2011ApJS..194....4B


Query : 2011ApJS..194....4B

2011ApJS..194....4B - Astrophys. J., Suppl. Ser., 194, 4 (2011/May-0)

A naive Bayes source classifier for X-ray sources.

BROOS P.S., GETMAN K.V., POVICH M.S., TOWNSLEY L.K., FEIGELSON E.D. and GARMIRE G.P.

Abstract (from CDS):

The Chandra Carina Complex Project (CCCP) provides a sensitive X-ray survey of a nearby starburst region over >1 deg2 in extent. Thousands of faint X-ray sources are found, many concentrated into rich young stellar clusters. However, significant contamination from unrelated Galactic and extragalactic sources is present in the X-ray catalog. We describe the use of a naive Bayes classifier to assign membership probabilities to individual sources, based on source location, X-ray properties, and visual/infrared properties. For the particular membership decision rule adopted, 75% of CCCP sources are classified as members, 11% are classified as contaminants, and 14% remain unclassified. The resulting sample of stars likely to be Carina members is used in several other studies, which appear in this special issue devoted to the CCCP.

Abstract Copyright: ∼

Journal keyword(s): methods: data analysis - methods: statistical - stars: pre-main sequence - X-rays: general - X-rays: stars

VizieR on-line data: <Available at CDS (J/ApJS/194/4): table5.dat>

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 1

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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 Carina Molecular Cloud Complex MoC 10 43 10 -59 38.2           ~ 97 0

Query : 2011ApJS..194....4B

Basic data :
NAME Carina Molecular Cloud Complex -- Molecular Cloud
Other object types:
otypes_help
MoC ()
ICRS coord. (ep=J2000) :
10 43 10.0 -59 38 12 [ ] E 2001ApJ...554..916B
FK4 coord. (ep=B1950 eq=1950) :
10 41 14.0 -59 22 27 [ ]
Gal coord. (ep=J2000) :
287.3633 -00.6995 [ ]
Angular size (arcmin):
90 90 ~ (~) D 2019ApJ...881...37P
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 146
Display criteria :

Identifiers (3) :
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NAME Carina Nebula Complex NAME Carina Molecular Cloud Complex NAME eta Car GMC

References (97 between 1850 and 2026) (Total 97)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Distance : 1   

   

Observing logs
ISO : 156   

   


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