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CCD photometry of variable stellar sources. Data reduction workflow, assessment of accuracy, case studies

vrijdag, 17 augustus, 2012 - 15:00
Campus: Brussels Humanities, Sciences & Engineering campus
Faculteit: Science and Bio-engineering Sciences
D
2.01
Taavi Tuvikene
doctoraatsverdediging

Photometric studies of variable stars nowadays involve observations with CCD cameras,
producing large amounts of CCD frames, which call for a highly automated data
reduction approach. As data often originate from a variety of telescopes and
instruments, the same reduction steps cannot always be applied to all data. Thus,
what is needed is not a fully automated pipeline, but rather a workflow, an organised
and consistent set of reduction procedures. A workflow for reducing heterogeneous
CCD data was developed in the framework of this thesis.

In order to check for systematic errors arising from data reduction, we carried out
comparative tests that involved independent reductions of the same CCD frames. We
found systematic discrepancies between light curves obtained with different software
packages and concluded that in order to achieve high accuracy, data should be reduced
in a consistent way, preferably using a single software package.

Part II of the thesis is devoted to five case studies involving CCD photometry of
variable stellar sources. We participated in observations of a stellar occultation
by Pluto's moon Charon in 2005. Recording such an event required fast photometry
together with accurate timing of CCD exposures. The occultation observations
eventually led to the determination of Charon's radius and density. The same observing
technique was also applied to the pulsating star CY Aquarii, producing a unique
high-resolution light curve over nearly two periods. We obtained a large amount of
photometric observations of CY Aquarii and presented a total of 155 new times of
maximum, which were analysed using an O–C diagram.

We discovered the variability of the Delta Scuti star GSC 08613–02122. Our results
revealed the presence of erratic amplitude and phase variations, which we showed not
to be of instrumental nor procedural origin. A deep study of the close binary star
GSC 04778 – 00152 was carried out, involving photometric and spectroscopic
observations. The star was found to have a 1-magnitude fainter visual companion about
2 arcseconds away from the binary. We derived the parameters of the binary system
from light-curve modelling.

Finally, we applied the workflow to a target for which it was initially designed –
the open cluster NGC 3293, known to contain 11 Beta Cephei-type pulsators and numerous
other variable stars. The cluster was photometrically monitored for a time span of
ten years (1997–2007), resulting in a massive set of over 22000 CCD frames. Careful
reduction and analysis led to the conclusion that truly constant stars among brighter
cluster members are rather rare. Special focus was given to the long-term variability
of the cluster stars.