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Magnetic activity and radial velocity filtering of young Suns: The weak-line T Tauri stars Par 1379 and Par 2244

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The authors thank the IDEX initiative at Universite Federale Toulouse Midi-Pyrenees (UFTMiP) for funding the STEPS collaboration programme between IRAP/OMP and ESO and for allocating a ‘Chaire d'Attractivite’ to GAJH,… Click to show full abstract

The authors thank the IDEX initiative at Universite Federale Toulouse Midi-Pyrenees (UFTMiP) for funding the STEPS collaboration programme between IRAP/OMP and ESO and for allocating a ‘Chaire d'Attractivite’ to GAJH, allowing her to regularly visit Toulouse to work on MaTYSSE data. SGG acknowledges support from the Science & Technology Facilities Council (STFC) via an Ernest Rutherford Fellowship [ST/J003255/1]. SHPA acknowledges financial support from CNPq, CAPES and Fapemig. This work has made use of the VALD, operated at Uppsala University, the Institute of Astronomy RAS in Moscow, and the University of Vienna, and the SVO Filter Profile Service supported from the Spanish MINECO through grant AyA2014-55216

Keywords: magnetic activity; filtering young; activity radial; velocity filtering; radial velocity; young suns

Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2017

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