papers

Publications (18)

cond-mat.str-el2020

Probing spin correlations using angle resolved photoemission in a coupled metallic/Mott insulator system

V. Sunko, F. Mazzola, S. Kitamura +16

A nearly free electron metal and a Mott insulating state can be thought of as opposite ends of possibilities for the motion of electrons in a solid. In the magnetic oxide metal PdC…

astro-ph.HE2009

Spin and Relativistic Phenomena Around Black Holes

L. Brenneman, J. M. Miller, K. Nandra +13

Since the seminal work of Penrose (1969) and Blandford & Znajek (1977), it has been realized that black hole spin may be an important energy source in astrophysics. The radio-loud/…

astro-ph.HE2013

Athena+: The first Deep Universe X-ray Observatory

D. Barret, K. Nandra, X. Barcons +31

The Advanced Telescope for High-energy Astrophysics (Athena+) is being proposed to ESA as the L2 mission (for a launch in 2028) and is specifically designed to answer two of the mo…

astro-ph2007

The XMM large scale structure survey: optical vs. X-ray classifications of active galactic nuclei and the unified scheme

O. Garcet, P. Gandhi, E. Gosset +25

Our goal is to characterize AGN populations by comparing their X-ray and optical classifications. We present a sample of 99 spectroscopically identified X-ray point sources in the…

astro-ph2002

The Galactic Plane Observed by XMM-Newton

A. Hands, R. Warwick, M. Watson +1

In A0-1 we proposed an ambitious long-term survey of selected regions of our Galaxy (the XGPS survey) using the EPIC CCD cameras on XMM-Newton. The first phase of the programme, wh…

astro-ph.HE2017

An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907

G. L. Israel, A. Belfiore, L. Stella +20

Ultraluminous x-ray sources (ULXs) in nearby galaxies shine brighter than any X-ray source in our Galaxy. ULXs are usually modeled as stellar-mass black holes (BHs) accreting at ve…