output
20032009
most citedFirst direct observation of Spin-textures in Topological Insulators : Spin-resolved ARPES as a probe of topological quantum spin Hall effect and Berry's phase

1.3k citations

Showing 2006Show all

51 papers · 1 filter

physics.ins-det200635 cited

A Vertex Trigger based on Cylindrical Multiwire Proportional Chambers

J. Becker, K. Bösiger, L. Lindfeld +14

The article describes the technical implementation and the performance of the z-vertex trigger (CIP2k), which is part of the H1-experiment at HERA.

hep-ph20068 cited

Heavy neutral MSSM Higgs Bosons at the PLC - a comparison of two analyses

M. Spira, P. Niezurawski, M. Krawczyk +1

Measurement of the heavy neutral MSSM Higgs bosons H and A production in the process gamma gamma --> A, H --> b anti-b at the Photon Linear Collider has been considered in two inde…

astro-ph200694 cited

X-rays from T Tau: A test case for accreting T Tauri stars

M. Guedel, S. L. Skinner, S. Yu. Mel'nikov +3

We test models for the generation of X-rays in accreting T Tauri stars (TTS), using X-ray data from the classical TTS T Tau. High-resolution spectroscopy from the Reflection Gratin…

astro-ph200644 cited

A nanoflare model of quiet Sun EUV emission

Anuschka Pauluhn, Sami K. Solanki

Nanoflares have been proposed as the main source of heating of the solar corona. However, detecting them directly has so far proved elusive, and extrapolating to them from the prop…

astro-ph200616 cited

Hard X-rays and Fluorescent Iron Emission from the Embedded Infrared Cluster in NGC 2071

Stephen L. Skinner, Audrey E. Simmons, Marc Audard +1

We present first results of XMM-Newton X-ray observations of the infrared cluster lying near the NGC 2071 reflection nebula in the Orion B region. This cluster is of interest becau…

astro-ph2006158 cited

X-ray Emission from T Tauri Stars and the Role of Accretion: Inferences from the XMM-Newton Extended Survey of the Taurus Molecular Cloud

A. Telleschi, M. Guedel, K. R. Briggs +2

T Tau stars display different X-ray properties depending on whether they are accreting (classical T Tau stars; CTTS) or not (weak-line T Tau stars; WTTS). We use data from the XMM-…