-
PDF
- Split View
-
Views
-
Cite
Cite
Katsuki Muraoka, Naoto Kojiguchi, Junpei Ito, Daisaku Nogami, Taichi Kato, Yusuke Tampo, Kenta Taguchi, Keisuke Isogai, Teófilo Arranz, John Blackwell, David Blane, Stephen M Brincat, Graeme Coates, Walter Cooney, Shawn Dvorak, Charles Galdies, Daniel Glomski, Franz-Josef Hambsch, Barbara Harris, John Hodge, Jose L Hernández-Verdejo, Marco Iozzi, Hiroshi Itoh, Seiichiro Kiyota, Darrell Lee, Magnus Larsson, Tapio Lahtinen, Gordon Myers, Berto Monard, Mario Morales Aimar, Masayuki Moriyama, Masanori Mizutani, Kazuo Nagai, Thabet AlQaissieh, Aldrin B s Gabuya, Mohammad Odeh, Carlos Perello, Andrew Pearce, Juan Miguel Perales, David Quiles, Filipp D Romanov, David J Lane, Michael Richmond, Nello Ruocco, Yasuo Sano, Mark Spearman, Richard Schmidt, Tonny Vanmunster, Pavol A Dubovsky, Richard Wagner, Guido Wollenhaupt, Joachim Lorenz, Gerhard Lehmann, Andrea Salewski, Guy Williamson, Erratum: Optical and soft X-ray light-curve analysis during the 2022 eruption of U Scorpii: Structural changes in the accretion disk, Publications of the Astronomical Society of Japan, 2024;, psae034, https://doi.org/10.1093/pasj/psae034
Close - Share Icon Share
In the original version of article [Publ. Astron. Soc. Japan (2024) 76(2); https://doi.org/10.1093/pasj/psae010], the email address was incorrectly typed during the production process. The PDF and HTML versions of the original article are updated with the correct email address upon the publication of this erratum.
