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J/A+AS/107/385      UV-excess objects Spacelab-1 survey IV.       (Tobin+, 1994)

The Spacelab-1 Very Wide Field Survey of UV-excess objects. IV. The performance of the instrument in combination with optical photometry as a means of identifying stars with peculiar properties TOBIN W., VITON M., SIVAN J.-P. <Astron. Astrophys. Suppl. Ser. 107, 385 (1994)> =1994A&AS..107..385T (SIMBAD/NED Reference)
ADC_Keywords: Surveys; Ultraviolet; Photometry, ultraviolet; Stars, blue Keywords: stars: fundamental parameters - Galaxy: stellar content - ultraviolet: stars - survey File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 149 109 Ultraviolet and Vuvby photometry for the completely-surveyed region indicated in Fig. 2 table1.tex 80 233 LaTeX version of table1 table4 149 139 Vuvby photometry for other stars table4.tex 80 227 LaTeX version of table4
Byte-by-byte Description of file: table1 table4
Bytes Format Units Label Explanations
3- 6 A4 --- WT WT number 8- 18 A11 --- Name Star name 20- 24 F5.2 --- y/V []? Johnson V magnitude obtained by transformation of observations obtained with the Stroemgren y filter 25 A1 --- u_y/V Uncertainty flag on y/V 27- 31 F5.3 --- e_y/V []? Internal error on y/V (1) 34- 39 F6.3 mag (b-y) []? (b-y) colour 41- 45 F5.3 mag e_(b-y) []? Internal error on (b-y) (1) 47- 52 F6.3 mag m1 []? m1 colour index 54- 58 F5.3 mag e_m1 []? Internal error on m1 (1) 60- 65 F6.3 mag c1 []? c1 colour index 67- 71 F5.3 mag e_c1 []? Internal error on c1 (1) 73- 74 I2 --- nObs []? Number of observations 77- 80 F4.2 mag m195 []? UV (195 nm) magnitude 82- 85 F4.2 mag e_m195 []? rms uncertainty on m195 (2) 86 A1 --- nem195 Note on e_m195 (3) 90-149 A60 --- Com. Comments (3)
Note (1): Single-star internal errors are reported for those stars for which any Stroemgren index exceeds 2.5 times the appropriate mean uncertainty reported in Table II Note (2): The error given to m195 magnitudes is twice the one derived by the CAPELLA software, see Viton et al (1991) Note (3): a uncertain error bar b VWFC image elongated, both HD 204779 and 204763 may contribute c CORAVEL data indicate possibly variable velocity d CORAVEL data indicate variable velocity e UV detection in fact due to WT026bis (Fig. 3, V≃12.5) which preliminary spectroscopy and CCD photometry has shown is a sdO star probably in binary association with a cooler companion f SAO 227683 excluded g SAO 227683 included h photometric and spectroscopic variable, suspected EB (see Prevot et al., 1993) + see Fig. 3 for finding .chart * see Viton et al. (1991)

(End) Patricia Bauer [CDS] 25-May-1994
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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