Pasadena / Boulder / Lyngby / Zurich / Santiago / Roma / Cambridge / Livermore / Bologna / Valpara´ıso / New Haven / /
Company
Draper / Jet Propulsion Laboratory / UK 18 Columbia Astrophysics Laboratory / Observational Cosmology Laboratory / Astrophysics Laboratory / Thomson / Konami / Wilson / Henkel / Italy 15 Lawrence Livermore National Laboratory / EFE / Space Sciences Laboratory / Wilder Laboratory / UK Propulsion Laboratory / NuSTAR Data Analysis Software / Leverhulme Trust / /
Country
Germany / Switzerland / Italy / Chile / United States / Denmark / Columbia / /
Facility
Durham University / Millennium Institute of Astrophysics / Space Science Institute / Jet Propulsion Laboratory / Stanford University / Georgia Institute of Technology / The Pennsylvania State University / Columbia University / Institute of Technology / Technical University of Denmark / DTU Space-National Space Institute / University Park / Dartmouth College / California Institute of Technology / Institute of Astronomy / Kavli Institute / University of California / Yale University / /
IndustryTerm
circumnuclear gas / energy range / operational energy range / rest-frame energy / gas accretion rate / accretion disk gas / imaging / energy / thick circumnuclear gas / even accounting / gas column / hot gas components / gas columns / fixed rest-frame line centroid energy / angular resolution infrared imaging / low-energy / high gas column densities / thick cold gas / /
Organization
Technical University of Denmark / California Institute of Technology / Columbia University / Max-Planck-Institut f¨ / Yale Center for Astronomy and Astrophysics / School of Physics / Harvard / Institute for Gravitation / University of California / Berkeley / Department of Physics / Dartmouth College / Institute for Astronomy / ASI Science Data Center / Yale University / Durham University / Department of Astronomy / The Pennsylvania State University / Davey Lab / Pontificia Universidad Catolica de Chile / Institute of Astronomy / Institute for Gravitation and the Cosmos / Stanford University / Millennium Institute of Astrophysics / National Aeronautics and Space Administration / Space Science Institute / Georgia Institute of Technology / Atlanta / Swiss National Science Foundation / Kavli Institute for Particle Astrophysics and Cosmology / Smithsonian Center for Astrophysics / Instituto de F´ısica / Cahill Center for Astrophysics / Center for Relativistic Astrophysics / Asia-Pacific Economic Cooperation / DTU Space-National Space Institute / /
Person
P. Gandhi / James R. Mullaney / Chris M. Harrison / T. Finally / Matteo Guainazzi / Della Ceca / Fred K.Y. Lo / RAY SPECTRAL FITTING / /
Position
driver / D.J. / model / Major / representative / /
Product
CH-8093 Zurich / /
ProgrammingLanguage
L / /
ProvinceOrState
M.B. / Maryland / New York / Connecticut / Pennsylvania / California / Georgia / Massachusetts / Colorado / New Hampshire / /
A P J IN PRESS Preprint typeset using LATEX style emulateapj v[removed]NUSTAR UNVEILS A COMPTON-THICK TYPE 2 QUASAR IN MRK 34 1