2014MNRAS.440.1982H

Query : 2014MNRAS.440.1982H

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):

We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1-5.7 d, masses of 0.5-2.8 MJup and radii of 1.1-1.4 RJup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent.

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

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Number of rows : 23
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 WASP-96 * 00 04 11.1376764240 -47 21 38.320831728     12.2     G8 50 0
2 WASP-96b Pl 00 04 11.1376764240 -47 21 38.320831728           ~ 94 0
3 HAT-P-19b Pl 00 38 04.0135699416 +34 42 41.553538560           ~ 74 1
4 CD-56 324b Pl 01 38 25.0565551464 -55 46 19.525595664           ~ 27 0
5 CD-56 324 PM* 01 38 25.0565551464 -55 46 19.525595664   11.31 10.57     G5 48 0
6 HAT-P-38 PM* 02 21 31.9803537360 +32 14 46.093339140   13.34 12.51 12.36   G 32 0
7 CD-50 777 * 02 39 35.4433933368 -50 00 28.879171596   10.08 9.48     F8 38 0
8 CD-50 777b Pl 02 39 35.4433933368 -50 00 28.879171596           ~ 30 0
9 CD-30 1019b Pl 02 44 09.6096023424 -30 10 08.563662228           ~ 36 1
10 WASP-98b Pl 03 53 42.9206066712 -34 19 41.585663208           ~ 32 0
11 WASP-98 * 03 53 42.9206066712 -34 19 41.585663208     13.0     G7 37 0
12 HAT-P-15b Pl 04 24 59.5350210144 +39 27 38.312978976           ~ 60 1
13 CPD-64 356 * 04 35 50.3301268152 -64 01 37.333851168   11.07 10.80     F2 46 0
14 CPD-64 356b Pl 04 35 50.3301268152 -64 01 37.333851168           ~ 49 0
15 CPD-23 1329 * 06 33 24.2671186968 -23 29 10.297934988   10.78 10.34     F6 50 0
16 CPD-23 1329b Pl 06 33 24.2671186968 -23 29 10.297934988           ~ 60 0
17 HAT-P-9b Pl 07 20 40.4564614032 +37 08 26.342829060           ~ 73 1
18 HAT-P-46 * 18 01 46.6085289960 -02 58 15.458098944   12.9 11.94 11.62 11.07 ~ 31 1
19 HAT-P-37 * 18 57 11.0562256392 +51 16 08.850467640   13.1 13.23 13.58   ~ 31 1
20 HATS-3b Pl 20 49 49.7853010920 -24 25 43.537820952           ~ 28 1
21 CD-48 14223b Pl 22 29 49.7355107880 -48 00 11.048684184           ~ 28 0
22 CD-48 14223 PM* 22 29 49.7355107880 -48 00 11.048684184   10.78 10.09     G2 39 0
23 BD+37 4734B PM* 22 57 46.8442481880 +38 40 30.358351704   10.82 9.87     G0V 189 1

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