K. Miike (Miyazaki U.), H. Negoro (Nihon U.), Y. Kawakubo (LSU),
M. Nakajima, M. Aoki, K. Kobayashi, R. Takagi, K, Asakura,
K, Seino, S. Mokumoto (Nihon U.),
T. Mihara, C. Guo, Y. Zhou, T. Tamagawa, M. Matsuoka (RIKEN),
T. Sakamoto, M. Serino, S. Sugita, H. Nishida, A. Yoshida (AGU),
Y. Tsuboi, W. Iwakiri, R. Sasaki, H. Kawai, Y. Okamoto, S. Kitakoga (Chuo U.),
M. Shidatsu (Ehime U.), N. Kawai, R. Adachi, M. Niwano (Tokyo Tech),
S. Nakahira, Y. Sugawara, S. Ueno, H. Tomida, M. Ishikawa, M. Tominaga, T. Nagatsuka (JAXA),
Y. Ueda, S. Yamada, S. Ogawa, K. Setoguchi, T. Yoshitake (Kyoto U.),
H. Tsunemi (Osaka U.), M. Yamauchi, K. Kurogi (Miyazaki U.),
T. Kawamuro (NAOJ), K. Yamaoka (Nagoya U.), M. Sugizaki (NAOC)
report on behalf of the MAXI team:
The MAXI/GSC nova alert system triggered on an uncatalogued X-ray transient source
at 10:30:18 UT on 2020 June 15.
Assuming that the source flux was constant over the transit,
we obtain the source position at
(R.A., Dec) = (153.421 deg, -5.158 deg) = (10 13 41, -05 09 28) (J2000)
with a statistical 90% C.L. elliptical error region
with long and short radii of 0.34 deg and 0.3 deg, respectively.
The roll angle of the long axis from the north direction is 180.0 deg counterclockwise.
Without assumptions on the source flux constancy, we obtain a rectangular error
box for the transient source with the following corners:
(R.A., Dec) = (152.024, -3.311) deg = (10 08 05, -03 18 39) (J2000)
(R.A., Dec) = (151.564, -3.753) deg = (10 06 15, -03 45 10) (J2000)
(R.A., Dec) = (153.538, -5.793) deg = (10 14 09, -05 47 34) (J2000)
(R.A., Dec) = (153.998, -5.350) deg = (10 15 59, -05 20 59) (J2000)
There is an additional systematic uncertainty of 0.1 deg (90% containment radius)
in both error regions.
The X-ray flux averaged over the scan was 85 +- 19 mCrab
(4.0-10.0keV, 1 sigma error).
There was no significant excess flux in the previous transit at 08:57 UT
and in the next transit at 12:03 UT with an upper limit of 20 mCrab for each.