2023A&A...678A.207M


Query : 2023A&A...678A.207M

2023A&A...678A.207M - Astronomy and Astrophysics, volume 678A207 (2023/10-1)

Characterizing planetary systems with SPIRou: M-dwarf planet-search survey and the multiplanet systems GJ 876 and GJ 1148.

MOUTOU C., DELFOSSE X., PETIT A.C., DONATI J.-F., ARTIGAU E., FOUQUE P., CARMONA A., OULD-ELHKIM M., ARNOLD L., COOK N.J., CADIEUX C., BELLOTTI S., BOISSE I., BOUCHY F., CHARPENTIER P., CORTES-ZULETA P., DOYON R., HEBRARD G., MARTIOLI E., MORIN J. and VANDAL T.

Abstract (from CDS):

SPIRou is a near-infrared spectropolarimeter and a high-precision velocimeter. The SPIRou Legacy Survey collected data from February 2019 to June 2022, half of the time devoted to a blind search for exoplanets around nearby cool stars. The aim of this paper is to present this program and an overview of its properties, and to revisit the radial velocity (RV) data of two multiplanet systems, including new visits with SPIRou. From SPIRou data, we can extract precise RVs using efficient telluric correction and line-by-line measurement techniques, and we can reconstruct stellar magnetic fields from the collection of polarized spectra using the Zeeman-Doppler imaging method. The stellar sample of our blind search in the solar neighborhood, the observing strategy, the RV noise estimates, chromatic behavior, and current limitations of SPIRou RV measurements on bright M dwarfs are described. In addition, SPIRou data over a 2.5-yr time span allow us to revisit the known multiplanet systems GJ 876 and GJ 1148. For GJ 876, the new dynamical analysis including the four planets is consistent with previous models and confirms that this system is deep in the Laplace resonance and likely chaotic. The large-scale magnetic map of GJ 876 over two consecutive observing seasons is obtained and shows a dominant dipolar field with a polar strength of 30 G, which defines the magnetic environment in which the inner planet with a period of 1.94 days is embedded. For GJ 1148, we refine the known two-planet model.

Abstract Copyright: © The Authors 2023

Journal keyword(s): stars: low-mass - planetary systems - methods: observational - techniques: radial velocities - techniques: polarimetric - stars: magnetic field

VizieR on-line data: <Available at CDS (J/A+A/678/A207): gj876.dat gj1148.dat>

Simbad objects: 61

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Number of rows : 61
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 G 158-27 PM* 00 06 43.1973190107 -07 32 17.019101068     13.837 13.605 10.15 M5.5V 257 0
2 HD 1326 PM* 00 18 22.8849799680 +44 01 22.637951588   9.61 8.14 7.3   M2V 602 0
3 HD 1326B PM* 00 18 25.8251408611 +44 01 38.092431857   12.84 11.04 10.3   M3.5V 317 0
4 G 31-53 PM* 00 28 39.4648750195 -06 39 49.179160254   13.71 12.23 11.885   dM4.0 84 0
5 Ross 318 PM* 01 02 32.2354294685 +71 40 47.336260174   11.736   9.1   M3.0V 192 0
6 G 175-34 PM* 04 31 11.5144294005 +58 58 37.463848495     10.98     M4.0V 175 0
7 HD 36395 PM* 05 31 27.3957852161 -03 40 38.024004501 10.626 9.443 7.968 6.996 5.913 M1.5Ve 574 0
8 G 192-13 PM* 06 01 11.0455145210 +59 35 49.884065409   13.31   10.7   M4.0V 128 0
9 HD 265866 PM* 06 54 48.9580633365 +33 16 05.438282419   11.47   9.650   M3V 277 0
10 G 112-50 PM* 07 51 54.6712965202 -00 00 12.259020776 15.86 14.95 13.26 11.9 10.17 M4.5V 71 0
11 G 111-47 PM* 07 58 12.7020660564 +41 18 13.314829358   13.67 13.912 11.698   M3.5V 125 0
12 G 51-15 PM* 08 29 49.3527921926 +26 46 33.624143059   16.87   14.736   M6.5Ve 326 0
13 LSPM J0840+3127 PM* 08 40 15.9834311184 +31 27 06.808923216   13.5   11.966   M3.5V 58 0
14 L 675-81 Pe* 08 40 59.2057867166 -23 27 22.592748045   13.2 11.975 11.637 9.37 M3.5V 180 1
15 HD 79211 PM* 09 14 24.6828466599 +52 41 10.902471910   7.966   6.8   M0V 341 0
16 LP 847-48 PM* 09 55 23.8624392916 -27 15 40.725133064 14.94 13.681 12.081 10.922 9.486 M3V 42 0
17 BD-03 2870 PM* 10 12 17.6682499584 -03 44 44.392042932 11.941 10.757 9.264 8.258 7.066 M2V 283 1
18 V* AD Leo PM* 10 19 36.2808181226 +19 52 12.010446571   10.82 9.52 9.19   dM3 1469 1
19 LP 731-58 PM* 10 48 12.6142508200 -11 20 09.610693470     15.784 16.01 11.25 M6.5V 198 0
20 Wolf 359 PM* 10 56 28.9208702274 +07 00 53.003285286 16.706 15.541 13.507 11.684 9.507 dM6 775 0
21 Ross 104 PM* 11 00 04.2570074282 +22 49 58.645009946 12.826 11.584 10.020 8.952 7.646 M4V 222 0
22 V* DS Leo BY* 11 02 38.3420210088 +21 58 01.700013360 12.246 11.049 9.572 8.638 7.634 M1.0Ve 269 0
23 HD 95735 PM* 11 03 20.1948195942 +35 58 11.576182057 10.030 8.960 7.520 5.99 4.79 M2+V 795 0
24 BD+44 2051 PM* 11 05 28.5769490063 +43 31 36.386948721 11.440 10.270   7.9   M1.0V 368 0
25 Ross 1003 PM* 11 41 44.6358403057 +42 45 07.102117090   13.36 13.795 11.524 9.18 M4.0V 172 1
26 Ross 905 PM* 11 42 11.0933350978 +26 42 23.650782778   12.06 10.613 10.272 8.24 M3V 750 1
27 G 254-29 PM* 11 47 41.3869161825 +78 41 28.176228837   12.741   10.0   M4.0V 208 0
28 Ross 128 PM* 11 47 44.3972681420 +00 48 16.400337591 14.223 12.905 11.153 9.859 8.184 dM4 484 0
29 G 122-49 PM* 11 50 57.7205259231 +48 22 38.561183125       12.95   M4.5V 176 0
30 G 13-22 PM* 12 14 16.5489621254 +00 37 26.362449419   15.40   13.309   M4.5Ve 98 0
31 Wolf 433 PM* 12 38 52.4410371789 +11 41 46.143038529 14.106 12.975 11.502 10.394 8.963 M3.5V 137 0
32 BD+11 2576 PM* 13 29 59.7858994351 +10 22 37.784532575 11.728 10.524 9.029 8.07 7.013 M1.0V 313 0
33 HD 122303 PM* 14 01 03.1882316643 -02 39 17.519814662 12.343 11.177 9.707 8.745 7.66 M0V 204 0
34 NAME Proxima Centauri PM* 14 29 42.9461331854 -62 40 46.164680672 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1483 0
35 NAME Proxima Centauri b Pl 14 29 42.9461331854 -62 40 46.164680672           ~ 445 0
36 BD-07 4003 BY* 15 19 26.8269387505 -07 43 20.189497466 13.403 11.76 10.560 9.461 8.911 M3V 717 2
37 HD 147379B BY* 16 16 45.3144811630 +67 15 22.481125328   12.20   10.310   M3.0V 173 0
38 BD+68 946 PM* 17 36 25.8993094605 +68 20 20.909627174 11.73 10.65   8.3   M3.0V 345 0
39 NAME Barnard's star BY* 17 57 48.4984700685 +04 41 36.113879676 12.497 11.24 9.511 8.298 6.741 M4V 907 2
40 LP 229-17 LM* 18 34 36.6521805504 +40 07 26.384102544       11.104   M4V 98 0
41 HD 173739 PM* 18 42 46.7043860406 +59 37 49.409446059   10.43 8.93     M3V 427 1
42 HD 173740 PM* 18 42 46.8946714770 +59 37 36.721161413   11.32 9.78     M3.5V 381 1
43 G 141-36 PM* 18 48 17.5373479643 +07 41 21.186505469   15.6   13.817   M5.0V 70 0
44 HD 180617 PM* 19 16 55.2565688720 +05 10 08.040554168 11.768 10.63 9.115 8.076 6.782 M3-V 475 0
45 Kepler-78b Pl 19 34 58.0137407208 +44 26 53.960186940           ~ 153 1
46 G 208-45 LM* 19 53 55.1405033909 +44 24 54.147256052   15.97 13.99 14.3 10.27 M6V 205 0
47 HD 189733b Pl 20 00 43.7129433648 +22 42 39.073143456           ~ 1610 1
48 G 144-25 PM* 20 40 33.8632524043 +15 29 58.730061366   15.13 13.41 12.1 10.36 M4.5V 114 0
49 HD 197481 BY* 20 45 09.5324974119 -31 20 27.237889841   10.05 8.627 9.078 6.593 M1VeBa1 1344 0
50 LSPM J2146+3813 PM* 21 46 22.0724658744 +38 13 04.977309828   13.3   11.867   M5V 69 0
51 IRAS 21500+5903 PM* 21 51 38.3194245194 +59 17 39.867862225   11.88 10.64     dM4.0 23 0
52 HD 209290 PM* 22 02 10.2750978279 +01 24 00.832158070 11.838 10.616 9.146 8.213 7.245 M0.5V 285 0
53 BD-05 5715 PM* 22 09 40.3443137051 -04 38 26.650757960 13.006 11.868 10.366 9.279 7.877 M3.5V 332 1
54 L 788-34 PM* 22 23 06.9968051575 -17 36 26.333040286   15.135 13.316 12.878 10.04 M4.5Ve 120 0
55 V* EV Lac PM* 22 46 49.7312610268 +44 20 02.374381562   11.85 10.26 9.89   M4.0Ve 993 2
56 BD-15 6290 BY* 22 53 16.7325836486 -14 15 49.304052185 12.928 11.749 10.192 9.013 7.462 M3.5V 1106 1
57 HD 216899 PM* 22 56 34.8046530863 +16 33 12.355636588 11.323 10.143 8.638 7.657 6.542 M1.5V 335 0
58 G 68-8 PM* 23 21 37.4486739614 +17 17 25.391139752 14.299 13.236 11.710 10.514 8.942 M3.5V 126 0
59 G 157-77 PM* 23 35 10.4624266947 -02 23 20.613547105   16.60 14.69 14.447   M5.0Ve 126 0
60 Ross 248 BY* 23 41 55.0363002516 +44 10 38.818911116   14.19   11.1   M5.0V 361 0
61 G 130-4 PM* 23 43 06.3118372752 +36 32 13.137302361     12.67 12.298   M4.5Ve 133 0

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