A limit on galactic extinction not correlated with far IR emission

  • Douglas P. Finkbeiner
  • David J. Schlegel
  • Marc Davis
Distant Hot Gas, SXRB Fluctuations, Dust, Gamma-Rays
Part of the Lecture Notes in Physics book series (LNP, volume 506)


We have reprocessed the IRAS and DIRBE full-sky 100 µm maps, using Hi as a zero-point, to produce a map of Galactic extinction. This map is cross-correlated with APM galaxy counts over the full APM region, including dusty regions of the sky not used to compute the APM correlation function in Maddox et al. (1990a). The angular correlation function, ω(θ), of galaxy counts is computed with and without the extinction correction, and is used to suggest that our map accounts for ∼90% of the dust-induced correlation in the APM region on scales from 2–10°. This is the first time that a limit has been placed on the correlation function of the extinction not represented in a given map.


Correlation Function Extinction Correction Corrected Count Zodiacal Light Angular Correlation Function 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer-Verlag 1998

Authors and Affiliations

  • Douglas P. Finkbeiner
    • 1
  • David J. Schlegel
    • 2
  • Marc Davis
    • 1
  1. 1.Departments of Physics and AstronomyUniversity of California at BerkeleyBerkeley
  2. 2.Department of PhysicsUniversity of DurhamDurhamUnited Kingdom

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