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Showing 1 to 13 of 13 for “"stellar activity"”.

  1. Unearth: Revealing the Effects of Stellar Activity on Exoplanet Host Stars

    … this thesis, I investigate the effect activity has on stellar spectra, using HARPS data of the well observed K1 V star α Centauri B. I compare spectra from high- and low-activity periods (as traced by log R′HK) of α Cen B. I produce ‘relative spectra’ by dividing the high-activity

    qu-belfast Repository record for Unearth: Revealing the Effects of Stellar Activity on Exoplanet Host Stars (opens in a new tab)

  2. Exoplanetary system WASP-3 : measurement of the projected spin-orbit angle and evidence for stellar activity

    … angle between the planetary orbital axis and the stellar rotation axis, ... degrees. I use the new photometric data to refine the system parameters. Additionally, I present evidence for stellar activity, as the spectra obtained on UT June 19, 2008 reveal an increase in radial velocity to a peak …

    mit Repository record for Exoplanetary system WASP-3 : measurement of the projected spin-orbit angle and evidence for stellar activity (opens in a new tab)

  3. Understand thy star, understand thy planet

    … Earth-analogue planets. However, it is now stellar activity that poses a critical challenge on the pathway to detect habitable Earth-like worlds. This thesis is therefore dedicated to understanding the effect stellar activity has on spectroscopically observed radial-velocity (RV) variations …

    qu-belfast Repository record for Understand thy star, understand thy planet (opens in a new tab)

  4. Precise radial velocities and simultaneous magnetic flux estimates from intensity spectra

    … smaller than 1 m/s are drowned out by the stars' activity. The detection of Earth analogues causing an RV effect of about 10 cm/s is, therefore, out of reach at the time of writing. A few avenues are being explored to resume the trend to detect ever lighter planets. These include improving (a) …

    cambridge Repository record for Precise radial velocities and simultaneous magnetic flux estimates from intensity spectra (opens in a new tab)

  5. Effects of starspots activity on optical and near infrared observations of planetary transits

    … thesis, I report on the effects that magnetic stellar activity of solar-type stars induces on stellar light curves involved in the photometric technique for the detection and characterization of transiting extra-solar planets that is one of the most effective detection methods, the first being …

    catania Repository record for Effects of starspots activity on optical and near infrared observations of planetary transits (opens in a new tab)

  6. Exoplanet Atmospheric Characterization using High-Precision Photometry

    … identify exoplanet's atmospheric scattering and stellar activity imprints on the transmission spectrum. Finally, I present a set of Kepler and K2 Ultra Short Period(USP)planets which shows secondary eclipse and phase curve variations. In extension to that I also explored to investigate the …

    catania Repository record for Exoplanet Atmospheric Characterization using High-Precision Photometry (opens in a new tab)

  7. Enshrouded Exoplanetary Systems

    … period planets can show anomalously low apparent stellar activity values caused by planetary mass-loss enshrouding the system. The resulting circumstellar absorption depresses the cores of the Ca II H&K lines, where the activity index log(R'<sub>HK</sub>) is measured. I searched for this effect in …

    the-open-u Repository record for Enshrouded Exoplanetary Systems (opens in a new tab)

  8. Spot evolution on the red giant star XX Triangulum

    Spots on stellar surfaces are thought to be stellar analogues of sunspots. Thus, starspots are direct manifestations of strong magnetic fields. Their decay rate is directly related to the magnetic diffusivity, which itself is a key quantity for the deduction of an activity cycle length. So far, no …

    potsdam-diss Repository record for Spot evolution on the red giant star XX Triangulum (opens in a new tab)

  9. Characterization of exoplanetary systems combining transit timing techniques and radial velocities: From secular perturbations to resonant chains

    … that challenge our understanding of stellar evolution and tidal dissipation. I then focus on sub-Neptune characterization in multi-planet systems, notably focusing on the multi-planet system HIP 41378, where I performed a joint dynamical modelling of the TTV and RV signals of the two …

    trento Repository record for Characterization of exoplanetary systems combining transit timing techniques and radial velocities: From secular perturbations to resonant chains (opens in a new tab)

  10. Ground-based transmission spectroscopy of three inflated Hot Jupiter exoplanets

    … photometrically to correct for influences of stellar activity if necessary. The obtained measurements of the three objects all favor featureless spectra. A variety of atmospheric compositions can explain the lack of a wavelength dependent absorption. But the broad trend of featureless spectra …

    potsdam-diss Repository record for Ground-based transmission spectroscopy of three inflated Hot Jupiter exoplanets (opens in a new tab)

  11. Optimising the Detection of Temperate, Terrestrial Planets around Ultra-Cool Dwarfs with SPECULOOS

    … image reduction, cross-matches with preexisting stellar catalogues, and performs precise aperture and differential photometry every night. With the SSO Pipeline, I address both the instrumental and atmospheric contamination that can prevent detecting small planets. I tackle the first and …

    cambridge Repository record for Optimising the Detection of Temperate, Terrestrial Planets around Ultra-Cool Dwarfs with SPECULOOS (opens in a new tab)

  12. Robotic telescopes & Doppler imaging : measuring differential rotation on long-period active stars

    Auf der Sonne sind viele Phänomene zu sehen die mit der solaren magnetischen Aktivität zusammenhängen. Das dafür zuständige Magnetfeld wird durch einen Dynamo erzeugt, der sich vermutlich am Boden der Konvektionszone in der sogenannten Tachocline befindet. Angetrieben wird der Dynamo teils von der …

    potsdam-diss Repository record for Robotic telescopes & Doppler imaging : measuring differential rotation on long-period active stars (opens in a new tab)

  13. Zeeman-Doppler Imaging of active late-type stars

    Stellare Magnetfelder spielen eine wichtige Rolle bei der Entstehung und Entwicklung von Sternen. Leider entziehen sie sich aber, aufgrund ihrer großen Entfernung zur Erde, einer direkten Beobachtung. Dies gilt zumindest für derzeitige und in naher Zukunft zur Verfügung stehende Instrumente. Um …

    potsdam-diss Repository record for Zeeman-Doppler Imaging of active late-type stars (opens in a new tab)