Tuğçe Kocabıyık

ORCID: 0000-0003-1188-4692
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About
Contact & Profiles
Research Areas
  • Pulsars and Gravitational Waves Research
  • High-pressure geophysics and materials
  • Astrophysical Phenomena and Observations
  • Spectroscopy Techniques in Biomedical and Chemical Research
  • Geophysics and Sensor Technology
  • Crystallography and Radiation Phenomena
  • Advanced Fiber Laser Technologies
  • Electron Spin Resonance Studies
  • Radio Astronomy Observations and Technology
  • Gamma-ray bursts and supernovae
  • Seismic Imaging and Inversion Techniques
  • Particle Accelerators and Free-Electron Lasers
  • Photoreceptor and optogenetics research
  • Blind Source Separation Techniques
  • Superconducting Materials and Applications

Istanbul University
2021-2025

Astronomy and Space
2025

We present a detailed spectral study of an intermittent-AMXP Aql X-1 during the \textit{pulse-on} and \textit{pulse-off} stages by using archival RXTE data. first perform temporal analysis Z$_n^2$ technique in three different energy bands, 3.0 -- 13.0~keV, 13.0 23.0~keV 23.0 33.0~keV, for last 128~s time segment data including region. show that pulse is most significant softest band. We, then, spectrum represented best via combination absorbed blackbody, disk blackbody gaussian line. modeled...

10.48550/arxiv.2501.04542 preprint EN arXiv (Cornell University) 2025-01-08

Abstract We present a detailed spectral study of an intermittent-AMXP Aql X-1 during the pulse-on and pulse-off stages by using archival RXTE data. first perform temporal analysis Z$_n^2$ technique in three different energy bands, 3.0 – 13.0 keV, 23.0 keV 33.0 for last 128 s time segment data including region. show that pulse is most significant softest band. We, then, spectrum represented best via combination absorbed blackbody, disk blackbody gaussian line. modeled four segments...

10.1093/mnras/staf041 article EN cc-by Monthly Notices of the Royal Astronomical Society 2025-01-09

We present a detailed systematic pulse search for three Intermittent-Accreting Millisecond X-ray Pulsars (Intermittent-AMXPs), HETE J1900.1-2455, SAX J1748.9-2021 & Aql X-1, via Z$_1^2$ and maximum likelihood (ML) techniques by using 16 years data of Rossi Timing Explorer/Proportional Counter Array (RXTE/PCA) in the energy range 3.0 - 13.0 keV. first performed scan technique millisecond sensitivities every 25 s time interval with 1 shifts to cover all set around detected frequencies given...

10.48550/arxiv.2502.03947 preprint EN arXiv (Cornell University) 2025-02-06

Abstract We report the temporal and spectral analysis of three thermonuclear X-ray bursts from 4U 1608−52, observed by Neutron Star Interior Composition Explorer (NICER) during just after outburst source in 2020. In two bursts, we detect secondary peaks 30 18 s initial peaks. The show a fast rise exponential decay-like shape resembling burst. Time-resolved reveals that peak flux, blackbody temperature, apparent emitting radius values are agreement with previously while same for tend toward...

10.3847/1538-4357/abe1ae article EN The Astrophysical Journal 2021-03-01
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