Table 3.
Open in new tab

The physical properties of HIP 113103.

ParameterValueSource
Identifiers|$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|HIP 113 103
TIC 121 490 076
TYC 8011-00766-1
2MASS J22541736-4300372
Gaia DR2 6 541 360 574 788 758 016
Astrometry
RA |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|22h54m17s.37Gaia Collaboration (2022)
Dec. |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−43°00′37″.25Gaia Collaboration (2022)
Parallax (mas) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|21.61785 ± 0.00024Gaia Collaboration (2022)
Proper motion
Gaia (2016.4) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|1.995 ± 0.020Gaia Collaboration (2022)
Gaia (2016.3) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|27.384 ± 0.021Gaia Collaboration (2022)
Hipparcos (1991.2) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|2.2 ± 1.5Perryman et al. (1997)
Hipparcos (1991.4) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|27.1 ± 1.3Perryman et al. (1997)
Hipparcos-Gaia average RA proper motion (mas yr−1) |$\ldots \ldots \ldots $|2.032 ± 0.048Brandt (2021)
Hipparcos-Gaia average Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots $|27.396 ± 0.038Brandt (2021)
Photometry
TESS (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9988 ± 0.0063Stassun et al. (2019)
B (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.907 ± 0.033Høg et al. (2000)
V (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.95 ± 0.03Høg et al. (2000)
J (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.195 ± 0.03Skrutskie et al. (2006)
H (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.67 ± 0.042Skrutskie et al. (2006)
K (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.557 ± 0.031Skrutskie et al. (2006)
Gaia G (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.6175 ± 0.0018Gaia Collaboration (2022)
GaiaBP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.1491 ± 0.0033Gaia Collaboration (2022)
GaiaRP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9353 ± 0.0039Gaia Collaboration (2022)
WISE W1 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.398 ± 0.033Cutri & et al. (2012)
WISE W2 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.538 ± 0.02Cutri & et al. (2012)
WISE W3 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.489 ± 0.017Cutri & et al. (2012)
WISE W4 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.395 ± 0.132Cutri & et al. (2012)
Kinematics and position
U (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|5.00 ± 0.17Propagated from Gaia1
V (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.635 ± 0.031Propagated from Gaia1
W (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−13.89 ± 0.32Propagated from Gaia1
Distance (pc) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|46.212 ± 0.086This paper
γCHIRON (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$12.845_{-0.013}^{+0.012}$|This paper
γMINERVA (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13.395_{-0.011}^{+0.010}$|This paper
JitterCHIRON (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$16_{-11}^{+20}$|This paper
JitterMINERVA (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13_{-9}^{+14}$|This paper
Physical properties
M⋆ (M⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.761 ± 0.038This paper
R⋆ (R⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.742 ± 0.013This paper
Teff (K) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4930 ± 100This paper
log g (cgs) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.6 ± 0.1This paper
[m/H] |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−0.1 ± 0.1This paper
vsin i (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|3 ± 1This paper
Rotation period (d) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.92 ± 0.23This paper
Gyrochronology age (Myr) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$470_{-110}^{+170}$|Based on the gyrochronology relationship from Bouma, Palumbo & Hillenbrand (2023)
Limb darkening coefficients (TESSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.463 ± 0.021Claret (2017)
Limb darkening coefficients (TESSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.182 ± 0.020Claret (2017)
Limb darkening coefficients (CHEOPSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.604 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (CHEOPSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.111 ± 0.022Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u1) |$\ldots \ldots \ldots $|0.350 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u2) |$\ldots \ldots \ldots $|0.287 ± 0.021Claret & Bloemen (2011)
ParameterValueSource
Identifiers|$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|HIP 113 103
TIC 121 490 076
TYC 8011-00766-1
2MASS J22541736-4300372
Gaia DR2 6 541 360 574 788 758 016
Astrometry
RA |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|22h54m17s.37Gaia Collaboration (2022)
Dec. |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−43°00′37″.25Gaia Collaboration (2022)
Parallax (mas) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|21.61785 ± 0.00024Gaia Collaboration (2022)
Proper motion
Gaia (2016.4) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|1.995 ± 0.020Gaia Collaboration (2022)
Gaia (2016.3) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|27.384 ± 0.021Gaia Collaboration (2022)
Hipparcos (1991.2) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|2.2 ± 1.5Perryman et al. (1997)
Hipparcos (1991.4) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|27.1 ± 1.3Perryman et al. (1997)
Hipparcos-Gaia average RA proper motion (mas yr−1) |$\ldots \ldots \ldots $|2.032 ± 0.048Brandt (2021)
Hipparcos-Gaia average Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots $|27.396 ± 0.038Brandt (2021)
Photometry
TESS (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9988 ± 0.0063Stassun et al. (2019)
B (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.907 ± 0.033Høg et al. (2000)
V (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.95 ± 0.03Høg et al. (2000)
J (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.195 ± 0.03Skrutskie et al. (2006)
H (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.67 ± 0.042Skrutskie et al. (2006)
K (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.557 ± 0.031Skrutskie et al. (2006)
Gaia G (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.6175 ± 0.0018Gaia Collaboration (2022)
GaiaBP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.1491 ± 0.0033Gaia Collaboration (2022)
GaiaRP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9353 ± 0.0039Gaia Collaboration (2022)
WISE W1 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.398 ± 0.033Cutri & et al. (2012)
WISE W2 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.538 ± 0.02Cutri & et al. (2012)
WISE W3 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.489 ± 0.017Cutri & et al. (2012)
WISE W4 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.395 ± 0.132Cutri & et al. (2012)
Kinematics and position
U (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|5.00 ± 0.17Propagated from Gaia1
V (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.635 ± 0.031Propagated from Gaia1
W (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−13.89 ± 0.32Propagated from Gaia1
Distance (pc) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|46.212 ± 0.086This paper
γCHIRON (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$12.845_{-0.013}^{+0.012}$|This paper
γMINERVA (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13.395_{-0.011}^{+0.010}$|This paper
JitterCHIRON (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$16_{-11}^{+20}$|This paper
JitterMINERVA (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13_{-9}^{+14}$|This paper
Physical properties
M⋆ (M⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.761 ± 0.038This paper
R⋆ (R⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.742 ± 0.013This paper
Teff (K) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4930 ± 100This paper
log g (cgs) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.6 ± 0.1This paper
[m/H] |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−0.1 ± 0.1This paper
vsin i (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|3 ± 1This paper
Rotation period (d) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.92 ± 0.23This paper
Gyrochronology age (Myr) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$470_{-110}^{+170}$|Based on the gyrochronology relationship from Bouma, Palumbo & Hillenbrand (2023)
Limb darkening coefficients (TESSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.463 ± 0.021Claret (2017)
Limb darkening coefficients (TESSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.182 ± 0.020Claret (2017)
Limb darkening coefficients (CHEOPSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.604 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (CHEOPSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.111 ± 0.022Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u1) |$\ldots \ldots \ldots $|0.350 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u2) |$\ldots \ldots \ldots $|0.287 ± 0.021Claret & Bloemen (2011)
1

Propagated from Gaia via the gal uvw function in the pyastronomy package (Czesla et al. 2019).

Table 3.
Open in new tab

The physical properties of HIP 113103.

ParameterValueSource
Identifiers|$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|HIP 113 103
TIC 121 490 076
TYC 8011-00766-1
2MASS J22541736-4300372
Gaia DR2 6 541 360 574 788 758 016
Astrometry
RA |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|22h54m17s.37Gaia Collaboration (2022)
Dec. |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−43°00′37″.25Gaia Collaboration (2022)
Parallax (mas) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|21.61785 ± 0.00024Gaia Collaboration (2022)
Proper motion
Gaia (2016.4) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|1.995 ± 0.020Gaia Collaboration (2022)
Gaia (2016.3) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|27.384 ± 0.021Gaia Collaboration (2022)
Hipparcos (1991.2) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|2.2 ± 1.5Perryman et al. (1997)
Hipparcos (1991.4) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|27.1 ± 1.3Perryman et al. (1997)
Hipparcos-Gaia average RA proper motion (mas yr−1) |$\ldots \ldots \ldots $|2.032 ± 0.048Brandt (2021)
Hipparcos-Gaia average Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots $|27.396 ± 0.038Brandt (2021)
Photometry
TESS (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9988 ± 0.0063Stassun et al. (2019)
B (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.907 ± 0.033Høg et al. (2000)
V (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.95 ± 0.03Høg et al. (2000)
J (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.195 ± 0.03Skrutskie et al. (2006)
H (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.67 ± 0.042Skrutskie et al. (2006)
K (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.557 ± 0.031Skrutskie et al. (2006)
Gaia G (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.6175 ± 0.0018Gaia Collaboration (2022)
GaiaBP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.1491 ± 0.0033Gaia Collaboration (2022)
GaiaRP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9353 ± 0.0039Gaia Collaboration (2022)
WISE W1 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.398 ± 0.033Cutri & et al. (2012)
WISE W2 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.538 ± 0.02Cutri & et al. (2012)
WISE W3 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.489 ± 0.017Cutri & et al. (2012)
WISE W4 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.395 ± 0.132Cutri & et al. (2012)
Kinematics and position
U (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|5.00 ± 0.17Propagated from Gaia1
V (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.635 ± 0.031Propagated from Gaia1
W (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−13.89 ± 0.32Propagated from Gaia1
Distance (pc) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|46.212 ± 0.086This paper
γCHIRON (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$12.845_{-0.013}^{+0.012}$|This paper
γMINERVA (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13.395_{-0.011}^{+0.010}$|This paper
JitterCHIRON (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$16_{-11}^{+20}$|This paper
JitterMINERVA (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13_{-9}^{+14}$|This paper
Physical properties
M⋆ (M⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.761 ± 0.038This paper
R⋆ (R⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.742 ± 0.013This paper
Teff (K) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4930 ± 100This paper
log g (cgs) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.6 ± 0.1This paper
[m/H] |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−0.1 ± 0.1This paper
vsin i (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|3 ± 1This paper
Rotation period (d) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.92 ± 0.23This paper
Gyrochronology age (Myr) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$470_{-110}^{+170}$|Based on the gyrochronology relationship from Bouma, Palumbo & Hillenbrand (2023)
Limb darkening coefficients (TESSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.463 ± 0.021Claret (2017)
Limb darkening coefficients (TESSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.182 ± 0.020Claret (2017)
Limb darkening coefficients (CHEOPSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.604 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (CHEOPSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.111 ± 0.022Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u1) |$\ldots \ldots \ldots $|0.350 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u2) |$\ldots \ldots \ldots $|0.287 ± 0.021Claret & Bloemen (2011)
ParameterValueSource
Identifiers|$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|HIP 113 103
TIC 121 490 076
TYC 8011-00766-1
2MASS J22541736-4300372
Gaia DR2 6 541 360 574 788 758 016
Astrometry
RA |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|22h54m17s.37Gaia Collaboration (2022)
Dec. |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−43°00′37″.25Gaia Collaboration (2022)
Parallax (mas) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|21.61785 ± 0.00024Gaia Collaboration (2022)
Proper motion
Gaia (2016.4) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|1.995 ± 0.020Gaia Collaboration (2022)
Gaia (2016.3) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|27.384 ± 0.021Gaia Collaboration (2022)
Hipparcos (1991.2) RA proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|2.2 ± 1.5Perryman et al. (1997)
Hipparcos (1991.4) Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots \ldots$|27.1 ± 1.3Perryman et al. (1997)
Hipparcos-Gaia average RA proper motion (mas yr−1) |$\ldots \ldots \ldots $|2.032 ± 0.048Brandt (2021)
Hipparcos-Gaia average Dec. proper motion (mas yr−1) |$\ldots \ldots \ldots \ldots $|27.396 ± 0.038Brandt (2021)
Photometry
TESS (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9988 ± 0.0063Stassun et al. (2019)
B (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.907 ± 0.033Høg et al. (2000)
V (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.95 ± 0.03Høg et al. (2000)
J (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.195 ± 0.03Skrutskie et al. (2006)
H (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.67 ± 0.042Skrutskie et al. (2006)
K (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.557 ± 0.031Skrutskie et al. (2006)
Gaia G (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.6175 ± 0.0018Gaia Collaboration (2022)
GaiaBP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|10.1491 ± 0.0033Gaia Collaboration (2022)
GaiaRP (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|8.9353 ± 0.0039Gaia Collaboration (2022)
WISE W1 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.398 ± 0.033Cutri & et al. (2012)
WISE W2 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.538 ± 0.02Cutri & et al. (2012)
WISE W3 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.489 ± 0.017Cutri & et al. (2012)
WISE W4 (mag) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|7.395 ± 0.132Cutri & et al. (2012)
Kinematics and position
U (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|5.00 ± 0.17Propagated from Gaia1
V (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.635 ± 0.031Propagated from Gaia1
W (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−13.89 ± 0.32Propagated from Gaia1
Distance (pc) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|46.212 ± 0.086This paper
γCHIRON (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$12.845_{-0.013}^{+0.012}$|This paper
γMINERVA (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13.395_{-0.011}^{+0.010}$|This paper
JitterCHIRON (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$16_{-11}^{+20}$|This paper
JitterMINERVA (m s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$13_{-9}^{+14}$|This paper
Physical properties
M⋆ (M⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.761 ± 0.038This paper
R⋆ (R⊙) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.742 ± 0.013This paper
Teff (K) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4930 ± 100This paper
log g (cgs) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|4.6 ± 0.1This paper
[m/H] |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|−0.1 ± 0.1This paper
vsin i (km s−1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|3 ± 1This paper
Rotation period (d) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|9.92 ± 0.23This paper
Gyrochronology age (Myr) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $||$470_{-110}^{+170}$|Based on the gyrochronology relationship from Bouma, Palumbo & Hillenbrand (2023)
Limb darkening coefficients (TESSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.463 ± 0.021Claret (2017)
Limb darkening coefficients (TESSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.182 ± 0.020Claret (2017)
Limb darkening coefficients (CHEOPSu1) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.604 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (CHEOPSu2) |$\ldots \ldots \ldots \ldots \ldots \ldots \ldots \ldots $|0.111 ± 0.022Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u1) |$\ldots \ldots \ldots $|0.350 ± 0.021Claret & Bloemen (2011)
Limb darkening coefficients (LCO z’ band u2) |$\ldots \ldots \ldots $|0.287 ± 0.021Claret & Bloemen (2011)
1

Propagated from Gaia via the gal uvw function in the pyastronomy package (Czesla et al. 2019).

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