Extending the high-resolution X-ray spectroscopy of Line Emission Mapper to UV/optically-bright sources

Author:

Drake Jeremy J.1,Bandler Simon R.2,Barbera Marco3,Bozzo Enrico4,Dunn William R.5,Garraffo Cecilia6,Gauron Thomas6,Genolet Ludovic4,Houston Janice6,Kelley Richard L.2,Kilbourne Caroline A.2,Kraft Ralph P.6,Leutenegger Maurice A.2,Lo Cicero Ugo3,McEntee Seán C.7,Patnaude Daniel J.6

Affiliation:

1. Lockheed Martin, Palo Alto, California, United States

2. NASA Goddard Space Flight Center, Greenbelt, Maryland, United States

3. Università degli Studi di Palermo, Dipartimento di Fisica e Chimica “E. Segré,” Palermo, Italy

4. University of Geneva, Department of Astronomy, Versoix, Switzerland

5. University College London, Department of Physics and Astronomy, London, United Kingdom

6. Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts, United States

7. Dublin Institute for Advanced Studies, School of Cosmic Physics, DIAS Dunsink Observatory, Dublin, Ireland

Funder

NASA James Webb Space Telescope

Publisher

SPIE-Intl Soc Optical Eng

Reference33 articles.

1. Line Emission Mapper (LEM): probing the physics of cosmic ecosystems;Kraft,2022

2. Line Emission Mapper: an X-ray probe mission concept to study the cosmic ecosystems and the physics of galaxy formation

3. Breakthroughs in cool star physics with the Line Emission Mapper X-ray Probe;Drake,2023

4. Addressing outstanding problems in the physics of massive stars with the Line Emission Mapper X-ray Probe;Drake,2023

5. Revolutionary solar system science enabled by the Line Emission Mapper X-ray Probe;Dunn,2023

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