Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Gioia Rau"'
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 1, p 16 (2023)
The Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph treasury program Advanced Spectral Library enables investigations of the characteristics and dynamics of the wind and chromosphere of cool stars using high-quality spectral data. T
Externí odkaz:
https://doaj.org/article/94ea11525c32456d858f31d643a1ad92
Autor:
Greg Olmschenk, David P. Bennett, Ian A. Bond, Weicheng Zang, Youn Kil Jung, Jennifer C. Yee, Etienne Bachelet, Leading authors, Fumio Abe, Richard K. Barry, Aparna Bhattacharya, Hirosane Fujii, Akihiko Fukui, Yuki Hirao, Stela Ishitani Silva, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Naoki Koshimoto, Yutaka Matsubara, Sho Matsumoto, Shota Miyazaki, Brandon Munford, Yasushi Muraki, Arisa Okamura, Clément Ranc, Nicholas J. Rattenbury, Yuki Satoh, Takahiro Sumi, Daisuke Suzuki, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, The MOA Collaboration, Michael D. Albrow, Sang-Mok Cha, Sun-Ju Chung, Andrew Gould, Cheongho Han, Kyu-Ha Hwang, Dong-Jin Kim, Hyoun-Woo Kim, Seung-Lee Kim, Chung-Uk Lee, Dong-Joo Lee, Yongseok Lee, Byeong-Gon Park, Richard W. Pogge, Yoon-Hyun Ryu, In-Gu Shin, Yossi Shvartzvald, The KMTNet Collaboration, Grant Christie, Tony Cooper, John Drummond, Jonathan Green, Steve Hennerley, Jennie McCormick, L. A. G. Monard, Tim Natusch, Ian Porritt, Thiam-Guan Tan, The MicroFUN Collaboration, Shude Mao, Dan Maoz, Matthew T. Penny, Wei Zhu, The MAP Follow-Up Collaboration, V. Bozza, Arnaud Cassan, Martin Dominik, Markus Hundertmark, R. Figuera Jaimes, K. Kruszyńska, K. A. Rybicki, R. A. Street, Y. Tsapras, Joachim Wambsganss, Ł. Wyrzykowski, P. Zieliński, The OMEGA Collaboration, Gioia Rau
Publikováno v:
The Astronomical Journal, Vol 165, Iss 4, p 175 (2023)
We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass. With a mass ratio $q={3.17}_{-0.26}^{+0.28}\times {10}^{-4}$ , the
Externí odkaz:
https://doaj.org/article/7071297452874f4699f42ea1eb0bd198
Autor:
David T. Leisawitz, Taro Matsuo, Gregory Mosby, Peter A. R. Ade, Rachel Akeson, Dale J. Fixsen, Qian Gong, Hidehiro Kaneda, Stephen F. Maher, Lee G. Mundy, Shunsuke Ota, Gioia Rau, Elmer H. Sharp, Toru Shimokawa, Johannes G. Staguhn, Carole E. Tucker, Gerard T. van Belle
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI.
Autor:
Leonid Pogorelyuk, Paul Serra, Shreeyam Kacker, Sophia Vlahakis, Nicholas Belsten, Gioia Rau, Kenneth G. Carpenter, Laurent Pueyo, John D. Monnier, Ewan Douglas, Kerri Cahoy
Publikováno v:
Optical and Infrared Interferometry and Imaging VIII.
Autor:
Stefan Kraus, Eric Lagadec, E. Cannon, Florentin Millour, Guy Perrin, A. de Koter, John D. Monnier, Andrea Chiavassa, Xavier Haubois, Claudia Paladini, Narsireddy Anugu, Peter Scicluna, Andrea K. Dupree, L. Decin, Philippe Stee, Bruno Lopez, Gioia Rau, M. Montargès, William C. Danchi, K. Kravchenko, S. T. Ridgway, Ryan P. Norris, J. Sanchez-Bermudez, Pierre Kervella, Faustine Cantalloube, J-B. Le Bouquin, Markus Wittkowski
Publikováno v:
Nature
Nature, Nature Publishing Group, 2021, 594 (7863), pp.365-368. ⟨10.1038/s41586-021-03546-8⟩
Nature, 594(7863), 365-368. Nature Publishing Group
Nature, Nature Publishing Group, 2021, 594 (7863), pp.365-368. ⟨10.1038/s41586-021-03546-8⟩
Nature, 594(7863), 365-368. Nature Publishing Group
Red supergiants are the most common final evolutionary stage of stars that have initial masses between 8 and 35 times that of the Sun1. During this stage, which lasts roughly 100,000 years1, red supergiants experience substantial mass loss. However,
Autor:
Greg Olmschenk, David P. Bennett, Ian A. Bond, Weicheng Zang, Youn Kil Jung, Jennifer C. Yee, Etienne Bachelet, Fumio Abe, Richard K. Barry, Aparna Bhattacharya, Hirosane Fujii, Akihiko Fukui, Yuki Hirao, Stela Ishitani Silva, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Naoki Koshimoto, Yutaka Matsubara, Sho Matsumoto, Shota Miyazaki, Brandon Munford, Yasushi Muraki, Arisa Okamura, Clément Ranc, Nicholas J. Rattenbury, Yuki Satoh, Takahiro Sumi, Daisuke Suzuki, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Michael D. Albrow, Sang-Mok Cha, Sun-Ju Chung, Andrew Gould, Cheongho Han, Kyu-Ha Hwang, Dong-Jin Kim, Hyoun-Woo Kim, Seung-Lee Kim, Chung-Uk Lee, Dong-Joo Lee, Yongseok Lee, Byeong-Gon Park, Richard W. Pogge, Yoon-Hyun Ryu, In-Gu Shin, Yossi Shvartzvald, Grant Christie, Tony Cooper, John Drummond, Jonathan Green, Steve Hennerley, Jennie McCormick, L. A. G. Monard, Tim Natusch, Ian Porritt, Thiam-Guan Tan, Shude Mao, Dan Maoz, Matthew T. Penny, Wei Zhu, V. Bozza, Arnaud Cassan, Martin Dominik, Markus Hundertmark, R. Figuera Jaimes, K. Kruszyńska, K. A. Rybicki, R. A. Street, Y. Tsapras, Joachim Wambsganss, Ł. Wyrzykowski, P. Zieliński, Gioia Rau
We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass. With a mass ratio q = 3.17 − 0.26 + 0.28 × 10 − 4 , the plane
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b68fe9ba654959416d09800398273d1
Autor:
Stela Ishitani Silva, Clément Ranc, David P. Bennett, Ian A. Bond, Weicheng Zang, Fumio Abe, Richard K. Barry, Aparna Bhattacharya, Hirosane Fujii, Akihiko Fukui, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Naoki Koshimoto, Yutaka Matsubara, Sho Matsumoto, Shota Miyazaki, Yasushi Muraki, Greg Olmschenk, Arisa Okamura, Nicholas J. Rattenbury, Yuki Satoh, Takahiro Sumi, Daisuke Suzuki, Taiga Toda, Paul. J. Tristram, Aikaterini Vandorou, Hibiki Yama, Andreea Petric, Todd Burdullis, Pascal Fouqué, Shude Mao, Matthew T. Penny, Wei Zhu, Gioia Rau
Publikováno v:
The Astronomical Journal. 164:118
We report the light-curve analysis for the event MOA-2020-BLG-135, which leads to the discovery of a new Neptune-class planet, MOA-2020-BLG-135Lb. With a derived mass ratio of $q=1.52_{-0.31}^{+0.39} \times 10^{-4}$ and separation $s\approx1$, the pl
Autor:
Steven B. Charnley, Anthony F. J. Moffat, Laurent Loinard, Gioia Rau, Gerd Weigelt, Martin A. Cordiner, Noel D. Richardson, Augusto Damineli, M. Y. Palmer, Andrea Mehner, Thomas I. Madura, Patrick W. Morris, Jose H. Groh, Theodore R. Gull, Michael F. Corcoran
The complex circumstellar environment around the massive binary and luminous blue variable η Carinae is known to harbor numerous light molecules, emitting most strongly in rotational states with upper level energies to ~300 K. In circumstellar gas,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c9f132236469e1dfc31d4592f472b02
https://resolver.caltech.edu/CaltechAUTHORS:20200401-070803450
https://resolver.caltech.edu/CaltechAUTHORS:20200401-070803450
Autor:
Kenneth G, Carpenter, Gioia, Rau
Publikováno v:
Proceedings of the International Astronomical Union. International Astronomical Union.
Stencel et al. (1986) analyzed IUE spectra of a modest set of cool stars and found that they continue to produce chromospheres even in the presence of high dust levels in their outer atmospheres. This reversed the previous results of Jennings (1973)
Autor:
Gioia Rau, Stela Ishitani Silva, Ethan Kruse, Edward Wyrwas, Richard K. Barry, Brian P. Powell, Greg Olmschenk, Jeremy D. Schnittman, Veselin B. Kostov, Thomas Barclay, Luca Cacciapuoti
Publikováno v:
The Astronomical Journal. 161:273
The Transiting Exoplanet Survey Satellite (TESS) mission measured light from stars in ~75% of the sky throughout its two year primary mission, resulting in millions of TESS 30-minute cadence light curves to analyze in the search for transiting exopla