Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Export to PDF

Submillimeter Array Polarimetry with Hertz

  • Authors: C. Darren Dowell, Roger H. Hildebrand, David A. Schleuning, John E. Vaillancourt, Jessie L. Dotson, Giles Novak, Tom Renbarger, and Martin Houde

Dowell et al. 1998 The Astrophysical Journal 504 588.

  • Provider: AAS Journals

Caption: Fig. 5.

Extinction curve of G34.3 from observations in 1997 April. The signal, observed with a single pixel centered on the source, is plotted vs. the atmospheric optical depth at 225 GHz measured by the CSO radiometer. Each point corresponds to an average signal during a 5 minute file. The signal has been normalized to 1.0 at τ = 0. The linear fit shown has a slope of −26.9.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions