Zobrazeno 1 - 10
of 68
pro vyhledávání: '"Hsiao Hsiang-Yao"'
Autor:
Chen, Ting-Wan, Yang, Sheng, Srivastav, Shubham, Moriya, Takashi J., Smartt, Stephen J., Rest, Sofia, Rest, Armin, Lin, Hsing Wen, Miao, Hao-Yu, Cheng, Yu-Chi, Aryan, Amar, Cheng, Chia-Yu, Fraser, Morgan, Huang, Li-Ching, Lee, Meng-Han, Lai, Cheng-Han, Liu, Yu Hsuan, K, Aiswarya Sankar., Smith, Ken W., Stevance, Heloise F., Wang, Ze-Ning, Anderson, Joseph P., Angus, Charlotte R., de Boer, Thomas, Chambers, Kenneth, Duan, Hao-Yuan, Erasmus, Nicolas, Gao, Hua, Herman, Joanna, Hou, Wei-Jie, Hsiao, Hsiang-Yao, Huber, Mark E., Lin, Chien-Cheng, Lin, Hung-Chin, Magnier, Eugene A., Man, Ka Kit, Moore, Thomas, Ngeow, Chow-Choong, Nicholl, Matt, Ou, Po-Sheng, Pignata, Giuliano, Shiau, Yu-Chien, Sommer, Julian Silvester, Tonry, John L., Wang, Xiao-Feng, Young, David R., Yeh, You-Ting, Zhang, Jujia
We present the discovery and early observations of the nearby Type II supernova (SN) 2024ggi in NGC 3621 at 6.64 +/- 0.3 Mpc. The SN was caught 5.8 (+1.9 -2.9) hours after its explosion by the ATLAS survey. Early-phase, high-cadence, and multi-band p
Externí odkaz:
http://arxiv.org/abs/2406.09270
Autor:
Dietrich, Jeremy, Apai, Dániel, Schlecker, Martin, Hardegree-Ullman, Kevin K., Rackham, Benjamin V., Kurtovic, Nicolas, Molaverdikhani, Karan, Gabor, Paul, Henning, Thomas, Chen, Wen-Ping, Mancini, Luigi, Bixel, Alex, Gibbs, Aidan, Boyle, Richard P., Brown-Sevilla, Samantha, Burn, Remo, Delage, Timmy N., Flores-Rivera, Lizxandra, Franceschi, Riccardo, Pichierri, Gabriele, Savvidou, Sofia, Syed, Jonas, Bruni, Ivan, Ip, Wing-Huen, Ngeow, Chow-Choong, Tsai, An-Li, Lin, Chia-Lung, Hou, Wei-Jie, Hsiao, Hsiang-Yao, Lin, Chi-Sheng, Lin, Hung-Chin, Basant, Ritvik
Earth-sized exoplanets that transit nearby, late spectral type red dwarfs will be prime targets for atmospheric characterization in the coming decade. Such systems, however, are difficult to find via wide-field transit surveys like Kepler or TESS. Co
Externí odkaz:
http://arxiv.org/abs/2302.04138
Autor:
Hasegawa, Sunao, Kuroda, Daisuke, Kitazato, Kohei, Kasuga, Toshihiro, Sekiguchi, Tomohiko, Takato, Naruhisa, Aoki, Kentaro, Arai, Akira, Choi, Young-Jun, Fuse, Tetsuharu, Hanayama, Hidekazu, Hattori, Takashi, Hsiao, Hsiang-Yao, Kashikawa, Nobunari, Kawai, Nobuyuki, Kawakami, Kyoko, Kinoshita, Daisuke, Larson, Steve, Lin, Chi-Sheng, Miyasaka, Seidai, Miura, Naoya, Nagayama, Shogo, Nagumo, Yu, Nishihara, Setsuko, Ohba, Yohei, Ohta, Kouji, Ohyama, Youichi, Okumura, Shin-Ichiro, Sarugaku, Yuki, Shimizu, Yasuhiro, Takagi, Yuhei, Takahashi, Jun, Toda, Hiroyuki, Urakawa, Seitaro, Usui, Fumihiko, Watanabe, Makoto, Weissman, Paul, Yanagisawa, Kenshi, Yang, Hongu, Yoshida, Michitoshi, Yoshikawa, Makoto, Ishiguro, Masateru, Abe, Masanao
Sample return from the near-Earth asteroid known as 25143 Itokawa was conducted as part of the Hayabusa mission, with a large number of scientific findings being derived from the returned samples. Following the Hayabusa mission, Hayabusa2 was planned
Externí odkaz:
http://arxiv.org/abs/1810.03706
Autor:
Kato, Taichi, Ishioka, Ryoko, Isogai, Keisuke, Kimura, Mariko, Imada, Akira, Miller, Ian, Masumoto, Kazunari, Nishino, Hirochika, Kojiguchi, Naoto, Kawabata, Miho, Sakai, Daisuke, Sugiura, Yuki, Furukawa, Hisami, Yamamura, Kenta, Kobayashi, Hiroshi, Matsumoto, Katsura, Wang, Shiang-Yu, Chou, Yi, Ngeow, Chow-Choong, Chen, Wen-Ping, Panwar, Neelam, Lin, Chi-Sheng, Hsiao, Hsiang-Yao, Guo, Jhen-Kuei, Lin, Chien-Cheng, Omarov, Chingis, Kusakin, Anatoly, Krugov, Maxim, Starkey, Donn R., Pavlenko, Elena P., Antonyuk, Kirill A., Sosnjvskij, Aleksei A., Antonyuk, Oksana I., Pit, Nikolai V., Baklanov, Alex V., Babina, Julia V., Itoh, Hiroshi, Padovan, Stefano, Akazawa, Hidehiko, Kafka, Stella, de Miguel, Enrique, Pickard, Roger D., Kiyota, Seiichiro, Shugarov, Sergey Yu., Chochol, Drahomir, Krushevska, Viktoriia, Sekeras, Matej, Pikalova, Olga, Sabo, Richard, Dubovsky, Pavol A., Kudzej, Igor, Ulowetz, Joseph, Dvorak, Shawn, Stone, Geoff, Tordai, Tamas, Dubois, Franky, Logie, Ludwig, Rau, Steve, Vanaverbeke, Siegfried, Vanmunster, Tonny, Oksanen, Arto, Maeda, Yutaka, Kasai, Kiyoshi, Katysheva, Natalia, Morelle, Etienne, Neustroev, Vitaly V., Sjoberg, George
We observed RZ LMi, which is renowned for the extremely (~19d) short supercycle and is a member of a small, unusual class of cataclysmic variables called ER UMa-type dwarf novae, in 2013 and 2016. In 2016, the supercycles of this object substantially
Externí odkaz:
http://arxiv.org/abs/1609.08791
Autor:
Ngeow, Chow-Choong, Lee, Chien-Hsiu, Yang, Michael Ting-Chang, Lin, Chi-Sheng, Hsiao, Hsiang-Yao, Cheng, Yu-Chi, Lin, Zhong-Yi, Lin, I-Ling, Kanbur, Shashi M., Ip, Wing-Huen
The ultra-long period Cepheids (ULPCs) are classical Cepheids with pulsation periods exceeding $\approx 80$ days. The intrinsic brightness of ULPCs are ~1 to ~3 mag brighter than their shorter period counterparts. This makes them attractive in future
Externí odkaz:
http://arxiv.org/abs/1501.02456
Publikováno v:
2022 IEEE 24th Electronics Packaging Technology Conference (EPTC).
Publikováno v:
2022 IEEE 24th Electronics Packaging Technology Conference (EPTC).
Publikováno v:
2022 IEEE 24th Electronics Packaging Technology Conference (EPTC).
Publikováno v:
2022 IEEE 24th Electronics Packaging Technology Conference (EPTC).
Autor:
Soon Wee Ho, Hsiao Hsiang-Yao, Lau Boon Long, Sharon Lim Pei Siang, Lim Teck Guan, Chai Tai Chong
Publikováno v:
2022 IEEE 72nd Electronic Components and Technology Conference (ECTC).