NICER Discovery that SRGA J144459.2–604207 Is an Accreting Millisecond X-Ray Pulsar
Chakrabarty, Deepto; Ray, Paul S.; Wolff, Michael T.; Arzoumanian, Zaven; Guillot, Sebastien; Buisson, D. J. K.; Papitto, Alessandro; Güver, Tolga; Hare, Jeremy; Ferrara, Elizabeth C.; Altamirano, Diego; Sanna, Andrea; Jaisawal, Gaurava K.; Gendreau, Keith C.; Malacaria, Christian; Ng, Mason; Strohmayer, Tod E.; Illiano, Giulia; Boztepe, Tuğba; Albayati, Arianna C.
United States, Italy, United Kingdom, Turkey, France, Denmark, Switzerland
Abstract
We present the discovery, with the Neutron Star Interior Composition Explorer (NICER), that SRGA J144459.2‑604207 is a 447.9 Hz accreting millisecond X-ray pulsar (AMXP), which underwent a 4 week long outburst starting on 2024 February 15. The AMXP resides in a 5.22 hr binary, orbiting a low-mass companion donor with M d > 0.1 M ⊙. We report on the temporal and spectral properties from NICER observations during the early days of the outburst, from 2024 February 21 through 2024 February 23, during which NICER also detected a type I X-ray burst that exhibited a plateau lasting ∼6 s. The spectra of the persistent emission were well described by an absorbed thermal blackbody and power-law model, with blackbody temperature kT ≈ 0.9 keV and power-law photon index Γ ≈ 1.9. Time-resolved burst spectroscopy confirmed the thermonuclear nature of the burst, where an additional blackbody component reached a maximum temperature of nearly kT ≈ 3 keV at the peak of the burst. We discuss the nature of the companion as well as the type I X-ray burst.