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Hugh Jones Hugh Jones Frequency of low-mass exoplanets .. what about the non-detections? SIMON O’TOOLE (AAO/HERTFORDSHIRE), CHRIS TINNEY, JEREMY BAILEY, ROB WITTENMYER (UNSW), PAUL BUTLER (CARNEGIE), BRAD CARTER (SOUTHERN QUEENSLAND)

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Frequency of low-mass exoplanets .. what about the non-detections?. Hugh Jones. SIMON O’TOOLE (AAO/HERTFORDSHIRE), CHRIS TINNEY, JEREMY BAILEY, ROB WITTENMYER (UNSW), PAUL BUTLER (CARNEGIE), BRAD CARTER (SOUTHERN QUEENSLAND). Planet mass function. Jupiter. Earth. Neptune. - PowerPoint PPT Presentation

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Page 1: Hugh Jones

Hugh JonesHugh Jones

Frequency of low-mass exoplanets .. what about

the non-detections?

SIMON O’TOOLE (AAO/HERTFORDSHIRE), CHRIS TINNEY, JEREMY BAILEY, ROB

WITTENMYER (UNSW), PAUL BUTLER (CARNEGIE), BRAD CARTER (SOUTHERN

QUEENSLAND)

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Planet mass functionPlanet mass function

Earth Neptune Jupiter

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Exoplanet distributionsExoplanet distributions

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AAPS (Anglo-Australian Planet AAPS (Anglo-Australian Planet Search)Search)

Nearly 300 nights over last 10 years on 250, V< 7.7 F, G, K, M IV, V stars selected on CaHK and observed with S/N=200 has yielded more than 30 nearby exoplanets (and 18 spectroscopic binaries)

Recent programme of operational upgradesObserving sequencerAutomated iodine cellExposure meter

Near future – fibre feed

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Many ‘noise’ componentsMany ‘noise’ componentse.g., asteroseismological e.g., asteroseismological

signalsignal

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asteroseismological signal function asteroseismological signal function of L/Mof L/M

Based on Sun, Kjeldsen et al. 2008, Alpha Cen A varies by ~20%

plus ~10% over Solar cycle

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Strategy continuous long Strategy continuous long blocks of telescope timeblocks of telescope time

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48 night 48 night run on 24 run on 24 bright starsbright stars

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ExoplanetsExoplanets

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Development of robust Development of robust simulation system for AAPS simulation system for AAPS datadata

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Differences between by star-by-Differences between by star-by-star simulations star simulations

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Differences between by star-by-Differences between by star-by-star simulations star simulations

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DetectabiliDetectability on 48 ty on 48 night runnight run

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Detectability sensitive to mass Detectability sensitive to mass functionfunction

0.01 -10 MJ lines of increasing thickness

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Mass function dN/dM ~MMass function dN/dM ~M-1-1 (~17% of planets host planets with >3 M(~17% of planets host planets with >3 MEE and <16 days) and <16 days)

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ConclusionsConclusions

Simulation system can provide assessment of exoplanetary architectures based on RV data

With multiple telescopes and long campaigns (1m/s precision) can constrain Saturn mass planets out to 6 AUNeptune mass planets out to 1 AUSuper-Earths out to 0.3 AUEarth-mass planets out to 0.1 AU