research


Introduction

Since 1999, I have been employed at NASA's Goddard Space Flight Center, where I have been involved in the operations and data analysis of the XMM-Newton X-ray/UV/optical satellite observatory and, most-recently, with the development of the Swift gamma-ray burst mission. This working environment has also resulted in expertise with the current Chandra and RXTE missions, and familiarity with the upcoming Astro E2 and Constellation-X projects. This fleet of space missions provides a host of exciting teaching and research opportunities for university-based teams. They provide the basis for a set of vibrant, rapidly-evolving research areas in high-energy astrophysics and are the current sources of an enormous data archive that stretches back to the beginning of high-energy observations in astronomy, forty years ago.

NASA's Swift mission 1. gamma-ray bursts in the Swift era
X-ray spectroscopy with XMM-Newton and Chandra 2. high-resolution x-ray spectroscopy
Multi-wavelength analysis of high-energy sources 3. multi-instrument observations of high-energy sources
Astrotomography of accreting sources 4. astrotomography of accreting sources
Accretion disk atmospheres 5. accretion disk atmospheres


Martin Still (Martin.Still@gsfc.nasa.gov)              Last modified on Sunday, 09-Nov-2003 07:30:51 EST