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J/A+A/602/A89       Star clusters in the Magellanic Clouds       (Perren+, 2017)

Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA. Perren G.I., Piatti A.E., Vazquez R.A. <Astron. Astrophys. 602, A89 (2017)> =2017A&A...602A..89P (SIMBAD/NED BibCode)
ADC_Keywords: Magellanic Clouds ; Clusters, open; Clusters, globular ; Photometry, CCD Keywords: galaxies: fundamental parameters - galaxies: star clusters: general - Magellanic Clouds - methods: statistical - catalogs - techniques: photometric Abstract: To produce an homogeneous catalog of astrophysical parameters of 239 resolved star clusters located in the Small and Large Magellanic Clouds, observed in the Washington photometric system. The cluster sample was processed with the recently introduced Automated Stellar Cluster Analysis (ASteCA) package, which ensures both an automatized and a fully reproducible treatment, together with a statistically based analysis of their fundamental parameters and associated uncertainties. The fundamental parameters determined with this tool for each cluster, via a color-magnitude diagram (CMD) analysis, are: metallicity, age, reddening, distance modulus, and total mass. We generated an homogeneous catalog of structural and fundamental parameters for the studied cluster sample, and performed a detailed internal error analysis along with a thorough comparison with values taken from twenty-six published articles. We studied the distribution of cluster fundamental parameters in both Clouds, and obtained their age-metallicity relationships. The ASteCA package can be applied to an unsupervised determination of fundamental cluster parameters; a task of increasing relevance as more data becomes available through upcoming surveys. Description: Fundamental parameters for 150 Large Magellanic Cloud and 89 Small Magellanic Cloud clusters. All clusters were analyzed via C,T1 Washington photometry by the ASteCA package. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file clusters.dat 100 239 Fundamental parameters for 239 Magellanic Clouds star clusters
Byte-by-byte Description of file: clusters.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name Star cluster name 10- 12 A3 --- Galaxy [LMC SMC] Magellanic Cloud identification 14- 26 F13.9 deg RAdeg Right ascension J2000 (decimal degrees) 28- 40 F13.9 deg DEdeg Declination J2000 (decimal degrees) 42- 45 F4.1 pc Radius Adopted radius in parsecs 47- 51 F5.2 --- [Fe/H] Metallicity (1) 53- 56 F4.2 --- e_[Fe/H] Metallicity error 58- 61 F4.2 [yr] log(Age) Logarithm of age 63- 66 F4.2 [yr] e_log(Age) Logarithmic age error 68- 72 F5.3 mag E(B-V) E(B-V) extinction 74- 78 F5.3 mag e_E(B-V) E(B-V) extinction error 80- 84 F5.2 mag mu0 Distance modulus 86- 89 F4.2 mag emu0 Distance modulus error 91- 95 I5 Msun Mass Mass 97-100 I4 Msun e_Mass Mass error
Note (1): Solar metallicity adopted is z=0.0152 following Bressan et al. (2012MNRAS.427..127B)
Acknowledgements: Gabriel I. Perren, gabrielperren(at)gmail.com References: Perren et al., ASteCA: Automated Stellar Cluster Analysis, 2015A&A...576A...6P
(End) Gabriel I. Perren [IALP, Argentina], Patricia Vannier [CDS] 07-Feb-2017
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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