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pubs: FellWalker - another "cf splits sources" reference
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Although obviously this reference makes no mention of FellWalker.
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David Berry committed Jul 18, 2014
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30 changes: 30 additions & 0 deletions pubs/fellwalker/fellwalker.bib
@@ -1,3 +1,33 @@
@ARTICLE{2006Enoch,
author = {{Enoch}, M.~L. and
{Young}, K.~E. and
{Glenn}, J. and
{Evans}, N.~J. and
{Golwala}, S. and
{Sargent}, A.~I. and
{Harvey}, P. and
{Aguirre}, J. and
{Goldin}, A. and
{Haig}, D. and
{Huard}, T.~L. and
{Lange}, A. and
{Laurent}, G. and
{Maloney}, P. and
{Mauskopf}, P. and
{Rossinot}, P. and
{Sayers}, J.},
title = "{Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. I. Perseus}",
journal = {\apj},
year = 2006,
volume = 638,
pages = {293-313},
eprint = {astro-ph/0510202},
archivePrefix = "arXiv",
doi = {10.1086/498678},
adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...638..293E},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@Article{2014Jenness,
author = {Tim Jenness and others},
title = "{Learning from 25 years of the extensible
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3 changes: 2 additions & 1 deletion pubs/fellwalker/fellwalker.tex
Expand Up @@ -536,7 +536,8 @@ \section{Comparing FellWalker and CLUMPFIND}
This concluded that, under the conditions used in the study, FellWalker
is less likely than CLUMPFIND to split up large clumps, and is less
likely to create false clump detections. A similar conclusion was reached
by \cite{2014Christie} for 3-dimensional data.
by \cite{2014Christie} for 3-dimensional data. The tendency for CLUMPFIND
to split sources has also been noted by \cite{2006Enoch}.

An independent illustration of this for 2-dimensional data is presented in
Fig.~\ref{fig:comp1}, which shows a field of artificial Gaussian clumps,
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