins, Karen A., Rogers, James G., Bouma, Luke G., Douglas, Stephanie T., Quinn, Samuel N., Fairnington, Tyler R., Krüger, Joachim, Shporer, Avi, Collins, Kevin I., Srdoc, Gregor, Schwarz, Richard P., Relles, Howard M., Barkaoui, Khalid, McLeod, Kim K., Schneider, Alayna, Narita, Norio, Fukui, Akihiko, Sefako, Ramotholo, Fong, William, Mireles, Ismael, Torres, Guillermo, Ricker, George R., Seager, Sara, Winn, Joshua N.
Observing and characterizing young planetary systems can aid in unveiling the evolutionary mechanisms that sculpt the mature exoplanet population. As an all-sky survey, NASA's Transiting Exoplanet Survey Satellite (TESS) has expanded the known young
Externí odkaz:
http://arxiv.org/abs/2407.19680
Autor:
Korth, Judith, Chaturvedi, Priyanka, Parviainen, Hannu, Carleo, Ilaria, Endl, Michael, Guenther, Eike W., Nowak, Grzegorz, Persson, Carina, MacQueen, Phillip J., Mustill, Alexander J., Cabrera, Juan, Cochran, William D., Lillo-Box, Jorge, Hobbs, David, Murgas, Felipe, Greklek-McKeon, Michael, Kellermann, Hanna, Hébrard, Guillaume, Fukui, Akihiko, Pallé, Enric, Jenkins, Jon M., Twicken, Joseph D., Collins, Karen A., Quinn, Samuel N., Šubjak, Ján, Beck, Paul G., Gandolfi, Davide, Mathur, Savita, Deeg, Hans J., Latham, David W., Albrecht, Simon, Barrado, David, Boisse, Isabelle, Bouy, Hervé, Delfosse, Xavier, Demangeon, Olivier, García, Rafael A., Hatzes, Artie P., Heidari, Neda, Ikuta, Kai, Kabáth, Petr, Knutson, Heather A., Livingston, John, Martioli, Eder, Morales-Calderón, María, Morello, Giuseppe, Narita, Norio, Orell-Miquel, Jaume, Osborne, Hanna L. M., Palakkatharappil, Dinil B., Pinter, Viktoria, Redfield, Seth, Relles, Howard M., Schwarz, Richard P., Seager, Sara, Shporer, Avi, Skarka, Marek, Srdoc, Gregor, Stangret, Monika, Thomas, Luis, Van Eylen, Vincent, Watanabe, Noriharu, Winn, Joshua N.
We report the discovery and characterization of a small planet, TOI-1408 c, on a 2.2-day orbit located interior to a previously known hot Jupiter, TOI-1408 b ($P=4.42$ d, $M=1.86\pm0.02\,M_\mathrm{Jup}$, $R=2.4\pm0.5\,R_\mathrm{Jup}$) that exhibits g
Externí odkaz:
http://arxiv.org/abs/2407.17798
Autor:
Gaidos, E., Parviainen, H., Esparza-Borges, E., Fukui, A., Isogai, K., Kawauchi, K., de Leon, J., Mori, M., Murgas, F., Narita, N., Palle, E., Watanabe, N.
Context: Rocky planets on ultra-short period orbits can have surface magma oceans and rock-vapour atmospheres in which dust can condense. Observations of that dust can inform about the composition surface conditions on these objects. Aims: We constra
Externí odkaz:
http://arxiv.org/abs/2407.17372
Autor:
Konishi, Ayu, Muraoka, Kazuyuki, Tokuda, Kazuki, Fujita, Shinji, Fukui, Yasuo, Yamada, Rin I., Demachi, Fumika, Tachihara, Kengo, Kobayashi, Masato I. N., Kuno, Nario, Tsuge, Kisetsu, Sano, Hidetoshi, Miura, Rie E., Kawamura, Akiko, Onishi, Toshikazu
The evolution of giant molecular clouds (GMCs), the main sites of high-mass star formation, is an essential process to unravel the galaxy evolution. Using a GMC catalogue of M33 from ALMA-ACA survey, we classified 848 GMCs into three types based on t
Externí odkaz:
http://arxiv.org/abs/2407.17018
Autor:
Giles-Donovan, N., Chen, Y., Fukui, H., Manjo, T., Ishikawa, D., Baron, A. Q. R., Chi, S., Zhong, H., Cao, S., Tang, Y., Wang, Y., Lu, X., Song, Y., Birgeneau, R. J.
Employing inelastic X-ray scattering and neutron scattering techniques, we observed nematic and magnetic phase transitions with distinct characters in K$_{5}$Fe$_{4}$Ag$_{6}$Te$_{10}$. Upon cooling, the nematic order undergoes a strongly first-order
Externí odkaz:
http://arxiv.org/abs/2407.14706
Autor:
Rybicki, Krzysztof A., Shvartzvald, Yossi, Yee, Jennifer C., Novati, Sebastiano Calchi, Ofek, Eran O., Bond, Ian A., Beichman, Charles, Bryden, Geoff, Carey, Sean, Henderson, Calen, Zhu, Wei, Fausnaugh, Michael M., Wibking, Benjamin, Udalski, Andrzej, Poleski, Radek, Mróz, Przemek, Szymański, Michal K., Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Skowron, Jan, Ulaczyk, Krzysztof, Iwanek, Patryk, Wrona, Marcin, Ryu, Yoon-Hyun, Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Shin, In-Gu, Yang, Hongjing, Zang, Weicheng, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Abe, Fumio, Barry, Richard, Bennett, David P., Bhattacharya, Aparna, Fukui, Akihiko, Hamada, Ryusei, Hamada, Shunya, Hamasaki, Naoto, Hirao, Yuki, Silva, Stela Ishitani, Itow, Yoshitaka, Kirikawa, Rintaro, Koshimoto, Naoki, Matsubara, Yutaka, Miyazaki, Shota, Muraki, Yasushi, Nagai, Tutumi, NUNOTA, Kansuke, Olmschenk, Greg, Ranc, Clement, Rattenbury, Nicholas J., Satoh, Yuki K., Sumi, Takahiro, Suzuki, Daisuke, Tristram, Paul . J., Vandorou, Aikaterini, Yama, Hibiki, Wyrzykowski, Lukasz, Howil, Kornel, Kruszyńska, Katarzyna
In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of $\sim 950$ microlensing events observed by the Spitzer Space Telescope between 2014 and 2019. In this study we focus on a sub-sample of
Externí odkaz:
http://arxiv.org/abs/2407.13740
Autor:
Barber, Madyson G., Thao, Pa Chia, Mann, Andrew W., Vanderburg, Andrew, Mori, Mayuko, Livingston, John H., Fukui, Akihiko, Narita, Norio, Kraus, Adam L., Tofflemire, Benjamin M., Newton, Elisabeth R., Winn, Joshua N., Jenkins, Jon M., Seager, Sara, Collins, Karen A., Twicken, Joseph D.
The youngest ($<$50 Myr) planets are vital to understand planet formation and early evolution. The 17 Myr system HIP 67522 is already known to host a giant ($\simeq$10$R_\oplus$) planet on a tight orbit. In the discovery paper, Rizzuto et al. 2020 re
Externí odkaz:
http://arxiv.org/abs/2407.04763