2017ApJ...840L..17G


Query : 2017ApJ...840L..17G

2017ApJ...840L..17G - Astrophys. J., 840, L17-L17 (2017/May-2)

Removing visual bias in filament identification: a new goodness-of measure.

GREEN C.-E., CUNNINGHAM M.R., DAWSON J.R., JONES P.A., NOVAK G. and FISSEL L.M.

Abstract (from CDS):

Different combinations of input parameters to filament identification algorithms, such as disperse and filfinder, produce numerous different output skeletons. The skeletons are a one-pixel-wide representation of the filamentary structure in the original input image. However, these output skeletons may not necessarily be a good representation of that structure. Furthermore, a given skeleton may not be as good of a representation as another. Previously, there has been no mathematical "goodness-of-fit" measure to compare output skeletons to the input image. Thus far this has been assessed visually, introducing visual bias. We propose the application of the mean structural similarity index (MSSIM) as a mathematical goodness-of-fit measure. We describe the use of the MSSIM to find the output skeletons that are the most mathematically similar to the original input image (the optimum, or "best," skeletons) for a given algorithm, and independently of the algorithm. This measure makes possible systematic parameter studies, aimed at finding the subset of input parameter values returning optimum skeletons. It can also be applied to the output of non-skeleton-based filament identification algorithms, such as the Hessian matrix method. The MSSIM removes the need to visually examine thousands of output skeletons, and eliminates the visual bias, subjectivity, and limited reproducibility inherent in that process, representing a major improvement upon existing techniques. Importantly, it also allows further automation in the post-processing of output skeletons, which is crucial in this era of "big data."

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): ISM: structure - methods: data analysis - methods: statistical - stars: formation - techniques: image processing - techniques: image processing

Simbad objects: 1

goto Full paper

goto View the references in ADS

Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Vela C Cld 08 57 -43.2           ~ 193 0

Query : 2017ApJ...840L..17G

Basic data :
NAME Vela C -- Cloud
Other object types:
otypes_help
Cld (VMR)
ICRS coord. (ep=J2000) :
08 57 00.0 -43 12 00 [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
08 55 11.2 -43 00 23 [ ]
Gal coord. (ep=J2000) :
264.4344 +01.4774 [ ]
SIMBAD within arcmin
Overlay Simbad points in this preview
Back
All CDSPortal (CDSPortal)

Send to sendBySAMP sendBySAMP

sedIcon
within arcsec sed-help-icon

Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 233
Display criteria :

Identifiers (4) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

NAME Vela C NAME Vela-C Molecular Cloud NAME Vela C Cloud VMR C

References (193 between 1850 and 2026) (Total 193)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
Follow new references on this object
                Reference summaries :

                from: to:

                 or select by : (not exhaustive, explanation here)


Collections of Measurements Description of Measurements

Distance : 1   

   


Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience


To bookmark this query, right click on this link: simbad:objects in 2017ApJ...840L..17G and select 'bookmark this link' or equivalent in the popup menu