wakai
is the Japanese word for young.
This repo contains several youth indicators and other tools to constrain exoplanet ages.
-
10 Myr
- Upper Sco
- TW Hya
- nu Cha (11)
- Beta Pic (23)
-
15 - 25 Myr
- Sco-Cen
-
50 Myr
- Tuc-Hor
- IC 2391
- IC 2602
-
100- 150 Myr
- Pisces-Eridani (120)
- Pleiades (125)
- AB Dor (150)
-
250 Myr
- M 34 (220 Myr)
- Melange I
- Group X
-
300 Myr
- NGC 3532
-
400 Myr
- M 48 (450 Myr)
-
600 - 800 Myr
- Praesepe (670)
- Hyades (730)
-
1 Gyr
- NGC 6811
-
2.5 Gyr
- NGC 6819
- Ruprecht 147 (2.7 Gyr)
See notebooks/cluster_catalog.ipynb
- See Morton+2015 using isochrones v2 code for MIST model
- See Vines & Jenkins 2022 using ARIADNE code for several models
- See Squicciarini & Bonavita using MADYS code
- See Sagear+2024 using zoomies code
- See Tofflemire+2021 using comove code
- Gagne+2018 using BANYAN SIGMA code
- See Barner & Mann 2023 using Gaia excess uncertainty variability code
- See Bouma+2023 using gyro-interp code
- See Angus+2018 using stardate code
- See also Astraea code
- Barnes 2007
- Mamajek & Hillenbrand 2008
- Angus+2015
- log(R'_HK)
- S_HK index: ratio of narrow flux to the background continuum flux
- See description in Isaacson & Fischer (2010)
- Ca II K: 3933.5 Å
- Ca II H: 3968.5 Å
- H epsilon: 3970 Å
- See Stanford-Moore+2020 using BAFFLES code
- See Jeffries+2023 using EAGLES code
- See activity-age relations of Mamajek & Hillenbrand (2008)
- 6562.8 Å
- 5889.95 and 5895.92Å
- Wood+2023
- Li I resonance: 6708 Å: 6707.78 & 6707.91 Å
- See description in Bouma+2022a
- Pleiades: Bouvier+2018
- Hyades & Praesepe: Cummings+2017
- detection by GALEX with (NUV, 1750–2750 Å) and far-UV (FUV, 1350–1750 Å)
- (NUV-J) and (J − K) colors and the empirical relations presented in Findeisen+2011
- Linder+2019: See Fig. 10 in Dong+2022
- B-V
- V-K_s
- M 48 (Barnes+2015)
- M 34 (Meibom+2011)
- Rebull+2016
- Rebull+2017
- Melange: Tofflemire+2021
- NGC 3532: Fritzewski+2021
- Group X: Newton+2022 & Messina+2022
- Praesepe: Rampalli+2021
- Pleiades: Curtis+2020
- Pis-Eri: Curtis+2019
- NGC 6811: Curtis+2019
- Stars with TESS contamination ratios > 0.2, RUWE > 1.3 (likely binary), or C*>0.04 (corrected GBP and GRP flux excess factor) were not analyzed and are not included in figures. C* calculated from phot_bp_rp_excess_factor following Riello et al. (2021, Table 2 and Equation (6)).
- See Jeffries+2023 using EAGLES code
- Pleiades: Soderblom+1993 & Bouvier+2018
- IC 2391/2602: Randich+2001
- young moving groups: Mentuch+2008 & Kraus+2014
- Praesepe: Cummings+2017
- Group X: Newton+2022 & Messina+2022
- violin plot e.g. Fig. 14 in David+2018
- weighted posterior distribution e.g. Stanford-Moore+2020