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Thermonuclear Superburst of MAXI J1752−457 Observed with NinjaSat and MAXI

  • Authors: Amira Aoyama, Teruaki Enoto, Takuya Takahashi, Sota Watanabe, Tomoshi Takeda, Wataru Iwakiri, Kaede Yamasaki, Satoko Iwata, Naoyuki Ota, Arata Jujo, Toru Tamagawa, Tatehiro Mihara, Chin-Ping Hu, Akira Dohi, Nobuya Nishimura, Motoko Serino, Motoki Nakajima, Takao Kitaguchi, Yo Kato, Nobuyuki Kawai

Amira Aoyama et al 2025 The Astrophysical Journal Letters 986 .

  • Provider: AAS Journals

Caption: Figure 3.

The fitted X-ray spectra of MAXI/GSC and NinjaSat/GMC using the absorbed blackbody model. The time spans A, B, and C correspond to MAXI/GSC, with no markers. The time spans D, F, and H correspond to NinjaSat/GMC, represented by circular markers. The time spans are shown in Figure 2(a). The upper panel displays the unfolded spectrum, while the lower panel shows the ratio of the data to the best-fitting model (see Table 1).

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