Luke Filor

ORCID: 0009-0004-9156-7893
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About
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Research Areas
  • Astrophysical Phenomena and Observations
  • Astronomical Observations and Instrumentation
  • Mechanics and Biomechanics Studies
  • Pulsars and Gravitational Waves Research
  • Astrophysics and Star Formation Studies

We aim at characterizing the population of low-luminosity X-ray sources in Galactic plane by studying their spectra and periodic signals light curves. are performing an survey disk using XMM-Newton, source XMMU J173029.8-330920 was serendipitously discovered our campaign. performed a follow-up observation pre-approved NuSTAR target opportunity time. used various phenomenological models xspec for spectral modeling. also computed Lomb-Scargle periodogram to search periodicity. A Monte Carlo...

10.48550/arxiv.2407.03025 preprint EN arXiv (Cornell University) 2024-07-03

Aims. We aim to characterise the population of low-luminosity X-ray sources in Galactic plane by studying their spectra and periodic signals light curves. Methods. are performing an survey disc using XMM-Newton , source XMMU J173029.8–330920 was serendipitously discovered our campaign. performed a follow-up observation pre-approved NuSTAR target opportunity time. used various phenomenological models XSPEC for spectral modelling. also computed Lomb-Scargle periodogram search periodicity. A...

10.1051/0004-6361/202449228 article EN cc-by Astronomy and Astrophysics 2024-07-23

We present the first $\textit{NuSTAR}$ X-ray observation of EF Eri, a well-known polar system. The was conducted in conjunction with $\textit{NICER}$, shortly after Eri entered high accretion state following an unprecedented period low activity lasting 26 years since 1997. detected hard emission up to 50 keV flux $1.2\times10^{-10}$ ergs s$^{-1}$ cm$^{-2}$ ($3\rm{-}50 keV$). Folded lightcurves exhibit single peak $\sim65\%$ spin modulation throughout $3\rm{-}50$ band. found no evidence QPO...

10.48550/arxiv.2412.11273 preprint EN arXiv (Cornell University) 2024-12-15
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