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Astronomy Science Data Kepler data, sensor pos 41 Search for micro variables, object 4, 5, 6, Kepler data pos 41

Coordinates/Direction :	RA: 290.427033o, DEC: +43.624771o. Angle calculator
Object size :	sensor about 1 x 1 degrees
Object magnitude :	-
Object :	Area of Cygnus, Lyra and Draco
Date :	2009-08-19 to 2013-04-08
Lens/telescope :	Kepler Space observatory
Film/CCD :	Sensor position 41 (from sensor 41, 42, 43, 44), Kepler data, credits: STScI
Filter/Wavelength :	420 to 900 nm
Exp. time :	27 minutes x 44 frames
Image process tool :	AstroImageJ, Fitswork, Irfanview
Processing :	Multi aperture analyze
Site :	Space
Comment :	This time I'm concentrating me of the left middle part of the area.
More to know :

Crop around analyze area

Object size :	crop area about 0.3 x 0.3 degrees
Object magnitude :	-
Object :	Area of Cygnus, Lyra and Draco
Date :	2009-08-19 to 2013-04-08
Lens/telescope :	Kepler Space observatory
Film/CCD :	Sensor position 41 (from sensor 41, 42, 43, 44), Kepler data, credits: STScI
Filter/Wavelength :	420 to 900 nm
Exp. time :	27 minutes x 44 frames
Image process tool :	AstroImageJ, Fitswork, Irfanview
Processing :	Multi aperture analyze
Site :	Space
Comment :	These time it's the stars with label T8, T10 and T11 that we analyze. The T1 star was oversaturated and not usable.
Object :	T8= KIC 8095028, star T10= KIC 8095275, eclipsing binary T11= KIC 8095110, eclipsing binary of Algol type
More to know :	T8, KIC 8095028: http://simbad.u-strasbg.fr/ simbad ... T10, KIC 8095275: http://simbad.u-strasbg.fr/ simbad ... T11, KIC 8095110: http://simbad.u-strasbg.fr/ simbad ...

Differential Photometry of variable star with micro variations

Image process tool :	AstroImageJ, Irfanview
Processing :	Multi aperture analyze
Site :	Space
Comment :	The T objects are offset along the Y-axis. As you can see they show different wave pattern compare to the reference stars at bottom. I have now sent these data to Hans and Thomas for further analyze. Now waiting exited if they find some of these star to be unknown. I come back about this in a few days.
More to know :	Semi regular variable star, Wikipedia: https://en.wikipedia.org/ wiki/ Semiregular variable star

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