J/ApJ/772/L2     Keck/HIRES radial velocities for HD 97658     (Dragomir+, 2013)

MOST detects transits of HD 97658b, a warm, likely volatile-rich super-Earth. Dragomir D., Matthews J.M., Eastman J.D., Cameron C., Howard A.W., Guenther D.B., Kuschnig R., Moffat A.F.J., Rowe J.F., Rucinski S.M., Sasselov D., Weiss W.W. <Astrophys. J., 772, L2 (2013)> =2013ApJ...772L...2D 2013ApJ...772L...2D
ADC_Keywords: Radial velocities ; Stars, double and multiple Keywords: planets and satellites: formation; planets and satellites: interiors; stars: individual: HD 97658; techniques: photometric Abstract: Through photometric monitoring of the extended transit window of HD 97658b with the MOST space telescope, we have found that this exoplanet transits with an ephemeris consistent with that predicted from radial velocity measurements. The mid-transit times are 5.6σ earlier than those of the unverified transit-like signals reported in 2011, and we find no connection between the two sets of events. The transit depth together with our determined stellar radius (R*=0.703-0.034+0.039R) indicates a 2.34-0.150.18R super-Earth. When combined with the radial velocity determined mass of 7.86±0.73M, our radius measure allows us to derive a planet density of 3.44-0.82+0.91g/cm3. Models suggest that a planet with our measured density has a rocky core that is enveloped in an atmosphere composed of lighter elements. The star of the HD 97658 system is the second brightest known to host a transiting super-Earth, facilitating follow-up studies of this not easily daunted, warm and likely volatile-rich exoplanet. Description: Since the publication of Dragomir et al. (2012, J/ApJ/759/L41), we have obtained four new Keck HIRES radial velocity measurements. These were acquired and reduced using the same techniques as in Howard et al. (2011ApJ...730...10H 2011ApJ...730...10H). Objects: -------------------------------------------------------------------- RA (ICRS) DE Designation(s) (Period) -------------------------------------------------------------------- 11 14 33.16 +25 42 37.4 HD 97658 = TYC 1981-1168-1 (P=9.4909) -------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 27 174 Radial velocities for HD 97658 -------------------------------------------------------------------------------- See also: J/ApJ/759/L41 : New radial velocities of HD 97658 (Dragomir+, 2012) J/ApJ/754/37 : HD 192263 radial velocities and photometry (Dragomir+, 2012) J/A+A/533/A114 : Transit of super-Earth 55 Cnc e (Demory+, 2011) J/PASP/123/412 : Exoplanet Orbit Database (Wright+, 2011) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 F15.6 d BJD Barycentric Julian Date (BJD-2440000) 17- 22 F6.2 m/s RVel [-12.7/12.7] Radial velocity 24- 27 F4.2 m/s e_RVel [0.4/1.7] Uncertainty in RVel -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 05-Feb-2015
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