Eliana Amazo-Gómez 1, 2, 3, Julián Alvarado-Gómez3 Jeremy J. Drake 3, Alexander I. Shapiro 1 Sami K. Solanki 1,4 1 Max Planck Institute for Solar System Research 2 Georg-August Universität Göttingen 3 HarvarD-Smithsonian Center for Astrophysics 4 Kyung Hee University IOTA HOROLOGII: FAR BEYOND THE SUN CAMPAING LONG TERM SIMULTANEOUS MULTI-TECHNIQUE MULTI-WAVELENGHT FOLLOW UP Ca II H&K Since late 2002RV data Since late 1992 Cycle period 1.6 yrs. (Metcalfe et al. 2010) Giant exoplanet (Kürster et al. 2000) Ø Coronal X-rays (XMM-Newton - poster #68 S. Raetz) Ø Astrosphere (HST) Ø Chromospheric, Magnetic FielD, RV, , Magnetic FielD, RV, Age, Inclination Age, Inclination (HARPSpol) Ø Rotation perioD, Gyrochronology, F/S (TESS, F/S (TESS)) Eliana M. Amazo-Gómez TESS Science Conference I 2 ROTATION PERIOD ANALYSIS S2 TESS LC Eliana M. Amazo-Gómez TESS Science Conference I 3 SOLAR CASE FOR PSEUDO-ISOLATED MAGNETIC FEATURES Spots Facular region Infl. 1 Infl. 2 Prot = 26.65 ± 2.368 D Prot = 27.84 ± 2.47 D TSI: TIM/SORCE Observations Amazo-Gómez et al. SubmitteD Eliana M. Amazo-Gómez TESS Science Conference I 4 Period, days Period, days 90 30 5 1 90 30 5 1 -0 10-0 10 10-1 10-1 10-2 SPOT DOM. 10-2 -3 10 10-3 -4 Norm. Power Norm. Power 10 TR 10-4 0.1 1.0 10.0 Factor 0.1 1.0 10.0 1.0 - � 1.0 0.8 0.8 16.1d, 49.8d 0.6 FACULAE DOM. 32.3d 0.4 GPS 0.6 0.4 31.6d Norm. Power 0.2 0.0 Norm. Power 0.2 0.1 1.0 10.0 0.0 0.1 1.0 10.0 1.10 Infl. 1 1.08 1.05 Infl. 2 1.06 1.04 Gradient 1.00 1.02 5.6d 0.95 Gradient 1.00 7.4d 0.98 0.1 1.0 10.0 4.0d Frequency, µHz 0.96 0.1 1.0 10.0 Linear Decay of spots Frequency, µHz Lifetime: 90 D, 50d, 20d, 12d - Spot component of variability - Facular component of variability Shapiro, Amazo-Gómez et al. SubmitteD - Total variability Eliana M. Amazo-Gómez TESS Science Conference I 5 FACULAE TO SPOT RATIO MORE ACTIVE Factor - � LESS ACTIVE Shapiro et al. SubmitteD Amazo-Gómez et al. SubmitteD �⨀ = IPGPS/Prot = 0.158 Faculae/Spot⨀ ratio ~ 3 ��Hor = 0.191 F/S�Hor ~ 0.74 Eliana M. Amazo-Gómez TESS Science Conference I 6 GYROCHRONOLOGY APPROACH McQuillan et al. 2014 Prot = 7.42 [d] & Teff ~ 6189 [K] Age < 1 Gyr Eliana M. Amazo-Gómez TESS Science Conference I 7 LITHIUM AGE-DATING MelenDez et al. 2013 Lithium age-dating → 600 - 1000 [Myr] Vsini fitting → 6.0 [Km/s] Teff → 6189 [K] Log g → 4.45 � = 49° ± 8° Eliana M. Amazo-Gómez TESS Science Conference I 8 MULTI-TECHNIQUE FOLLOW UP K-LINE CORE H-LINE CORE Amazo-Gómez + In prep. Eliana M. Amazo-Gómez TESS Science Conference I 9 MULTI-TECHNIQUE FOLLOW UP AlvaraDo-Gómez + In prep. Amazo-Gómez + In prep. Eliana M. Amazo-Gómez TESS Science Conference I 10 • Comprehensive stellar analysis requires simultaneous multi-techniques, multi- wavelength data. • Valuable information to characterize magnetism anD activity, helpful for dealing with stellar noise in exoplanetary hunting. • GPS methoD works not just for the determination of stellar rotational periods, but also to interpret stellar surfaces –> F/S ratio. • Better understanding of the stars woulD allow more realistic exoplanet characterizations. Eliana M. Amazo-Gómez TESS Science Conference I 11 Eliana M. Amazo-Gómez TESS Science Conference I 12 SATIRE moDel : Spectral And Total IrraDiance REconstruction SoliD angle Spectral facular contrast Spectral spot contrast Quiet Sun Faculae fraction area contribution Spot fraction area contribution i – i-th active region t – evolution time Eliana M. Amazo-Gómez TESS Science Conference I 13 Spots Facular region TIM/SORCE Amazo-Gómez et al. In prep Eliana M. Amazo-Gómez TESS Science Conference I 14 TSI: VIRGO/SOHO Current methods With GPS Eliana M. Amazo-Gómez TESS Science Conference I 15 Rotation periods from real Solar twins will allow us to characterize stellar systems • Stellar activity with maybe closser Earth twins • Stellar Dynamo • Stellar evolution • Gyrochronology • + Vsin -> Inclination • Phase for exoplanet unDerstanDing • AbunDance fitting • Using GPS: Facula/Spot ratio - McQuillan et al. 2014 - GPS Eliana M. Amazo-Gómez TESS Science Conference I 16 This work) [ Days ] This work) [ Days ] PerioD ( PerioD ( Amazo-Gómez et al. (in Prep.) Eliana M. Amazo-Gómez TESS Science Conference I 17 Amazo-Gómez et al. In prep Eliana M. Amazo-Gómez TESS Science Conference I 18 Inclination angle = 62.43 deg Vsini = 2.4 Km/s Period PS = 14.86 days Period In1 = 17.01 days Period In2 = 15.60 days Inflection 1 = 11.46 days Inflection 2 = 4.61 days Inflection 3 = 4.61 days Ratio 1 = 0.77 Ratio 2 = 0.31 Ratio 3 = 0.31 Eliana M. Amazo-Gómez TESS Science Conference I 19 Amazo-Gómez et al. In prep Eliana M. Amazo-Gómez TESS Science Conference I 20.