X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

Kavli Affiliate: Fukun Liu| Summary: We present a multi-epoch study of the extreme X-ray variability of the type~1 quasar SDSS~J000532.84+200717.4 using archival observations from textitXMM-Newton, textitSwift/XRT, textitEP-FXT, and textitROSAT, together with new optical spectroscopy and multi-wavelength photometry. The 0.2–10~keV X-ray flux exhibits a transition from a high state to a subsequent low state, declining by […]


Continue.. X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

Kavli Affiliate: Fukun Liu| Summary: We present a multi-epoch study of the extreme X-ray variability of the type~1 quasar SDSS~J000532.84+200717.4 using archival observations from textitXMM-Newton, textitSwift/XRT, textitEP-FXT, and textitROSAT, together with new optical spectroscopy and multi-wavelength photometry. The 0.2–10~keV X-ray flux exhibits a transition from a high state to a subsequent low state, declining by […]


Continue.. X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

Kavli Affiliate: Fukun Liu| Summary: We present a multi-epoch study of the extreme X-ray variability of the type~1 quasar SDSS~J000532.84+200717.4 using archival observations from textitXMM-Newton, textitSwift/XRT, textitEP-FXT, and textitROSAT, together with new optical spectroscopy and multi-wavelength photometry. The 0.2–10~keV X-ray flux exhibits a transition from a high state to a subsequent low state, declining by […]


Continue.. X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

A Novel Method to Construct Frequency-Domain Gravitational Waveform for Accelerating Sources

Kavli Affiliate: Xian Chen| Summary: Accurately modeling the inspiral-merger-ringdown (IMR) signal of coalescing compact objects is essential for the test of general relativity. However, it is known that astrophysical environments can distort gravitational-wave (GW) signal and, if ignored, may bias parameter estimation or even our understanding of gravity. Previous studies suggest that various astrophysical environmental […]


Continue.. A Novel Method to Construct Frequency-Domain Gravitational Waveform for Accelerating Sources

High dimensional alpha test for linear factor pricing model with $L_q$-norm

Kavli Affiliate: Feng Long| Summary: We consider testing zero pricing errors in high-dimensional linear factor pricing models. Existing methods are mainly based on either an $L_2$ statistic, which is effective under dense alternatives, or an $L_infty$ statistic, which is powerful under very sparse alternatives. To bridge these two regimes, we develop a class of $L_q$-based […]


Continue.. High dimensional alpha test for linear factor pricing model with $L_q$-norm

Direct N-body simulations of rotating and extremely massive Population III star clusters

Kavli Affiliate: Rainer Spurzem | Summary:Aims. We present eight direct N-body simulations with NBODY6++GPU of extremely massive, initially rotating Population III star clusters with 1.01 x 10^5 stars. Methods. Our models include primordial binaries, a continuous initial mass function, differential rotation, tidal mass loss, updated fitting formulae for extremely massive metal-poor Population III stars, and […]


Continue.. Direct N-body simulations of rotating and extremely massive Population III star clusters

Direct N-body simulations of rotating and extremely massive Population III star clusters

Kavli Affiliate: Rainer Spurzem | Summary:Aims. We present eight direct N-body simulations with NBODY6++GPU of extremely massive, initially rotating Population III star clusters with 1.01 x 10^5 stars. Methods. Our models include primordial binaries, a continuous initial mass function, differential rotation, tidal mass loss, updated fitting formulae for extremely massive metal-poor Population III stars, and […]


Continue.. Direct N-body simulations of rotating and extremely massive Population III star clusters

Formation and disruption of wide binaries in star clusters revealed by N-body simulations

Kavli Affiliate: Rainer Spurzem | Summary:Wide (soft) binaries are expected to be rapidly disrupted in dense stellar environments, yet they are observed in both the Galactic field and open clusters (OCs). In this paper, we investigate the formation and disruption of wide binaries in star clusters using direct N-body simulations. We perform simulations containing 10,000 […]


Continue.. Formation and disruption of wide binaries in star clusters revealed by N-body simulations

Formation and disruption of wide binaries in star clusters revealed by N-body simulations

Kavli Affiliate: Rainer Spurzem | Summary:Wide (soft) binaries are expected to be rapidly disrupted in dense stellar environments, yet they are observed in both the Galactic field and open clusters (OCs). In this paper, we investigate the formation and disruption of wide binaries in star clusters using direct N-body simulations. We perform simulations containing 10,000 […]


Continue.. Formation and disruption of wide binaries in star clusters revealed by N-body simulations

The cold molecular gas regulates the activity of active galactic nuclei in massive galaxies

Kavli Affiliate: Luis Ho | Summary:The physical quantities that directly regulate AGN feedback in massive galaxies remain poorly understood. Observations of molecular gas surrounding AGNs suggest that this gas serves as a fuel source for AGN activity. Accordingly, we study the relationship between AGN activity and molecular gas properties. In this study, we analyze a […]


Continue.. The cold molecular gas regulates the activity of active galactic nuclei in massive galaxies