J/MNRAS/535/2562 Stellar surface inform. from CaII H&K lines (Cretignier+, 2024)

Stellar surface information from the Ca II H&K lines. II. Defining better activity proxies. Cretignier M., Hara N.C., Pietrow A.G.M., Zhao Y., Yu H., Dumusque X., Sozzetti A., Lovis C., Aigrain S. <Mon. Not. R. Astron. Soc. 535, 2562-2584 (2024)> =2024MNRAS.535.2562C 2024MNRAS.535.2562C (SIMBAD/NED BibCode)
ADC_Keywords: Stars, atmospheres ; Stars, activity ; Models ; Spectroscopy Keywords: line: profiles - methods: data analysis - techniques: spectroscopic - stars: activity - stars: chromospheres Abstract: In our former paper I (Cretignier et al., 2024MNRAS.527.2940C 2024MNRAS.527.2940C, Cat. J/MNRAS/527/2940), we showed on the Sun that different active regions possess unique intensity profiles on the Ca II H & K lines. We now extend the analysis by showing how those properties can be used on real stellar observations, delivering more powerful activity proxies for radial velocity correction. More information can be extracted on rotational timescale from the Ca II H & K lines than the classical indicators: S-index and log(R'HK). For high-resolution HARPS observations of alpha Cen B, we apply a principal and independent component analysis on the Ca II H & K spectra time-series to disentangle the different sources that contribute to the disk-integrated line profiles. While the first component can be understood as a denoised version of the Mount-Wilson S-index, the second component appears as powerful activity proxies to correct the RVs induced by the inhibition of the convective blueshift in stellar active regions. However, we failed to interpret the extracted component into a physical framework. We conclude that a more complex kernel or bandpass than the classical triangular of the Mount Wilson convention should be used to extract activity proxies. To this regard, we provide the first principal component activity profile obtained across the spectral type sequence between M1V to F9V type stars. Description: We propose here below to extract the different activity components on the spectra time-series of chromospheric lines such as the Ca II H & K lines by using algorithms designed to solve the blind source separation (BSS) problem. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table_e1.dat 28 107 Stars used for the E1 empirical profiles model_e1.dat 250 90 E1 empirical profiles tab_cenb.dat 130 298 HD128621 extracted time-series spm_cenb.dat 1799 800 HD128621 spectra time-series difference with the master quiet reference spectrum -------------------------------------------------------------------------------- See also: J/MNRAS/527/2940 : Solar activity components intensity profiles (Cretignier+ 2024) Byte-by-byte Description of file: table_e1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Index [0/106] Index of the table 5- 15 A11 --- Name Star name 17- 23 A7 --- Inst Instrument 25- 28 I4 K Teff [3451/5934] Stellar effective temperature -------------------------------------------------------------------------------- Byte-by-byte Description of file: model_e1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Index [0/89] Index of the table 4- 13 F10.6 km/s Wavelength [-34,34] Wavelength in km/s 15- 22 F8.6 --- model-T3500 [0/1] E1 profile at 3500K 24- 32 F9.6 --- model-T3600 [-0.1/1] E1 profile at 3600K 34- 42 F9.6 --- model-T3700 [-0.1/1] E1 profile at 3700K 44- 52 F9.6 --- model-T3800 [-0.1/1] E1 profile at 3800K 54- 61 F8.6 --- model-T3900 [0/1] E1 profile at 3900K 63- 70 F8.6 --- model-T4000 [0/1] E1 profile at 4000K 72- 79 F8.6 --- model-T4100 [0/1] E1 profile at 4100K 81- 88 F8.6 --- model-T4200 [0/1] E1 profile at 4200K 90- 97 F8.6 --- model-T4300 [0/1] E1 profile at 4300K 99-106 F8.6 --- model-T4400 [0/1] E1 profile at 4400K 108-115 F8.6 --- model-T4500 [0/1] E1 profile at 4500K 117-124 F8.6 --- model-T4600 [0/1] E1 profile at 4600K 126-133 F8.6 --- model-T4700 [0/1] E1 profile at 4700K 135-142 F8.6 --- model-T4800 [0/1] E1 profile at 4800K 144-151 F8.6 --- model-T4900 [0/1] E1 profile at 4900K 153-160 F8.6 --- model-T5000 [0/1] E1 profile at 5000K 162-169 F8.6 --- model-T5100 [0/1] E1 profile at 5100K 171-178 F8.6 --- model-T5200 [0/1] E1 profile at 5200K 180-187 F8.6 --- model-T5300 [0/1] E1 profile at 5300K 189-196 F8.6 --- model-T5400 [0/1] E1 profile at 5400K 198-205 F8.6 --- model-T5500 [0/1] E1 profile at 5500K 207-214 F8.6 --- model-T5600 [0/1] E1 profile at 5600K 216-223 F8.6 --- model-T5700 [0/1] E1 profile at 5700K 225-232 F8.6 --- model-T5800 [0/1] E1 profile at 5800K 234-241 F8.6 --- model-T5900 [0/1] E1 profile at 5900K 243-250 F8.6 --- model-T6000 [0/1] E1 profile at 6000K -------------------------------------------------------------------------------- Byte-by-byte Description of file: tab_cenb.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Index [0/297] Index of the table 5- 16 F12.6 d BJD Barycentric Julian date (BJD-2400000) 18- 26 F9.6 m/s RV CCF radial velocity 28- 35 F8.6 m/s e_RV CCF RV error 37- 45 F9.6 --- PCA1 F1 coefficient time-serie from principal component analysis (PCA) method 47- 54 F8.6 --- e_PCA1 F1 PCA error 56- 64 F9.6 --- PCA2 F2 coefficient time-serie from principal component analysis (PCA) method 66- 73 F8.6 --- e_PCA2 F2 PCA error 75- 83 F9.6 --- ICA1 F1 coefficient time-serie from independent component analysis (ICA) method 85- 92 F8.6 --- e_ICA1 F1 ICA error 94-102 F9.6 --- ICA2 F2 coefficient time-serie from independent component analysis (ICA) method 104-111 F8.6 --- e_ICA2 F2 ICA error 113-121 F9.6 m/s Vspan CCF VSPAN 123-130 F8.6 m/s e_Vspan CCF VSPAN error -------------------------------------------------------------------------------- Byte-by-byte Description of file: spm_cenb.dat 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Spectrum at time index = 256 1555-1559 F5.2 % spec-258 Spectrum at time index = 257 1561-1565 F5.2 % spec-259 Spectrum at time index = 258 1567-1571 F5.2 % spec-260 Spectrum at time index = 259 1573-1577 F5.2 % spec-261 Spectrum at time index = 260 1579-1583 F5.2 % spec-262 Spectrum at time index = 261 1585-1589 F5.2 % spec-263 Spectrum at time index = 262 1591-1595 F5.2 % spec-264 Spectrum at time index = 263 1597-1601 F5.2 % spec-265 Spectrum at time index = 264 1603-1607 F5.2 % spec-266 Spectrum at time index = 265 1609-1613 F5.2 % spec-267 Spectrum at time index = 266 1615-1619 F5.2 % spec-268 Spectrum at time index = 267 1621-1625 F5.2 % spec-269 Spectrum at time index = 268 1627-1631 F5.2 % spec-270 Spectrum at time index = 269 1633-1637 F5.2 % spec-271 Spectrum at time index = 270 1639-1643 F5.2 % spec-272 Spectrum at time index = 271 1645-1649 F5.2 % spec-273 Spectrum at time index = 272 1651-1655 F5.2 % spec-274 Spectrum at time index = 273 1657-1661 F5.2 % spec-275 Spectrum at time index = 274 1663-1667 F5.2 % spec-276 Spectrum at time index = 275 1669-1673 F5.2 % spec-277 Spectrum at time index = 276 1675-1679 F5.2 % spec-278 Spectrum at time index = 277 1681-1685 F5.2 % spec-279 Spectrum at time index = 278 1687-1691 F5.2 % spec-280 Spectrum at time index = 279 1693-1697 F5.2 % spec-281 Spectrum at time index = 280 1699-1703 F5.2 % spec-282 Spectrum at time index = 281 1705-1709 F5.2 % spec-283 Spectrum at time index = 282 1711-1715 F5.2 % spec-284 Spectrum at time index = 283 1717-1721 F5.2 % spec-285 Spectrum at time index = 284 1723-1727 F5.2 % spec-286 Spectrum at time index = 285 1729-1733 F5.2 % spec-287 Spectrum at time index = 286 1735-1739 F5.2 % spec-288 Spectrum at time index = 287 1741-1745 F5.2 % spec-289 Spectrum at time index = 288 1747-1751 F5.2 % spec-290 Spectrum at time index = 289 1753-1757 F5.2 % spec-291 Spectrum at time index = 290 1759-1763 F5.2 % spec-292 Spectrum at time index = 291 1765-1769 F5.2 % spec-293 Spectrum at time index = 292 1771-1775 F5.2 % spec-294 Spectrum at time index = 293 1777-1781 F5.2 % spec-295 Spectrum at time index = 294 1783-1787 F5.2 % spec-296 Spectrum at time index = 295 1789-1793 F5.2 % spec-297 Spectrum at time index = 296 1795-1799 F5.2 % spec-298 Spectrum at time index = 297 -------------------------------------------------------------------------------- Acknowledgements: Michael Cretignier, Michael.cretignier(at)physics.ox.ac.uk References: Cretignier et al., Paper I 2024MNRAS.527.2940C 2024MNRAS.527.2940C, Cat. J/MNRAS/527/2940
(End) Patricia Vannier [CDS] 31-Oct-2024
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