Unveiling the Nature of Superorbital Modulation of SMC X-1 using NinjaSat
Chin-Ping Hu, Naoyuki Ota, Takuya Takahashi, Tomoshi Takeda, Teruaki Enoto, Toru Tamagawa, Biswajit Paul, Sota Watanabe, Wataru Iwakiri, Tatehiro Mihara, Amira Aoyama, Satoko Iwata, Kaede Yamasaki, Takayuki Kita, Soma Tsuchiya, Mayu Ichibakase

TL;DR
This study uses NinjaSat CubeSat observations to analyze the superorbital modulation of SMC X-1, revealing that the modulation is mainly geometric, with stable spectral properties and variable pulse profiles, demonstrating CubeSat's scientific potential.
Contribution
First complete measurement of spin-up rate and spectral evolution across a superorbital cycle in SMC X-1 using CubeSat data, indicating geometric obscuration as the primary modulation mechanism.
Findings
Spin-up rate remains consistent during high states.
Spectral shape is stable throughout the cycle.
Pulse profile varies with superorbital phase.
Abstract
We report a long-term, high-cadence timing and spectral observation of the X-ray pulsar SMC X-1 using NinjaSat, a 6U CubeSat in low-Earth orbit, covering nearly a full superorbital cycle. SMC X-1 is a high-mass X-ray binary exhibiting a 0.7 s X-ray pulsar and a non-stationary superorbital modulation with periods ranging from approximately 40 to 65 days. Its peak luminosity of ~\lumcgs\ makes it a local analogue of ultraluminous X-ray pulsars powered by supercritical accretion. We find that the spin-up rate during the high state remains consistent with the long-term average, with no significant correlation between spin-up rate and flux. This result indicates that the modulation is primarily geometric rather than accretion-driven. The hardness ratio and spectral shape are stable throughout the entire superorbital cycle, supporting obscuration by optically thick material…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Astronomy and Astrophysical Research
