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J/A+AS/104/379    Integrated Photometry of open clusters      (Battinelli+ 1994)

Integrated photometric properties of open clusters BATTINELLI P., BRANDIMARTI A., CAPUZZO-DOLCETTA R. <Astron. Astrophys. Suppl. Ser. 104, 379 (1994)> =1994A&AS..104..379B
Keywords: clusters: open and associations - techniques: photometric ADC_Keywords: Clusters, open; Photometry Abstract: Galactic open clusters provide an abundant sample of stellar aggregates of various sizes, ages and metal abundances, apt to constitute a template for comparison with star systems in other galaxies. In this paper we present and discuss a standard methodology to synthesize U,B,V fluxes and colours, and apply it to a set of 138 open clusters. Results are compared with previous ones available in the literature. We were able to calibrate a mass-luminosity relation by which we evaluated the mass of ∼ 400 open clusters, leading to a well defined present-day mass function. The number-complete sample of galactic open clusters presented in Battinelli & Capuzzo-Dolcetta (1992AJ....103.1596B) is enlarged of a 15%. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 62 138 Magnitude, colour and mass refs.dat 93 106 References to table1 table2.dat 65 115 Galactic coordinates, distance and age
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name *Open cluster name 9- 12 I4 --- n Number of members stars 13- 18 F6.2 mag Mv Integrated magnitude 20- 24 F5.2 mag (B-V)0 (B-V)0 colour in decimal log 26- 30 F5.2 mag (U-B)0 ? (U-B)0 colour in decimal log 32- 35 F4.2 [solMass] logM Mass in decimal log 37- 42 A6 --- Notes *Notes on integrated photometry 43- 62 A20 --- r_Notes Comma-separated references, see file refs.dat
Note on Name: Bas=Basel, Ber=Berkeley, Bla=Blanco, Boc=Bochum, Byu=Byurakan, Col=Collinder, Fei=Feinstein, Hog=Hogg, Hya=Hyades, Lyn=Lynga, Mar=Markarian, N=NGC, Pis=Pismis, Ple=Pleiades, Ros=Roslund, Rup=Ruprecht, Tra=Trapezium, Upg=Upgren, VdH=van den Bergh & Hagen, Wat=Waterloo, Wes=Westerlund. Note on Notes: The symbols refer to other authors who give integrated photometry: b= Spassova N.M. & Baev P.V. =1985Ap&SS.112..111S g= Gray D.F. =1965AJ.....70..362G l= Lynga G. 1987, Lund Catalogue of Open Cluster Data, 5th ed., CDS Catalogue V/92 p= Pandey A.K., Bhatt B.C., Mahra H.S. & Sagar R. =1989MNRAS.236..263P s= Sagar R., Joshi U.C. & Sinvhal S.D. 1983, Bull. Astron. Soc. India 11, 44 Symbol c stands for clusters in the "complete" sample and symbol : stands for uncertain values. Hog 17 is included in the sample due to BCD determination based on a higher number of members (41).
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 3 I3 --- RefNo [1,106]+ Reference number 5- 23 A19 --- BibCode Coded Reference 25- 93 A69 --- Text Text of reference
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name *Open cluster name 10- 15 F6.2 deg GLON Galactic longitude l 17- 22 F6.2 deg GLAT Galactic latitude b 24- 27 I4 pc d Projected distance to the Sun 29- 35 F7.2 pc z Height on the galactic plane 37- 41 F5.1 arcmin D Angular diameter 45- 48 F4.2 [yr] Log(t) ? Logarithmic age 53- 57 F5.2 mag (B-V)to ? Turn-off colour 61- 64 F4.2 mag E(B-V) Reddening
Note on Name: Bas=Basel, Ber=Berkeley, Bla=Blanco, Boc=Bochum, Byu=Byurakan, Col=Collinder, Fei=Feinstein, Hog=Hogg, Hya=Hyades, Lyn=Lynga, Mar=Markarian, N=NGC, Pis=Pismis, Ple=Pleiades, Ros=Roslund, Rup=Ruprecht, Tra=Trapezium, Upg=Upgren, VdH=van den Bergh & Hagen, Wat=Waterloo, Wes=Westerlund.
History: * 18-Jan-1994: first archived at CDS (Patricia Bauer) * 24-Jan-1999: references added (Francois Ochsenbein)
(End) Patricia Bauer, Francois Ochsenbein [CDS] 24-Jan-1999
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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