The Cosmic History of Black Hole Growth from Deep Multiwavelength Surveys

We construct a one-loop effective metric describing the evaporation phase of a Schwarzschild black hole in a spherically symmetric null- dust model.. This is achieved by quantising

As a first step, we verify the analysis procedure using simu- lated point-like sources with the computed spectra correspond- ing to (1) the inner part of the lunar disk (the total

In this article we compute explicitly the first-order α 0 (fourth order in derivatives) corrections to the charge-to-mass ratio of the extremal Reissner-Nordstr¨ om black hole

• Analysis of long-term variability of high-energy sources in the optical and X-ray bands, using INTEGRAL observations from IBIS (the gamma-ray imager), JEM-X (the X-ray monitor)

The difficulty stems from the fact that the measurement of orbits at the Galactic center requires understanding 5 major components: (1) the astrophysical content near the black

These properties of the LIGO black hole binaries would come naturally from early universe models of PBH formation from large peaks in the matter power spectrum, arising both in

Díaz Soto has raised the point about banning religious garb in the ―public space.‖ He states, ―for example, in most Spanish public Universities, there is a Catholic chapel

By measuring the two-point correlation function of galaxy populations that differ in redshift, color, luminosity, star-formation history and bias, and using high-resolution