Charlottesville / Minneapolis / Pasadena / Boston / INDEBETOUW ET / Whitewater / Madison / Cambridge / Laramie / /
Company
Jet Propulsion Laboratory / 2MASS / /
Country
Netherlands / United States / /
Currency
pence / /
Facility
University of Virginia / Spitzer Science Center / Space Science Institute / GLIMPSE pipeline / Boston University / Jet Propulsion Laboratory / College Park / Analysis Center/ California Institute of Technology / Campbell Hall / Analysis Center/California Institute of Technology / University of Minnesota / University of Massachusetts / University of Maryland / University of Wyoming / California Institute of Technology / Infrared Space Observatory / University of California / University of Wisconsin / University of Colorado / /
IndustryTerm
power-law regime / power-law extinction curve / universal extinction law / power-law wavelength dependence / power law / /
Organization
California Institute of Technology / University of Massachusetts / National Science Foundation / University of Maryland / Spitzer Science Center / Physics Department / Department of Physics and Astronomy / University of Colorado / University of California / Berkeley / University of Maryland / College Park / Department of Astronomy / University of Virginia / Radio Astronomy Lab / University of Wyoming / National Aeronautics and Space Administration / Astronomy Department / NASA’s Earth Science Technology Office / Space Science Institute / American Astronomical Society / Institute for Astrophysical Research / Boston University / University of Minnesota / University of Wisconsin / /
Person
Bruce Draine / Spencer Jones / Stephan Jansen / ESA SP / /
ProvinceOrState
Wisconsin / Minnesota / Virginia / Alabama / Wyoming / Maryland / California / Massachusetts / Colorado / /
PublishedMedium
The Astrophysical Journal / /
Technology
AV / ESA / Spectroscopy / fit algorithm / recombination / /
The Astrophysical Journal, 619:931–938, 2005 February 1 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE WAVELENGTH DEPENDENCE OF INTERSTELLAR EXTINCTION FROM 1.25 TO 8.0 m USING G