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A CATALOG OF LOW-MASS STAR-FORMING CORES OBSERVED WITH SHARC-II AT 350 μm

  • Authors: Akshaya Suresh, Michael M. Dunham, Héctor G. Arce, Neal J. Evans II, Tyler L. Bourke, Manuel Merello, and Jingwen Wu

2016 The Astronomical Journal 152 36.

  • Provider: AAS Journals

Caption: Figure 2.

Histogram showing the distance between measured peak positions for sources that were each observed twice in our Monte Carlo model, as explained in detail in the text. The mean distance is 1.2 and the median distance is 1.1 (both in arbitrary units). Since the model assumed a pointing rms of 1, we find that the mean of this distribution is 20% larger than the underlying rms of the pointing model.

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