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 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 (Kürster et al. 2000)

Ø Coronal X-rays (XMM-Newton - poster #68 S. Raetz) Ø Astrosphere (HST) Ø Chromospheric, Magnetic Field, , Magnetic Field, RV, RV, Age, Inclination Age, Inclination (HARPSpol) Ø Rotation period, Gyrochronology, F/S , F/S (TESS(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 Eliana M. Amazo �-Factor � � Amazo Shapiro et al. Submitted � ⨀ Hor = IP - Gómez = 0.191 - Gómez et al. Submitted MORE ACTIVE GPS / Prot = 0.158 FACULAE TO SPOT RATIO TESS Science Conference I Faculae/Spot LESS ACTIVE F/S ⨀ � Hor ratio ~ 3 ~ 0.74 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 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 twins • Stellar dynamo • • 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