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MAXI/GSC detection of new outbursts from Swift J1753.5-0127 and RX J1709.5-2639 (XTE J1709-267)

ATel #16283; H. Negoro (Nihon U.), S. Ogawa (JAXA), S. Urabe (Chuo U.), M. Nakajima, K. Kobayashi, M. Tanaka, Y. Soejima, Y. Kudo (Nihon U.), T. Mihara, T. Kawamuro, S. Yamada, T. Tamagawa, N. Kawai, M. Matsuoka (RIKEN), T. Sakamoto, M. Serino, S. Sugita, H. Hiramatsu, H. Nishikawa, A. Yoshida (AGU), Y. Tsuboi, S. Nawa, N. Nemoto, E. Goto (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, T. Kurihara (JAXA), Y. Ueda, K. Setoguchi, T. Yoshitake, Y. Nakatani, Y. Okada (Kyoto U.), M. Yamauchi, Y. Hagiwara, Y. Umeki, Y. Otsuki (Miyazaki U.), K. Yamaoka (Nagoya U.), Y. Kawakubo (LSU), M. Sugizaki (NAOC), and W. Iwakiri (Chiba U.)
on 12 Oct 2023; 05:44 UT
Credential Certification: Hitoshi Negoro (negoro@phys.cst.nihon-u.ac.jp)

Subjects: X-ray, Black Hole, Neutron Star, Transient

Referred to by ATel #: 16308, 16314, 16427

The MAXI/GSC nova alert system triggered on X-ray increase from the black hole X-ray binary Swift J1753.5-0127 at 01:09 (UT) on October 12, 2023. This new outburst from Swift J1753.5-0127 was first detected in optical with the LCO network on September 28 (ATel #16262). Faint X-ray emission less than 1 mCrab was detected from October 1 to 5 with Chandra/ACIS-S and Swift/XRT (ATel #16272), and radio emission was also observed on October 6 (ATel #16281).

The source has been slightly visible since October 6 with the GSC. Average 2-4 keV and 4-10 keV X-ray fluxes from October 6 to 11 are (1.3+/-0.3)e-2 photons/cm2/s (~6 mCrab) and (0.3+/0.3)e-2 photons/cm2/s (~3 mCrab), respectively. No rapid increase was observed during the period.

The alert system also triggered on a new X-ray outburst from the low-mass X-ray binary RX J1709.5-2639 (AKA XTE J1709-267) at 14:23 (UT) on October 9, 2023. The source flux is rapidly increasing and currently about 30-40 mCrab in the 2-10 keV band. RX J1709.5-2639 exhibited outbursts every 2-3 years, and this is the 7th detection of outbursts from this source with the MAXI/GSC. The last outburst was on September, 2020 (ATel #14047).

MAXI data of Swift J1753.5-0127