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J/A+A/458/997   Abundances for 6 transiting planet host stars   (Santos+, 2006)

Chemical abundances for the transiting planet host stars OGLE-TR-10, 56, 111, 113, 132 and TrES-1. Abundances in different galactic populations. Santos N.C., Ecuvillon A., Israelinan G., Mayor M., Melo C., Queloz D., Udry S., Ribeiro J.P., Jorge S. <Astron. Astrophys. 458, 997 (2006)> =2006A&A...458..997S
ADC_Keywords: Abundances, [Fe/H] - Abundances, peculiar - Planets Keywords: Stars: abundances ; Stars: fundamental parameters ; planetary systems ; Galaxy: abundances ; solar neighbourhood Abstract: We used the UVES spectrograph (VLT-UT2 telescope) to obtain high-resolution spectra of 6 stars hosting transiting planets, namely for OGLE-TR-10, 56, 111, 113, 132, and TrES-1. These spectra are now used to derive and discuss the chemical abundances for C, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Cu, and Zn. Description: In table2, the line-lists and atomic parameters used in the chemical analysis are presented. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 17 51 28.2 -29 52 35 OGLE-TR-10 = OGLE-TR 10 17 56 35.5 -29 32 21 OGLE-TR-56 = OGLE-TR 56 10 53 17.9 -61 24 20 OGLE-TR-111 = OGLE-TR 111 10 52 24.4 -61 26 49 OGLE-TR-113 = OGLE-TR 113 10 50 34.7 -61 57 26 OGLE-TR-132 = OGLE-TR 132 19 04 09.8 +36 37 56 TrES-1 = NAME TrES-1 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 103 6 Stellar parameters and metallicities table2.dat 27 136 Line-list and atomic parameters tables.dat 33 114 Derived abundances for the 6 stars (tables 3-6 of the paper) table7.dat 81 6 Stellar I magnitudes, stellar radii, galactic coordinates, derived distances, X, Y, Z, Rg galactic coordinates, adopted interstellar extinction, and systemic radial-velocities for the 6 stars studied
See also: J/A+A/356/590 : The CORALIE survey for extrasolar planets II (Udry+, 2000) J/A+A/375/205 : The CORALIE survey for extrasolar planets V (Naef+ 2001) J/A+A/379/999 : The CORALIE survey for extrasolar planets. VI (Santos+ 2001) J/A+A/388/632 : The CORALIE survey for extrasolar planets. VII (Pepe+, 2002) J/A+A/390/267 : The CORALIE survey for extrasolar planets VIII (Udry+, 2002) J/A+A/392/215 : The CORALIE survey for extrasolar planets. IX. (Santos+ 2002) J/A+A/398/363 : Statistical properties of exoplanets II (Santos+, 2003) J/A+A/406/373 : The CORALIE survey for extrasolar planets. XI (Santos+, 2003) J/A+A/415/391 : The CORALIE survey for extrasolar planets. XII (Mayor+, 2004) J/A+A/415/1153 : [Fe/H] for 98 extra-solar planet-host stars (Santos+, 2004) J/A+A/438/251 : Abundances in stars with giant planets (Beirao+, 2005) J/A+A/449/723 : Abundances in atmospheres of stars with planets (Gilli+, 2006) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Name Star name 13- 16 I4 K Teff Effective temperature 18- 20 I3 K e_Teff rms uncertainty on Teff 22- 25 F4.2 [cm/s2] logg Surface gravity 27- 30 F4.2 [cm/s2] e_logg rms uncertainty on logg 32- 35 F4.2 km/s Vt Turbulent velocity 37- 40 F4.2 km/s e_Vt rms uncertainty on Vt 42- 45 F4.2 [Sun] [Fe/H] Metallicity 47- 50 F4.2 [Sun] e_[Fe/H] rms uncertainty on [Fe/H] 52- 53 I2 --- o_FeI Number of Fe I lines used in analysis 55- 56 I2 --- o_FeII Number of Fe I lines used in analysis 58- 61 F4.2 --- e_FeI Dispersion of abundances given by FeI lines 63- 66 F4.2 --- e_FeII Dispersion of abundances given by FeII lines 68-103 A36 ---- Ref Reference
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 7 F7.2 0.1nm Lambda Wavelength of spectral line 9- 13 F5.3 eV Xlow Lower excitation potential 15- 21 F7.4 [-] loggf Oscillator strength value 23- 27 A5 --- El Element and ionization stage
Byte-by-byte Description of file: tables.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Name Star name 13- 17 A5 --- El Element 18 A1 --- l_[El/H] Limit flag on [El/H] 19- 23 F5.2 [Sun] [El/H] ?=- Abundance 25- 28 F4.2 [Sun] e_[El/H] ?=- rms uncertainty on [El/H] 30- 31 I2 --- o_[El/H] ?=- Number of lines used in analysis 33 A1 --- n_[El/H] [*] Note (1)
Note (1): For OGLE-TR-113, the Cu abundance was obtained only from the 5380Å, the uncertainty was derived based on an estimate of the measured EW. For TrES-1, only the 6757Å line of sulphur was measured.
Byte-by-byte Description of file: table7.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Name Name 13- 17 F5.2 mag Imag I magnitude (1) 19- 23 F5.3 solRad Rad Star radius 25- 32 F8.4 deg GLON Galactic longitude 34- 40 F7.4 deg GLAT Galactic latitude 42- 45 I4 pc Dist0 Distance derived considering null extinction 47- 50 I4 pc Dist Distance 52- 56 I5 pc X X galactic coordinate 58- 61 I4 pc Y Y galactic coordinate 63- 65 I3 pc Z Z galactic coordinate 67- 70 I4 pc Radg Galactocentric distance 72- 75 F4.2 mag AV Adopted interstellar extinction 77- 80 F4.1 km/s RV Systemic radial velocity 81 A1 --- r_RV References for RV (2)
Note (1): For TrES-1, the I magnitude was derived from the V magnitude (V=11.79) and the known effective temperature. Note (2): References for radial velocities as follows: a = Bouchy et al. (2005A&A...431.1105B) b = Pont et al. (2004A&A...426L..15P) c = Bouchy et al. (2004A&A...421L..13B) d = This paper
Acknowledgements: Nuno C. Santos, nuno(at)oal.ul.pt
(End) Nuno C. Santos [Lisbon Obs., Portugal], Patrica Vannier [CDS] 19-Oct-2006
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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