2019AJ....157..113B


Query : 2019AJ....157..113B

2019AJ....157..113B - Astron. J., 157, 113-113 (2019/March-0)

Predicted number, multiplicity, and orbital dynamics of TESS M-dwarf exoplanets.

BALLARD S.

Abstract (from CDS):

We present a study of the M-dwarf exoplanetary systems forthcoming from NASA's TESS mission. While the mission's footprint is too complex to be characterized by a single detection completeness, we extract ensemble completeness functions that recover the planet detections from previous work for stars between 3200 and 4000 K. We employ these completeness functions, together with a dual-population planet occurrence model that includes compact multiple planetary systems, to infer anew the planet yield. We predict both the number of M-dwarf planets likely from TESS and their system architectures. We report four main findings. First, TESS will likely detect more planets orbiting M dwarfs that previously predicted. Around stars with effective temperatures between 3200 and 4000 K, we predict that TESS will find 1274 ± 241 planets orbiting 1026 ± 182 stars, a 1.2-fold increase over previous predictions. Second, TESS will find two or more transiting planets around 20% of these host stars, a number similar to the multiplicity yield of NASA's Kepler mission. Third, TESS light curves in which one or more planets are detected will often contain transits of additional planets below the detection threshold of TESS. Among a typical set of 200 TESS hosts to one or more detected planets, 93 ± 17 transiting planets will be missed. Transit follow-up efforts with the photometric sensitivity to detect an Earth or larger around a mid-M dwarf, even with very modest period completeness, will readily result in additional planet discoveries. Fourth, the strong preference of TESS for systems of compact multiples indicates that TESS planets will be dynamically cooler on average than Kepler planets, with 90% of TESS planets residing in orbits with e < 0.15. We include both (1) a predicted sample of planets detected by TESS orbiting stars between 3200 and 4000 K, including additional nontransiting planets, or transiting and undetected planets orbiting the same star and (2) sample completeness functions for use by the community.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): eclipses - planetary systems - planets and satellites: detection

VizieR on-line data: <Available at CDS (J/AJ/157/113): table2.dat>

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 1

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Number of rows : 1
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 L 119-213 PM* 22 41 58.1171811377 -69 10 08.320741850   17.3 15.26 13.74 11.88 ~ 73 0

Query : 2019AJ....157..113B

Basic data :
L 119-213 -- High Proper Motion Star
Other object types:
otypes_help
PM* (2016ApJ,LHS,...), * (2021MNRAS,CNS5,...), Er* (2020AJ), Ro* (2020ApJ), NIR (2MASS), MIR (WISEA)
ICRS coord. (ep=J2000) :
22 41 58.1171811377 -69 10 08.320741850 (Optical) [ 0.0154 0.0148 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
22 38 20.8385121729 -69 25 14.255914214 [ 0.0154 0.0148 90 ]
Gal coord. (ep=J2000) :
318.2538446332079 -43.9075545056190 [ 0.0154 0.0148 90 ]
Proper motions mas/yr :
334.419 -726.986 [0.021 0.020 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -10.642 [0.500] / z(spectroscopic) -0.000035 [0.000002] / cz -10.64 [0.50]
   (Opt) A 2022ApJ...935..104M
Parallaxes (mas):
67.2123 [0.0187] A 2020yCat.1350....0G
Fluxes (8) :
B 17.3 [~] E ~
V 15.26 [~] D 2024AJ....167..196K
R 13.74 [~] D 2024AJ....167..196K
G 13.364960 [0.002834] C 2020yCat.1350....0G
I 11.88 [~] D 2024AJ....167..196K
J 10.046 [0.023] C 2003yCat.2246....0C
H 9.477 [0.023] C 2003yCat.2246....0C
K 9.145 [0.023] C 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
Display criteria :

Identifiers (13) :
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LHS 3844 L 119-213 TIC 410153553 Gaia DR2 6385548541499112448
CNS5 5600 2MASS J22415815-6910089 TOI-136
LEHPM 5027 NAME-IAU Batsu WISEA J224158.77-691015.9
LFT 1732 NLTT 54534 Gaia DR3 6385548541499112448

References (73 between 1850 and 2026) (Total 73)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 1    Distance : 2    Var : 1    Fe/H : 2    Plx : 2    PM : 8   

   


External archives :

Link by name to the catalogue in VizieR :

LHS 3844 2MASS J22415815-6910089 NLTT 54534 WISEA J224158.77-691015.9 Gaia DR3 6385548541499112448
Gaia DR2 6385548541499112448

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