John Barnes - Centre for Astrophysics Research (CAR) - University ...

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John Barnes - Centre for Astrophysics Research (CAR) - University ...

John Barnes - Centre for Astrophysics Research (CAR) - University ...

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ROPS RVs <strong>for</strong> eight M5.5-M8 dwarfs• 4 epochs spread over 6 nights: 5.1 – 18.6 ms

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Bayesian inference of T Tauri star properties using multi-wavelength ...

Spectro- Astrometry of Herbig Ae/Be Binary Systems

Name Organisation Monday Tuesday Wednesday Thursday Abbott ...

ROPS RVs <strong>for</strong> eight M5.5-M8 dwarfs• 4 epochs spread over 6 nights: 5.1 – 18.6 ms

Sensitivities• For UVES - 5 ms -1 - 1, 2, 3- K* sensitivities3,6,9 M at M6V2,4,6 M at M9V

Page 1 and 2: Red Optical Planet Survey (R PS):A
Page 3 and 4: • Kepler planet candidates:M dwar
Page 5 and 6: VisibleRed opticalNear infrared Y-b
Page 7 and 8: RV sensitivity in the red-optical
Page 9 and 10: Deconvolution S/N in a single spect
Page 11 and 12: Proxima Centauri - a training datas
Page 13 and 14: Proxima Centauri Archival UVES data
Page 15: Poisson limited precision usingdeco
Page 19: Summary• Initial 2 night study of