2022A&A...658A.141V


Query : 2022A&A...658A.141V

2022A&A...658A.141V - Astronomy and Astrophysics, volume 658A141-141 (2022/2-1)

Robust statistical tools for identifying multiple stellar populations in globular clusters in the presence of measurement errors. A case study: NGC 2808.

VALLE G., DELL'OMODARME M. and TOGNELLI E.

Abstract (from CDS):


Context. The finding of multiple stellar populations (MPs), which are defined by patterns in the stellar element abundances, is considered today a distinctive feature of globular clusters. However, while data availability and quality have improved in the past decades, this is not always true for the techniques that are adopted to analyse them, which creates problems of objectivity for the claims and reproducibility.
Aims. Using NGC 2808 as test case, we show the use of well-established statistical clustering methods. We focus our analysis on the red giant branch phase, where two data sets are available in the recent literature for low- and high-resolution spectroscopy.
Methods. We adopted hierarchical clustering and partition methods. We explicitly addressed the usually neglected problem of measurement errors, for which we relied on techniques that were recently introduced in the statistical literature. The results of the clustering algorithms were subjected to a silhouette width analysis to compare the performance of the split into different numbers of MPs.
Results. For both data sets the results of the statistical pipeline are at odds with those reported in the literature. Two MPs are detected for both data sets, while the literature reports five and four MPs from high- and low-resolution spectroscopy, respectively. The silhouette analysis suggests that the population substructure is reliable for high-resolution spectroscopy data, while the actual existence of MP is questionable for the low-resolution spectroscopy data. The discrepancy with literature claims can be explained with the different methods that were adopted to characterise MPs. By means of Monte Carlo simulations and multimodality statistical tests, we show that the often adopted study of the histogram of the differences in some key elements is prone to multiple false-positive findings.
Conclusions. The adoption of statistically grounded methods, which adopt all the available information to split the data into subsets and explicitly address the problem of data uncertainty, is of paramount importance to present more robust and reproducible research.

Abstract Copyright: © ESO 2022

Journal keyword(s): methods: statistical - stars: evolution - stars: abundances - globular clusters: general - globular clusters: individual: NGC 2808

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 NGC 2808 GlC 09 12 03.10 -64 51 48.6           ~ 1540 0

Query : 2022A&A...658A.141V

Basic data :
NGC 2808 -- Globular Cluster
Other object types:
otypes_help
* (CPD,GCRV,...), GlC (2013A&A,GCl), Cl* (C,[KPS2012]), IR (IRAS)
ICRS coord. (ep=J2000) :
09 12 03.10 -64 51 48.6 (Optical) [ ] D 2010AJ....140.1830G
FK4 coord. (ep=B1950 eq=1950) :
09 11 04.42 -64 39 24.9 [ ]
Gal coord. (ep=J2000) :
282.19303 -11.25259 [ ]
Proper motions mas/yr :
1.02 0.28 [0.01 0.01 90] C 2019MNRAS.482.5138B
Radial velocity / Redshift / cz :
V(km/s) 103.7 [0.3] / z(spectroscopic) 0.000346 [0.000001] / cz 103.72 [0.30]
   (Opt) A 2018MNRAS.478.1520B
Parallaxes (mas):
0.112 [0.010] C 2021MNRAS.505.5978V
Angular size (arcmin):
13.8 13.8 90 (Opt) D 1989Sci...246.1066D
Fluxes (1) :
K 3.06 [~] D 2008MNRAS.389.1924F
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

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: 1320
: 186 Display criteria :

Identifiers (11) :
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NGC 2808 CPD-64 1012 HD 79627 IRAS F09110-6439
AKARI-IRC-V1 J0912036-645148 GCl 13 HR 3671 [KPS2012] MWSC 1636
C 0911-646 GCRV 3437 E IRAS 09110-6439

References (1540 between 1850 and 2026) (Total 1540)
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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Collections of Measurements Description of Measurements

Velocities : 5    Distance : 3    Fe/H : 17    Plx : 2    PM : 3   

   

Observing logs
IUE : 2    XMM : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : NGC 2808

Link by name to the catalogue in VizieR :

NGC 2808 AKARI-IRC-V1 J0912036-645148 CPD-64 1012 HD 79627 HR 3671
IRAS 09110-6439 IRAS F09110-6439

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