ASTEROSEISMOLOGY WITH SUPERWASP · ASTEROSEISMOLOGY WITH SUPERWASP Daniel L Holdsworth University...
Transcript of ASTEROSEISMOLOGY WITH SUPERWASP · ASTEROSEISMOLOGY WITH SUPERWASP Daniel L Holdsworth University...
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ASTEROSEISMOLOGY WITH
SUPERWASPDaniel L Holdsworth
University of Central Lancashire [email protected]
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SUPER WIDE ANGLE SEARCH FOR PLANETS
SuperWASP is a UK based consortium performing the worlds largest survey for transiting extrasolar planets
Over 150 planets discovered so far…
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THE WASP INSTRUMENTS
Fully Automatic:
Roll-off roof system
8 cameras mounted in a 2x4 configuration
Standard 200mm telephoto lenses
8x8 degree FOV
13.7” Pixel size
Broadband filters
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FILTER RESPONSE FUNCTION
4000-7000Å
Ideal for transiting planets
Not ideal for hot stars
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OBSERVING STRATEGY
Capable of observing entire sky in ~40 min
Takes two 30s exposures back-to-back
Focuses on pre-programmed ‘hot spots’
Returns to the same patch of sky every ~10 mins
Typically 3000 data point per season of 100-150 days 5
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OBSERVATIONS
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SUPERWASP PHOTOMETRY
Automated photometry extraction pipeline
USNO B1.0 input catalogue
3.5 pixel aperture = 48”
Transformed to Tycho-2 V magnitudescorrected for primary & secondary extinction
Systematics removed with SysRem (Tamuz+ 2005)
Better than 1% for V<11.5 nd 0.5% for V<9.4Pollacco+ 2006
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SUPER WIDE ANGLE SEARCH FOR PLANETS
>31 million stars
Multi-season multi-site photometry
Large database of time-series photometry
Statistical studies of variable stars
Find ‘rare’ pulsators
Pulsations!
http://astro.phys.au.dk/%7Ejcd/HELAS/puls_HR/ 8
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WASP CAPABILITIES
Dependant on:
Blending
Magnitude
Noise
Data length
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Detection limit of ~0.5mmag for V<11
Holdsworth 2015
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WHAT’S IN THE ARCHIVE?
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LOW-FREQUENCY VARIABLES
~80,000 targets with frequencies 5-50d-1
Plagued by aliasing
Harmonics of binaries
Require a star-by-star analysis
Studies include:
Pulsations in Am stars (Smalley+ 2011)
Am binary stars (Smalley+ 2014)
λ Boo stars with γ Dor & δ Sct pulsations (Paunzen+ 2014, 2015)
Rotational modulation of CP stars (Bernhard+2015)
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See Paul’s talk next & Barry’s on Friday
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HIGH-FREQUENCY VARIABLES
These include some of the rarer pulsating stars:
The roAp stars
Short period δ Sct stars
Compact pulsators
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HIGH-FREQUENCY VARIABLES
These include some of the rarer pulsating stars:
The roAp stars
Short period δ Sct stars
Compact pulsators
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PMS STARS
HD 34282
Pre-main sequence star
IR excess
High-frequency δ Sct pulsations
79.5 & 71.3 d-1
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Amando+ 2004
See Konstanze’s talk on Thursday
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SDBV STARS
Able to probe to at least 1440 d-1
Noise is not fully characterised
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At least 3 newly identified
p and g modes in single starHoldsworth+ in prep
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WASP DATA TO SUPPLEMENT KEPLER (K2/TESS) OBSERVATIONS
KIC 7106205
Amplitude variable star (Bowman & Kurtz 2014)
Amplitude drops from ~5mmag to 0.5mmag
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See Dominic’s talk tomorrow
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WASP DATA TO SUPPLEMENT KEPLER (K2/TESS) OBSERVATIONS
KIC 7106205
Amplitude variable star (Bowman & Kurtz 2015)
Amplitude drops from ~5mmag to 0.5mmag
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WASP DATA TO SUPPLEMENT KEPLER (K2/TESS) OBSERVATIONS
KIC 7106205
Amplitude variable star (Bowman & Kurtz 2015)
Amplitude drops from ~5mmag to 0.5mmag
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SUMMARY
Over 31 million objects
‘All’-sky coverage in approx. V-band
Test for variability in the range of minutes to a decade
Caution: large pixels make blending an issue
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Ideal for extending Kepler/K2/TESS observations andproposing targets for the K2/TESS missions!!