collaborators

6 papers

astro-ph.HE2026

Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613

Ruican Ma, Federico Vincentelli, Diego Altamirano +5

We present a timing analysis of the black hole transient Swift J1727.8-1613 during its intermediate state. We use coordinated broadband X-ray observations from Insight-HXMT (2-150…

astro-ph.HE2026

Discovery of a quasi-periodic oscillation non-harmonically related to the Type-C QPO in the hard intermedidate state of MAXI J1820+070

Pei Jin, Mariano Méndez, Federico García +2

We present a detailed timing analysis of the transition from the hard-intermediate state (HIMS) to the soft-intermediate state (SIMS) in MAXI J1820+070 using NICER observations. Th…

astro-ph.HE2026

Multiwavelength Analysis of the Einstein Probe X-ray Transient EP240305a

Ruican Ma, Ye Li, Lian Tao +32

We report multiwavelength observations of EP240305a, an uncatalogued X-ray transient detected by the Einstein Probe on March 5, 2024. The source exhibits distinct characteristics a…

astro-ph.HE2026

Unveiling hidden millihertz quasi-periodic oscillations in 1A 0535+262

Zihan Yang, Ruican Ma, Mariano Méndez +9

Be/X-ray binary pulsars show transient outbursts and complex timing behaviour, including millihertz quasi-periodic oscillations (QPOs), whose physical origin and energy dependence…

astro-ph.HE2025

Gaussian process analysis of type-B quasiperiodic oscillations in the black hole X-ray binary MAXI J1348-630

Yiran Wang, Ruican Ma, Haiyun Zhang +1

We analyzed Insight-HXMT data of the black hole X-ray binary MAXI J1348-630 during the type-B QPO phase of its 2019 outburst. Using the Gaussian process method, we applied an addit…

astro-ph.HE2025

The nature of an imaginary quasi-periodic oscillation in the soft-to-hard transition of MAXI J1820+070

Candela Bellavita, Mariano Méndez, Federico García +2

A recent study shows that if the power spectra (PS) of accreting compact objects consist of a combination of Lorentzian functions that are coherent in different energy bands but in…