2013AJ....146..113B


Query : 2013AJ....146..113B

2013AJ....146..113B - Astron. J., 146, 113 (2013/November-0)

HATS-3b: an inflated hot Jupiter transiting an f-type star.

BAYLISS D., ZHOU G., PENEV K., BAKOS G.A., HARTMAN J.D., JORDAN A., MANCINI L., MOHLER-FISCHER M., SUC V., RABUS M., BEKY B., CSUBRY Z., BUCHHAVE L., HENNING T., NIKOLOV N., CSAK B., BRAHM R., ESPINOZA N., NOYES R.W., SCHMIDT B., CONROY P., WRIGHT D.J., TINNEY C.G., ADDISON B.C., SACKETT P.D., SASSELOV D.D., LAZAR J., PAPP I. and SARI P.

Abstract (from CDS):

We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V = 12.4 F dwarf star. HATS-3b has a period of P = 3.5479 days, mass of Mp= 1.07 MJ, and radius of Rp= 1.38 R J. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsin i = 9.0 km/s), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low-/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transiting planet candidates produced by the HATSouth survey. We show that this important step in discovering planets produces log g and Teff parameters at a precision suitable for efficient candidate vetting, as well as efficiently identifying stellar mass eclipsing binaries with radial velocity semi-amplitudes as low as 1 km/s.

Abstract Copyright:

Journal keyword(s): planetary systems - stars: individual (HATS-3, GSC 6926-00454) - techniques: photometric - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/AJ/146/113): table4.dat table5.dat>

Simbad objects: 16

goto Full paper

goto View the references in ADS

Number of rows : 16
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 HD 20453 * 03 21 30.6181217400 +67 35 29.368756680   9.02 8.89     A0 3 0
2 HD 26297 Pe* 04 09 03.4178692512 -15 53 27.056905800   8.55 7.47 7.09   G5/6IVw 148 0
3 V* HP Eri LP* 04 38 55.7330378304 -13 20 48.133934448 10.91 9.72 8.33     G8/K0IIIwF7 128 0
4 HD 36702 Pe* 05 31 52.2291576648 -38 33 24.045172128   9.53 8.38     F0wG/K 71 0
5 HATS-1 * 11 42 06.0806028384 -23 21 17.431249716   12.729 12.059 12.08 11.38 ~ 31 1
6 HATS-2 * 11 46 57.3702458424 -22 33 46.817348148   14.53 13.62 13.40   ~ 33 1
7 V* TY Vir LP* 11 51 50.1113014296 -05 45 44.183830536   9.668 7.97 7.57   G3Ibp 117 0
8 HD 122956 PM* 14 05 13.0244442888 -14 51 25.455804480   8.18 7.25 6.88   G6IV/VwF6 147 0
9 HD 197286 PM* 20 44 10.2208462488 -39 13 30.855881604   9.98 9.50     F5V 72 1
10 HATS-3b Pl 20 49 49.7852629888 -24 25 43.539819512           ~ 18 1
11 HATS-3 * 20 49 49.7853010920 -24 25 43.537820952   12.45 12.43     ~ 18 1
12 WASP-46 * 21 14 56.8598669520 -55 52 18.458085144   13.0   13.06 12.29 G6 37 1
13 WASP-4 PM* 23 34 15.0857248317 -42 03 41.047972591   13.51 12.48 11.9   G7V 154 1
14 CD-40 15273 PM* 23 51 31.0839097560 -39 54 24.258188484   12.15 11.33 10.896 10.10 K4V 48 1
15 WASP-5 V* 23 57 23.7564672192 -41 16 37.743700800   12.808 12.146 12.058 11.44 G4V 108 1
16 CD-35 16019 PM* 23 59 36.0711872328 -35 01 52.923618408   10.49 9.87 9.91   G6 96 0

To bookmark this query, right click on this link: simbad:objects in 2013AJ....146..113B and select 'bookmark this link' or equivalent in the popup menu


2022.10.01-23:35:11

© Université de Strasbourg/CNRS

    • Contact