2016A&A...588A.144W


Query : 2016A&A...588A.144W

2016A&A...588A.144W - Astronomy and Astrophysics, volume 588A144-144 (2016/4-1)

The SOPHIE search for northern extrasolar planets.

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

Abstract (from CDS):

Radial velocity planet search surveys of nearby solar-type stars have shown a strong scarcity of brown dwarf companions within ∼5AU. There is presently no comprehensive explanation for this lack of brown dwarf companions; therefore, increasing the sample of such objects is crucial to understand their formation and evolution. Based on precise radial velocities obtained using the SOPHIE spectrograph at Observatoire de Haute-Provence we characterise the orbital parameters of 15 companions to solar-type stars and constrain their true mass using astrometric data from the Hipparcos space mission. The nine companions not shown to be stellar in nature have minimum masses ranging from ∼13 to 70MJup, and are well distributed across the planet/brown dwarf mass regime, making them an important contribution to the known population of massive companions around solar-type stars. We characterise six companions as stellar in nature with masses ranging from a minimum mass of 76±4MJup to a mass of 0.35±0.03M☉. The orbital parameters of two previously known substellar candidates are improved.

Abstract Copyright: © ESO, 2016

Journal keyword(s): techniques: radial velocities - stars: general - brown dwarfs

VizieR on-line data: <Available at CDS (J/A+A/588/A144): stars.dat rv.dat>

Simbad objects: 83

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Number of rows : 83
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 KELT-1b Pl 00 01 26.9168207928 +39 23 01.784206464           ~ 149 0
2 BD+73 27 * 00 40 23.5472357568 +74 46 01.924645260   10.47 9.08     K0 4 0
3 HD 4747 SB* 00 49 26.7604733944 -23 12 44.868742449 8.244 7.927 7.155 6.732 6.344 G8/K0V 226 0
4 HD 5388B LM* 00 55 11.8899595488 -47 24 21.477151800           ~ 17 1
5 CD-23 395b Pl 01 06 02.0495101320 -22 27 11.350993068           ~ 20 1
6 UCAC3 259-9416 PM* 01 07 56.7182938704 +39 14 58.041886704       12.65   ~ 4 0
7 HD 6664 PM* 01 07 58.7593768464 +39 15 09.287829936   8.34 7.78     G1V 44 0
8 HD 10069b Pl 01 37 25.0332798696 -45 40 40.374717456           ~ 444 1
9 HD 13507b BD? 02 12 55.0057 +40 40 06.023           ~ 7 1
10 HD 14348b Pl? 02 19 52.9249941168 +31 20 14.917557336           ~ 2 0
11 HD 14651b Pl? 02 22 00.8541987312 +04 44 48.326313696           ~ 1 0
12 HD 16760C LM* 02 42 21.3134499936 +38 37 07.231908072           ~ 24 1
13 HD 22781b Pl 03 40 49.5243423552 +31 49 34.652692848           ~ 14 1
14 BD+57 793b Pl 04 21 52.7048156328 +57 49 01.889294952           ~ 234 1
15 HD 283668 PM* 04 27 52.9092842784 +24 26 41.877432536   10.32   8.8   K2 73 0
16 HD 283668b Pl? 04 27 52.9092842784 +24 26 41.877432536           ~ 4 0
17 HD 30246b Pl 04 46 30.3856235280 +15 28 19.360077276           ~ 6 0
18 HD 30339b Pl? 04 49 33.3469509960 +53 21 56.555449056           ~ 1 0
19 BD+73 275 SB* 05 13 16.1000774784 +73 29 28.262833548   9.74 8.98     G5 24 0
20 * pi. Men b Pl 05 37 09.8868446714 -80 28 08.834553264           ~ 82 1
21 HD 38529c Pl 05 46 34.9131388488 +01 10 05.502949860           ~ 84 1
22 HD 39392b Pl? 05 53 18.9954417360 +22 04 19.744402476           ~ 3 0
23 HD 39392 PM* 05 53 18.9954417360 +22 04 19.744402476   8.94 8.38     F8 28 0
24 BD+39 1560B BD? 06 15 31.420 +39 55 54.59           ~ 4 0
25 BD+39 1560 * 06 15 31.4242273512 +39 55 54.633420228   10.321 9.792 9.705   F7V 16 0
26 CoRoT-15b BD? 06 28 27.8204 +06 11 10.477   17.012 15.997 15.807   ~ 49 1
27 NAME Tyc 2949-557-1B LM* 06 47 41.077 +42 00 33.60           ~ 2 0
28 HD 50761 PM* 06 58 14.3056545144 +58 36 06.928896600   8.64 8.13     F8 23 0
29 HD 51813 Em* 06 58 59.0650330464 +05 32 06.600205644   9.27 8.67     G 41 0
30 HD 52756b Pl? 07 00 29.5974807720 -41 22 47.306259516           ~ 2 0
31 HD 56709 PM* 07 21 55.9194983376 +60 19 32.996795232   7.98 7.56     F5 37 0
32 HD 72946 ** 08 35 51.2666658240 +06 37 21.954760284 8.23 7.77 7.08     G8-V 147 1
33 HAT-P-13c Pl 08 39 31.8072358440 +47 21 07.273799280           ~ 53 1
34 HD 77065b Pl? 09 00 47.4452587799 +21 27 13.363366500           ~ 3 0
35 HD 77065 SB* 09 00 47.4452587799 +21 27 13.363366500   9.65   8.3   K2 56 0
36 BD+26 1888 PM* 09 02 30.6358324992 +25 53 21.898972572       8.9   K7 31 0
37 BD+26 1888b Pl? 09 02 30.6358324992 +25 53 21.898972572           ~ 1 0
38 HD 89707b Pl? 10 20 49.9823777315 -15 28 47.688646996           ~ 2 0
39 HD 91669B BD? 10 34 54.43 -13 47 16.6           ~ 6 0
40 HD 92320b Pl? 10 40 56.9112399672 +59 20 33.010773432           ~ 2 0
41 HD 106270b Pl 12 13 37.2858514992 -09 30 48.176202312           ~ 21 1
42 TYC 2534-698-1 Em* 13 03 22.0021613016 +35 05 25.382751324   11.40 10.70     G2V 9 2
43 NAME TYC 2534-698-1b Pl? 13 03 22.0021613016 +35 05 25.382751324           ~ 1 0
44 HD 114762C LM* 13 12 19.7410686234 +17 31 01.630334317           ~ 134 0
45 BD+48 2155B BD? 13 50 07.269 +47 49 15.96           ~ 3 0
46 HD 122562b Pl 14 02 21.1634920056 +20 52 52.743793584           ~ 3 0
47 HD 122562 PM* 14 02 21.1634920056 +20 52 52.743793584   8.70 7.69     G5 39 0
48 HD 132032 SB* 14 56 43.9313642304 +13 08 57.146074404 8.850 8.710 8.110     G5 39 0
49 HD 132032b Pl? 14 56 43.9313642304 +13 08 57.146074404           ~ 1 0
50 HD 131664b Pl 15 00 06.0800617968 -73 32 07.189532412           ~ 24 1
51 HD 134113b Pl? 15 07 46.5004807478 +08 52 47.202473395           ~ 2 0
52 HD 134113 SB* 15 07 46.5004807478 +08 52 47.202473395   8.83   7.9   F9 143 0
53 HD 134133 * 15 07 52.1353863888 +13 41 49.770712320   11.38 10.38     K0 4 0
54 HD 134169 SB* 15 08 18.0570477216 +03 55 50.144061360 8.14 8.22 7.70     F7V 220 0
55 HD 136118b Pl 15 18 55.4722661904 -01 35 32.592572196           ~ 38 1
56 HD 137510b Pl? 15 25 53.2697518752 +19 28 50.545457724           ~ 13 0
57 HD 156846b Pl 17 20 34.3108875144 -19 20 01.491746388           ~ 31 1
58 MARVELS-4 SB* 17 34 33.7444326648 +29 58 05.610696888   11.170 10.533 10.369   G0IV 11 0
59 MARVELS-4B BD? 17 34 33.76 +29 58 06.2           ~ 4 0
60 HD 160508b Pl? 17 39 12.6964195992 +26 45 27.143740584           ~ 2 0
61 HD 160508 SB* 17 39 12.6964195992 +26 45 27.143740584   8.62 8.11     F8V 38 0
62 HD 162020b Pl 17 50 38.3557484304 -40 19 06.072311784           ~ 60 1
63 MOA 2007-BLG-197b Pl? 18 07 04.729 -31 56 46.77           ~ 2 0
64 HD 167665 SB* 18 17 23.7587105112 -28 17 20.218638480   6.87 6.36     F9VFe-0.8CH-0.4+T4 125 0
65 HD 168443c Pl 18 20 03.9332862096 -09 35 44.614653900           ~ 96 1
66 CoRoT-27b Pl 18 33 58.9993615272 +05 32 18.324717936           ~ 24 0
67 CoRoT-33b Pl? 18 38 33.9102478176 +05 37 28.786272924           ~ 25 0
68 HD 174457b Pl? 18 50 02.0580006528 +15 18 41.432514516           ~ 1 0
69 CoRoT-3b Pl 19 28 13.2642131544 +00 07 18.613986132           ~ 148 1
70 KOI-415b Pl? 19 33 13.4494812696 +41 36 22.965562764           ~ 45 0
71 Kepler-492b Pl 19 41 59.1967605000 +42 32 16.400455944           ~ 46 0
72 Kepler-39b Pl 19 47 50.4745594512 +46 02 03.499726272           ~ 73 1
73 HD 190228b Pl 20 03 00.7726656864 +28 18 24.687065520           ~ 46 1
74 HD 189310b Pl? 20 13 16.4278229424 -82 01 41.316970620           ~ 1 0
75 HD 191760b Pl? 20 13 26.7462823536 -46 12 03.708889200           ~ 2 1
76 HD 202206b Pl 21 14 57.7686051936 -20 47 21.161521320           ~ 57 1
77 HD 209262b Pl? 22 01 54.1216802952 +04 46 13.615669488           ~ 2 0
78 HD 211847b Pl 22 20 55.7384451240 -41 25 48.384652332           ~ 9 0
79 BD+24 4697 SB* 23 01 39.3230252832 +25 47 16.549446732       9.2   K2 30 0
80 BD+24 4697b Pl? 23 01 39.3230252832 +25 47 16.549446732           ~ 2 0
81 HD 217786b Pl 23 03 08.2057849080 -00 25 46.666955676           ~ 17 1
82 HD 219077b Pl 23 14 06.5877117106 -62 42 00.008075788           ~ 17 1
83 WASP-30b BD? 23 53 38.054 -10 07 05.12           ~ 55 1

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