Populations¶
An exoplanet Population
is designed to be a (hopefully!) relatively easy way to interact with data for a group of exoplanet systems. Here we step through the basics of how we can explore a population of planets, access standardized planet properties, and filter subsets of planet populations.
Getting started¶
The exoatlas
package contains the tools we will use, and astropy.units
will help us handle unit conversions for calculations.
import exoatlas as ea
import astropy.units as u
ea.version()
'0.6.6'
Create a Population
¶
Now, to get started, we'll make a population that contains all confirmed transiting exoplanets. We can read more about the different populations we can create over one the Creating page. When we create this population, the code will download a table of the latest data from the NASA Exoplanet Archive.
pop = ea.TransitingExoplanets()
What's inside a Population
?¶
The core ingredient to an exoplanet Population
is a table of planet properties that have been standardized and populated with astropy units. This pop.table
table is an astropy Table, so its contents can be accessed or modified as any other astropy Table
. This .table
table is created by processing the raw data from the archive, providing slightly more verbose names, and attaching units.
pop.table
name | hostname | letter | gaia_id | number_of_stars | number_of_planets | discovery_method | discovery_year | discovery_publication | discovery_facility | ra | dec | pmra | pmdec | systemic_rv_upper_limit | systemic_rv | systemic_rv_uncertainty_upper | systemic_rv_uncertainty_lower | systemic_rv_reference | distance | distance_uncertainty_upper | distance_uncertainty_lower | distance_reference | detected_in_rv | detected_in_pulsar | detected_in_pulsation_timing | detected_in_transit | detected_in_astrometry | detected_in_orbital_brightness_modulations | detected_in_microlensing | detected_in_eclipse_timing_variations | detected_in_imaging | detected_in_disk_kinematics | is_controversial | shows_ttv | stellar_spectral_type | stellar_teff_upper_limit | stellar_teff | stellar_teff_uncertainty_upper | stellar_teff_uncertainty_lower | stellar_teff_reference | stellar_radius | stellar_radius_uncertainty_upper | stellar_radius_uncertainty_lower | stellar_radius_reference | stellar_mass | stellar_mass_uncertainty_upper | stellar_mass_uncertainty_lower | stellar_mass_reference | stellar_age_lower_limit | stellar_age_upper_limit | stellar_age | stellar_age_uncertainty_upper | stellar_age_uncertainty_lower | stellar_age_reference | stellar_metallicity_lower_limit | stellar_metallicity_upper_limit | stellar_metallicity | stellar_metallicity_uncertainty_upper | stellar_metallicity_uncertainty_lower | stellar_metallicity_reference | stellar_luminosity | stellar_luminosity_uncertainty_upper | stellar_luminosity_uncertainty_lower | stellar_luminosity_reference | stellar_logg_lower_limit | stellar_logg | stellar_logg_uncertainty_upper | stellar_logg_uncertainty_lower | stellar_logg_reference | stellar_density | stellar_density_uncertainty_upper | stellar_density_uncertainty_lower | stellar_density_reference | stellar_vsini_lower_limit | stellar_vsini_upper_limit | stellar_vsini | stellar_vsini_uncertainty_upper | stellar_vsini_uncertainty_lower | stellar_vsini_reference | stellar_rotation_period_lower_limit | stellar_rotation_period_upper_limit | stellar_rotation_period | stellar_rotation_period_uncertainty_upper | stellar_rotation_period_uncertainty_lower | stellar_rotation_period_reference | magnitude_u | magnitude_u_uncertainty_upper | magnitude_u_uncertainty_lower | magnitude_u_reference | magnitude_g | magnitude_g_uncertainty_upper | magnitude_g_uncertainty_lower | magnitude_g_reference | magnitude_r | magnitude_r_uncertainty_upper | magnitude_r_uncertainty_lower | magnitude_r_reference | magnitude_i | magnitude_i_uncertainty_upper | magnitude_i_uncertainty_lower | magnitude_i_reference | magnitude_z | magnitude_z_uncertainty_upper | magnitude_z_uncertainty_lower | magnitude_z_reference | magnitude_V | magnitude_V_uncertainty_upper | magnitude_V_uncertainty_lower | magnitude_V_reference | magnitude_B | magnitude_B_uncertainty_upper | magnitude_B_uncertainty_lower | magnitude_B_reference | magnitude_IC | magnitude_IC_uncertainty_upper | magnitude_IC_uncertainty_lower | magnitude_IC_reference | magnitude_J | magnitude_J_uncertainty_upper | magnitude_J_uncertainty_lower | magnitude_J_reference | magnitude_H | magnitude_H_uncertainty_upper | magnitude_H_uncertainty_lower | magnitude_H_reference | magnitude_K | magnitude_K_uncertainty_upper | magnitude_K_uncertainty_lower | magnitude_K_reference | magnitude_W1 | magnitude_W1_uncertainty_upper | magnitude_W1_uncertainty_lower | magnitude_W1_reference | magnitude_W2 | magnitude_W2_uncertainty_upper | magnitude_W2_uncertainty_lower | magnitude_W2_reference | magnitude_W3 | magnitude_W3_uncertainty_upper | magnitude_W3_uncertainty_lower | magnitude_W3_reference | magnitude_W4 | magnitude_W4_uncertainty_upper | magnitude_W4_uncertainty_lower | magnitude_W4_reference | magnitude_gaia | magnitude_gaia_uncertainty_upper | magnitude_gaia_uncertainty_lower | magnitude_gaia_reference | magnitude_T | magnitude_T_uncertainty_upper | magnitude_T_uncertainty_lower | magnitude_T_reference | magnitude_kep | magnitude_kep_uncertainty_upper | magnitude_kep_uncertainty_lower | magnitude_kep_reference | period_lower_limit | period_upper_limit | period | period_uncertainty_upper | period_uncertainty_lower | period_reference | semimajoraxis_lower_limit | semimajoraxis | semimajoraxis_uncertainty_upper | semimajoraxis_uncertainty_lower | semimajoraxis_reference | eccentricity_lower_limit | eccentricity_upper_limit | eccentricity | eccentricity_uncertainty_upper | eccentricity_uncertainty_lower | eccentricity_reference | argument_of_periastron | argument_of_periastron_uncertainty_upper | argument_of_periastron_uncertainty_lower | argument_of_periastron_reference | inclination_lower_limit | inclination_upper_limit | inclination | inclination_uncertainty_upper | inclination_uncertainty_lower | inclination_reference | radius_lower_limit | radius | radius_uncertainty_upper | radius_uncertainty_lower | radius_reference | mass_lower_limit | mass_upper_limit | mass | mass_uncertainty_upper | mass_uncertainty_lower | mass_reference | density_lower_limit | density_upper_limit | density | density_uncertainty_upper | density_uncertainty_lower | density_reference | number_of_transmission_measurements | number_of_emission_measurements | transit_midpoint | transit_midpoint_uncertainty_upper | transit_midpoint_uncertainty_lower | transit_midpoint_reference | transit_duration_upper_limit | transit_duration | transit_duration_uncertainty_upper | transit_duration_uncertainty_lower | transit_duration_reference | transit_scaled_radius | transit_scaled_radius_uncertainty_upper | transit_scaled_radius_uncertainty_lower | transit_scaled_radius_reference | transit_depth_lower_limit | transit_depth | transit_depth_uncertainty_upper | transit_depth_uncertainty_lower | transit_depth_reference | transit_scaled_semimajoraxis_lower_limit | transit_scaled_semimajoraxis | transit_scaled_semimajoraxis_uncertainty_upper | transit_scaled_semimajoraxis_uncertainty_lower | transit_scaled_semimajoraxis_reference | transit_impact_parameter_lower_limit | transit_impact_parameter_upper_limit | transit_impact_parameter | transit_impact_parameter_uncertainty_upper | transit_impact_parameter_uncertainty_lower | transit_impact_parameter_reference | rv_semiamplitude_lower_limit | rv_semiamplitude_upper_limit | rv_semiamplitude | rv_semiamplitude_uncertainty_upper | rv_semiamplitude_uncertainty_lower | rv_semiamplitude_reference | msini_lower_limit | msini_upper_limit | msini | msini_uncertainty_upper | msini_uncertainty_lower | msini_reference | projected_obliquity_upper_limit | projected_obliquity | projected_obliquity_uncertainty_upper | projected_obliquity_uncertainty_lower | projected_obliquity_reference | obliquity_lower_limit | obliquity_upper_limit | obliquity | obliquity_uncertainty_upper | obliquity_uncertainty_lower | obliquity_reference | tidyname | tidyhostname |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
deg | deg | mas / yr | mas / yr | km / s | km / s | km / s | pc | pc | pc | K | K | K | solRad | solRad | solRad | solMass | solMass | solMass | Gyr | Gyr | Gyr | solLum | solLum | solLum | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | mag | d | d | d | AU | AU | AU | deg | deg | deg | deg | deg | deg | earthRad | earthRad | earthRad | earthMass | earthMass | earthMass | g / cm3 | g / cm3 | g / cm3 | d | d | d | h | h | h | m / s | m / s | m / s | earthMass | earthMass | earthMass | deg | deg | deg | deg | deg | deg | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
str29 | str27 | str1 | object | int64 | int64 | str29 | int64 | str42 | str60 | float64 | float64 | float64 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str33 | int64 | int64 | int64 | int64 | int64 | int64 | int64 | int64 | int64 | int64 | int64 | int64 | object | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str44 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str44 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str34 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str36 | float64 | float64 | float64 | str36 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | str33 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | int64 | int64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | str44 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str42 | float64 | float64 | float64 | float64 | float64 | str44 | float64 | float64 | float64 | float64 | str44 | float64 | float64 | float64 | float64 | float64 | str25 | str24 | str22 |
55 Cnc e | 55 Cnc | e | Gaia DR2 704967037090946688 | 2 | 5 | Radial Velocity | 2004 | McArthur et al. 2004 | McDonald Observatory | 133.1468373 | 28.3298154 | -485.872 | -233.651 | nan | 27.40949 | 8e-05 | -8e-05 | Bourrier + Hébrard 2014 | 12.5855 | 0.0124 | -0.0123 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | G8V | nan | 5172.0 | 18.0 | -18.0 | Bourrier et al. 2018 | 0.943 | 0.01 | -0.01 | Bourrier et al. 2018 | 0.905 | 0.015 | -0.015 | Bourrier et al. 2018 | nan | nan | 5.5 | 2.5 | -2.5 | Marcy et al. 2002 | nan | nan | 0.35 | 0.1 | -0.1 | Bourrier et al. 2018 | 0.6354040812391201 | 0.018288399568609694 | 0.015201317721428378 | Knapp et al. 2020 | nan | 4.43 | 0.02 | -0.02 | Bourrier et al. 2018 | 1.521203 | 0.007049 | -0.007049 | Crida et al. 2018 | nan | 1.23 | nan | nan | nan | Bourrier et al. 2018 | nan | nan | 38.8 | 0.05 | -0.05 | Bourrier et al. 2018 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 5.95084 | 0.023 | -0.023 | TICv8 | 6.816 | 0.019 | -0.019 | TICv8 | nan | nan | nan | TICv8 | 4.768 | 0.244 | -0.244 | TICv8 | 4.265 | 0.234 | -0.234 | TICv8 | 4.015 | 0.036 | -0.036 | TICv8 | nan | 0.318 | nan | Cutri et al. 2014 | nan | 0.174 | nan | Cutri et al. 2014 | nan | 0.015 | nan | Cutri et al. 2014 | nan | nan | nan | Cutri et al. 2014 | 5.72973 | 0.0008523 | -0.0008523 | TICv8 | 5.2058 | 0.0061 | -0.0061 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 0.7365474 | 1.3e-06 | -1.4e-06 | Bourrier et al. 2018 | nan | 0.01544 | 5e-05 | -5e-05 | Bourrier et al. 2018 | nan | nan | 0.05 | 0.03 | -0.03 | Bourrier et al. 2018 | 86.0 | 30.7 | -33.4 | Bourrier et al. 2018 | nan | nan | 83.59 | 0.47 | -0.44 | Bourrier et al. 2018 | nan | 1.875 | 0.029 | -0.029 | Bourrier et al. 2018 | nan | nan | 7.99 | 0.32 | -0.33 | Bourrier et al. 2018 | nan | nan | 6.66 | 0.43 | -0.4 | Bourrier et al. 2018 | 4 | 19 | 2457063.2096 | 0.0006 | -0.0004 | Bourrier et al. 2018 | nan | 1.5439 | 0.0027 | -0.0026 | Zhao et al. 2023 | 0.0182 | 0.0002 | -0.0002 | Bourrier et al. 2018 | nan | 0.00038467330000000003 | 4.1906e-06 | -4.1906e-06 | ExoFOP-TESS TOI | nan | 3.52 | 0.01 | -0.01 | Bourrier et al. 2018 | nan | nan | 0.39 | 0.03 | -0.03 | Bourrier et al. 2018 | nan | nan | 6.02 | 0.24 | -0.23 | Bourrier et al. 2018 | nan | nan | 9.3759380065 | 0.4449597698 | -0.4449597698 | Rosenthal et al. 2021 | nan | 72.4 | 12.7 | -11.5 | Bourrier + Hébrard 2014 | nan | nan | 23.0 | 15.0 | -12.0 | Zhao et al. 2023 | 55cnce | 55cnc |
AU Mic b | AU Mic | b | Gaia DR2 6794047652729201024 | 1 | 3 | Transit | 2020 | Plavchan et al. 2020 | Transiting Exoplanet Survey Satellite (TESS) | 311.2911369 | -31.34245 | 281.424 | -359.895 | nan | -6.31031 | 0.28682 | -0.28682 | Gaia DR2 | 9.7221 | 0.004625 | -0.004625 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 1 | M1 | nan | 3678.0 | 90.0 | -88.0 | Wittrock et al. 2023 | 0.744 | 0.023 | -0.021 | Wittrock et al. 2023 | 0.51 | 0.028 | -0.027 | Wittrock et al. 2023 | nan | nan | 0.0201 | 0.0025 | -0.0024 | Wittrock et al. 2023 | nan | nan | 0.23 | 0.24 | -0.3 | Wittrock et al. 2023 | 0.09160095468444289 | 0.01038776039345075 | 0.010364559304247104 | Wittrock et al. 2023 | nan | 4.404 | 0.026 | -0.031 | Wittrock et al. 2023 | 1.75 | 0.14 | -0.16 | Wittrock et al. 2023 | nan | nan | 8.5 | 0.2 | -0.2 | Donati et al. 2023 | nan | nan | 4.856 | 0.003 | -0.003 | Donati et al. 2023 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 8.81 | 0.1 | -0.1 | TICv8 | 10.209 | 0.036 | -0.036 | TICv8 | nan | nan | nan | Plavchan et al. 2020 | 5.436 | 0.017 | -0.017 | TICv8 | 4.831 | 0.016 | -0.016 | TICv8 | 4.529 | 0.02 | -0.02 | TICv8 | nan | 0.277 | nan | Cutri et al. 2014 | nan | 0.166 | nan | Cutri et al. 2014 | nan | 0.014 | nan | Cutri et al. 2014 | nan | nan | nan | Cutri et al. 2014 | 7.84038 | 0.000731 | -0.000731 | TICv8 | 6.755 | 0.032 | -0.032 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 8.46308 | 6e-05 | -6e-05 | Wittrock et al. 2023 | nan | 0.0649 | 0.0012 | -0.0012 | Wittrock et al. 2023 | nan | nan | 0.00577 | 0.00101 | -0.00101 | Wittrock et al. 2023 | 88.4304 | 0.0578 | -0.0578 | Wittrock et al. 2023 | nan | nan | 89.57917 | 0.37639 | -0.37639 | Wittrock et al. 2023 | nan | 3.95677019 | 0.14571675 | -0.14571675 | Wittrock et al. 2023 | nan | nan | 20.12 | 1.57 | -1.72 | Cale et al. 2021 | nan | nan | 1.32 | 0.19 | -0.2 | Cale et al. 2021 | 0 | 0 | 2458525.04109 | 0.00052 | -0.00051 | Wittrock et al. 2023 | nan | 3.4927 | 0.0074 | -0.0067 | Wittrock et al. 2023 | 0.0488 | 0.001 | -0.001 | Wittrock et al. 2023 | nan | 0.002379 | 0.0001 | -9.900000000000001e-05 | Wittrock et al. 2023 | nan | 18.79 | 0.5 | -0.59 | Wittrock et al. 2023 | nan | nan | 0.134 | 0.096 | -0.089 | Wittrock et al. 2023 | nan | nan | 10.23 | 0.88 | -0.91 | Cale et al. 2021 | nan | 57.2094 | nan | nan | nan | Plavchan et al. 2020 | nan | -4.7 | 6.8 | -6.4 | Hirano et al. 2020 | nan | nan | nan | nan | nan | -- | aumicb | aumic |
AU Mic c | AU Mic | c | Gaia DR2 6794047652729201024 | 1 | 3 | Transit | 2021 | Martioli et al. 2021 | Transiting Exoplanet Survey Satellite (TESS) | 311.2911369 | -31.34245 | 281.424 | -359.895 | nan | -6.31031 | 0.28682 | -0.28682 | Gaia DR2 | 9.7221 | 0.004625 | -0.004625 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | M1 | nan | 3678.0 | 90.0 | -88.0 | Wittrock et al. 2023 | 0.744 | 0.023 | -0.021 | Wittrock et al. 2023 | 0.51 | 0.028 | -0.027 | Wittrock et al. 2023 | nan | nan | 0.0201 | 0.0025 | -0.0024 | Wittrock et al. 2023 | nan | nan | 0.23 | 0.24 | -0.3 | Wittrock et al. 2023 | 0.09160095468444289 | 0.01038776039345075 | 0.010364559304247104 | Wittrock et al. 2023 | nan | 4.404 | 0.026 | -0.031 | Wittrock et al. 2023 | 1.75 | 0.14 | -0.16 | Wittrock et al. 2023 | nan | nan | 8.5 | 0.2 | -0.2 | Donati et al. 2023 | nan | nan | 4.856 | 0.003 | -0.003 | Donati et al. 2023 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 8.81 | 0.1 | -0.1 | TICv8 | 10.209 | 0.036 | -0.036 | TICv8 | nan | nan | nan | Plavchan et al. 2020 | 5.436 | 0.017 | -0.017 | TICv8 | 4.831 | 0.016 | -0.016 | TICv8 | 4.529 | 0.02 | -0.02 | TICv8 | nan | 0.277 | nan | Cutri et al. 2014 | nan | 0.166 | nan | Cutri et al. 2014 | nan | 0.014 | nan | Cutri et al. 2014 | nan | nan | nan | Cutri et al. 2014 | 7.84038 | 0.000731 | -0.000731 | TICv8 | 6.755 | 0.032 | -0.032 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 18.85969 | 8e-05 | -8e-05 | Wittrock et al. 2023 | nan | 0.1108 | 0.002 | -0.002 | Wittrock et al. 2023 | nan | nan | 0.00338 | 0.00164 | -0.00164 | Wittrock et al. 2023 | 223.2844 | 1.6836 | -1.6836 | Wittrock et al. 2023 | nan | nan | 89.22655 | 0.21654 | -0.21654 | Wittrock et al. 2023 | nan | 2.52202066 | 0.24659758 | -0.24659758 | Wittrock et al. 2023 | nan | nan | 9.6 | 2.07 | -2.31 | Cale et al. 2021 | nan | nan | 1.22 | 0.26 | -0.29 | Cale et al. 2021 | 0 | 0 | 2458342.224 | 0.0019 | -0.0018 | Wittrock et al. 2023 | nan | 4.236 | 0.029 | -0.029 | Wittrock et al. 2023 | 0.0311 | 0.0028 | -0.0028 | Wittrock et al. 2023 | nan | 0.00097 | 0.00017999999999999998 | -0.00017 | Wittrock et al. 2023 | nan | 32.05 | 0.86 | -1.0 | Wittrock et al. 2023 | nan | nan | 0.3 | 0.13 | -0.19 | Wittrock et al. 2023 | nan | nan | 3.68 | 0.87 | -0.86 | Cale et al. 2021 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | aumicc | aumic |
BD+05 4868 A b | BD+05 4868 A | b | Gaia DR2 2700378125204437760 | 2 | 1 | Transit | 2025 | Hon et al. 2025 | Transiting Exoplanet Survey Satellite (TESS) | 326.8614036 | 6.6053185 | 205.457 | 106.6 | nan | -25.6 | 0.2 | -0.2 | Hon et al. 2025 | 43.5687 | 0.0975 | -0.0971 | TICv8 | 0 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | K V | nan | 4596.0 | 65.0 | -64.0 | Hon et al. 2025 | 0.69 | 0.02 | -0.02 | Hon et al. 2025 | 0.7 | 0.02 | -0.02 | Hon et al. 2025 | nan | nan | 11.1 | 1.7 | -3.0 | Hon et al. 2025 | nan | nan | -0.05 | 0.08 | -0.05 | Hon et al. 2025 | 0.19199945679542882 | 0.0049337811718140135 | 0.005066409697938046 | Hon et al. 2025 | nan | 4.6 | 0.03 | -0.02 | Hon et al. 2025 | 2.994175 | 0.94744 | -0.701929 | TICv8 | nan | 3.0 | nan | nan | nan | Hon et al. 2025 | nan | nan | nan | nan | nan | -- | 15.6057 | 0.0093455 | -0.0093455 | TICv8 | 10.9218 | 0.0005589 | -0.0005589 | TICv8 | 9.76663 | 0.0004225 | -0.0004225 | TICv8 | 9.4008 | 0.0008059 | -0.0008059 | TICv8 | 12.014 | 0.0091291 | -0.0091291 | TICv8 | 10.158 | 0.01 | -0.01 | TICv8 | 11.212 | 0.0714143 | -0.0714143 | TICv8 | nan | nan | nan | TICv8 | 8.113 | 0.027 | -0.027 | TICv8 | 7.567 | 0.034 | -0.034 | TICv8 | 7.448 | 0.026 | -0.026 | TICv8 | 7.225 | 0.035 | -0.035 | TICv8 | 7.339 | 0.02 | -0.02 | TICv8 | 7.284 | 0.017 | -0.017 | TICv8 | 7.247 | 0.14 | -0.14 | TICv8 | 9.84152 | 0.000476 | -0.000476 | TICv8 | 9.1886 | 0.006 | -0.006 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 1.271869 | 1e-06 | -1e-06 | Hon et al. 2025 | nan | 0.0208 | 0.0003 | -0.0003 | Hon et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | 6.2 | nan | nan | nan | Hon et al. 2025 | nan | nan | nan | nan | nan | -- | 0 | 0 | 2460556.2892 | 0.0003 | -0.0003 | Hon et al. 2025 | nan | nan | nan | nan | -- | nan | nan | nan | -- | nan | 0.013999999999999999 | 0.006 | -0.006 | Hon et al. 2025 | nan | 6.4 | 0.2 | -0.2 | Hon et al. 2025 | nan | nan | nan | nan | nan | -- | nan | 4.5 | nan | nan | nan | Hon et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | bd054868ab | bd054868a |
BD+20 594 b | BD+20 594 | b | Gaia DR2 58200934326315136 | 1 | 1 | Transit | 2016 | Espinoza et al. 2016 | K2 | 53.6511231 | 20.5990205 | 36.5714 | -51.3647 | nan | -20.33638 | 0.00073 | -0.00073 | Espinoza et al. 2016 | 179.461 | 1.257 | -1.24 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | G | nan | 5766.0 | 99.0 | -99.0 | Stassun et al. 2017 | 1.08 | 0.06 | -0.06 | Stassun et al. 2017 | 1.67 | 0.4 | -0.4 | Stassun et al. 2017 | nan | nan | 3.34 | 1.95 | -1.49 | Espinoza et al. 2016 | nan | nan | nan | nan | nan | Stassun et al. 2017 | 0.8799945855058902 | 0.13849503603116636 | 0.12901212793130012 | Espinoza et al. 2016 | nan | 4.5 | 0.08 | -0.08 | Stassun et al. 2017 | 1.89 | 0.34 | -0.34 | Stassun et al. 2017 | nan | nan | 3.3 | 0.31 | -0.31 | Espinoza et al. 2016 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | 0.039 | nan | Espinoza et al. 2016 | nan | 0.05 | nan | Espinoza et al. 2016 | nan | 0.54 | nan | Espinoza et al. 2016 | nan | nan | nan | TICv8 | 10.849 | 0.012 | -0.012 | TICv8 | 11.765 | 0.161 | -0.161 | TICv8 | nan | nan | nan | TICv8 | 9.770001 | 0.022 | -0.022 | TICv8 | 9.432 | 0.022 | -0.022 | TICv8 | 9.368 | 0.018 | -0.018 | TICv8 | 9.31 | 0.024 | -0.024 | TICv8 | 9.344 | 0.02 | -0.02 | TICv8 | 9.332 | 0.038 | -0.038 | TICv8 | 8.976 | 0.527 | -0.527 | TICv8 | 10.8644 | 0.000249 | -0.000249 | TICv8 | 10.4021 | 0.006 | -0.006 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 41.6855 | 0.003 | -0.003 | Stassun et al. 2017 | nan | 0.241 | 0.019 | -0.017 | Espinoza et al. 2016 | nan | nan | nan | nan | nan | Stassun et al. 2017 | nan | nan | nan | -- | nan | nan | 89.55 | 0.16 | -0.16 | Stassun et al. 2017 | nan | 2.57807 | 0.11209 | -0.11209 | Stassun et al. 2017 | nan | nan | 22.2481 | 9.5349 | -9.5349 | Stassun et al. 2017 | nan | nan | 7.89 | 3.4 | -3.1 | Espinoza et al. 2016 | 0 | 0 | 2457068.52877 | 0.002801 | -0.002798 | Mayo et al. 2018 | nan | nan | nan | nan | -- | 0.02204 | 0.00058 | -0.00057 | Espinoza et al. 2016 | nan | 0.00049 | 2.5e-05 | -2.5e-05 | Stassun et al. 2017 | nan | 55.8 | 3.3 | -3.3 | Stassun et al. 2017 | nan | nan | nan | nan | nan | -- | nan | nan | 3.1 | 1.1 | -1.1 | Stassun et al. 2017 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | bd20594b | bd20594 |
BD-14 3065 b | BD-14 3065 A | b | Gaia DR2 3751877374435102720 | 3 | 1 | Transit | 2024 | Šubjak et al. 2024 | Transiting Exoplanet Survey Satellite (TESS) | 153.6696689 | -15.6428372 | -5.60772 | 7.07846 | nan | nan | nan | nan | -- | 589.423 | 16.599 | -15.729 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | None | nan | 6935.0 | 90.0 | -90.0 | Šubjak et al. 2024 | 2.35 | 0.08 | -0.08 | Šubjak et al. 2024 | 1.41 | 0.05 | -0.05 | Šubjak et al. 2024 | nan | nan | 2.24 | 0.26 | -0.26 | Šubjak et al. 2024 | nan | nan | -0.34 | 0.05 | -0.05 | Šubjak et al. 2024 | 11.481536214968829 | 0.7931164239977552 | 0.7931164239977552 | Šubjak et al. 2024 | nan | 3.85 | 0.03 | -0.03 | Šubjak et al. 2024 | 0.223 | 0.013 | -0.014 | Šubjak et al. 2024 | nan | nan | 22.0 | 3.0 | -3.0 | Šubjak et al. 2024 | nan | nan | 4.3 | 0.2 | -0.2 | Šubjak et al. 2024 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 11.1 | 0.013 | -0.013 | TICv8 | 11.484 | 0.18 | -0.18 | TICv8 | nan | nan | nan | TICv8 | 10.143 | 0.026 | -0.026 | TICv8 | 9.975 | 0.026 | -0.026 | TICv8 | 9.932 | 0.026 | -0.026 | TICv8 | 9.842 | 0.023 | -0.023 | TICv8 | 9.866 | 0.02 | -0.02 | TICv8 | 9.852 | 0.049 | -0.049 | TICv8 | 9.062 | 0.536 | -0.536 | TICv8 | 10.91 | 0.001617 | -0.001617 | TICv8 | 10.6311 | 0.0081 | -0.0081 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 4.2889731 | 5.2e-06 | -5.2e-06 | Šubjak et al. 2024 | nan | 0.0656 | 0.0026 | -0.0026 | Šubjak et al. 2024 | nan | nan | 0.066 | 0.0098 | -0.011 | Šubjak et al. 2024 | 54.0 | 6.0 | -9.1 | Šubjak et al. 2024 | nan | nan | 80.78 | 0.24 | -0.3 | Šubjak et al. 2024 | nan | 21.59 | 1.05 | -1.05 | Šubjak et al. 2024 | nan | nan | 3932.0 | 290.0 | -280.0 | Šubjak et al. 2024 | nan | nan | 2.15 | 0.53 | -0.48 | Šubjak et al. 2024 | 0 | 0 | 2459313.48578 | 0.00076 | -0.00076 | Šubjak et al. 2024 | nan | 3.086 | 0.041 | -0.041 | Šubjak et al. 2024 | 0.0843 | 0.0023 | -0.0022 | Šubjak et al. 2024 | nan | 0.00649 | 0.00023 | -0.0002 | Šubjak et al. 2024 | nan | 6.01 | 0.12 | -0.13 | Šubjak et al. 2024 | nan | nan | 0.9099 | 0.0092 | -0.0079 | Šubjak et al. 2024 | nan | nan | 1210.0 | 71.0 | -71.0 | Šubjak et al. 2024 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | bd143065b | bd143065a |
CoRoT-1 b | CoRoT-1 | b | Gaia DR2 3105507886130792448 | 1 | 1 | Transit | 2008 | Barge et al. 2008 | CoRoT | 102.0798591 | -3.1021394 | -6.01462 | 0.54713 | nan | 23.354 | 0.008 | -0.008 | Barge et al. 2008 | 787.909 | 23.491 | -23.491 | TICv8 | 1 | 0 | 0 | 1 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | G0 V | nan | 5950.0 | 150.0 | -150.0 | Barge et al. 2008 | 1.11 | 0.05 | -0.05 | Barge et al. 2008 | 0.95 | 0.15 | -0.15 | Barge et al. 2008 | nan | nan | 1.6 | 0.5 | -0.5 | Bonomo et al. 2017 | nan | nan | -0.3 | 0.25 | -0.25 | Barge et al. 2008 | 1.9857748224761653 | 0.13392605012025915 | 0.14361957098932537 | Gaia DR2 | nan | 4.25 | 0.3 | -0.3 | Barge et al. 2008 | 0.93 | 0.027 | -0.027 | Southworth 2011 | nan | nan | 5.2 | 1.0 | -1.0 | Barge et al. 2008 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 13.623 | 0.114 | -0.114 | TICv8 | 14.158 | 0.053 | -0.053 | TICv8 | nan | nan | nan | TICv8 | 12.462 | 0.029 | -0.029 | TICv8 | 12.218 | 0.026 | -0.026 | TICv8 | 12.149 | 0.027 | -0.027 | TICv8 | 12.098 | 0.023 | -0.023 | TICv8 | 12.136 | 0.023 | -0.023 | TICv8 | 12.29 | 0.338 | -0.338 | TICv8 | nan | nan | nan | TICv8 | 13.457 | 0.000477 | -0.000477 | TICv8 | 13.0501 | 0.0165 | -0.0165 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 1.5089557 | 6.4e-06 | -6.4e-06 | Barge et al. 2008 | nan | 0.02752 | 0.00022 | -0.00023 | Bonomo et al. 2017 | nan | nan | nan | nan | nan | Barge et al. 2008 | nan | nan | nan | -- | nan | nan | 85.1 | 0.5 | -0.5 | Barge et al. 2008 | nan | 16.7 | 0.9 | -0.9 | Barge et al. 2008 | nan | nan | 327.35 | 38.14 | -38.14 | Barge et al. 2008 | nan | nan | 0.38 | 0.05 | -0.05 | Barge et al. 2008 | 6 | 7 | 2454159.4532 | 0.0001 | -0.0001 | Barge et al. 2008 | nan | 2.373 | 0.245 | -0.245 | ExoFOP-TESS TOI | 0.1388 | 0.0021 | -0.0021 | Barge et al. 2008 | nan | 0.0192654 | 0.00058737 | -0.0005785520000000001 | Barge et al. 2008 | nan | 4.92 | 0.08 | -0.08 | Barge et al. 2008 | nan | nan | 0.35 | 0.08 | -0.08 | Pont et al. 2010 | nan | nan | 188.0 | 11.0 | -11.0 | Barge et al. 2008 | nan | nan | nan | nan | nan | -- | nan | 77.0 | 11.0 | -11.0 | Pont et al. 2010 | nan | nan | nan | nan | nan | -- | corot1b | corot1 |
CoRoT-10 b | CoRoT-10 | b | Gaia DR2 4263752921128319616 | 1 | 1 | Transit | 2010 | Bonomo et al. 2010 | CoRoT | 291.0636813 | 0.7460143 | -3.19635 | -22.735 | nan | 15.33 | 0.007 | -0.007 | Bonomo et al. 2010 | 338.386 | 3.9865 | -3.9865 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | K1 V | nan | 5075.0 | 75.0 | -75.0 | Bonomo et al. 2010 | 0.79 | 0.05 | -0.05 | Bonomo et al. 2010 | 0.89 | 0.05 | -0.05 | Bonomo et al. 2010 | nan | 3.0 | nan | nan | nan | Bonomo et al. 2010 | nan | nan | 0.26 | 0.07 | -0.07 | Bonomo et al. 2010 | 0.18789706657349484 | 0.005139869935972136 | 0.005282644100860251 | Gaia DR2 | nan | 4.65 | 0.1 | -0.1 | Bonomo et al. 2010 | 3.32 | 0.7 | -0.7 | Bonomo et al. 2010 | nan | nan | 2.0 | 0.5 | -0.5 | Bonomo et al. 2010 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | 0.03 | nan | Bonomo et al. 2010 | nan | 0.03 | nan | Bonomo et al. 2010 | nan | nan | nan | TICv8 | 15.293 | 0.137 | -0.137 | TICv8 | 17.344 | 0.166 | -0.166 | TICv8 | nan | nan | nan | TICv8 | 12.527 | 0.025 | -0.025 | TICv8 | 11.929 | 0.028 | -0.028 | TICv8 | 11.782 | 0.021 | -0.021 | TICv8 | 11.64 | 0.022 | -0.022 | TICv8 | 11.752 | 0.023 | -0.023 | TICv8 | 11.396 | 0.213 | -0.213 | TICv8 | nan | nan | nan | TICv8 | 14.6645 | 0.000329 | -0.000329 | TICv8 | 13.8215 | 0.006 | -0.006 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 13.2406 | 0.0002 | -0.0002 | Bonomo et al. 2010 | nan | 0.1055 | 0.0021 | -0.0021 | Bonomo et al. 2010 | nan | nan | 0.53 | 0.04 | -0.04 | Bonomo et al. 2010 | 218.9 | 6.4 | -6.4 | Bonomo et al. 2010 | nan | nan | 88.55 | 0.2 | -0.2 | Bonomo et al. 2010 | nan | 10.87 | 0.78 | -0.78 | Bonomo et al. 2010 | nan | nan | 874.0 | 50.85 | -50.85 | Bonomo et al. 2010 | nan | nan | 3.7 | 0.83 | -0.83 | Bonomo et al. 2010 | 0 | 0 | 2454273.3436 | 0.0012 | -0.0012 | Bonomo et al. 2010 | nan | 2.98 | 0.06 | -0.06 | Bonomo et al. 2010 | 0.1269 | 0.0038 | -0.0038 | Bonomo et al. 2010 | nan | 0.0161036 | 0.000978881 | -0.000949999 | Bonomo et al. 2010 | nan | 31.33 | 2.15 | -2.15 | Bonomo et al. 2010 | nan | nan | 0.85 | 0.03 | -0.03 | Bonomo et al. 2010 | nan | nan | 301.0 | 10.0 | -10.0 | Bonomo et al. 2010 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | corot10b | corot10 |
CoRoT-11 b | CoRoT-11 | b | Gaia DR2 4285511294172309504 | 1 | 1 | Transit | 2010 | Gandolfi et al. 2010 | CoRoT | 280.6872998 | 5.9376586 | 1.91873 | -5.24175 | nan | -1.342 | 0.041 | -0.041 | Gandolfi et al. 2012 | 655.037 | 24.947 | -23.209 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | F6 V | nan | 6440.0 | 120.0 | -120.0 | Gandolfi et al. 2010 | 1.37 | 0.03 | -0.03 | Gandolfi et al. 2010 | 1.27 | 0.05 | -0.05 | Gandolfi et al. 2010 | nan | nan | 2.0 | 1.0 | -1.0 | Gandolfi et al. 2010 | nan | nan | -0.03 | 0.08 | -0.08 | Gandolfi et al. 2010 | 2.385228555525889 | 0.12461783002101087 | 0.1315379915823363 | Gaia DR2 | nan | 4.22 | 0.23 | -0.23 | Gandolfi et al. 2010 | 0.69 | 0.02 | -0.02 | Gandolfi et al. 2010 | nan | nan | 40.0 | 5.0 | -5.0 | Gandolfi et al. 2010 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | 0.019 | nan | Gandolfi et al. 2010 | nan | 0.053 | nan | Gandolfi et al. 2010 | nan | nan | nan | TICv8 | 12.897 | 0.114 | -0.114 | TICv8 | 13.529 | 0.029 | -0.029 | TICv8 | nan | nan | nan | TICv8 | 11.589 | 0.021 | -0.021 | TICv8 | 11.416 | 0.029 | -0.029 | TICv8 | 11.248 | 0.022 | -0.022 | TICv8 | 11.173 | 0.022 | -0.022 | TICv8 | 11.265 | 0.021 | -0.021 | TICv8 | 11.47 | 0.206 | -0.206 | TICv8 | nan | nan | nan | TICv8 | 12.841 | 0.000336 | -0.000336 | TICv8 | 12.419 | 0.0216 | -0.0216 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 2.99433 | 1.1e-05 | -1.1e-05 | Gandolfi et al. 2010 | nan | 0.0436 | 0.005 | -0.005 | Gandolfi et al. 2010 | nan | nan | nan | nan | nan | Gandolfi et al. 2010 | nan | nan | nan | -- | nan | nan | 83.17 | 0.15 | -0.15 | Gandolfi et al. 2010 | nan | 16.03 | 0.34 | -0.34 | Gandolfi et al. 2010 | nan | nan | 740.51 | 108.06 | -108.06 | Gandolfi et al. 2010 | nan | nan | 0.99 | 0.15 | -0.15 | Gandolfi et al. 2010 | 0 | 0 | 2454597.679 | 0.0003 | -0.0003 | Gandolfi et al. 2010 | nan | 2.5009 | 0.0144 | -0.0144 | Gandolfi et al. 2010 | 0.107 | 0.0005 | -0.0005 | Gandolfi et al. 2010 | nan | 0.011449 | 0.00010725 | -0.00010675 | Gandolfi et al. 2010 | nan | 6.89 | 0.08 | -0.08 | Gandolfi et al. 2010 | nan | nan | 0.818 | 0.008 | -0.008 | Gandolfi et al. 2010 | nan | nan | 280.0 | 40.0 | -40.0 | Gandolfi et al. 2010 | nan | nan | nan | nan | nan | -- | nan | 0.1 | 2.6 | -2.6 | Gandolfi et al. 2012 | nan | nan | nan | nan | nan | -- | corot11b | corot11 |
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XO-2 N b | XO-2 N | b | Gaia DR2 934346809278715776 | 2 | 3 | Transit | 2007 | Burke et al. 2007 | XO | 117.0267691 | 50.2251472 | -29.7313 | -154.272 | nan | 46.9329 | 0.0017 | -0.0017 | Damasso et al. 2015 | 154.273 | 1.459 | -1.433 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | K0 V | nan | 5340.0 | 32.0 | -32.0 | Yalçınkaya et al. 2024 | 0.99 | 0.009 | -0.009 | Crouzet et al. 2012 | nan | nan | nan | Crouzet et al. 2012 | nan | nan | 7.8 | 1.2 | -1.3 | Bonomo et al. 2017 | nan | nan | 0.43 | 0.05 | -0.05 | Bonomo et al. 2017 | 0.8161500282610129 | 0.040253639716392633 | 0.02726798843533413 | Baluev et al. 2015 | nan | 4.433 | 0.008 | -0.008 | Crouzet et al. 2012 | 1.41 | 0.04 | -0.039 | Crouzet et al. 2012 | nan | nan | 1.07 | 0.09 | -0.09 | Bonomo et al. 2017 | nan | nan | 28.6 | 1.3 | -1.3 | Bonomo et al. 2017 | 14.9353 | 0.0067085 | -0.0067085 | TICv8 | 14.8008 | 0.0100065 | -0.0100065 | TICv8 | 14.4984 | 0.0114432 | -0.0114432 | TICv8 | 10.8006 | 0.0004149 | -0.0004149 | TICv8 | 13.0957 | 0.0152614 | -0.0152614 | TICv8 | 11.246 | 0.011 | -0.011 | TICv8 | 11.947 | 0.161 | -0.161 | TICv8 | nan | 0.012 | nan | Damasso et al. 2015 | 9.744 | 0.022 | -0.022 | TICv8 | 9.34 | 0.026 | -0.026 | TICv8 | 9.308 | 0.021 | -0.021 | TICv8 | 9.24 | 0.022 | -0.022 | TICv8 | 9.31 | 0.019 | -0.019 | TICv8 | 9.236 | 0.038 | -0.038 | TICv8 | 8.833 | 0.443 | -0.443 | TICv8 | 10.9718 | 0.000514 | -0.000514 | TICv8 | 10.4467 | 0.0061 | -0.0061 | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | nan | nan | Crouzet et al. 2012 | nan | nan | nan | nan | Crouzet et al. 2012 | nan | nan | 0.028 | 0.038 | -0.022 | Knutson et al. 2014 | 261.0 | 11.0 | -71.0 | Knutson et al. 2014 | nan | nan | 88.01 | 0.33 | -0.28 | Crouzet et al. 2012 | nan | 11.130537 | 0.134508 | -0.134508 | Crouzet et al. 2012 | nan | nan | 179.89178 | 7.94575 | -7.94575 | Crouzet et al. 2012 | nan | nan | 0.715 | 0.041 | -0.04 | Crouzet et al. 2012 | 5 | 1 | 2454508.73829 | 0.00014 | -0.00016 | Crouzet et al. 2012 | nan | 2.6839 | 0.0066 | -0.0077 | Crouzet et al. 2012 | 0.10304 | 0.00037 | -0.00037 | Crouzet et al. 2012 | nan | 0.013363 | 0.000135919 | -0.000135919 | ExoFOP-TESS TOI | nan | 7.986 | 0.074 | -0.073 | Crouzet et al. 2012 | nan | nan | 0.28 | 0.036 | -0.044 | Crouzet et al. 2012 | nan | nan | 90.17 | 0.82 | -0.82 | Bonomo et al. 2017 | nan | nan | nan | nan | nan | -- | nan | 7.0 | 11.0 | -11.0 | Damasso et al. 2015 | nan | nan | 27.0 | 12.0 | -27.0 | Damasso et al. 2015 | xo2nb | xo2n |
XO-3 b | XO-3 | b | Gaia DR2 470650560777348352 | 1 | 1 | Transit | 2007 | Johns-Krull et al. 2008 | XO | 65.4695814 | 57.8172095 | -2.51565 | 4.00264 | nan | -12.03 | 0.007 | -0.007 | Garai et al. 2017 | 213.053 | 2.724 | -2.658 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | F5V | nan | 6429.0 | 50.0 | -50.0 | Stassun et al. 2017 | 1.54 | 0.11 | -0.11 | Stassun et al. 2017 | 0.58 | 0.14 | -0.14 | Stassun et al. 2017 | nan | nan | 2.82 | 0.58 | -0.82 | Bonomo et al. 2017 | nan | nan | nan | nan | nan | Stassun et al. 2017 | 5.083115757753529 | 0.9883116467510756 | 0.7379565292237721 | Wong et al. 2014 | nan | 3.95 | 0.06 | -0.06 | Stassun et al. 2017 | 0.22 | 0.02 | -0.02 | Stassun et al. 2017 | nan | nan | 18.54 | 0.17 | -0.17 | Kokori et al. 2023 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 9.854 | 0.004 | -0.004 | TICv8 | 10.274 | 0.054 | -0.054 | TICv8 | nan | nan | nan | TICv8 | 9.013 | 0.029 | -0.029 | TICv8 | 8.845 | 0.018 | -0.018 | TICv8 | 8.791 | 0.019 | -0.019 | TICv8 | 8.754 | 0.023 | -0.023 | TICv8 | 8.765 | 0.02 | -0.02 | TICv8 | 8.736 | 0.025 | -0.025 | TICv8 | 8.372 | 0.284 | -0.284 | TICv8 | 9.73889 | 0.000258 | -0.000258 | TICv8 | 9.441 | 0.006 | -0.006 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 3.19154 | 0.00014 | -0.00014 | Stassun et al. 2017 | nan | 0.0476 | 0.0005 | -0.0005 | Johns-Krull et al. 2008 | nan | nan | 0.29 | 0.0 | 0.0 | Stassun et al. 2017 | 349.35 | 0.67 | -0.68 | Bonomo et al. 2017 | nan | nan | 79.32 | 1.36 | -1.36 | Stassun et al. 2017 | nan | 15.80469 | 1.34508 | -1.34508 | Stassun et al. 2017 | nan | nan | 2316.9807 | 378.2177 | -378.2177 | Stassun et al. 2017 | nan | nan | 8.09 | 0.89 | -0.89 | Southworth 2010 | 0 | 3 | 2457417.98678 | 0.00013 | -0.00013 | Kokori et al. 2023 | nan | 2.5032 | 0.024 | -0.0192 | Tsantaki et al. 2014 | 0.08825 | 0.00037 | -0.00037 | Wong et al. 2014 | nan | 0.0089 | 0.00078 | -0.00078 | Stassun et al. 2017 | nan | 4.95 | 0.18 | -0.18 | Stassun et al. 2017 | nan | nan | 0.696 | 0.028 | -0.033 | Patel + Espinoza 2022 | nan | nan | 1488.0 | 10.0 | -10.0 | Stassun et al. 2017 | nan | nan | 4138.12585914 | 203.41018048 | -203.41018048 | Johns-Krull et al. 2008 | nan | 37.3 | 3.7 | -3.7 | Winn et al. 2009 | nan | nan | nan | nan | nan | -- | xo3b | xo3 |
XO-4 b | XO-4 | b | Gaia DR2 990291507088739072 | 1 | 1 | Transit | 2010 | Southworth 2010 | Lowell Observatory | 110.3880285 | 58.2681094 | -16.9894 | 5.31035 | nan | 1.63576 | 0.52851 | -0.52851 | Gaia DR2 | 272.655 | 2.914 | -2.855 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | F5 V | nan | 6397.0 | 70.0 | -70.0 | Stassun et al. 2017 | 1.45 | 0.09 | -0.09 | Stassun et al. 2017 | 1.1 | 0.22 | -0.22 | Stassun et al. 2017 | nan | nan | 2.1 | 0.6 | -0.6 | Kokori et al. 2023 | nan | nan | nan | nan | nan | Stassun et al. 2017 | 3.4322585851325806 | 0.053266674636098764 | 0.05413601205597574 | Gaia DR2 | nan | 4.18 | 0.03 | -0.03 | Stassun et al. 2017 | 0.5 | 0.02 | -0.02 | Stassun et al. 2017 | nan | nan | 8.8 | 0.5 | -0.5 | Bonomo et al. 2017 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 10.814 | 0.008 | -0.008 | TICv8 | 11.149 | 0.111 | -0.111 | TICv8 | nan | nan | nan | TICv8 | 9.667 | 0.021 | -0.021 | TICv8 | 9.476 | 0.022 | -0.022 | TICv8 | 9.406 | 0.023 | -0.023 | TICv8 | 9.373 | 0.022 | -0.022 | TICv8 | 9.398 | 0.021 | -0.021 | TICv8 | 9.378 | 0.04 | -0.04 | TICv8 | nan | nan | nan | TICv8 | 10.5131 | 0.000383 | -0.000383 | TICv8 | 10.1653 | 0.0061 | -0.0061 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 4.12508 | 4e-06 | -4e-06 | Stassun et al. 2017 | nan | 0.05524 | 0.00027 | -0.00028 | Bonomo et al. 2017 | nan | nan | nan | nan | nan | Stassun et al. 2017 | 240.0 | 39.0 | -160.0 | Knutson et al. 2014 | nan | nan | 88.8 | 0.6 | -0.6 | Stassun et al. 2017 | nan | 14.01125 | 0.89672 | -0.89672 | Stassun et al. 2017 | nan | nan | 451.3186 | 60.3877 | -60.3877 | Stassun et al. 2017 | nan | nan | 0.83 | 0.1 | -0.088 | Bonomo et al. 2017 | 0 | 1 | 2456878.47303 | 0.00023 | -0.00023 | Kokori et al. 2023 | nan | 4.454 | 0.056 | -0.056 | ExoFOP-TESS TOI | 0.0881 | 0.0007 | -0.0007 | Kokori et al. 2023 | nan | 0.0078000000000000005 | 0.00012 | -0.00012 | Stassun et al. 2017 | nan | 7.68 | 0.11 | -0.11 | Stassun et al. 2017 | nan | nan | nan | nan | nan | -- | nan | nan | 168.6 | 6.2 | -6.2 | Stassun et al. 2017 | nan | nan | nan | nan | nan | -- | nan | -46.7 | 8.1 | -6.1 | Narita et al. 2010 | nan | nan | nan | nan | nan | -- | xo4b | xo4 |
XO-5 b | XO-5 | b | Gaia DR2 920308932010648448 | 1 | 1 | Transit | 2008 | Burke et al. 2008 | XO | 116.7163868 | 39.0944695 | -21.5254 | -23.9055 | nan | -9.84207 | 1.51936 | -1.51936 | Gaia DR2 | 276.211 | 3.919 | -3.812 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | G8 V | nan | 5430.0 | 70.0 | -70.0 | Smith 2015 | 1.13 | 0.03 | -0.03 | Smith 2015 | 1.04 | 0.03 | -0.03 | Smith 2015 | nan | nan | 8.5 | 0.8 | -0.8 | Kokori et al. 2023 | nan | nan | 0.05 | 0.06 | -0.06 | Smith 2015 | 0.8709635899560807 | 0.08021871115093801 | 0.08021871115093801 | Ment et al. 2018 | nan | 4.35 | 0.02 | -0.02 | Smith 2015 | 1.01 | 0.06 | -0.06 | Smith 2015 | nan | nan | 1.8 | 0.5 | -0.5 | Kokori et al. 2023 | nan | nan | nan | nan | nan | -- | 15.3529 | 0.0075771 | -0.0075771 | TICv8 | 15.008 | 0.0116719 | -0.0116719 | TICv8 | 11.9889 | 0.000865 | -0.000865 | TICv8 | 11.8207 | 0.0008332 | -0.0008332 | TICv8 | 13.6561 | 0.016259 | -0.016259 | TICv8 | 12.198 | 0.092 | -0.092 | TICv8 | 12.899 | 0.056 | -0.056 | TICv8 | nan | nan | nan | TICv8 | 10.774 | 0.019 | -0.019 | TICv8 | 10.443 | 0.021 | -0.021 | TICv8 | 10.345 | 0.018 | -0.018 | TICv8 | 10.333 | 0.024 | -0.024 | TICv8 | 10.381 | 0.02 | -0.02 | TICv8 | 10.292 | 0.067 | -0.067 | TICv8 | nan | nan | nan | TICv8 | 11.9498 | 0.000237 | -0.000237 | TICv8 | 11.4556 | 0.0061 | -0.0061 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 4.1877558 | 6e-07 | -6e-07 | Smith 2015 | nan | 0.0515 | 0.0005 | -0.0005 | Smith 2015 | nan | nan | nan | nan | nan | Smith 2015 | 331.01 | 0.72 | -0.72 | Ment et al. 2018 | nan | nan | 86.8 | 0.2 | -0.2 | Smith 2015 | nan | 12.78 | 0.34 | -0.34 | Smith 2015 | nan | nan | 378.2 | 9.53 | -9.53 | Smith 2015 | nan | nan | 1.06 | 0.08 | -0.08 | Smith 2015 | 0 | 0 | 2456864.3129 | 0.0002 | -0.0002 | Smith 2015 | nan | 3.1176 | 0.0168 | -0.0168 | Smith 2015 | 0.1039 | 0.0007 | -0.0007 | Smith 2015 | nan | 0.0108 | 0.0001 | -0.0001 | Smith 2015 | nan | 9.85 | 0.03 | -0.03 | Kokori et al. 2023 | nan | nan | 0.55 | 0.03 | -0.03 | Smith 2015 | nan | nan | 146.0 | 3.0 | -3.0 | Smith 2015 | nan | nan | 331.81452 | 10.80622 | -10.80622 | Ment et al. 2018 | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | xo5b | xo5 |
XO-6 b | XO-6 | b | Gaia DR2 1114308481600798336 | 1 | 1 | Transit | 2016 | Crouzet et al. 2017 | XO | 94.7929552 | 73.8275672 | -16.6426 | -22.5927 | nan | -1.58475 | 1.14501 | -1.14501 | Gaia DR2 | 235.479 | 2.443 | -2.393 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | F5 | nan | 6720.0 | 100.0 | -100.0 | Crouzet et al. 2017 | 1.93 | 0.18 | -0.18 | Crouzet et al. 2017 | 1.47 | 0.06 | -0.06 | Crouzet et al. 2017 | nan | nan | 1.88 | 0.9 | -0.2 | Crouzet et al. 2017 | nan | nan | -0.07 | 0.1 | -0.1 | Crouzet et al. 2017 | 3.436687157499013 | 0.05001183238665306 | 0.050724026202285784 | Gaia DR2 | nan | 4.04 | 0.1 | -0.1 | Crouzet et al. 2017 | 1.0 | 0.056 | -0.056 | Crouzet et al. 2017 | nan | nan | 48.0 | 3.0 | -3.0 | Crouzet et al. 2017 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 10.247 | 0.004 | -0.004 | TICv8 | 10.678 | 0.056 | -0.056 | TICv8 | nan | nan | nan | TICv8 | 9.471 | 0.02 | -0.02 | TICv8 | 9.266 | 0.017 | -0.017 | TICv8 | 9.246 | 0.02 | -0.02 | TICv8 | 9.213 | 0.023 | -0.023 | TICv8 | 9.232 | 0.021 | -0.021 | TICv8 | 9.34 | 0.037 | -0.037 | TICv8 | nan | nan | nan | TICv8 | 10.191 | 0.000329 | -0.000329 | TICv8 | 9.88278 | 0.006 | -0.006 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 3.7650007 | 8.1e-06 | -8.1e-06 | Crouzet et al. 2017 | nan | 0.0815 | 0.0077 | -0.0077 | Crouzet et al. 2017 | nan | nan | nan | nan | nan | Crouzet et al. 2017 | nan | nan | nan | -- | nan | nan | 86.0 | 0.2 | -0.2 | Crouzet et al. 2017 | nan | 23.20263 | 2.46598 | -2.46598 | Crouzet et al. 2017 | nan | 1398.452 | nan | nan | nan | Crouzet et al. 2017 | nan | 0.62 | nan | nan | nan | Crouzet et al. 2017 | 0 | 0 | 2456652.71245 | 0.00055 | -0.00055 | Crouzet et al. 2017 | nan | 2.9 | 0.1 | -0.1 | Crouzet et al. 2017 | 0.11 | 0.006 | -0.006 | Crouzet et al. 2017 | nan | 0.014735 | 7.2808e-05 | -7.2808e-05 | ExoFOP-TESS TOI | nan | 9.08 | 0.17 | -0.17 | Crouzet et al. 2017 | nan | nan | 0.633 | 0.034 | -0.034 | Crouzet et al. 2017 | nan | 450.0 | nan | nan | nan | Crouzet et al. 2017 | nan | nan | nan | nan | nan | -- | nan | -20.7 | 2.3 | -2.3 | Crouzet et al. 2017 | nan | nan | nan | nan | nan | -- | xo6b | xo6 |
XO-7 b | XO-7 | b | Gaia DR2 2303332931542914048 | 1 | 1 | Transit | 2019 | Crouzet et al. 2020 | XO | 277.4780753 | 85.2333208 | -15.3542 | 24.4608 | nan | -12.983 | 0.015 | -0.015 | Crouzet et al. 2020 | 234.149 | 1.194 | -1.181 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | G0 V | nan | 6250.0 | 100.0 | -100.0 | Crouzet et al. 2020 | 1.48 | 0.022 | -0.022 | Crouzet et al. 2020 | 1.405 | 0.059 | -0.059 | Crouzet et al. 2020 | nan | nan | 1.18 | 0.98 | -0.71 | Crouzet et al. 2020 | nan | nan | 0.432 | 0.057 | -0.057 | Crouzet et al. 2020 | 2.699727932818183 | 0.02467892257418971 | 0.02492757670591958 | Gaia DR2 | nan | 4.246 | 0.023 | -0.023 | Crouzet et al. 2020 | 0.451084 | 0.10508 | -0.093724 | TICv8 | nan | nan | 6.0 | 1.0 | -1.0 | Crouzet et al. 2020 | nan | nan | 3.62 | 0.12 | -0.12 | Knudstrup et al. 2024 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 10.521 | 0.006 | -0.006 | TICv8 | 11.229 | 0.087 | -0.087 | TICv8 | nan | nan | nan | TICv8 | 9.557 | 0.024 | -0.024 | TICv8 | 9.308 | 0.03 | -0.03 | TICv8 | 9.241 | 0.024 | -0.024 | TICv8 | 9.16 | 0.023 | -0.023 | TICv8 | 9.192 | 0.02 | -0.02 | TICv8 | 9.109 | 0.026 | -0.026 | TICv8 | 9.215 | 0.444 | -0.444 | TICv8 | 10.4575 | 0.000449 | -0.000449 | TICv8 | 10.0521 | 0.0061 | -0.0061 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 2.8641424 | 4.3e-06 | -4.3e-06 | Crouzet et al. 2020 | nan | 0.04421 | 0.00062 | -0.00062 | Crouzet et al. 2020 | nan | nan | 0.038 | 0.033 | -0.033 | Crouzet et al. 2020 | nan | nan | nan | -- | nan | nan | 83.45 | 0.29 | -0.29 | Crouzet et al. 2020 | nan | 15.389957 | 0.291434 | -0.291434 | Crouzet et al. 2020 | nan | nan | 225.34147 | 10.80622 | -10.80622 | Crouzet et al. 2020 | nan | nan | 0.34 | 0.027 | -0.027 | Crouzet et al. 2020 | 0 | 0 | 2457917.47503 | 0.00045 | -0.00045 | Crouzet et al. 2020 | nan | 2.772 | 0.0336 | -0.0336 | Crouzet et al. 2020 | 0.09532 | 0.00093 | -0.00093 | Crouzet et al. 2020 | nan | 0.00909 | 0.00017999999999999998 | -0.00017999999999999998 | Crouzet et al. 2020 | nan | 6.43 | 0.14 | -0.14 | Crouzet et al. 2020 | nan | nan | 0.709 | 0.023 | -0.023 | Crouzet et al. 2020 | nan | nan | 80.5 | 3.2 | -3.2 | Crouzet et al. 2020 | nan | nan | nan | nan | nan | -- | nan | 0.0 | 20.0 | -14.0 | Knudstrup et al. 2024 | nan | nan | 70.0 | 1.7 | -1.7 | Knudstrup et al. 2024 | xo7b | xo7 |
ZTF J1230-2655 b | ZTF J1230-2655 | b | Gaia DR2 3475360576690175616 | 1 | 1 | Transit | 2025 | Parsons et al. 2025 | Zwicky Transient Facility | 187.5689308 | -26.9309608 | -42.1958 | -7.67328 | nan | nan | nan | nan | -- | 186.69 | 15.112 | -13.034 | TICv8 | 0 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | None | nan | 10000.0 | 110.0 | -110.0 | Parsons et al. 2025 | 0.0123 | 0.0002 | -0.0002 | Parsons et al. 2025 | 0.646 | 0.017 | -0.017 | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | Calculated Value | nan | 8.07 | 0.05 | -0.05 | Parsons et al. 2025 | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 18.9116 | 0.046 | -0.046 | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 18.8866 | 0.002415 | -0.002415 | TICv8 | 18.8086 | 0.0214 | -0.0214 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 0.23597766 | 9.5e-07 | -9.5e-07 | Parsons et al. 2025 | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | -- | nan | nan | 86.7 | 0.3 | -0.3 | Parsons et al. 2025 | nan | 13.78704626 | 0.00560449 | -0.00560449 | Parsons et al. 2025 | nan | 7024.0077947 | nan | nan | nan | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | 0 | 0 | 2460432.5478805 | 3.2e-06 | -3.2e-06 | Parsons et al. 2025 | nan | nan | nan | nan | -- | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | 1.4 | 0.012 | -0.012 | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | nan | 9000.0 | nan | nan | nan | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | ztfj12302655b | ztfj12302655 |
ZTF J1828+2308 b | ZTF J1828+2308 | b | Gaia DR2 4529477698683435264 | 1 | 1 | Transit | 2025 | Parsons et al. 2025 | Zwicky Transient Facility | 277.2031946 | 23.1439121 | -5.96713 | -19.8677 | nan | nan | nan | nan | -- | 201.827 | 5.77 | -5.464 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | None | nan | 15900.0 | 75.0 | -75.0 | Parsons et al. 2025 | 0.0131 | 0.0002 | -0.0002 | Parsons et al. 2025 | 0.61 | 0.004 | -0.004 | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | Calculated Value | nan | 8.05 | 0.05 | -0.05 | Parsons et al. 2025 | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 18.0447 | 0.0459 | -0.0459 | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 18.0258 | 0.001293 | -0.001293 | TICv8 | 18.1336 | 0.0121 | -0.0121 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 0.1120067 | 8.7e-07 | -8.7e-07 | Parsons et al. 2025 | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | nan | nan | nan | -- | nan | nan | 88.9 | 0.4 | -0.4 | Parsons et al. 2025 | nan | 11.13051784 | 0.21297063 | -0.21297063 | Parsons et al. 2025 | nan | nan | 6356.56814 | 317.828407 | -317.828407 | Parsons et al. 2025 | nan | nan | nan | nan | nan | Calculated Value | 0 | 0 | 2460431.6494044 | 2e-07 | -2e-07 | Parsons et al. 2025 | nan | nan | nan | nan | -- | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | 0.838 | 0.002 | -0.002 | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | 10500.0 | 1100.0 | -1100.0 | Parsons et al. 2025 | nan | nan | nan | nan | nan | -- | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | ztfj18282308b | ztfj18282308 |
pi Men c | HD 39091 | c | Gaia DR2 4623036865373793408 | 1 | 3 | Transit | 2018 | Gandolfi et al. 2018 | Transiting Exoplanet Survey Satellite (TESS) | 84.2992798 | -80.4646041 | 311.187 | 1048.84 | nan | 10.70916 | 0.00039 | -0.00039 | Kokori et al. 2023 | 18.2702 | 0.0226 | -0.0226 | TICv8 | 1 | 0 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | G0 V | nan | 5998.0 | 62.0 | -62.0 | Damasso et al. 2020 | 1.17 | 0.02 | -0.02 | Damasso et al. 2020 | 1.07 | 0.04 | -0.04 | Damasso et al. 2020 | nan | nan | 3.92 | 1.03 | -0.98 | Damasso et al. 2020 | nan | nan | 0.09 | 0.04 | -0.04 | Damasso et al. 2020 | 1.4440093323399628 | 0.01984997754585799 | 0.020149223438509115 | Venner et al. 2021 | nan | 4.43 | 0.1 | -0.1 | Damasso et al. 2020 | 0.944584 | 0.056393 | -0.056393 | Damasso et al. 2020 | nan | nan | 3.34 | 0.07 | -0.07 | Damasso et al. 2020 | nan | nan | nan | nan | nan | -- | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | nan | nan | nan | TICv8 | 5.65 | 0.03 | -0.03 | TICv8 | 6.252 | 0.021 | -0.021 | TICv8 | nan | nan | nan | TICv8 | 4.869 | 0.272 | -0.272 | TICv8 | 4.424 | 0.226 | -0.226 | TICv8 | 4.241 | 0.027 | -0.027 | TICv8 | nan | 0.329 | nan | Cutri et al. 2014 | nan | 0.16 | nan | Cutri et al. 2014 | nan | 0.02 | nan | Cutri et al. 2014 | nan | nan | nan | Cutri et al. 2014 | 5.5128 | 0.0019464 | -0.0019464 | TICv8 | 5.1054 | 0.0063 | -0.0063 | TICv8 | nan | nan | nan | TICv8 | nan | nan | 6.267852 | 1.6e-05 | -1.6e-05 | Damasso et al. 2020 | nan | 0.068 | 0.0008 | -0.0008 | Damasso et al. 2020 | nan | nan | nan | nan | nan | Damasso et al. 2020 | nan | nan | nan | Damasso et al. 2020 | nan | nan | 87.05 | 0.15 | -0.15 | Damasso et al. 2020 | nan | 2.11 | 0.05 | -0.05 | Damasso et al. 2020 | nan | nan | 4.3 | 0.7 | -0.7 | Damasso et al. 2020 | nan | nan | 2.8 | 0.5 | -0.5 | Damasso et al. 2020 | 0 | 0 | 2458519.8068 | 0.0003 | -0.0003 | Damasso et al. 2020 | nan | 2.969 | 0.03 | -0.032 | Gandolfi et al. 2018 | 0.0165 | 0.0001 | -0.0001 | Damasso et al. 2020 | nan | 0.000321 | 7.4565000000000005e-06 | -7.4565000000000005e-06 | ExoFOP-TESS TOI | nan | 12.5 | 0.3 | -0.3 | Damasso et al. 2020 | nan | nan | 0.614 | 0.018 | -0.018 | Gandolfi et al. 2018 | nan | nan | 1.5 | 0.2 | -0.2 | Damasso et al. 2020 | nan | nan | 3.496112477 | 0.317828407 | -0.317828407 | Feng et al. 2022 | nan | nan | nan | nan | -- | nan | nan | nan | nan | nan | -- | pimenc | hd39091 |
How do we access planet properties?¶
The main way to access planet properties within a Population
is with its methods. That is, we can access an array of the values for some property x
by calling pop.x()
. Behind the scenes, the population will look to see if there is a column called "x"
in the standardized table and return that column, or it will do a calculation using some of the internal data. For example, we can get an array of planet names with:
pop.name()
array(['55 Cnc e', 'AU Mic b', 'AU Mic c', ..., 'ZTF J1230-2655 b', 'ZTF J1828+2308 b', 'pi Men c'], shape=(4424,), dtype='<U29')
pop.radius()
pop.get("radius")
We also have access to quantities that are not directly included in the table itself but can be calculated from them. For example, we can get an array of the amount of insolation that the planets receive from their stars as:
pop.insolation()
In this case, the insolation is calculated from the planet's orbital separation and the luminosity of the star (which is itself calculated from the stellar effective temperature and radius).
If information needed to do a calculation is missing, exoatlas
will try to estimate them from other available information. In the .insolation
case, some planets had no semimajor axes defined in the .table
table, but we were able to calculate this quantity from the orbital period, the stellar mass, and Newton's Version of Kepler's 3rd Law.
With this toolkit, you can now access the data you need to make some pretty fundamental plots in exoplanetary science. For example:
import matplotlib.pyplot as plt
plt.loglog(pop.relative_insolation(), pop.radius(), ".")
plt.xlabel("Flux Received (relative to Earth)")
plt.ylabel("Planet Radius (Earth radii)");
Why is everything a function?¶
Many bits of data are simply columns in a giant table, so it might feel a little unnecessary to have to call them as functions. However, others that depend on calculations might need to have custom keyword inputs and/or options to specify, so they need to be callable. For consistency, we just make everything act like a function.
For example, equilibrium temperature depends on assumed albedo, so it's nice to be able to provide that as a keyword:
pop.teq()
pop.teq(albedo=0.7)
Or, for some calculations, there's a kludge
option that allows missing masses and/or radii to be replaced with reasonable (but horribly imprecise!) theoretical estimates. We can see this making a difference if we look at a population with imprecise or missing mass estimates, and try to calculate the estimate transmission spectroscopy signal (see Observing), which depends on the planet's surface gravity, and therefore its mass. By default, nothing will be calculated for planets without masses; if kludge=True
, planet's without masses will use estimated masses instead!
b = ea.BadMass()
b.transmission_signal()
b.transmission_signal(kludge=True)
How do we retrieve uncertainties?¶
We will often want to know the uncertainty on a particular quantity. We can retrieve this either with the .get_uncertainty()
method, or by appending _uncertainty
to the name of a quantity. For core table quantities, uncertainties are extracted directly from the table.
sigma = pop.get_uncertainty("radius")
sigma
sigma = pop.radius_uncertainty()
sigma
For more details about how uncertainties are calculated and propagated, please see Uncertainties.
How do we access some sub-population of planets?¶
Often we'll want to pull out some subset of a population. We might want a smaller sample of planets, or all the planets that meet some particular criterion, or maybe the properties of one individual planet. In our experience with numpy
arrays or astropy
tables, we've often done this by indexing (x[0]
or x[[0, 1, 5]]
), slicing (x[3:30]
), or masking (x[some_array > some_other_array]
).
We can apply the same methods to a Population
, creating smaller populations by indexing, slicing, or masking. Anything we can do with a Population
we can do with one of these sub-Population
s that we create.
pop
✨ Transiting Exoplanets | 4424 elements ✨
one_planet = pop[0]
one_planet
✨ Transiting Exoplanets | 1 elements ✨
one_planet.name(), one_planet.radius(), one_planet.insolation()
(array(['55 Cnc e'], dtype='<U29'), <Quantity [1.875] earthRad>, <Quantity [3627994.74216773] W / m2>)
prime_planets = pop[[2, 3, 5, 7, 11, 13, 17, 19, 23]]
prime_planets
✨ Transiting Exoplanets | 9 elements ✨
first_ten = pop[:10]
first_ten
✨ Transiting Exoplanets | 10 elements ✨
every_other_exoplanet = pop[::2]
every_other_exoplanet
✨ Transiting Exoplanets | 2212 elements ✨
import astropy.units as u
small = pop[pop.radius() < 4 * u.Rearth]
small
✨ Transiting Exoplanets | 3007 elements ✨
Additionally, we can extract an individual planet or a list of planets by indexing the population with planet name(s). This is using astropy tables' .loc
functionality, with "name"
being used as an index.
cute_planet = pop["GJ 1214b"]
cute_planet
✨ GJ 1214b | 1 elements ✨
cute_planets = pop[["LHS 1140b", "GJ 1214b", "GJ 436b"]]
cute_planets
✨ LHS 1140b+GJ 1214b+GJ 436b | 3 elements ✨
Systems of planets can also be extracted via name using the hostname
.
pop["TRAPPIST-1"]
✨ TRAPPIST-1 | 7 elements ✨
Unfortunately it's not possible (right now) to mix and match selecting objects via both the planet name and the host name at the same time. Sorry!
How do we add new quantities?¶
Obviously sometimes we might sometimes want to add additional quantities into a population, for filtering or calculating or visualizing.
.add_column
for arrays¶
For static quantities, we could just add a new column to the internal .table
astropy Table, it's a little more graceful to use the .add_column
wrapper. This both adds the data into .table
and registers a new method that can be used to extract it (or calculate its uncertainties).
s = ea.SolarSystem()
new_column_name = "is_inhabited"
new_column_data = (s.name() == "Earth") * 1
new_column_uncertainty = (s.name() != "Earth") * 0.01
s.add_column(
name=new_column_name, data=new_column_data, uncertainty=new_column_uncertainty
)
We can see that our column was added, both to the table and as a callable column method.
s.table["is_inhabited"]
0 |
0 |
1 |
0 |
0 |
0 |
0 |
0 |
s.table["is_inhabited_uncertainty"]
0.01 |
0.01 |
0.0 |
0.01 |
0.01 |
0.01 |
0.01 |
0.01 |
s.is_inhabited()
array([0, 0, 1, 0, 0, 0, 0, 0])
s.is_inhabited_uncertainty()
array([0.01, 0.01, 0. , 0.01, 0.01, 0.01, 0.01, 0.01])
.add_calculation
for functions¶
For quantities we want to calculate on the fly, we can define a new function and then assign it to a method name inside our population using .add_calculation
. If we want to be able to propagate uncertainties, we will need to pass the distribution
keyword into all ingredient quantities that go into the calculation, and set its default for the function overall to False
. This says that when the method is being called normally, it should just return quantity arrays, but when it's being called inside of an uncertainty propagation calculation, everything will be treated as a quantity distributions.
import numpy as np
def f(self, distribution=False):
"""
Surface Area (m)
Calculate the surface area of a planet,
based on its radius.
"""
return 4 * np.pi * self.radius(distribution=distribution)
pop.add_calculation(name="surface_area", function=f)
pop.surface_area()
pop.surface_area_uncertainty()
How do we get help on available quantities?¶
It's super important to be able to know exactly what the quantity we're retrieving represents. There are few tools for quick documentation.
Short descriptions of some common attributes can printed with the help()
function. This will return a dictionary containing 1-line summaries of all quantities that can be accessed for the Population
.
pop.help(['quantities'])
⚖️ The available quantities are: airmass = Airmass (unitless) altaz = Altitude, Azimuth (astropy.coordinates.SkyCoord) angular_separation = Maximum Angular Separation (a/D, arcseconds) argument_of_periastron = Planet Orbital Argument of Periastron ($\omega$, degrees) dec = The table quantity 'dec', with units of 'deg'. density = Planet Density (m/s**2) depth_snr = Transit Depth S/N depth_uncertainty = Transit/Eclipse Depth Uncertainty (unitless) detected_in_astrometry = The table quantity 'detected_in_astrometry'. detected_in_disk_kinematics = The table quantity 'detected_in_disk_kinematics'. detected_in_eclipse_timing_variations = The table quantity 'detected_in_eclipse_timing_variations'. detected_in_imaging = The table quantity 'detected_in_imaging'. detected_in_microlensing = The table quantity 'detected_in_microlensing'. detected_in_orbital_brightness_modulations = The table quantity 'detected_in_orbital_brightness_modulations'. detected_in_pulsar = The table quantity 'detected_in_pulsar'. detected_in_pulsation_timing = The table quantity 'detected_in_pulsation_timing'. detected_in_rv = The table quantity 'detected_in_rv'. detected_in_transit = The table quantity 'detected_in_transit'. discovery_facility = The table quantity 'discovery_facility'. discovery_method = The table quantity 'discovery_method'. discovery_publication = The table quantity 'discovery_publication'. discovery_year = The table quantity 'discovery_year'. distance = The table quantity 'distance', with units of 'pc'. distance_modulus = Distance Modulus ($\mu$, magnitudes) eccentricity = Planet Orbital Eccentricity (e, unitless) emission_signal = Thermal Emission Eclipse Signal (unitless) emission_snr = Thermal Emission Eclipse Depth S/N escape_parameter = Jeans Atmospheric Escape Parameter (unitless) escape_velocity = Planet Escape Velocity (km/s) gaia_id = The table quantity 'gaia_id'. hostname = The table quantity 'hostname'. imaging_contrast = Reflected Light Imaging Contrast (unitless) impact_velocity = Very Approximately Estimated Impact Velocity (km/s) inclination = The table quantity 'inclination', with units of 'deg'. insolation = Planet Insolation (S, W/m**2) is_controversial = The table quantity 'is_controversial'. kludge_mass = Planet Mass or msini (Earth masses) kludge_radius = Planet Radius or Estimated Planet Radius (Earth radii) kludge_stellar_age = System Age (Gyr) letter = The table quantity 'letter'. log_relative_insolation = log(Relative Planet Insolation) magnitude_B = The table quantity 'magnitude_B', with units of 'mag'. magnitude_H = The table quantity 'magnitude_H', with units of 'mag'. magnitude_IC = The table quantity 'magnitude_IC', with units of 'mag'. magnitude_J = The table quantity 'magnitude_J', with units of 'mag'. magnitude_K = The table quantity 'magnitude_K', with units of 'mag'. magnitude_T = The table quantity 'magnitude_T', with units of 'mag'. magnitude_V = The table quantity 'magnitude_V', with units of 'mag'. magnitude_W1 = The table quantity 'magnitude_W1', with units of 'mag'. magnitude_W2 = The table quantity 'magnitude_W2', with units of 'mag'. magnitude_W3 = The table quantity 'magnitude_W3', with units of 'mag'. magnitude_W4 = The table quantity 'magnitude_W4', with units of 'mag'. magnitude_g = The table quantity 'magnitude_g', with units of 'mag'. magnitude_gaia = The table quantity 'magnitude_gaia', with units of 'mag'. magnitude_i = The table quantity 'magnitude_i', with units of 'mag'. magnitude_kep = The table quantity 'magnitude_kep', with units of 'mag'. magnitude_r = The table quantity 'magnitude_r', with units of 'mag'. magnitude_u = The table quantity 'magnitude_u', with units of 'mag'. magnitude_z = The table quantity 'magnitude_z', with units of 'mag'. mass = The table quantity 'mass', with units of 'earthMass'. mass_estimated_from_radius_assuming_chen_and_kipping = Estimated Planet Mass (Earth masses) mass_estimated_from_radius_assuming_rockyish = Planet Mass (M_earth) msini = The table quantity 'msini', with units of 'earthMass'. name = The table quantity 'name'. number_of_emission_measurements = The table quantity 'number_of_emission_measurements'. number_of_planets = The table quantity 'number_of_planets'. number_of_stars = The table quantity 'number_of_stars'. number_of_transmission_measurements = The table quantity 'number_of_transmission_measurements'. obliquity = The table quantity 'obliquity', with units of 'deg'. orbital_velocity = Planet Orbital Velocity (km/s) period = The table quantity 'period', with units of 'd'. planet_luminosity = Planet Luminosity (K) pmdec = The table quantity 'pmdec', with units of 'mas / yr'. pmra = The table quantity 'pmra', with units of 'mas / yr'. projected_obliquity = The table quantity 'projected_obliquity', with units of 'deg'. ra = The table quantity 'ra', with units of 'deg'. radius = The table quantity 'radius', with units of 'earthRad'. radius_estimated_from_mass_assuming_chen_and_kipping = Estimated Planet Radius (Earth radii) reflection_signal = Reflection Eclipse Signal (unitless) reflection_snr = Reflected Light Eclipse Depth S/N relative_cumulative_xuv_insolation = Relative Cumulative XUV Insolation relative_escape_velocity = Planet Escape Velocity (relative to Earth) relative_insolation = Relative Planet Insolation (S/S_Earth) rv_semiamplitude = The table quantity 'rv_semiamplitude', with units of 'm / s'. scale_height = Atmospheric Scale Height (km) scaled_radius = Scaled Planet Radius ((Rp/Rs), unitless) scaled_radius_from_radii = Scaled Planet Radius ((Rp/Rs), unitless) scaled_semimajoraxis = Planet Scaled Semi-major Axis (a/R*, unitless) scaled_semimajoraxis_from_semimajoraxis = Planet Scaled Semi-major Axis (a/R*, unitless) semimajoraxis = Planet Semi-major Axis (a, AU) semimajoraxis_from_period = Planet Semi-major Axis (a, AU) semimajoraxis_from_transit_scaled_semimajoraxis = Planet Semi-major Axis (a, AU) shows_ttv = The table quantity 'shows_ttv'. stellar_age = The table quantity 'stellar_age', with units of 'Gyr'. stellar_brightness = Stellar Brightness (photons/s/m^2/micron) stellar_brightness_in_telescope_units = Stellar Brightness (photons/telescope/hour) stellar_density = The table quantity 'stellar_density'. stellar_logg = The table quantity 'stellar_logg'. stellar_luminosity = Stellar Luminosity (L*, Lsun) stellar_luminosity_from_radius_and_teff = Stellar Luminosity (L*, Lsun) stellar_mass = The table quantity 'stellar_mass', with units of 'solMass'. stellar_metallicity = The table quantity 'stellar_metallicity'. stellar_radius = The table quantity 'stellar_radius', with units of 'solRad'. stellar_rotation_period = The table quantity 'stellar_rotation_period'. stellar_spectral_type = The table quantity 'stellar_spectral_type'. stellar_teff = The table quantity 'stellar_teff', with units of 'K'. stellar_vsini = The table quantity 'stellar_vsini'. surface_area = Surface Area (m) surface_gravity = Planet Surface Gravity (m/s**2) systemic_rv = The table quantity 'systemic_rv', with units of 'km / s'. table = targeted_fractional_uncertainty_precision = teq = Planet Equilibrium Temperature (K) tidyhostname = The table quantity 'tidyhostname'. tidyname = The table quantity 'tidyname'. transit_depth = Transit Depth ((Rp/Rs)**2, unitless) transit_depth_from_radii = Transit Depth ((Rp/Rs)**2, unitless) transit_duration = Transit Duration (days) transit_duration_from_orbit = Transit Duration (days) transit_impact_parameter = Planet Impact Parameter (b) transit_impact_parameter_from_inclination = Planet Semi-major Axis (a, AU) transit_midpoint = The table quantity 'transit_midpoint', with units of 'd'. transit_scaled_radius = The table quantity 'transit_scaled_radius'. transit_scaled_semimajoraxis = The table quantity 'transit_scaled_semimajoraxis'. transmission_signal = Transmission Transit Signal (2*H*Rp/Rs**2, unitless) transmission_snr = Transmission Spectroscopy Transit Depth S/N
Most quantities will have docstrings associated with them, which you can view either with ?
, or in some tools like jupyter lab
, typing the method name and then shift + tab
, or hovering the cursor over it.
?pop.mass
?pop.teq
Explore!¶
That's about it. For more information about different pre-defined populations see Creating, and for more about pre-packaged visualizations see Visualizing.