J/AJ/164/88        THYME. VIII. MELANGE-3 candidate members      (Barber+, 2022)

Transit Hunt for Young and Maturing Exoplanets (THYME). VIII. A Pleiades-age Association Harboring Two Transiting Planetary Systems from Kepler. Barber M.G., Mann A.W., Bush J.L., Tofflemire B.M., Kraus A.L., Krolikowski D.M., Vanderburg A., Fields M.J., Newton E.R., Owens D.A., Thao Pa C. <Astron. J., 164, 88 (2022)> =2022AJ....164...88B 2022AJ....164...88B
ADC_Keywords: Associations, stellar; Spectral types; Parallaxes, trigonometric; Proper motions; Radial velocities; Spectra, optical; Infrared Keywords: Transits ; Stellar associations ; Early stellar evolution ; Stellar evolution ; Exoplanet evolution ; Stellar dynamics Abstract: Young planets provide a window into the early stages and evolution of planetary systems. Ideal planets for such research are in coeval associations, where the parent population can precisely determine their ages. We describe a young association (MELANGE-3) in the Kepler field, which harbors two transiting planetary systems (KOI-3876 and Kepler-970). We identify MELANGE-3 by searching for kinematic and spatial overdensities around Kepler planet hosts with high levels of lithium. To determine the age and membership of MELANGE-3, we combine new high-resolution spectra with archival light curves, velocities, and astrometry of stars near KOI-3876 spatially and kinematically. We use the resulting rotation sequence, lithium levels, and color-magnitude diagram of candidate members to confirm the presence of a coeval 105±10Myr population. MELANGE-3 may be part of the recently identified Theia 316 stream. For the two exoplanet systems, we revise the stellar and planetary parameters, taking into account the newly determined age. Fitting the 4.5yr Kepler light curves, we find that KOI-3876b is a 2.0±0.1 R⊕ planet on a 19.58day orbit, while Kepler-970b is a 2.8±0.2R⊕ planet on a 16.73day orbit. KOI-3876 was previously flagged as an eclipsing binary, which we rule out using radial velocities from APOGEE and statistically validate the signal as planetary in origin. Given its overlap with the Kepler field, MELANGE-3 is valuable for studies of spot evolution on year timescales, and both planets contribute to the growing work on transiting planets in young stellar associations. Description: We observed KOI-3876 and 22 association candidates with the Coude spectrograph on the Harlan J.Smith 2.7m telescope at the McDonald Observatory. The Robert G.Tull Coude is a cross-dispersed echelle spectrograph, delivering an R∼60000 spectral resolution from 3400-10000Å using the 1.2" slit. Observations were taken over three nights from two observing runs, on 2021 July 9 and 2021 August 26 and 27. Objects: ----------------------------------------------------- RA (ICRS) DE Designation(s) ----------------------------------------------------- 19 18 30.0 +40 42 31 MELANGE-3 = NAME MELANGE-3 ----------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 120 1006 Candidate members of MELANGE-3 -------------------------------------------------------------------------------- See also: II/328 : AllWISE Data Release (Cutri+ 2013) I/337 : Gaia DR1 (Gaia Collaboration, 2016) IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019) III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) V/146 : LAMOST DR1 catalogs (Luo+, 2015) V/164 : LAMOST DR5 catalogs (Luo+, 2019) J/AJ/142/112 : KIC photometric calibration (Brown+, 2011) J/ApJ/733/L9 : Stellar rotation for 71 NGC 6811 members (Meibom+, 2011) J/ApJ/756/185 : Kepler TTVs. V. 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The BANYAN Σ algorithm (Gagne+, 2018) J/AJ/156/102 : TESS Input Catalog and Candidate Target List (Stassun+, 2018) J/ApJS/245/13 : CDIPS. I. LCs from TESS sectors 6 and 7 (Bouma+, 2019) J/A+A/632/A37 : Well sampled stars FEROS+HARPS radial velocities (Brems+, 2019) J/ApJ/879/49 : Rotation periods for 171 Gaia members NGC6811 (Curtis+, 2019) J/ApJ/879/100 : K2 rotation periods Hyades & Praesepe members (Douglas+, 2019) J/AJ/158/122 : Local structure & star formation history of MW (Kounkel+, 2019) J/A+A/628/A66 : alpha Persei, Pleiades and Praesepe clusters (Lodieu+, 2019) J/ApJ/871/63 : How to constrain your M dwarf II. Nearby binaries (Mann+, 2019) J/A+A/622/L13 : Stellar stream in Gaia DR2 discovery (Meingast+, 2019) J/ApJS/244/21 : Surface rotation & activity of Kepler stars. I. (Santos+, 2019) J/AJ/159/280 : Gaia-Kepler stellar properties catalog.I. 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(Petigura+, 2022) Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- Gaia Gaia EDR3 identifier 21- 29 F9.5 deg RAdeg [279/302] Right Ascension (J2016) 31- 38 F8.5 deg DEdeg [30/47] Declination (J2016) 40- 45 F6.3 mag Gmag [7.67/20.4] Gaia EDR3 G band magnitude 47- 51 F5.3 km/s Voff [0/5] Tangential velocity offset 53- 56 A4 --- SpType Spectral type (1) 58 A1 --- TESS? Has TESS light curve? (2) 60 A1 --- Kepler? Has Kepler light curve? (2) 62- 66 F5.3 mas plx [2.66/3.61] Parallax 68- 72 F5.3 mas e_plx [0.009/0.5] Uncertainty in plx 74- 79 F6.3 d Prot [0.16/44.5]? Rotational period 81- 85 F5.3 d e_Prot [0.003/6]? Uncertainty in Prot 87- 93 A7 --- r_Prot Reference flag on Prot (3) 95 A1 --- l_Li [<] Limit flag on Li 96-100 F5.1 10-13m Li [20/206]? LiI 6708Å equivalent width (mA) 102-105 F4.1 10-13m e_Li [9/21]? Uncertainty in mA 107-112 F6.2 km/s RVel [-71.7/18.4]? Radial velocity 114-118 F5.2 km/s e_RVel [0.02/18]? Uncertainty in RVel 120 I1 --- r_RVel [5/9]? Reference flag on RVel (4) -------------------------------------------------------------------------------- Note (1): Assigned based on the star's BP-RP color and the table from Pecaut & Mamajek, 2013, J/ApJS/208/9. Note (2): Of sufficient quality for running the Notch transit-search pipeline. Note (3): References as follows: 1 = McQuillan+, 2013, J/MNRAS/432/1203 and 2014, J/ApJS/211/24M 2 = Nielsen+, 2013, J/A+A/557/L10 3 = Santos+, 2021, J/ApJS/255/17 and 2019, J/ApJS/244/21 4 = This work. Note (4): References as follows: 5 = Coude 6 = LAMOSTDR5 7 = Gaia DR2 8 = APOGEE DR16 9 = CKS -------------------------------------------------------------------------------- History: From electronic version of the journal References: Newton et al. Paper I. 2019ApJ...880L..17N 2019ApJ...880L..17N Rizzuto et al. Paper II. 2020AJ....160...33R 2020AJ....160...33R Mann et al. Paper III. 2020AJ....160..179M 2020AJ....160..179M Newton et al. Paper IV. 2021AJ....161...65N 2021AJ....161...65N Cat. J/AJ/161/65 Tofflemire et al. Paper V. 2021AJ....161..171T 2021AJ....161..171T Cat. J/AJ/161/171 Mann et al. Paper VI. 2022AJ....163..156M 2022AJ....163..156M Cat. J/AJ/163/156 Newton et al. Paper VII. 2022AJ....164..115N 2022AJ....164..115N Cat. J/AJ/164/115 Barber et al. Paper VIII. 2022AJ....164...88B 2022AJ....164...88B This catalog Wood et al. Paper IX. 2023AJ....165...85W 2023AJ....165...85W Cat. J/AJ/165/85 Thao et al. Paper X. 2024AJ....168...41T 2024AJ....168...41T Cat. J/AJ/168/41 Capistrant et al. Paper XI. 2024AJ....167...54C 2024AJ....167...54C
(End) Prepared by [AAS], Coralie Fix [CDS], 08-Nov-2022
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