Ohio University / MMT Observatory / Pennsylvania State University / University of Arizona / Cerro Tololo Inter-American Observatory / Ohio State University / South African Astronomical Observatory / University of Texas / Kitt Peak National Observatory / Mamalahoa Highway / W. H. Keck Observatory / University of Virginia / Space Telescope Science Institute / Chandra observatory / Observatory Multiwavelength Project / Michigan State University / University Avenue / Steward Observatory / University Park / pipeline XPIPE / Johns Hopkins University / National Optical Astronomy Observatory / University of Wisconsin-Madison / /
IndustryTerm
required optical imaging time / on-axis chip / circumnuclear gas / energy bands / power-law slopes / high-energy universe / high gas columns / well-defined wide-area survey products / aspect solutions / reasonable power-law slopes / imaging / search radius / energy / nightly photometric solutions / by-products / power-law photon index / hot diffuse gas / energy dependence / power law / image processing strategies / deep imaging / high-energy spectrum / deposited energy / gas reservoirs / photon energy / winddriven gas / energy range / gas-rich protogalaxies / assumed power-law continuum / optical imaging campaign / energy-dependent vignetting / aim point chip / higher energy / accretion radiation energy density / optical imaging / /
NaturalFeature
Ly forest / Mount Hopkins / /
Organization
Association of Universities for Research / Ohio University / Athens / Space Telescope Science Institute / Center for Astrophysical Sciences / University of Virginia / Ohio State University / Smithsonian Center for Astrophysics / University of Texas / ID PI / Michigan State University / Department of Astronomy and Astrophysics / National Science Foundation / XMM-Newton Survey Science Center / Harvard / Department of Physics and Astronomy / Pennsylvania State University / Institute for Advanced Study / Johns Hopkins University / California Association for Research / American Astronomical Society / University of Arizona / University of Wisconsin / School of Natural Sciences / /
Person
RAY IMAGE / RAY TO OPTICAL SOURCE MATCHING / James Higdon / Chandra FoV / Ray Surveys / Kitt Peak / / /
Position
standard source model / the source and chip / representative / Visiting Astronomer / /
Product
SExtractor / sources / /
ProvinceOrState
Ohio / Virginia / Alabama / Michigan / California / Arizona / Texas / New Jersey / Wisconsin / Maryland / Pennsylvania / Manitoba / /
PublishedMedium
Astronomy and Astrophysics / /
Technology
radiation / aim point chip / S/N / X-ray / FI chips / on-axis chip / four chips / six chips / spectroscopy / The ACIS CCD chips / FI chip / broadband / image processing / BI chips / S/ N / simulation / /
A The Astrophysical Journal Supplement Series, 150:43–71, 2004 January # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE CHANDRA MULTIWAVELENGTH PROJECT: OPTICAL FOLLOW-UP OF SEREN