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J/MNRAS/403/1491 Integrated magnitudes of synthetic star clusters (Pandey+ 2010)

Integrated parameters of star clusters: a comparison of theory and observations. Pandey A.K., Sandhu T.S., Sagar R., Battinelli P. <Mon. Not. R. Astron. Soc., 403, 1491-1506 (2010)> =2010MNRAS.403.1491P
ADC_Keywords: Clusters, open ; Magellanic Clouds ; Photometry, UBVRI ; Models Keywords: open clusters and associations: general - galaxies: star clusters Abstract: This paper presents integrated magnitudes and colours for synthetic clusters. The integrated parameters have been obtained for the whole cluster population as well as for the main-sequence (MS) population of star clusters. We have also estimated observed integrated magnitudes and colours of the MS population of galactic open clusters, Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) star clusters. Description: We have generated synthetic colour-magnitude diagram (CMDs) of open clusters (Sandhu, Pandey & Sagar 2003A&A...408..515S) using stellar evolutionary models by Girardi et al. (2002A&A...391..195G). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 80 136 Integrated magnitude and colours of synthetic cluster (MS population) obtained in the present work table2.dat 80 136 Integrated magnitude and colours of synthetic cluster (whole population) obtained in the present work table3.dat 60 66 Observed MS integrated magnitude and colours of galactic clusters obtained in the present work table4.dat 46 685 Observed MS integrated magnitude and colours of LMC clusters obtained in the present work table5.dat 46 229 Observed MS integrated magnitude and colours of SMC clusters obtained in the present work
See also: B/ocl : Optically visible open clusters and Candidates (Dias+ 2002-2010) VII/103 : Galactic Globular Clusters (Monella 1985) J/A+A/438/1163 : Catalogue of Open Cluster Data (COCD) (Kharchenko+, 2005) J/AcA/48/175 : OGLE SMC star clusters BVI photometry (Pietrzynski+ 1998) J/AcA/49/521 : OGLE LMC star clusters BVI photometry (Pietrzynski+, 1999) Byte-by-byte Description of file: table[12].dat
Bytes Format Units Label Explanations
1- 4 F4.2 --- X [2.35] Mass function Slope 6- 10 F5.3 --- Z Metallicity (0.02, 0.001, 0.004, 0.008) 12- 15 F4.1 [yr] logt Age 17- 22 F6.3 mag (U-V)0 Deredenned U-V colour index 24- 28 F5.3 mag e_(U-V)0 rms uncertainty on (U-V)0 30- 35 F6.3 mag (U-B)0 Deredenned U-B colour index 37- 41 F5.3 mag e_(U-B)0 rms uncertainty on (U-B)0 43- 48 F6.3 mag (B-V)0 Deredenned B-V colour index 50- 54 F5.3 mag e_(B-V)0 rms uncertainty on (B-V)0 56- 61 F6.3 mag (V-R)0 Deredenned V-R colour index 63- 67 F5.3 mag e_(V-R)0 rms uncertainty on (V-R)0 69- 74 F6.3 mag (V-I)0 Deredenned V-I colour index 76- 80 F5.3 mag e_(V-I)0 rms uncertainty on (V-I)0
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Cluster Cluster name 10- 14 F5.2 mag m-M Distance modulus 16- 19 F4.2 mag E(B-V) Redenning 21- 24 F4.2 [yr] logt Age 26- 30 F5.2 mag VMAG Absolute V magnitude 32- 36 F5.2 mag (U-V)0 ?=- Deredenned U-V colour index 38- 42 F5.2 mag (U-B)0 ?=- Deredenned U-B colour index 44- 48 F5.2 mag (B-V)0 ?=- Deredenned B-V colour index 50- 54 F5.2 mag (V-R)0 ?=- Deredenned V-R colour index 56- 60 F5.2 mag (V-I)0 ?=- Deredenned V-I colour index
Byte-by-byte Description of file: table[45].dat
Bytes Format Units Label Explanations
1- 7 A7 --- OGLE OGLE-ID, LMCNNNN or SMCNNNN (1) 9- 18 A10 --- Cluster Other name 20- 23 F4.2 [yr] logt ?=- Age 25- 29 F5.2 mag VMAG Absolute V magnitude 31- 35 F5.2 mag (V-I)0 ?=- Deredenned V-I colour index 37- 41 F5.2 mag (B-V)0 ?=- Deredenned B-V colour index 43- 46 I4 --- N Number of stars used to calculate the integrated parameters
Note (1): Clusters identified as <OGLE-CL LMC NNN> (Pietrzynski et al., Cat. J/AcA/49/521) and <OGLE-CL SMC NNN> (Pietrzynski et al., Cat. J/AcA/48/175) in Simbad.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 04-Oct-2010
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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