CRA Seminar: Dr. Stefano Marchesi (Clemson University)

Title: A multi-observatory X-ray approach to characterize heavily obscured AGNs According to the different models of Cosmic X-ray Background (CXB), the diffuse X-ray emission observed in the 1 to ~200-300 keV band, is mainly caused by accreting supermassive black holes, the so-called active Galactic Nuclei (AGN). Particularly, at the peak of the CXB (~30 keV) … Continue reading "CRA Seminar: Dr. Stefano Marchesi (Clemson University)"

CRA Seminar: Mahdi Bagheri (University of New Hampshire)

Monte Carlo Simulation and Balloon-Borne Observation of Energetic Radiations and Electromagnetic Fields from Thunderstorms and Lightning   Mahdi Bagheri Space Science Center and Physics Department, University of New Hampshire   Abstract: Lightning is one of the most energetic geophysical phenomena, producing the brightest light and loudest sound commonly occurring on Earth. Because of its high … Continue reading "CRA Seminar: Mahdi Bagheri (University of New Hampshire)"

CRA Cosmic Coffee: Mathilda Avirett-Mackenzie

Howey N201/202 837 State Street, Atlanta, GA, United States

Title: The Evolving X-ray Spectrum of Active Galactic Nuclei Abstract: The cosmic X-ray background (XRB) spectrum and active galaxy number counts encode essential information about the spectral evolution of active galactic nuclei (AGNs) and have been successfully modeled by XRB synthesis models for many years. Recent measurements of the 8–24 keV AGN number counts by … Continue reading "CRA Cosmic Coffee: Mathilda Avirett-Mackenzie"

CRA seminar: Prof. Shane Davis (University of Virginia)

Title: How Black Holes Dine above the Eddington "Limit" without Overeating or Excessive Belching Abstract The study of super-Eddington accretion is essential to our understanding of the growth of super-massive black holes in the early universe, the accretion of tidally disrupted stars, and the nature of ultraluminous X-ray sources. Unfortunately, this mode of accretion is … Continue reading "CRA seminar: Prof. Shane Davis (University of Virginia)"

CRA Seminar: Prof. Huan Yang (Perimeter Institute)

Probing neutron star physics with gravitational wave detections The recent detection of the binary neutron star merger event (GW170817) has marked the beginning of multi-messenger astronomy with gravitational waves. In this talk I will briefly review current findings associated with GW170817 and introduce new opportunities from future detections. In the first part, I will explain … Continue reading "CRA Seminar: Prof. Huan Yang (Perimeter Institute)"