White Dwarf Variability Determiningabbott/REU/Wolf_finaltalk.pdf · 2020. 7. 31. · White Dwarf...
Transcript of White Dwarf Variability Determiningabbott/REU/Wolf_finaltalk.pdf · 2020. 7. 31. · White Dwarf...
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Determining White DwarfVariability
Participant: Shania WolfAdvisers: Dr. Kilic, Alekzander Kosakowski
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Overview: ● Introduction○ White dwarfs, variable stars
● The Missions:○ ASASSN & TESS
● Research Goal● Data Acquisition● Methods● ASASSN & TESS Comparisons● Discoveries● Future
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All About White Dwarfs
● Very small, dim, late-stage stars○ Fate of low/medium mass MS stars
● Earth-sized radius, but sun-sized mass
Graphic via: AStronomy.Swin.eduGraphic via: ESA.int
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All About Variable Stars
● Varying brightness○ Intrinsic
■ Caused by the star itself■ Ex: Pulsations, eruptions
○ Extrinsic■ Other bodies affecting star■ Ex: Eclipsing binaries, sunspots
● Any stellar type
Graphic via: Exoplanet.sg
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TESS Mission
Main science objective: ● Discover transiting exoplanets orbiting stars
>12th magnitudeCamera specs: ● Pixel scale: 21 arcseconds per pixel
Cadence: How often they take images & sky coveragePros:● Space based● Less noise● Continuous data
Cons:● Large pixel scale● Surveys some regions more frequently than
others
Graphic via: TESS.MIT.edu
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ASAS-SN Mission
Main science Objective:● Discover supernovae and other
astronomical transients >17th magnitude
Pixel scale: ● 7.8 arcseconds per pixel
CAdencePros:● Small pixel scale● Can survey entire sky every day
Cons: ● Ground-Based
○ Aliasing● Can only observe at night● Noisy
Image via: Astronomy.Ohio-State.edu
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Research Goal:
Discover variable white dwarfs using ASASSN & TESS targets
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Data Acquisition
● Obtained from ASAS-SN &
TESS Surveys○ White dwarfs determined
from Gentile-Fusillo et al. (2019) based on GAIA■ DR2
○ There are 500,000 WD in dataset
○ Our total targets: 8,500■ <17th magnitude due to
ASASSN & TESS restrictions Gentile-Fusillo et al. (2019)
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Methods:
● Data plotted using code by Alekzander Kosakowski & Shania Wolf
○ Produces light curves ->
■ Detection of variable targets
● Lomb-Scargle
■ Significance >20
● Significance is peak/mean power
● < 20 start getting into noise
● Check literature for targets○ Simbad, Vizier
● If not, we likely discovered the target
Target: 4670655408301574144
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ASASSN Targets’ Significance
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TESS Targets’ Significance
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Target Comparison: 1099005032089977984
ASASSN TESS
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Target Comparison: 4670655408301574144
ASASSN TESS
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Discoveries
By the Numbers:
● 44 variables found by both ASASSN &
TESS
● 98 variables found by ASASSN
● 179 variables found by TESS
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Interesting Findings:
Cataclysmic Variable: 2134077749400112128
Eclipsing Binary: 2791084432881749760
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Interesting Findings:
RR Lyrae: 5574654180530308736
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What’s Next?
● Expand limits on significance
● Follow up observations on discoveries
○ If no spectroscopy
● Constrain parameters of each object
● Publish
Acknowledgements:
● Dr. Kilic & Alekzander Kosakowski
● OU REU Program:
○ Dr. Abbot
○ Dr. Strauss Image via: Palomar Observatory/STScI/WikiSky
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Questions?