MAXI/GSC upper limit of SN 2023ixf in M 101
ATel #16044; N. Kawai (RIKEN), M. Serino (AGU), H. Negoro (Nihon U.), T. Mihara (RIKEN), M. Nakajima, K. Kobayashi, M. Tanaka, Y. Soejima, Y. Kudo (Nihon U.), T. Kawamuro, S. Yamada, T. Tamagawa, M. Matsuoka (RIKEN), T. Sakamoto, M. Serino, S. Sugita, H. Hiramatsu, H. Nishikawa, A. Yoshida (AGU), Y. Tsuboi, S. Urabe, S. Nawa, N. Nemoto (Chuo U.), M. Shidatsu (Ehime U.), I. Takahashi, M. Niwano, S. Sato, N. Higuchi, Y. Yatsu (Tokyo Tech), S. Nakahira, S. Ueno, H. Tomida, M. Ishikawa, S. Ogawa, T. Kurihara (JAXA), Y. Ueda, K. Setoguchi, T. Yoshitake, Y. Nakatani (Kyoto U.), M. Yamauchi, Y. Hagiwara, Y. Umeki, Y. Otsuki (Miyazaki U.), K. Yamaoka (Nagoya U.), Y. Kawakubo (LSU), M. Sugizaki (NAOC), W. Iwakiri (Chiba U.) report on behalf of the MAXI team:
on 22 May 2023; 13:24 UT
Credential Certification: Tatehiro Mihara (mihara@crab.riken.jp)
Subjects: X-ray, Supernovae
Referred to by ATel #: 16060
We report the X-ray upper limits of SN 2023ixf in M 101 observed with MAXI/GSC.
MJD of the scan, 1-sigma upper limits in 2-10 keV,
60079.565351 <12 mCrab,
60082.725611 <12 mCrab.
Each scan is for about 60 seconds.
The observation condition for M 101 around the explosion time was not good.
There was no observation between the two data and after the second one.