THE PHOTOMETRY GROUP
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Transcript of THE PHOTOMETRY GROUP
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THE PHOTOMETRY GROUPTeam members:Ivana BariiDino BekteeviNeven GoleniLucija abariTeam leaders:Aleksandar CikotaDijana VrbanecIntroductionPhotometry is a procedure of measuring visible light in units that are weighted according to the sensitivity of the human eyeVariables - stars that change their brightnessSome stars vary in brightness because of physical changes, such as pulsations or eruptions and the others vary in light output due to eclipses or stellar rotation
Our aimsReduce 20Gb of data from Tel Aviv Observatory and search for variable stars (18 nights)Plot light curves of all stars (35 000)Check all the light curves for variable starsDeterming if those stars are unknownPhotometry in CanopusApproximately determine variable stars typesPhotometry of an exoplanet Check mira stars
Pythonlearning basics of Pythonwriting a script for sorting images
MaxIm DLcalibrating photos of variable stars
Plot script in Pythonmanipulates data created by the photometry script and creates graphical preview of numeric data
Variable stars plotsWe checked all the plots (35 000)Found 80 variable stars
7Variable stars
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9Output dataScript that prints out right ascension, declination, and magnitude
10AAVSOAmerican association of variable stars observersWeb page that contains a list of variable starswww.aavso.org contains VSX
11Canopus Program for plotting precise light curves
User is able to read time, magnitude, and derived period
Exoplanet XO-2Exoplanet or extrasolar planet is a planet thatevolves around other star (not Sun)There are several ways of detecting exoplanets:- the transit photometry method our method- the spectroscopic method- astrometry method- gravity lensing
198 photos of XO-2 taken in the night of 07/03/2009 from La Sagra observatorya lot of noise on images because of bad weatherPlotting light curve in CanopusDetermining all orbital parameters of the extrasolar planet XO-2 from its light curve
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Mira variablessearch for new LPV-s (long period variables or mira ( Ceti) stars) that were considered as potential miras in Vinjan Observatory databaseCheck in other databasesPython- extracting star names and coordinates from Vinjan Observatory mira database listSearch in SDSS and SIMBADMira variables - SDSS
Mira variables - SIMBAD
Future goalsTo publish new variable stars that we have found and their light curves in JAAVSO (Journal of the AAVSO)
Finish the search for new mira variables
Thank you for your attention!Any questions?22