other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2014MNRAS.440.1982H - Mon. Not. R. Astron. Soc., 440, 1982-1992 (2014/May-3)
Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b.
HELLIER C., ANDERSON D.R., COLLIER CAMERON A., DELREZ L., GILLON M., JEHIN E., LENDL M., MAXTED P.F.L., PEPE F., POLLACCO D., QUELOZ D., SEGRANSAN D., SMALLEY B., SMITH A.M.S., SOUTHWORTH J., TRIAUD A.H.M.J., UDRY S. and WEST R.G.
Abstract (from CDS):
The host stars are of spectral type F2-G8. Five have metallicities of [Fe/H] from -0.03 to +0.23, while WASP-98 has a metallicity of -0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project.
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): planetary systems
VizieR on-line data: <Available at CDS (J/MNRAS/440/1982): stars.dat tablea.dat>
Simbad objects: 23
To bookmark this query, right click on this link: simbad:2014MNRAS.440.1982H and select 'bookmark this link' or equivalent in the popup menu