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CCD Observations and Preliminary Analysis of the “End-of-the-Line” W UMa Eclipsing Binary V523 Cas Presenting Authors: Russell M. Genet, Orion Observatory Thomas C. Smith, Dark Ridge Observatory Contributing Authors: Dirk Terrell, Southwest Research Institute Laurance Doyle, SETI Institute
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Program Overview First year “pilot” Concentrated on two W UMa binaries Complete light curves every night Often from two observatories Primary science goal Study changes in light curve shapes Secondary science goals Precise seasonal ephemeredes Consider hot “Jupiter” transits Technical goals Develop analytical tools Explore photometric precision
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Presentation Outline Introduction to W UMa Binaries Observations and Reduction V523 Cas Preliminary Analysis V523 Cas “Movie” Question & Answers Russ Tom Russ Tom All
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Presentation Outline Introduction to W UMa Binaries Observations and Reduction V523 Cas Preliminary Analysis V523 Cas “Movie” Question & Answers Russ Tom Russ Tom All
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Photometric / Magnetic Variability Intrinsic Period Changes Third – Body Period Changes Planetary Transits Introduction to W UMa Binaries
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Photometric / Magnetic Variability Intrinsic Period Changes Third – Body Period Changes Planetary Transits Introduction to W UMa Binaries
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W UMa’s Binaries Over contact Dissimilar stars Common envelope Yet nearly same temperature Very Different masses Huge transfer of energy Large to small
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Color – Period Relationship
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AW More evolved Higher masses Thicker envelopes Unevolved Lower masses Cannot achieve equilibrium Period changes Light curve variability Brighter star Dimmer star A and W Type W-UMa Binaries
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W Type W UMa Variability Large Rosby number Fast rotators Long convection turnover times For single stars Late Slow rotator For W UMa Late Fast rotator Ideal “laboratories” for magnetic activity Revealed through changing light curves “Movies” instead of disjointed snapshots
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Bright Northern Short Period W UMa’s
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Photometric / Magnetic Variability Intrinsic Period Changes Third – Body Period Changes Planetary Transits Introduction to W UMa Binaries
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Intrinsic Period Changes Angular Momentum Loss Gravitational radiation Mass loss Magnetic breaking Mass transfer between stars Applegate effect
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Photometric / Magnetic Variability Intrinsic Period Changes Third – Body Period Changes Planetary Transits Introduction to W UMa Binaries
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SETI Visit with Laurance Doyle
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Barycenters
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V523 Cas Long-Term O-C
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CM Dra Program
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Photometric / Magnetic Variability Intrinsic Period Changes Third – Body Period Changes Planetary Transits Introduction to W UMa Binaries
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Transit Perspective II I Inclination Angle
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High Inclination W UMa Stars
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Solar Radii vs. Line-of-Sight Inclination Angle
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Three Transit Plots
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Presentation Outline Introduction to W UMa Binaries Observations and Reduction V523 Cas Preliminary Analysis V523 Cas “Movie” Question & Answers Russ Tom Russ Tom All
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Dark Ridge Observatory (DRO)
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Orion Observatory (OO)
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Image Reduction Flowchart
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DRO/OO Observational Database 2004
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Light-Curve Database
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Raw Text File to Raw Excel 25K Sub buildPhase() ' use the getPhase function to populate the phase field Dim myDb As Database Dim myRs As Recordset Set myDb = CurrentDb() Set myRs = myDb.OpenRecordset("Select * from tblLightCurve", dbOpenDynaset) Do While Not myRs.EOF myRs.Edit myRs.Fields("Phase").Value = getPhase(myRs.Fields("HJD").Value).phase myRs.Fields("Cycle").Value = getPhase(myRs.Fields("HJD").Value).Cycle myRs.Update myRs.MoveNext Loop MsgBox "Done" End Sub Sub buildAdjustedPhase() ' use the getPhase function to populate the phase field Dim myDb As Database 1 2 3 Raw Source Database 1a
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Presentation Outline Introduction to W UMa Binaries Observations and Reduction V523 Cas Preliminary Analysis V523 Cas “Movie” Question & Answers Russ Tom Russ Tom All
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V523 Cas Preliminary Analysis
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Analysis Considerations Specialized analysis Complete light curves only Many complete curves Multiple observatories Preliminary Analysis not completed No ensemble photometry yet Automation Not just labor efficiency Parametric outer loop In conjunction with WD (Terrell)
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Edits and Adjustments
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25K Database24,761 Bad Weather-3,232 C&K Zeros-54 3-Sigma Cuts-173 V-C Outliers-54 21K Database21,248 Edits and Adjustments
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Beginning and Ending Database Rows
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Typical DRO 21K Database Light Curve
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Typical OO 21K Database Light Curve
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Classical Analysis
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Robert Nelson’s Minima23
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V523 Cas Seasonal O-C
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Phase-Binned Analysis
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Eclipsing Binary Phases 0.000.250.500.000.750.25
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HJD to Phase Transformation Epoch – JD Obs Period {} = Φ Epoch = 2453234.63551606 Period = 0.23369537
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21K Data Point Phase Plot V523 Cas
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Phase Binning Epoch – JD Obs Period {} = Φ
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Phase – Binned Analysis I...
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Phase – Binned Analysis II... Difference Engine...
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V523 Cas 2004 Season Master Curve Utilizing the Binning Method
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Symmetry Analysis
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Symmetry Algorithm … … Y 2 = Y 1 + (X 2 – X 1 )(Y 3 – Y 1 ) (X 3 – X 1 ) Σ N S=1 (Y 2 L – Y 2 R) =... …… N132N123 X1X1 X1X1 X2X2 X3X3 X2X2 X3X3 LeftRight Y1Y1 Y3Y3 Y2Y2 Y1Y1 Y3Y3 Y2Y2
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Total Phase
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Secondary Minima Narrow
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First Maxima Narrow
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Presentation Outline Introduction to W UMa Binaries Observations and Reduction V523 Cas Preliminary Analysis V523 Cas “Movie” Question & Answers Russ Tom Russ Tom All
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Making the Movie 35 pictures were created from the binned, zero-shifted V-C plots. The pictures have been arranged in chronological order to represent the nightly results and to show the night-to- night changes in the shapes of the light curves as compared to the master season curve created from all 21K observations. The following 35 frames represent a visual depiction of those changes in a somewhat dynamic show.
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots
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Frame 1
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 2
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 3
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 4
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 5
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 6
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 7
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 8
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 9
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 10
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 11
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 12
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 13
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 14
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 15
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 16
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 17
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 18
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 19
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 20
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 21
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 22
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 23
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 25
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 26
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 28
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 29
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 30
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 31
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 32
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 33
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 34
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V523 Cas 2004 Seasonal Movie of Binned Difference Plots Frame 35
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Preliminary Conclusions Changes in light curve shapes Definite changes September to December Possible changes within August and September Small O-C variations Difficult to detect within season But likely between seasons May detect distant “Jupiters” (over several years) Transits Several W UMa candidates Detection difficult due to changing times of transit / spots
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Potential Future Efforts Dirk Terrell, Darth’s other side! The Master Modeler… Photometric precision Parametric analysis / automation Data archives to AAVSO Give V1191 Cyg THE treatment Between season comparisions Wilson – Devinney Analysis With his extensive Galactic travels we asked the expert for his assistance with the WD analysis.
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Questions & Answers Genet / Smith V523 Cas 2004 Seasonal Report
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