Access to Astronomical Catalogues

← Click to display the menu
J/A+A/511/A45  HD 147018, 171238 and 204313 radial velocities (Segransan+, 2010)

The CORALIE survey for southern extrasolar planets. XVI. Discovery of a planetary system around HD 147018 and of two long period and massive planets orbiting HD 171238 and HD 204313. Segransan D., Udry S., Mayor M., Naef D., Pepe F., Queloz D., Santos N.C., Demory B-O., Figueira P., Gillon M., Marmier M., Megevand D., Sosnowska D., Tamuz O., Triaud A.H.M.J. <Astron. Astrophys. 511, A45 (2010)> =2010A&A...511A..45S
ADC_Keywords: Stars, G-type ; Radial velocities ; Planets Keywords: planetary systems - binaries: visual - techniques: radial velocities - stars: individual: HD 147018 - stars: individual: HD 171238 - stars: individual: HD 204313 Abstract: We report the detection of a double planetary system around HD140718 as well as the discovery of two long period and massive planets orbiting HD171238 and HD204313. Those discoveries were made with the CORALIE Echelle spectrograph mounted on the 1.2-m Euler Swiss telescope located at La Silla Observatory, Chile. The planetary system orbiting the nearby G9 dwarf HD147018 is composed of an eccentric inner planet (e=0.47) with twice the mass of Jupiter (2.1MJup) and with an orbital period of 44.24-days. The outer planet is even more massive (6.6MJup) with a slightly eccentric orbit (e=0.13) and a period of 1008-days. The planet orbiting HD171238 has a minimum mass of 2.6MJup, a period of 1523-days and an eccentricity of 0.40. It orbits a G8 dwarfs at 2.5AU. The last planet, HD204313 b, is a 4.0 MJup-planet with a period of 5.3-years and has a low eccentricity (e=0.13). It orbits a G5 dwarfs at 3.1AU. The three parent stars are metal rich, which further strengthened the case that massive planets tend to form around metal rich stars. Description: We present here radial-velocity measurements for 3 low mass stars: HD 147018, HD 171238 and HD204313. These radial velocities were obtained using the CORALIE echelle spectrograph mounted on the 1.2-m Euler Swiss telescope at the ESO-La Silla Observatory (Chile). Objects: -------------------------------------------------------------- RA (2000) DE Designation(s) (files) -------------------------------------------------------------- 16 23 00.1 -61 41 20 HD 147018 = HIP 80250 (table1.dat) 18 34 43.7 -28 04 20 HD 171238 = HIP 91085 (table2.dat) 21 28 12.2 -21 43 35 HD 204313 = HIP 106006 (table3.dat) -------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 37 101 Radial velocity measurements for HD 147018 table2.dat 37 99 Radial velocity measurements for HD 171238 table3.dat 37 97 Radial velocity measurements for HD 204313
See also: J/A+A/356/590 : CORALIE survey for extrasolar planets. II (Udry+, 2000) J/A+A/375/205 : CORALIE survey for extrasolar planets. V (Naef+ 2001) J/A+A/379/999 : CORALIE survey for extrasolar planets. VI (Santos+ 2001) J/A+A/388/632 : CORALIE survey for extrasolar planets. VII (Pepe+, 2002) J/A+A/390/267 : CORALIE survey for extrasolar planets. VIII (Udry+, 2002) J/A+A/392/215 : CORALIE survey for extrasolar planets. IX (Santos+ 2002) J/A+A/406/373 : CORALIE survey for extrasolar planets. XI (Santos+, 2003) J/A+A/415/391 : CORALIE survey for extrasolar planets. XII (Mayor+, 2004) J/A+A/447/1159 : CORALIE survey for extrasolar planets. XIV (Eggenberger+ 2006) J/A+A/480/L33 : CORALIE survey for extrasolar planets. XV (Tamuz+ 2008) Byte-by-byte Description of file: table1.dat table2.dat table3.dat
Bytes Format Units Label Explanations
1- 14 F14.6 d BJD Barycentric Julian date 17- 25 F9.5 km/s RV Barycentric radial velocity (1) 27- 33 F7.5 km/s e_RV Full RV uncertainty 35- 37 A3 -- Inst [C98,C07] Instrument (2)
Note (1): The CORALIE Echelle spectrograph was upgraded in July 2007 which affected the instrument zero point. We decided to refer to the original CORALIE as CORALIE-98 and to the upgraded one as CORALIE-07. When using both set of data, the instrumental zero point should be adjusted. Note (2): Instrument used as follows: C98 = CORALIE-98 C07 = CORALIE-07
Acknowledgements: Damien Segransan, Damien.Segransan(at) References: Queloz et al., Paper I 2000A&A...354...99Q Udry et al., Paper II 2000A&A...356..590U, Cat. J/A+A/356/590 Santos et al., Paper III 2000A&A...356..599S Santos et al., Paper IV 2000A&A...361..265S Santos et al., Paper V 2001A&A...375..205S, Cat. J/A+A/375/205 Santos et al., Paper VI 2001A&A...379..999S, Cat. J/A+A/379/999 Pepe et al., Paper VII 2002A&A...388..632P, Cat. J/A+A/388/632 Udry et al., Paper VIII 2002A&A...390..267U, Cat. J/A+A/390/267 Santos et al., Paper IX 2002A&A...392..215S, Cat. J/A+A/392/215 Udry et al., Paper X 2003A&A...407..679U Santos et al., Paper XI 2003A&A...406..373S, Cat. J/A+A/406/373 Mayor et al., Paper XII 2004A&A...415..391M, Cat. J/A+A/415/391 Correia et al., Paper XIII 2005A&A...440..751C Eggenberger et al., Paper XIV 2006A&A...447.1159E, Cat. J/A+A/447/1159 Tamuz et al., Paper XV 2008A&A...480L..33T, Cat. J/A+A/480/L33
(End) Patricia Vannier [CDS] 29-Jan-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

catalogue service