Taejon / Tucson / Urbana / Silverman et / La Serena / Cambridge / Garching / /
Company
Multiband / /
Country
Germany / Chile / United States / Korea / /
Facility
Space Science Institute / CERN Program Library / University of Illinois / ASCA observatory / Einstein Observatory / University of Arizona / Steward Observatory / Cerro Tololo Inter-American Observatory / National Optical Astronomy Observatory / Kitt Peak National Observatory / National Optical Astronomical Observatory / /
IndustryTerm
energy band detections / deep imaging campaign / respective energy selection band / energy bands / heasarc .nasa.gov/docs /software /tools /pimms.html / deep optical imaging / spectroscopy products / soft and hard energy bands / wider energy band / Energy production / quality optical imaging / optical imaging / /
MusicGroup
Selection / X-ray / Newton / Soft / /
Organization
Harvard / Astrophysics / Korea Astronomy and Space Science Institute / Max-Planck-Institut fu¨r / Department of Astronomy / University of Illinois / International Center for Astrophysics / American Astronomical Society / Smithsonian Center for Astrophysics / University of Arizona / CTIO BLANCO / /
Person
Ray Flux Limit / Ray Survey / Chandra Large / Chandra Deep / Koji Mukai / BLACK HOLES AT HIGH REDSHIFT / RAY SURVEYS / Chandra Chandra Chandra Chandra / Ray Band Hard / Ray Surveys Hard-Band / / /
The Astrophysical Journal, 679:118Y139, 2008 May 20 # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE LUMINOSITY FUNCTION OF X-RAYYSELECTED ACTIVE GALACTIC NUCLEI: EVOLUTION OF SUPERMA