SIMBAD references

2017A&A...601A...9R - Astronomy and Astrophysics, volume 601A9-9 (2017/5-1)

The SOPHIE search for northern extrasolar planets. XII. Three giant planets suitable for astrometric mass determination with Gaia.

REY J., HEBRARD G., BOUCHY F., BOURRIER V., BOISSE I., SANTOS N.C., ARNOLD L., ASTUDILLO-DEFRU N., BONFILS X., BORGNIET S., COURCOL B., DELEUIL M., DELFOSSE X., DEMANGEON O., DIAZ R.F., EHRENREICH D., FORVEILLE T., MARMIER M., MOUTOU C., PEPE F., SANTERNE A., SAHLMANN J., SEGRANSAN D., UDRY S. and WILSON P.A.

Abstract (from CDS):

We present new radial velocity measurements for three low-metallicity solar-like stars observed with the SOPHIE spectrograph and its predecessor ELODIE, both installed at the 193 cm telescope of the Haute-Provence Observatory, allowing the detection and characterization of three new giant extrasolar planets in intermediate periods of 1.7 to 3.7yr. All three stars, HD 17674, HD 42012 and HD 29021 present single giant planetary companions with minimum masses between 0.9 and 2.5MJup. The range of periods and masses of these companions, along with the distance of their host stars, make them good targets to look for astrometric signals over the lifetime of the new astrometry satellite Gaia. We discuss the preliminary astrometric solutions obtained from the first Gaia data release.

Abstract Copyright: © ESO, 2017

Journal keyword(s): techniques: radial velocities - planetary systems - brown dwarfs - stars: individual: HD 17674 - stars: individual: HD 29021 - stars: individual: HD 42012 - stars: individual: HD 42012

VizieR on-line data: <Available at CDS (J/A+A/601/A9): table5.dat table6.dat table7.dat>

Simbad objects: 11

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